The QWeak experiment at Jefferson Lab aims to measure the weak charge of the proton to 4% precision through parity-violating electron scattering. It collected data by shooting a highly polarized electron beam at a liquid hydrogen target and precisely measuring the tiny left-right asymmetry in scattered electrons. The experiment pushed precision by reducing systematic uncertainties in beam polarization and helicity-correlated effects to the parts-per-billion level. It also pushed intensity limits with a high-power cryotarget and event rates up to 800 MHz by using an integration mode of data collection over many polarization windows. Preliminary results from the completed experiment will be released in fall 2017.
Parity-Violating and Parity-Conserving Asymmetries in ep and eN scattering in...Wouter Deconinck
This document summarizes the QWeak experiment, which aimed to measure the weak charge of the proton to 1% accuracy by measuring tiny parity-violating asymmetries in electron-proton scattering. It discusses the challenges of measuring part-per-billion asymmetries with percent-level precision. Preliminary results from a subset of the data were in agreement with the Standard Model prediction of the proton's weak charge. Further analysis is ongoing to understand background effects and improve uncertainties. The full dataset will allow a more precise test of the Standard Model at the precision frontier.
UCSD NANO 266 Quantum Mechanical Modelling of Materials and Nanostructures is a graduate class that provides students with a highly practical introduction to the application of first principles quantum mechanical simulations to model, understand and predict the properties of materials and nano-structures. The syllabus includes: a brief introduction to quantum mechanics and the Hartree-Fock and density functional theory (DFT) formulations; practical simulation considerations such as convergence, selection of the appropriate functional and parameters; interpretation of the results from simulations, including the limits of accuracy of each method. Several lab sessions provide students with hands-on experience in the conduct of simulations. A key aspect of the course is in the use of programming to facilitate calculations and analysis.
Our new paper on exciton interference in hexagonal boron nitride is online. In this paper we show that the excitonic peak at finite momentum is formed by the superposition of two groups of transitions that we call KM and MK′ from the k-points involved in the transitions. These two groups contribute to the peak intensity with opposite signs, each damping the contributions of the other. The variations in number and amplitude of these transitions determine the changes in intensity of the peak. Our results unveil the non-trivial relation between valley physics and excitonic dispersion in h-BN.
1) The document discusses lattice vibrations (phonons) in solids, including models for heat capacity. It describes Einstein's model of independent harmonic oscillators and Debye's more accurate model treating the solid as a continuous elastic medium.
2) Key aspects of the Debye model include treating the solid as having a spectrum of vibrational frequencies up to a maximum cutoff, and integrating over these frequencies to determine properties like heat capacity.
3) The document also discusses phonon momentum, dispersion relations, vibrational modes in lattices with diatomic bases, and the use of Brillouin zones to describe vibrational properties in periodic solids.
1. Hartree-Fock theory describes molecules using a linear combination of atomic orbitals to approximate molecular orbitals. It treats electrons as independent particles moving in the average field of other electrons.
2. The Hartree-Fock method involves iteratively solving the Fock equations until self-consistency is reached between the input and output orbitals. This approximates electron correlation by including an average electron-electron repulsion term.
3. The Hartree-Fock method satisfies the Pauli exclusion principle through the use of Slater determinants, which are antisymmetric wavefunctions that go to zero when the spatial or spin coordinates of any two electrons are identical.
This document discusses phonons and lattice vibrations in crystalline solids. It begins by introducing phonons as quantized vibrational energy states that propagate through the lattice. It then covers topics like modeling atomic vibrations, phonon dispersion relations, vibrational modes, and the density of phonon states. The document also discusses how phonons contribute to various thermodynamic and transport properties of solids, including specific heat, thermal expansion, and thermal conductivity. It compares the Debye and Einstein models for the phonon density of states and explains how phonon-phonon scattering influences thermal conductivity.
Parity-Violating and Parity-Conserving Asymmetries in ep and eN scattering in...Wouter Deconinck
This document summarizes the QWeak experiment, which aimed to measure the weak charge of the proton to 1% accuracy by measuring tiny parity-violating asymmetries in electron-proton scattering. It discusses the challenges of measuring part-per-billion asymmetries with percent-level precision. Preliminary results from a subset of the data were in agreement with the Standard Model prediction of the proton's weak charge. Further analysis is ongoing to understand background effects and improve uncertainties. The full dataset will allow a more precise test of the Standard Model at the precision frontier.
UCSD NANO 266 Quantum Mechanical Modelling of Materials and Nanostructures is a graduate class that provides students with a highly practical introduction to the application of first principles quantum mechanical simulations to model, understand and predict the properties of materials and nano-structures. The syllabus includes: a brief introduction to quantum mechanics and the Hartree-Fock and density functional theory (DFT) formulations; practical simulation considerations such as convergence, selection of the appropriate functional and parameters; interpretation of the results from simulations, including the limits of accuracy of each method. Several lab sessions provide students with hands-on experience in the conduct of simulations. A key aspect of the course is in the use of programming to facilitate calculations and analysis.
Our new paper on exciton interference in hexagonal boron nitride is online. In this paper we show that the excitonic peak at finite momentum is formed by the superposition of two groups of transitions that we call KM and MK′ from the k-points involved in the transitions. These two groups contribute to the peak intensity with opposite signs, each damping the contributions of the other. The variations in number and amplitude of these transitions determine the changes in intensity of the peak. Our results unveil the non-trivial relation between valley physics and excitonic dispersion in h-BN.
1) The document discusses lattice vibrations (phonons) in solids, including models for heat capacity. It describes Einstein's model of independent harmonic oscillators and Debye's more accurate model treating the solid as a continuous elastic medium.
2) Key aspects of the Debye model include treating the solid as having a spectrum of vibrational frequencies up to a maximum cutoff, and integrating over these frequencies to determine properties like heat capacity.
3) The document also discusses phonon momentum, dispersion relations, vibrational modes in lattices with diatomic bases, and the use of Brillouin zones to describe vibrational properties in periodic solids.
1. Hartree-Fock theory describes molecules using a linear combination of atomic orbitals to approximate molecular orbitals. It treats electrons as independent particles moving in the average field of other electrons.
2. The Hartree-Fock method involves iteratively solving the Fock equations until self-consistency is reached between the input and output orbitals. This approximates electron correlation by including an average electron-electron repulsion term.
3. The Hartree-Fock method satisfies the Pauli exclusion principle through the use of Slater determinants, which are antisymmetric wavefunctions that go to zero when the spatial or spin coordinates of any two electrons are identical.
This document discusses phonons and lattice vibrations in crystalline solids. It begins by introducing phonons as quantized vibrational energy states that propagate through the lattice. It then covers topics like modeling atomic vibrations, phonon dispersion relations, vibrational modes, and the density of phonon states. The document also discusses how phonons contribute to various thermodynamic and transport properties of solids, including specific heat, thermal expansion, and thermal conductivity. It compares the Debye and Einstein models for the phonon density of states and explains how phonon-phonon scattering influences thermal conductivity.
Direct and indirect excitations in boron nitride: atomic structure and electr...Claudio Attaccalite
This document discusses the optical properties of boron nitride (BN) as studied through many-body perturbation theory and electron energy loss spectroscopy (EELS) experiments. It finds that BN has an indirect bandgap of 5.79 eV according to calculations, and a sharp exciton mode is visible in EELS between 0.4-1 Å-1 momentum transfer. Many-body calculations reveal the exciton has reduced dispersion compared to the band structure, in good agreement with EELS data. Different stackings of BN layers are also considered, with ABC stacking found to have a very flat and possibly direct excitonic gap.
THE FEYNMAN-STUCKELBREG INTERPRETATION OF E<0 SOLUTIONSHusnain Ali
The document discusses relativistic quantum mechanics and the Klein-Gordon equation. It describes the Feynman-Stuckelberg interpretation of negative energy solutions to the Klein-Gordon equation, which interprets them as representing positive energy anti-particles moving forward in time. This resolves issues with negative probabilities and allows a consistent treatment of antiparticles. The interpretation is illustrated using a diagram of double electron scattering, showing it accounts for both time orderings through particle-antiparticle pair production and annihilation.
In recent years, there have been great interest in alkali-O2 batteries with extremely high specific energies. Li-O2 batteries offer the greatest theoretical specific energy, but currently suffer from large charging overpotentials and low power densities. Na-O2 offers a somewhat lower theoretical specific energy compared to Li-O2, but still a substantial improvement over today’s lithium-ion batteries. In this talk, we will demonstrate how first principles calculations can provide crucial insight into the workings of alkali-O2 batteries. We will elucidate a facile mechanism for recharging Li2O¬¬2 that is accessible at relatively low overpotentials of ~0.3-0.4V and is likely to be kinetically favored over Li2O2 decomposition. We will also demonstrate that sodium superoxide (NaO2) is predicted to be considerably more stable than sodium peroxide (Na2O2) at the nanoscale. Using first principles calculations, we derive the specific electrochemical conditions to nucleate and retain NaO2 and comment on the importance of considering the nanophase thermodynamics when optimizing an electrochemical system.
1. The Stern-Gerlach experiment discovered that silver atoms split into two beams, indicating the presence of an intrinsic "spin" angular momentum of 1/2 beyond orbital angular momentum.
2. Elementary particles are classified as fermions, with half-integer spin, and bosons, with integer spin. The spin of the electron is represented by a two-component spinor.
3. In a magnetic field, the spin precesses around the field direction at the Larmor frequency, independent of initial spin orientation. This principle underlies paramagnetic resonance and nuclear magnetic resonance spectroscopy.
This document discusses statistical mechanics and the distribution of energy among particles in a system. It provides 3 main types of statistical distributions based on the properties of identical particles: Maxwell-Boltzmann, Bose-Einstein, and Fermi-Dirac statistics. Maxwell-Boltzmann statistics applies to distinguishable particles, while Bose-Einstein and Fermi-Dirac apply to indistinguishable particles (bosons and fermions respectively), with the key difference being that fermions obey the Pauli exclusion principle. The document also discusses applications of these distributions, including the Maxwell-Boltzmann distribution law for molecular energies in an ideal gas.
The WKB approximation is a method to find approximate solutions to the Schrodinger equation. It was developed in 1926 by Wentzel, Kramer, and Brillouin. The approximation assumes the wavefunction is an exponentially varying function with amplitude and phase that change slowly compared to the de Broglie wavelength. It can be used to obtain approximate solutions and energy eigenvalues for systems where the classical limit is valid. The approximation breaks down near classical turning points where the particle's energy is equal to the potential energy. The document provides examples of using the WKB approximation to solve the time-independent Schrodinger equation in one dimension for cases where the particle's energy is both greater than and less than the potential energy.
UCSD NANO 266 Quantum Mechanical Modelling of Materials and Nanostructures is a graduate class that provides students with a highly practical introduction to the application of first principles quantum mechanical simulations to model, understand and predict the properties of materials and nano-structures. The syllabus includes: a brief introduction to quantum mechanics and the Hartree-Fock and density functional theory (DFT) formulations; practical simulation considerations such as convergence, selection of the appropriate functional and parameters; interpretation of the results from simulations, including the limits of accuracy of each method. Several lab sessions provide students with hands-on experience in the conduct of simulations. A key aspect of the course is in the use of programming to facilitate calculations and analysis.
The document discusses ab initio molecular dynamics simulation methods. It begins by introducing molecular dynamics and Monte Carlo simulations using empirical potentials. It then describes limitations of empirical potentials and the need for ab initio molecular dynamics which calculates the potential from quantum mechanics. The document outlines several ab initio molecular dynamics methods including Ehrenfest molecular dynamics, Born-Oppenheimer molecular dynamics, and Car-Parrinello molecular dynamics. It provides details on how these methods treat the quantum mechanical potential and classical nuclear motion.
The document summarizes a gamma ray spectroscopy lab experiment. Key findings include:
- Gamma rays from various radioactive samples were measured using a sodium iodide detector and spectrometer interface.
- A linear relationship was found between the gamma ray energies and their channel numbers on the spectrometer.
- All major gamma ray interactions (photoelectric effect, Compton scattering) were observed except pair production which requires higher energies.
- The unknown isotope was identified as Cesium-137 based on its measured energy of 655.5 keV, though the author initially disagreed with this assessment.
The document summarizes key concepts about the hydrogen atom from quantum mechanics. It begins by introducing the Schrödinger equation and how it can be applied and solved for the hydrogen atom potential. The solution involves separation of variables into radial, angular, and azimuthal components. This leads to the identification of three quantum numbers - principal (n), angular momentum (l), and magnetic (ml) - that characterize the possible energy states. Higher sections discuss properties like orbital shapes, spin, and transition selection rules between energy levels and electron probability distributions.
1) The experiment used gamma-ray spectroscopy to analyze spectra from various radioactive sources. Spectra were recorded at different photomultiplier tube voltages to study resolution and efficiency.
2) Analysis found the number of dynodes in the photomultiplier tube to be 6.5, and resolution R was determined to be inversely proportional to gamma ray energy as expected.
3) Activity of a potassium chloride sample was estimated using detector efficiency calculations, finding 1.7×10^17 40K nuclei, consistent with the expected amount.
This document discusses statistical thermodynamics and the partition function. It introduces the concept of microscopic configurations and their weights. The Boltzmann distribution relates the probability of a configuration to its weight, which depends on the energy levels and temperature. The partition function allows calculating thermodynamic properties like internal energy, entropy, and heat capacity from knowledge of the energy levels and degeneracies alone. It provides a statistical mechanical approach to thermodynamics.
1) De Broglie hypothesized that particles like electrons can behave as waves, with a wavelength given by λ = h/mv, where h is Planck's constant, m is the particle's mass, and v is its velocity.
2) This hypothesis provided an explanation for the quantization of angular momentum and energy levels in Bohr's model of the hydrogen atom.
3) Experiments have verified that electrons and other particles do exhibit wave-like properties such as interference and diffraction, confirming the wave-particle duality predicted by De Broglie's hypothesis.
This document introduces key concepts in statistical mechanics, including the idea that macroscopic properties are thermal averages of microscopic properties. It discusses common statistical ensembles like the microcanonical ensemble (isolated systems with constant energy) and the canonical ensemble (systems in equilibrium with a heat reservoir). The canonical partition function Z relates microscopic quantum mechanics to macroscopic thermodynamics and can be used to calculate thermodynamic variables. Properties like heat capacity can be derived from fluctuations in energy calculated from the partition function.
1) The Born-Oppenheimer approximation separates the molecular Schrodinger equation into electronic and nuclear parts based on the large mass difference between electrons and nuclei.
2) It assumes that over short time periods, electrons adjust instantaneously to nuclear motions. This allows treating electronic motions separately for fixed nuclear positions.
3) Solving the electronic Schrodinger equation for different nuclear configurations provides the potential energy surface for nuclear vibrations and rotations.
In computational physics and Quantum chemistry, the Hartree–Fock (HF) method also known as self consistent method is a method of approximation for the determination of the wave function and the energy of a quantum many-body system or many electron system in a stationary state
JC H2 Physics Formula List/Summary (all topics)John Jon
Some of the concepts might be out of syllabus but I believe most of it is still relevant. It is a very concise summary containing mostly formulas and the Laws that govern Physics. This was done by a Raffles Institution student. I hope you will find this beneficial!
Possible Inverse Isotope effect in High Tc Superconductors Using the Non Vari...IOSR Journals
This document discusses a theory proposing a possible inverse isotope effect in high-temperature superconductors. The theory uses a non-variational quasi-particle formulation to describe electron-electron pairing due to overlapping electron wave functions around iron ions, allowing singlet pair formation. The mathematical solution of the quadratic function yields a reversal of signs between stable and unstable energy solutions, leading to a predicted negative isotope effect exponent. This could challenge assertions that only positive exponents correspond to stable states.
Optimizing the Drell-Yan Trigger-CyclotronJackson Pybus
The document discusses optimizing the trigger logic for the STAR Forward Meson Spectrometer (FMS) detector to more efficiently detect electron-positron pairs from Drell-Yan processes. Simulations of Drell-Yan events were performed to test the current trigger layout, which was found to only detect 86% of relevant events. An altered trigger scheme is proposed, increasing the size of the top and bottom detector segments while decreasing the middle segments. This new scheme is predicted to improve the detection efficiency to 94% and the figure of merit by 19%, effectively adding 2.5 more weeks of data for the upcoming RHIC run.
APPLICATIONS OF ESR SPECTROSCOPY TO METAL COMPLEXESSANTHANAM V
This document discusses the applications of electron spin resonance (ESR) spectroscopy to study metal complexes. It outlines several key factors that influence the ESR spectra of metal complexes, including the nature of the metal ion, ligands, geometry, number of d electrons, and crystal field effects. It also describes how zero-field splitting and Jahn-Teller distortions can lead to splitting of electronic levels and influence the number and pattern of transitions observed in ESR spectra. Understanding these various effects is important for extracting information about electronic structure and bonding from ESR data of metal complexes.
Direct and indirect excitations in boron nitride: atomic structure and electr...Claudio Attaccalite
This document discusses the optical properties of boron nitride (BN) as studied through many-body perturbation theory and electron energy loss spectroscopy (EELS) experiments. It finds that BN has an indirect bandgap of 5.79 eV according to calculations, and a sharp exciton mode is visible in EELS between 0.4-1 Å-1 momentum transfer. Many-body calculations reveal the exciton has reduced dispersion compared to the band structure, in good agreement with EELS data. Different stackings of BN layers are also considered, with ABC stacking found to have a very flat and possibly direct excitonic gap.
THE FEYNMAN-STUCKELBREG INTERPRETATION OF E<0 SOLUTIONSHusnain Ali
The document discusses relativistic quantum mechanics and the Klein-Gordon equation. It describes the Feynman-Stuckelberg interpretation of negative energy solutions to the Klein-Gordon equation, which interprets them as representing positive energy anti-particles moving forward in time. This resolves issues with negative probabilities and allows a consistent treatment of antiparticles. The interpretation is illustrated using a diagram of double electron scattering, showing it accounts for both time orderings through particle-antiparticle pair production and annihilation.
In recent years, there have been great interest in alkali-O2 batteries with extremely high specific energies. Li-O2 batteries offer the greatest theoretical specific energy, but currently suffer from large charging overpotentials and low power densities. Na-O2 offers a somewhat lower theoretical specific energy compared to Li-O2, but still a substantial improvement over today’s lithium-ion batteries. In this talk, we will demonstrate how first principles calculations can provide crucial insight into the workings of alkali-O2 batteries. We will elucidate a facile mechanism for recharging Li2O¬¬2 that is accessible at relatively low overpotentials of ~0.3-0.4V and is likely to be kinetically favored over Li2O2 decomposition. We will also demonstrate that sodium superoxide (NaO2) is predicted to be considerably more stable than sodium peroxide (Na2O2) at the nanoscale. Using first principles calculations, we derive the specific electrochemical conditions to nucleate and retain NaO2 and comment on the importance of considering the nanophase thermodynamics when optimizing an electrochemical system.
1. The Stern-Gerlach experiment discovered that silver atoms split into two beams, indicating the presence of an intrinsic "spin" angular momentum of 1/2 beyond orbital angular momentum.
2. Elementary particles are classified as fermions, with half-integer spin, and bosons, with integer spin. The spin of the electron is represented by a two-component spinor.
3. In a magnetic field, the spin precesses around the field direction at the Larmor frequency, independent of initial spin orientation. This principle underlies paramagnetic resonance and nuclear magnetic resonance spectroscopy.
This document discusses statistical mechanics and the distribution of energy among particles in a system. It provides 3 main types of statistical distributions based on the properties of identical particles: Maxwell-Boltzmann, Bose-Einstein, and Fermi-Dirac statistics. Maxwell-Boltzmann statistics applies to distinguishable particles, while Bose-Einstein and Fermi-Dirac apply to indistinguishable particles (bosons and fermions respectively), with the key difference being that fermions obey the Pauli exclusion principle. The document also discusses applications of these distributions, including the Maxwell-Boltzmann distribution law for molecular energies in an ideal gas.
The WKB approximation is a method to find approximate solutions to the Schrodinger equation. It was developed in 1926 by Wentzel, Kramer, and Brillouin. The approximation assumes the wavefunction is an exponentially varying function with amplitude and phase that change slowly compared to the de Broglie wavelength. It can be used to obtain approximate solutions and energy eigenvalues for systems where the classical limit is valid. The approximation breaks down near classical turning points where the particle's energy is equal to the potential energy. The document provides examples of using the WKB approximation to solve the time-independent Schrodinger equation in one dimension for cases where the particle's energy is both greater than and less than the potential energy.
UCSD NANO 266 Quantum Mechanical Modelling of Materials and Nanostructures is a graduate class that provides students with a highly practical introduction to the application of first principles quantum mechanical simulations to model, understand and predict the properties of materials and nano-structures. The syllabus includes: a brief introduction to quantum mechanics and the Hartree-Fock and density functional theory (DFT) formulations; practical simulation considerations such as convergence, selection of the appropriate functional and parameters; interpretation of the results from simulations, including the limits of accuracy of each method. Several lab sessions provide students with hands-on experience in the conduct of simulations. A key aspect of the course is in the use of programming to facilitate calculations and analysis.
The document discusses ab initio molecular dynamics simulation methods. It begins by introducing molecular dynamics and Monte Carlo simulations using empirical potentials. It then describes limitations of empirical potentials and the need for ab initio molecular dynamics which calculates the potential from quantum mechanics. The document outlines several ab initio molecular dynamics methods including Ehrenfest molecular dynamics, Born-Oppenheimer molecular dynamics, and Car-Parrinello molecular dynamics. It provides details on how these methods treat the quantum mechanical potential and classical nuclear motion.
The document summarizes a gamma ray spectroscopy lab experiment. Key findings include:
- Gamma rays from various radioactive samples were measured using a sodium iodide detector and spectrometer interface.
- A linear relationship was found between the gamma ray energies and their channel numbers on the spectrometer.
- All major gamma ray interactions (photoelectric effect, Compton scattering) were observed except pair production which requires higher energies.
- The unknown isotope was identified as Cesium-137 based on its measured energy of 655.5 keV, though the author initially disagreed with this assessment.
The document summarizes key concepts about the hydrogen atom from quantum mechanics. It begins by introducing the Schrödinger equation and how it can be applied and solved for the hydrogen atom potential. The solution involves separation of variables into radial, angular, and azimuthal components. This leads to the identification of three quantum numbers - principal (n), angular momentum (l), and magnetic (ml) - that characterize the possible energy states. Higher sections discuss properties like orbital shapes, spin, and transition selection rules between energy levels and electron probability distributions.
1) The experiment used gamma-ray spectroscopy to analyze spectra from various radioactive sources. Spectra were recorded at different photomultiplier tube voltages to study resolution and efficiency.
2) Analysis found the number of dynodes in the photomultiplier tube to be 6.5, and resolution R was determined to be inversely proportional to gamma ray energy as expected.
3) Activity of a potassium chloride sample was estimated using detector efficiency calculations, finding 1.7×10^17 40K nuclei, consistent with the expected amount.
This document discusses statistical thermodynamics and the partition function. It introduces the concept of microscopic configurations and their weights. The Boltzmann distribution relates the probability of a configuration to its weight, which depends on the energy levels and temperature. The partition function allows calculating thermodynamic properties like internal energy, entropy, and heat capacity from knowledge of the energy levels and degeneracies alone. It provides a statistical mechanical approach to thermodynamics.
1) De Broglie hypothesized that particles like electrons can behave as waves, with a wavelength given by λ = h/mv, where h is Planck's constant, m is the particle's mass, and v is its velocity.
2) This hypothesis provided an explanation for the quantization of angular momentum and energy levels in Bohr's model of the hydrogen atom.
3) Experiments have verified that electrons and other particles do exhibit wave-like properties such as interference and diffraction, confirming the wave-particle duality predicted by De Broglie's hypothesis.
This document introduces key concepts in statistical mechanics, including the idea that macroscopic properties are thermal averages of microscopic properties. It discusses common statistical ensembles like the microcanonical ensemble (isolated systems with constant energy) and the canonical ensemble (systems in equilibrium with a heat reservoir). The canonical partition function Z relates microscopic quantum mechanics to macroscopic thermodynamics and can be used to calculate thermodynamic variables. Properties like heat capacity can be derived from fluctuations in energy calculated from the partition function.
1) The Born-Oppenheimer approximation separates the molecular Schrodinger equation into electronic and nuclear parts based on the large mass difference between electrons and nuclei.
2) It assumes that over short time periods, electrons adjust instantaneously to nuclear motions. This allows treating electronic motions separately for fixed nuclear positions.
3) Solving the electronic Schrodinger equation for different nuclear configurations provides the potential energy surface for nuclear vibrations and rotations.
In computational physics and Quantum chemistry, the Hartree–Fock (HF) method also known as self consistent method is a method of approximation for the determination of the wave function and the energy of a quantum many-body system or many electron system in a stationary state
JC H2 Physics Formula List/Summary (all topics)John Jon
Some of the concepts might be out of syllabus but I believe most of it is still relevant. It is a very concise summary containing mostly formulas and the Laws that govern Physics. This was done by a Raffles Institution student. I hope you will find this beneficial!
Possible Inverse Isotope effect in High Tc Superconductors Using the Non Vari...IOSR Journals
This document discusses a theory proposing a possible inverse isotope effect in high-temperature superconductors. The theory uses a non-variational quasi-particle formulation to describe electron-electron pairing due to overlapping electron wave functions around iron ions, allowing singlet pair formation. The mathematical solution of the quadratic function yields a reversal of signs between stable and unstable energy solutions, leading to a predicted negative isotope effect exponent. This could challenge assertions that only positive exponents correspond to stable states.
Optimizing the Drell-Yan Trigger-CyclotronJackson Pybus
The document discusses optimizing the trigger logic for the STAR Forward Meson Spectrometer (FMS) detector to more efficiently detect electron-positron pairs from Drell-Yan processes. Simulations of Drell-Yan events were performed to test the current trigger layout, which was found to only detect 86% of relevant events. An altered trigger scheme is proposed, increasing the size of the top and bottom detector segments while decreasing the middle segments. This new scheme is predicted to improve the detection efficiency to 94% and the figure of merit by 19%, effectively adding 2.5 more weeks of data for the upcoming RHIC run.
APPLICATIONS OF ESR SPECTROSCOPY TO METAL COMPLEXESSANTHANAM V
This document discusses the applications of electron spin resonance (ESR) spectroscopy to study metal complexes. It outlines several key factors that influence the ESR spectra of metal complexes, including the nature of the metal ion, ligands, geometry, number of d electrons, and crystal field effects. It also describes how zero-field splitting and Jahn-Teller distortions can lead to splitting of electronic levels and influence the number and pattern of transitions observed in ESR spectra. Understanding these various effects is important for extracting information about electronic structure and bonding from ESR data of metal complexes.
Parity-Violating and Parity-Conserving Asymmetries in ep and eN Scattering in...Wouter Deconinck
Invited workshop presentation at the Amherst Center for Fundamental Interactions at UMass Amherst. This presentation includes the official Qweak results and discussion of unofficial beam normal single spin asymmetries.
This document provides an overview of the key concepts in electrostatics, including:
- Electric force, electric fields, electric flux, Gauss' law, and electric potential are the main topics covered.
- The fundamental building blocks of matter are atoms, which can become charged by gaining or losing electrons.
- Charged objects interact via the electric force described by Coulomb's law. Electric fields are produced by charged objects and flux is a measure of the number of field lines passing through a surface.
- Conductors allow for the easy flow of charge, while insulators do not. Capacitors store charge and introduce the concept of electric potential.
Nucleon electromagnetic form factors at high-momentum transfer from Lattice QCDChristos Kallidonis
This document summarizes a presentation on calculating the nucleon electromagnetic form factors at high momentum transfer using lattice QCD. Key points:
1) Lattice QCD simulations were performed on two ensembles with different volumes but similar lattice spacing to calculate the nucleon form factors up to momentum transfers of 12 GeV^2.
2) Boosted nucleon states were used in the simulations to access higher momentum transfers while keeping nucleon energies low. Three-point correlation functions were calculated to extract the matrix elements.
3) Plateaus in the ratio of three-point to two-point functions were identified to obtain the form factors, and two-state fits were also used to account for excited state contributions.
This document summarizes a simulation of two electrons in silicon under an externally applied potential. The simulation models the electron wavefunctions in two dimensions using a Schrodinger-Poisson solver. It calculates the quadrupole interaction between electrons through iterative calculations of the electron wavefunctions and their electrostatic interactions. Results show the quadrupole coupling increases with more prolate wavefunctions and is sufficient for use in quantum logic gates at realistic scales. Future work could provide more accurate results at higher resolution or extend the simulation to three dimensions.
- Elements in the same group have similar properties due to having the same number of valence electrons. Atoms get smaller from left to right in a period as protons are added, and larger from top to bottom in a group as energy levels are added.
- Electronegativity, ionization energy, and electron affinity all generally increase from left to right across a period as the effective nuclear charge increases. Electronegativity also increases up a group as the distance from valence electrons to the nucleus decreases.
- Ionization energy increases from top to bottom within a group as it is easier to remove an electron from an atom with fewer energy levels. Electron affinity generally increases from left to right across a period and decreases
The document discusses room temperature superconductivity and summarizes past research on high temperature superconductivity. It also examines the electronic structure and superconducting properties of NaxCoO2. Specifically:
1) Prior research from the 1970s explored whether high temperature superconductivity was possible.
2) Calculations and experiments on NaxCoO2 suggest it has unusual magnetic and electronic properties, including spin fluctuations that may be important to superconductivity.
3) Studies of the superconducting state in NaxCoO2 indicate it is unconventional and not fully gapped, with triplet f-wave pairing being a leading hypothesis to explain experimental results.
Interatomic potentials are needed to model interactions between atoms and molecules in simulations. The most common approaches are semi-empirical potentials which make an educated guess about the potential energy surface and adjust parameters to experimental data. Common potentials include Lennard-Jones for non-bonded interactions and Morse for bonded interactions. However, pair potentials have limitations and fail to capture properties of metals where electrons are delocalized. Embedded-atom models provide a better description of metallic bonding. Specialized potentials are also developed for materials with directional bonding like silicon.
[L'angolo del PhD] Alessandro Palma - XXII Ciclo - 2009accatagliato
The first part of this work describes how to use Z -> e+e- events in order to calibrate the CMS electromagnetic calorimeter, which makes use of scintillating crystals in order to precisely measure the energy of electrons and photons coming from the proton-proton interactions.
Using the very precise knowledge of the Z mass coming from LEP experiments, it is possible to set the absolute scale of the calorimeter as well as calibrating regions of the calorimeter with various topologies, and finely correct the calorimeter response to electrons. Focus is put on the first weeks of data taking.
The second part of this work concentrates on the misidentification of the electric charge of electrons/positrons in CMS. It will be shown how it is possible to extract the charge misidentification rate from the first CMS data, this time relying on the fact that electrons coming from the Z decay are always oppositely-charged.
Measuring this charge misidentification rate not only allows to perform a real-time check of the reconstruction quality during data taking, but also has an important role in the study of some physics channels. One of the studies where the charge misidentification has an important in influence is the W+/W- cross section ratio, that represent a test of the Standard Model which does not need a precise knowledge of the machine luminosity, that will be difficult to achieve with the first data.
Nuclear chemistry deals with radioactive processes and transformations that occur within atom nuclei. It involves the study of radioactive decay, nuclear reactions, nuclear reactors, radioactive waste management, and applications of radioisotopes. Some key areas covered include alpha and beta decay, nuclear stability factors like binding energy and neutron-to-proton ratio, and nuclear reaction terms such as cross-section and fission.
Electron spin resonance (ESR) spectroscopy detects electron spin transitions in molecules containing unpaired electrons when irradiated with microwave radiation in the presence of a magnetic field. The ESR spectrum provides information about electron environments and interactions. Hyperfine splitting occurs when the electron spin interacts with nuclear spins, producing multiple peaks following Pascal's triangle. Superhyperfine splitting provides evidence of electron delocalization, appearing as overlapping multiplets. Anisotropic g-values from spin-orbit coupling depend on molecular orientation, shifting peak positions. Powder spectra show broadening from all orientations.
Electron Spin Resonance (ESR) SpectroscopyHaris Saleem
Electron Spin Resonance Spectroscopy
Also called EPR Spectroscopy
Electron Paramagnetic Resonance Spectroscopy
Non-destructive technique
Applications
Extensively used in transition metal complexes
Deviated geometries in crystals
Electron spin resonance (ESR) spectroscopy detects transitions between spin energy levels of unpaired electrons using microwave radiation. When an unpaired electron is near a nucleus with non-zero spin, the electron experiences a magnetic field from the nucleus that splits the ESR signal into multiple lines based on the nuclear spin. This splitting is called hyperfine coupling and provides information about electronic structure. Superhyperfine splitting occurs when the electron interacts with multiple equivalent nuclei and results in even finer splitting patterns. Anisotropic interactions like the g-tensor can also be observed in ESR and provide information about electronic environments.
This document discusses the potential for using quantum entanglement to enable novel communication techniques. Key points include:
- Entangled particles can exhibit non-local correlations even when separated, allowing potential advantages over traditional communication methods.
- Recent experiments have verified non-local correlations over distances up to 10km, but technical challenges remain in using entanglement for communication. Simply measuring one entangled particle does not convey enough information to the other.
- The document proposes approaches to modulate one entangled particle in a way that could be detected on the other, without disrupting the entanglement. This could enable communication if theoretical and experimental hurdles can be overcome.
- Further research is needed to understand how entanglement and correlations are
1. The document discusses quantum spin systems in copper minerals, focusing on geometrically frustrated lattices that can exhibit novel quantum phases like spin liquids.
2. It summarizes experiments on the S=1/2 kagome lattice material vesignieite, which shows plateaus in its magnetization curve and spin liquid behavior.
3. Future plans include further investigating the magnetic state of a distorted vesignieite material around half saturation and synthesizing larger crystals of the perfect kagome lattice vesignieite.
This document summarizes key concepts from Ohm's law, Gauss' law, and Faraday's law. It begins with an introduction to Ohm's law, relating current, voltage, and resistance. It then discusses Gauss' law and its applications to point charges and charge distributions. Finally, it covers Faraday's law, explaining magnetic flux, Lenz's law, and how changing magnetic flux induces an electromotive force. Key equations for each law are also provided.
ELECTROSTATICS:Coulomb's law, Electric field & problemsDr.SHANTHI K.G
This document provides an overview of the topics covered in the unit on electrostatics, including:
- Coulomb's law, electric fields, Gauss's law and applications.
- Electric potential, conductors and dielectrics in static electric fields.
- Boundary conditions and capacitance of parallel, cylindrical, and spherical capacitors.
- Electrostatic energy and Poisson's and Laplace's equations.
- Current density, Ohm's law, electromotive force, and Kirchhoff's laws.
It then goes on to define Coulomb's law, the electric field intensity, and the principle of superposition. Examples of calculating electric force and field due to point charges are also provided
This document provides an outline and overview of lecture 2 on electric fields and dipoles. It introduces the concept of electric fields to explain electrostatic interactions without instantaneous action at a distance. Electric field lines are defined to visualize electric fields, with field strength proportional to line density. Dipoles, such as water molecules, have a net electric field due to internal charge separation but no net charge. They experience a torque in external electric fields. Microwave ovens work by causing the rotation of polar water molecules through an oscillating electric field, generating heat through molecular collisions.
This document contains the syllabus for an electric circuits course taught by A. Mohamed Nazeer at PSG Polytechnic College. The syllabus covers topics including DC circuits, network theorems, AC circuits, three phase circuits, wiring, and books for study. DC circuits topics include electrical quantities, Ohm's law, Kirchhoff's laws, and simple circuit problems. Network theorems covered are Thevenin's, Norton's, superposition, and maximum power transfer. AC circuits discusses single phase circuits, sinusoidal waveforms, power, inductance, capacitance, and resonance. Three phase circuits focuses on balanced supply and load. Wiring covers different wire types, wiring types, testing, and earthing
Similar to The Qweak Experiment at Jefferson Lab (20)
A Vision for User-Centered Scientific Computing at Jefferson LabWouter Deconinck
Presentation in the Jefferson Lab Computing Seminar series, about the lab's users, their expectations and needs, and how we can align the scientific computing environment with those needs.
How Can Machine Learning Help Your Research Forward?Wouter Deconinck
Machine learning is a buzzwords that conjures up visions of programming gurus and data magicians solving problems with little effort while others balk at the black-box nature and lack of first principles understanding. In this talk I hope to introduce some ways in which you can start to use powerful machine learning algorithms to solve certain classes of problems in ways that may be more generic than traditional approaches. I will use examples from a range of fields to demonstrate the power of machine learning, even though those field with access to large data sets have lead the charge. I will highlight differences between machine learning in physics and other data sciences. Finally, I will point out why a solid understanding of the underlying physical principles is a necessity to use machine learning in research with any success.
Increasing enrollments in physics majors with required senior research projects often places unsustainable demands on a constant number of research faculty. At William & Mary we piloted several formats of scalable team-based senior design experiences for our new Engineering Physics and Applied Design track. We developed these scalable approaches to enable 3- to 5-person teams to work on physics design experiences outside the areas of research expertise of one faculty supervisor, with clear users outside the department, and with a management structure to allow individual assessment. Agile project management, an iterative and incremental approach to development, has turned out to be particularly effective. We work with month-long sprints. At the start the team plans the tasks to be completed on a tracking board. During the sprints the team meets for frequent 10-minute stand-up meetings. At the end the team demonstrates the incremental progress and sets the goals for the next sprint.
*This work was supported in part by the National Science Foundation under Grant No. DUE-1625872, supporting the American Physical Society PIPELINE project to create and document new approaches to teaching innovation and entrepreneurship in physics.
Physics Innovation & Entrepreneurship at a Liberal Arts UniversityWouter Deconinck
(1) Small makerspaces at liberal arts universities allow physics students to gain experience in interdisciplinary projects similar to careers outside of academia. (2) The PIPELINE Network brings together six institutions to develop new approaches to teaching innovation and entrepreneurship in physics. (3) While most physics bachelor's and PhD graduates do not become traditional academics, the curriculum focuses on preparing students for graduate school and does not address skills needed for other careers.
Presentation with Kevin Weng about our development and use of the Sharkduino animal data-logging tag platform for the study of sandbar sharks in the Chesapeake Bay and Virginia Eastern Shore.
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Invited presentation at the American Association of Physics Teacher's summer 2016 meeting. Through a list of initiatives we are encouraging physics students to explore entrepreneurship and interdisciplinary projects in their undergraduate curriculum. All materials licensed CC-BY-SA.
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This document summarizes the entrepreneurship and makerspace initiatives at a liberal arts university. It discusses the creation of makerspaces in various departments focused on rapid prototyping, 3D printing, and other tools. Examples include a physics makerspace, biology hackerspace, and art & design studio. Capstone projects involve interdisciplinary groups working on innovations like animal data logging tags. A new Engineering Physics and Applied Design concentration is being offered within the Physics degree. The university also supports entrepreneurship through competitions and spaces for student entrepreneurs.
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The document discusses sexual and gender diversity in physics departments. It defines key terms like gender, sexual orientation, and gender identity. It also discusses the importance of an inclusive campus climate and highlights research showing the negative impacts of discrimination. Specific challenges faced by LGBT+ faculty and students in STEM are presented. The document urges actions to promote inclusion, such as using inclusive language and including LGBT+ representatives. Overall it argues physics departments should work to improve their climate and support for LGBT+ individuals.
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Current descriptions of immersive learning cases are often difficult or impossible to compare. This is due to a myriad of different options on what details to include, which aspects are relevant, and on the descriptive approaches employed. Also, these aspects often combine very specific details with more general guidelines or indicate intents and rationales without clarifying their implementation. In this paper we provide a method to describe immersive learning cases that is structured to enable comparisons, yet flexible enough to allow researchers and practitioners to decide which aspects to include. This method leverages a taxonomy that classifies educational aspects at three levels (uses, practices, and strategies) and then utilizes two frameworks, the Immersive Learning Brain and the Immersion Cube, to enable a structured description and interpretation of immersive learning cases. The method is then demonstrated on a published immersive learning case on training for wind turbine maintenance using virtual reality. Applying the method results in a structured artifact, the Immersive Learning Case Sheet, that tags the case with its proximal uses, practices, and strategies, and refines the free text case description to ensure that matching details are included. This contribution is thus a case description method in support of future comparative research of immersive learning cases. We then discuss how the resulting description and interpretation can be leveraged to change immersion learning cases, by enriching them (considering low-effort changes or additions) or innovating (exploring more challenging avenues of transformation). The method holds significant promise to support better-grounded research in immersive learning.
The cost of acquiring information by natural selectionCarl Bergstrom
This is a short talk that I gave at the Banff International Research Station workshop on Modeling and Theory in Population Biology. The idea is to try to understand how the burden of natural selection relates to the amount of information that selection puts into the genome.
It's based on the first part of this research paper:
The cost of information acquisition by natural selection
Ryan Seamus McGee, Olivia Kosterlitz, Artem Kaznatcheev, Benjamin Kerr, Carl T. Bergstrom
bioRxiv 2022.07.02.498577; doi: https://doi.org/10.1101/2022.07.02.498577
JAMES WEBB STUDY THE MASSIVE BLACK HOLE SEEDSSérgio Sacani
The pathway(s) to seeding the massive black holes (MBHs) that exist at the heart of galaxies in the present and distant Universe remains an unsolved problem. Here we categorise, describe and quantitatively discuss the formation pathways of both light and heavy seeds. We emphasise that the most recent computational models suggest that rather than a bimodal-like mass spectrum between light and heavy seeds with light at one end and heavy at the other that instead a continuum exists. Light seeds being more ubiquitous and the heavier seeds becoming less and less abundant due the rarer environmental conditions required for their formation. We therefore examine the different mechanisms that give rise to different seed mass spectrums. We show how and why the mechanisms that produce the heaviest seeds are also among the rarest events in the Universe and are hence extremely unlikely to be the seeds for the vast majority of the MBH population. We quantify, within the limits of the current large uncertainties in the seeding processes, the expected number densities of the seed mass spectrum. We argue that light seeds must be at least 103 to 105 times more numerous than heavy seeds to explain the MBH population as a whole. Based on our current understanding of the seed population this makes heavy seeds (Mseed > 103 M⊙) a significantly more likely pathway given that heavy seeds have an abundance pattern than is close to and likely in excess of 10−4 compared to light seeds. Finally, we examine the current state-of-the-art in numerical calculations and recent observations and plot a path forward for near-future advances in both domains.
CLASS 12th CHEMISTRY SOLID STATE ppt (Animated)eitps1506
Description:
Dive into the fascinating realm of solid-state physics with our meticulously crafted online PowerPoint presentation. This immersive educational resource offers a comprehensive exploration of the fundamental concepts, theories, and applications within the realm of solid-state physics.
From crystalline structures to semiconductor devices, this presentation delves into the intricate principles governing the behavior of solids, providing clear explanations and illustrative examples to enhance understanding. Whether you're a student delving into the subject for the first time or a seasoned researcher seeking to deepen your knowledge, our presentation offers valuable insights and in-depth analyses to cater to various levels of expertise.
Key topics covered include:
Crystal Structures: Unravel the mysteries of crystalline arrangements and their significance in determining material properties.
Band Theory: Explore the electronic band structure of solids and understand how it influences their conductive properties.
Semiconductor Physics: Delve into the behavior of semiconductors, including doping, carrier transport, and device applications.
Magnetic Properties: Investigate the magnetic behavior of solids, including ferromagnetism, antiferromagnetism, and ferrimagnetism.
Optical Properties: Examine the interaction of light with solids, including absorption, reflection, and transmission phenomena.
With visually engaging slides, informative content, and interactive elements, our online PowerPoint presentation serves as a valuable resource for students, educators, and enthusiasts alike, facilitating a deeper understanding of the captivating world of solid-state physics. Explore the intricacies of solid-state materials and unlock the secrets behind their remarkable properties with our comprehensive presentation.
Anti-Universe And Emergent Gravity and the Dark UniverseSérgio Sacani
Recent theoretical progress indicates that spacetime and gravity emerge together from the entanglement structure of an underlying microscopic theory. These ideas are best understood in Anti-de Sitter space, where they rely on the area law for entanglement entropy. The extension to de Sitter space requires taking into account the entropy and temperature associated with the cosmological horizon. Using insights from string theory, black hole physics and quantum information theory we argue that the positive dark energy leads to a thermal volume law contribution to the entropy that overtakes the area law precisely at the cosmological horizon. Due to the competition between area and volume law entanglement the microscopic de Sitter states do not thermalise at sub-Hubble scales: they exhibit memory effects in the form of an entropy displacement caused by matter. The emergent laws of gravity contain an additional ‘dark’ gravitational force describing the ‘elastic’ response due to the entropy displacement. We derive an estimate of the strength of this extra force in terms of the baryonic mass, Newton’s constant and the Hubble acceleration scale a0 = cH0, and provide evidence for the fact that this additional ‘dark gravity force’ explains the observed phenomena in galaxies and clusters currently attributed to dark matter.
Microbial interaction
Microorganisms interacts with each other and can be physically associated with another organisms in a variety of ways.
One organism can be located on the surface of another organism as an ectobiont or located within another organism as endobiont.
Microbial interaction may be positive such as mutualism, proto-cooperation, commensalism or may be negative such as parasitism, predation or competition
Types of microbial interaction
Positive interaction: mutualism, proto-cooperation, commensalism
Negative interaction: Ammensalism (antagonism), parasitism, predation, competition
I. Mutualism:
It is defined as the relationship in which each organism in interaction gets benefits from association. It is an obligatory relationship in which mutualist and host are metabolically dependent on each other.
Mutualistic relationship is very specific where one member of association cannot be replaced by another species.
Mutualism require close physical contact between interacting organisms.
Relationship of mutualism allows organisms to exist in habitat that could not occupied by either species alone.
Mutualistic relationship between organisms allows them to act as a single organism.
Examples of mutualism:
i. Lichens:
Lichens are excellent example of mutualism.
They are the association of specific fungi and certain genus of algae. In lichen, fungal partner is called mycobiont and algal partner is called
II. Syntrophism:
It is an association in which the growth of one organism either depends on or improved by the substrate provided by another organism.
In syntrophism both organism in association gets benefits.
Compound A
Utilized by population 1
Compound B
Utilized by population 2
Compound C
utilized by both Population 1+2
Products
In this theoretical example of syntrophism, population 1 is able to utilize and metabolize compound A, forming compound B but cannot metabolize beyond compound B without co-operation of population 2. Population 2is unable to utilize compound A but it can metabolize compound B forming compound C. Then both population 1 and 2 are able to carry out metabolic reaction which leads to formation of end product that neither population could produce alone.
Examples of syntrophism:
i. Methanogenic ecosystem in sludge digester
Methane produced by methanogenic bacteria depends upon interspecies hydrogen transfer by other fermentative bacteria.
Anaerobic fermentative bacteria generate CO2 and H2 utilizing carbohydrates which is then utilized by methanogenic bacteria (Methanobacter) to produce methane.
ii. Lactobacillus arobinosus and Enterococcus faecalis:
In the minimal media, Lactobacillus arobinosus and Enterococcus faecalis are able to grow together but not alone.
The synergistic relationship between E. faecalis and L. arobinosus occurs in which E. faecalis require folic acid
Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary S...Sérgio Sacani
Wereport the study of a huge optical intraday flare on 2021 November 12 at 2 a.m. UT in the blazar OJ287. In the binary black hole model, it is associated with an impact of the secondary black hole on the accretion disk of the primary. Our multifrequency observing campaign was set up to search for such a signature of the impact based on a prediction made 8 yr earlier. The first I-band results of the flare have already been reported by Kishore et al. (2024). Here we combine these data with our monitoring in the R-band. There is a big change in the R–I spectral index by 1.0 ±0.1 between the normal background and the flare, suggesting a new component of radiation. The polarization variation during the rise of the flare suggests the same. The limits on the source size place it most reasonably in the jet of the secondary BH. We then ask why we have not seen this phenomenon before. We show that OJ287 was never before observed with sufficient sensitivity on the night when the flare should have happened according to the binary model. We also study the probability that this flare is just an oversized example of intraday variability using the Krakow data set of intense monitoring between 2015 and 2023. We find that the occurrence of a flare of this size and rapidity is unlikely. In machine-readable Tables 1 and 2, we give the full orbit-linked historical light curve of OJ287 as well as the dense monitoring sample of Krakow.
The debris of the ‘last major merger’ is dynamically youngSérgio Sacani
The Milky Way’s (MW) inner stellar halo contains an [Fe/H]-rich component with highly eccentric orbits, often referred to as the
‘last major merger.’ Hypotheses for the origin of this component include Gaia-Sausage/Enceladus (GSE), where the progenitor
collided with the MW proto-disc 8–11 Gyr ago, and the Virgo Radial Merger (VRM), where the progenitor collided with the
MW disc within the last 3 Gyr. These two scenarios make different predictions about observable structure in local phase space,
because the morphology of debris depends on how long it has had to phase mix. The recently identified phase-space folds in Gaia
DR3 have positive caustic velocities, making them fundamentally different than the phase-mixed chevrons found in simulations
at late times. Roughly 20 per cent of the stars in the prograde local stellar halo are associated with the observed caustics. Based
on a simple phase-mixing model, the observed number of caustics are consistent with a merger that occurred 1–2 Gyr ago.
We also compare the observed phase-space distribution to FIRE-2 Latte simulations of GSE-like mergers, using a quantitative
measurement of phase mixing (2D causticality). The observed local phase-space distribution best matches the simulated data
1–2 Gyr after collision, and certainly not later than 3 Gyr. This is further evidence that the progenitor of the ‘last major merger’
did not collide with the MW proto-disc at early times, as is thought for the GSE, but instead collided with the MW disc within
the last few Gyr, consistent with the body of work surrounding the VRM.
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...Sérgio Sacani
Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters
represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions
among stars.
Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate
the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars.
The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun.
Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically,
the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec.
Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within
and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation
were carried out using the ACIS-Extract software.
Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a
photon flux threshold of approximately 2 × 10−8 photons cm−2
s
−1
. The X-ray sources exhibit a highly concentrated spatial distribution,
with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known
massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...
The Qweak Experiment at Jefferson Lab
1. The QWeak Experiment at Jefferson Lab: Searching for TeV
Scale Physics by Measuring the Weak Charge of the Proton
Or, why measuring part-per-billion asymmetries
to percent-level accuracy is really hard. . .
Wouter Deconinck
William & Mary
Supported by the NSF under Grant Nos.
PHY-1206053 and PHY-1405857.
March 6, 2017
University of Tennessee, Knoxville
1
2. Precision Electroweak Tests of the Standard Model
Electroweak Interaction
Parity Symmetry and Parity Violation
Parity-Violating Electron Scattering
Measuring Small Asymmetries in Integration Mode
Parity-Violating Electroweak Experiments at Jefferson Lab
The QWeak Experiment
Cryotarget
Main Detectors
Tracking Detectors
Beam Polarimetry
First Determination of Proton’s Weak Charge
Progress of QWeak Data Analysis
The MOLLER Experiment
PV-DIS and SoLID Experiments
Summary
2
3. There are Two Main Classes of Standard Model Tests
Current status of the Standard Model
Standard Model is an effective low-energy theory of the
more fundamental underlying physics.
Complementary approaches to uncover the underlying physics
• Energy frontier: direct searches for new particles
• Precision or intensity frontier: indirect searches
Energy frontier
• Highest energies
• Few signature events
• E.g.: Tevatron, LHC
Precision or intensity frontier
• Modest or low energies
• High statistical power
• g − 2, EDM, ββ, rare decays
• Fundamental symmetries
3
5. Electroweak Interaction: An Introduction
Glashow–Weinberg–Salam theory of weak interaction
• Gauge symmetry: SU(2)L × U(1)Y
• Gauge couplings: g for SU(2)L, g for U(1)Y
• Left-handed leptons in doublets, right-handed in singlets
• Fundamental symmetry of left and right is broken
Parity symmetry is violated
• Weak interaction violates parity
• Electromagnetism satisfies parity
• Use parity-violation to measure internal
electroweak parameters
5
6. Electroweak Interaction: An Introduction
Glashow–Weinberg–Salam theory of weak interaction
• Gauge symmetry: SU(2)L × U(1)Y
• Gauge couplings: g for SU(2)L, g for U(1)Y
• Left-handed leptons in doublets, right-handed in singlets
• Fundamental symmetry of left and right is broken
Parity symmetry is violated
• Weak interaction violates parity
• Electromagnetism satisfies parity
• Use parity-violation to measure internal
electroweak parameters
5
7. Electroweak Interaction: An Introduction
Glashow–Weinberg–Salam theory of weak interaction
• Gauge symmetry: SU(2)L × U(1)Y
• Gauge couplings: g for SU(2)L, g for U(1)Y
• Left-handed leptons in doublets, right-handed in singlets
• Fundamental symmetry of left and right is broken
Electroweak symmetry breaking (Bµ, W i
µ → Aµ, Z0
µ, W ±
µ )
• Aµ, Z0
µ, W ±
µ are mixture of Bµ and W i
µ
• Gauge field Aµ remains massless (photon)
• Gauge fields Z0
µ, W ±
µ obtain mass (weak bosons)
• Weinberg angle θW describes how they mix
5
8. Electroweak Interaction: An Introduction
Glashow–Weinberg–Salam theory of weak interaction
• Gauge symmetry: SU(2)L × U(1)Y
• Gauge couplings: g for SU(2)L, g for U(1)Y
• Left-handed leptons in doublets, right-handed in singlets
• Fundamental symmetry of left and right is broken
Electroweak symmetry breaking (Bµ, W i
µ → Aµ, Z0
µ, W ±
µ )
sin2
θW =
g 2
g2 + g 2
= 0.23122 ± 0.00015 (at MZ ) ≈
1
4
Aµ = cos θW · Bµ + sin θW · W 3
µ (massless)
Z0
µ = − sin θW · Bµ + cos θW · W 3
µ (MZ ≈ 91.2 GeV)
W ±
µ = (W 1
µ iW 2
µ)/
√
2 (MW ≈ 80.4 GeV)
5
9. Electroweak Interaction: An Introduction
Glashow–Weinberg–Salam theory of weak interaction
• Gauge symmetry: SU(2)L × U(1)Y
• Gauge couplings: g for SU(2)L, g for U(1)Y
• Left-handed leptons in doublets, right-handed in singlets
• Fundamental symmetry of left and right is broken
Parity-violation neutral current (gV − γ5gA)
LNC
PV = −
GF
√
2
ge
A (¯eγµγ5e) · q gq
V (¯qγµ
q)
+ ge
V (¯eγµe) · q gq
A (¯qγµ
γ5q)
= −
GF
2
√
2
q C1q (¯eγµγ5e) · (¯qγµ
q)
+ q C2q (¯eγµe) · (¯qγµ
γ5q)
e e
Z, Z
q q
5
10. Electroweak Vector Charge of the Proton is Suppressed
Parity-violating electron scattering couplings
• Weak vector quark coupling: C1q = 2ge
A gq
V (γ5 on e vertex)
• Weak axial quark coupling: C2q = 2ge
V gq
A (γ5 on q vertex)
Particle Electric charge Weak vector charge (sin2
θW ≈ 1
4)
u +2
3 −2C1u = +1 − 8
3 sin2
θW ≈ +1
3
d −1
3 −2C1d = −1 + 4
3 sin2
θW ≈ −2
3
p(uud) +1 Qp
W = 1 − 4 sin2
θW ≈ 0
n(udd) 0 Qn
W = −1
Proton’s weak vector charge Qp
W is approximately zero
Accidental suppression of the proton’s weak charge in
Standard Model makes it more sensitive to new physics!
Access to these weak vector charges by using parity-violation
6
11. We Use Spin to Access Weak Charges in Parity-Violation
Parity transformation: Inversion of spatial vectors v → −v
• No change in the sign for angular momentum vectors (S)
Tests using parity-violating electron scattering
• Polarized electrons (spin S) on unpolarized target
• Instead of inverting r → −r, p → −p, but keeping S = S,
we leave r and p unchanged but flip polarization or spin S
Asymmetry APV between left and right scattering off nucleons
N
e
e
S
P
N
e
e
S
7
12. We Use Spin to Access Weak Charges in Parity-Violation
Parity transformation: Inversion of spatial vectors v → −v
• No change in the sign for angular momentum vectors (S)
Tests using parity-violating electron scattering
• Polarized electrons (spin S) on unpolarized target
• Instead of inverting r → −r, p → −p, but keeping S = S,
we leave r and p unchanged but flip polarization or spin S
Asymmetry APV between left and right scattering off nucleons
N
e
e
S
P
N
e
e
S
7
13. Difference in Cross Section is Encoded in Asymmetry.
Parity-violating asymmetry in electron scattering
• Difference between left- and right-handed scattering yield
APV =
σR − σL
σR + σL
N
e
e
S
P
N
e
e
S
• Electromagnetic component is identical, hence subtracted out
• Parity-violating electroweak and new physics remains in APV
8
14. Parity-Violating Asymmetry Reduces to the Weak Charge
Asymmetry between left and right helicity
APV =
σL − σR
σL + σR
with σ =
e e
γ
q q
+
e e
Z, . . .
q q
2
Interference of photon and weak boson exchange
MEM
∝
1
Q2
MNC
PV ∝
1
M2
Z + Q2
APV =
σR − σL
σR + σL
∝
MNC
PV
MEM
∝
Q2
M2
Z
when Q2
M2
Z
9
15. Parity-Violating Asymmetry Reduces to the Weak Charge
Asymmetry between left and right helicity
APV =
σL − σR
σL + σR
with σ =
e e
γ
q q
+
e e
Z, . . .
q q
2
Interference of photon and weak boson exchange for protons
APV (p) =
−GF Q2
4πα
√
2
GE GZ
E + τGMGZ
M − (1 − 4 sin2
θW ) GMGZ
A
(GE )2 + τ(GM)2
In the forward elastic limit Q2
→ 0, θ → 0 (plane wave)
APV (p)
Q2→0
−−−−→
−GF Q2
4πα
√
2
Qp
W + Q2
· B(Q2
) ≈ −230 ppb ∝ Qp
W
9
16. Parity-Violating Asymmetry Reduces to the Weak Charge
Asymmetry between left and right helicity
APV =
σL − σR
σL + σR
with σ =
e e
γ
q q
+
e e
Z, . . .
q q
2
Interference of photon and weak boson exchange for electrons
APV (e) = mE
GF
πα
√
2
4 sin2
θ
(3 + cos2 θ)2
Qe
W
Direct connection from asymmetry to weak charge of electron
APV (e) ≈ 35 ppb ∝ Qe
W
No hadronic uncertainty due to B(Q2) form factor term
9
17. Strategy to Measure Parts-Per-Billion: All The Events!
Event versus integration mode
• Event mode (the good ol’ nuclear/particle way)
• each event individually registered
• event selection or rejection possible
time0 100 ns
µA
• Integrating mode (current mode)
• high event rates possible (event every nanosecond!)
• no suppression of background events possible
time0 100 ns
µA
. . .
10
18. We Measure Time-Dependent Integrated Detector Signal
Current mode with 1 kHz helicity reversals
time [ms]0 1 2 3 4 5 6
current
≈ 6 µA + − + − + − polarization
asymmetry only 230 ppb
• Collect many polarization windows: 2 year long experiment
• Counting mode at 1 MHz would have taken 7000 years. . .
11
19. We Measure Time-Dependent Integrated Detector Signal
Current mode with 1 kHz helicity reversals
time [ms]
(zero several hundred km down)
0 1 2 3 4 5 6
current
≈ 6 µA + − + − + − polarization
asymmetry only 230 ppb
• Collect many polarization windows: 2 year long experiment
• Counting mode at 1 MHz would have taken 7000 years. . .
11
20. We Measure Time-Dependent Integrated Detector Signal
Current mode with 1 kHz helicity reversals
time [ms]
(zero several hundred km down)
0 1 2 3 4 5 6
current
≈ 6 µA + − + − + − polarization
asymmetry only 230 ppb
(counting noise ≈ 1000 times larger)
• Collect many polarization windows: 2 year long experiment
• Counting mode at 1 MHz would have taken 7000 years. . .
11
22. Parity-Violating Electroweak Experiments at Jefferson Lab
QWeak Experiment
• Measurement of Qp
W in ep → e p on protons in hydrogen
• Completed, preliminary results, full results in Fall 2017
• Ongoing analysis effort, constitutes the bulk of this talk
MOLLER Experiment
• Measurement of Qe
W in ee → e e on electrons in hydrogen
• Planned for running at Jefferson Lab 12 GeV
PV-DIS and SoLID Experiments
• Measurement of C1,2q in ep → e p on hydrogen, deuterium
• Completed at 6 GeV, planned at Jefferson Lab 12 GeV
13
26. The QWeak Experiment: Overview
• Precision measurement of a quantity suppressed by
fundamental symmetries (Qp
W ≈ 0, asymmetry of 230 ppb)
• Elastic scattering of electron beam on proton target to
measure the proton weak charge Qp
W to a precision of 4%
Pushing the envelope of intensity (more events)
• Higher beam current (150 µA versus usually < 100 µA)
• Longer cryo-target (35 cm versus 20 cm)
• Higher event rates up to 800 MHz (integration)
Pushing the envelope of precision (better measurements)
• Electron beam polarization precision of 1% at 1 GeV
• Helicity-correlated asymmetries at ppb level
17
27. The QWeak Experiment: Overview
Collimator-Magnet-Collimator focusing spectrometer
Triple Pb Collimator
System
LH Target
Drift
Chambers
8 Quartz Bar Detectors
Trigger
Scintillators8 Segment
Toroidal Magnet
High Density Shield Wall
2
“The Qweak Experimental Apparatus,” NIM A 781, 105 (2015);
http://dx.doi.org/10.1016/j.nima.2015.01.023
18
28. The QWeak Experiment: Overview
Collimator-Magnet-Collimator focusing spectrometer
“The Qweak Experimental Apparatus,” NIM A 781, 105 (2015);
http://dx.doi.org/10.1016/j.nima.2015.01.023
18
29. The QWeak Experiment: High Power Cryotarget
Operational Parameters
• Transverse flow: 2.8 m/s
• Target length: 35 cm
• Beam current: 150 µA
• Heating power: 2.5 kW
Design with CFD
Power for other cryotargets
19
30. The QWeak Experiment: High Power Cryotarget
Low-frequency ‘boiling’ noise
• Helicity flip rate 960 Hz →
240 Hz (quartet cycles)
• Target density fluctuations
at low frequencies occur
• Power spectrum of signal
Current dependence
• Additional noise smaller
than statistical width
• Consistent for different
current and beam rasters
• Current to 180 µA
20
31. The QWeak Experiment: Main Detector
Preradiated Čerenkov detector bars
• 8 fused silica radiators, 2 m long × 18 cm × 1.25 cm
• Pb preradiator tiles to reduce low-energy tracks (neutrals)
• Light collection: total internal reflection
• 5 inch PMTs with gain of 2000, low dark current
• 800 MHz electron rate per bar, defines counting noise
21
32. The QWeak Experiment: Kinematics in Event Mode
Reasons for a tracking system?
• Determine Q2, note: Ameas ∝ Q2 · Qp
W + Q2 · B(Q2)
• Main detector light output and Q2 position dependence
• Contributions from inelastic background events
Instrumentation of only two octants
• Horizontal drift chambers for front region (Va Tech)
• Vertical drift chambers for back region (W&M)
• Rotation allows measurements in all eight octants
Track reconstruction
• Straight tracks reconstructed in front and back regions
• Front and back partial tracks bridged through mag field
22
33. The QWeak Experiment: Improved Beam Polarimetry
Requirements on beam polarimetry
• Largest experimental uncertainty in QWeak experiment
• Systematic uncertainty of 1% (on absolute measurements)
Upgrade existing Møller polarimeter (e + e → e + e)
• Scattering off atomic electrons in magnetized iron foil
• Limited to separate, low current runs (I ≈ 1 µA)
Construction new Compton polarimeter (e + γ → e + γ)
• Compton scattering of electrons on polarized laser beam
• Continuous, non-destructive, high precision measurements
23
34. The QWeak Experiment: Improved Beam Polarimetry
Compton polarimeter
• Beam: 150 µA at 1.165 GeV
• Chicane: interaction region 57 cm below straight beam line
• Laser system: 532 nm green laser
• 10 W CW laser with low-gain cavity
• Photons: PbWO4 scintillator in integrating mode
• Electrons: Diamond strips with 200 µm pitch
24
35. The QWeak Experiment: Beam Polarimetry
Møller polarimetry
• New beamline, refurbished
• Invasive measurements
• Polarization larger than
anticipated: 86% to 88%
Compton polarimetry
• Excellent performance
• Continuous measurements
• Operates at full 180 µA
• Great statistical precision
25
36. Data Quality: Slow Helicity Reversal
λ/2-plate and Wien filter changes
• Insertable λ/2-plate (IHWP) in injector allows ‘analog’
flipping helicity frequently
• Wien filter: another way of flipping helicity (several weeks)
• Each ‘slug’ of 8 hours consists of same helicity conditions
• Preliminary asymmetries: 60 ppb blinded, not corrected, not
regressed! And only 8 of hundreds of slugs. . .
• Average asymmetries are consistent with sign change
26
37. Weak Charge in Preliminary Agreement with Prediction
First results based on subset of the data in 2013
• Publication in Phys. Rev. Lett. 111, 141803 (2013)
• Based on only 4% of the total data set: first experiment with
direct access to proton’s weak charge
• 25 times more data available: projected release in Fall 2017
Global analysis method by Young, Roche, Carlini, Thomas
• Fit of parity-violating asymmetry data on H, D, 4He, up to
Q2 = 0.63 GeV2, and rotated to zero forward angle
• Free parameters were C1u, C1d , strange charge radius ρs and
magnetic moment µs, and isoscalar axial form factor (zero at
tree level)
• Qp
W (PVES) = 0.064 ± 0.012 (our result with world data)
• Qp
W (SM) = 0.0710 ± 0.0007 (theoretical expectation)
27
38. First Determination of the Weak Charge of the Proton
Intercept of reduced asymmetry at Q2
= 0
APV = APV
A0
= Qp
W + Q2 · B(Q2, θ = 0) with A0 = − GF Q2
4πα
√
2
▲
▲
▲
0.0 0.1 0.2 0.3 0.4 0.5 0.6
0.0
0.1
0.2
0.3
0.4
■
■
■
✖
■
◆ This Experiment
■ HAPPEX
✖ SAMPLE
▲ PVA4
● G0
SM (prediction)
◆
Data Rotated to the Forward-Angle Limit
[GeV/c]Q
22
ç
ç
WA/A=Q+B(,θ=0)
p
0Q
2
Q
2
ep
28
39. Determination of the Weak Charge of the Proton
Extraction from just parity-violating electron scattering,
including the new QWeak results
Qp
W (PVES) = 0.064 ± 0.012
In agreement with prediction in the Standard Model
Qp
W (SM) = 0.0710 ± 0.0007
29
42. Determination of the Weak Vector Charges of the Quarks
Global fit of all atomic and electron scattering data
• Determination of weak charge of the proton
• Qp
W (PVES+APV) = 0.063 ± 0.012
• Qp
W (SM) = 0.0710 ± 0.0007
• Extraction of weak vector quark couplings possible
• C1u = −0.1835 ± 0.0054
• C1d = 0.3355 ± 0.0050
• Determination of weak charge of the neutron
• Qn
W (PVES+APV) = −0.975 ± 0.010
• Qn
W (SM) = −0.9890 ± 0.0007
32
43. Largest Uncertainties in Preliminary QWeak Result?
All uncertainties in ppb ∆Acorr δ(APV )
Beam polarization P -21 5
Kinematics Rtotal 5 9
Dilution 1/(1 − fi ) -7
Beam asymmetry -40 13
Transverse pol. AT 0 5
Detector non-linearity 0 4
Backgrounds: δ(fi ) δ(Ai )
Aluminum (b1) -58 4 8
Beamline (b2) 11 3 23
Neutrals (b3) 0 1 1
Inelastic (b4) 1 1 1
APV = Rtotal
Amsr
P − fi Ai
1 − fi
33
44. Largest Uncertainties in Preliminary QWeak Result?
All uncertainties in ppb ∆Acorr δ(APV )
Beam polarization P -21 5
Kinematics Rtotal 5 9
Dilution 1/(1 − fi ) -7
Beam asymmetry -40 13
Transverse pol. AT 0 5
Detector non-linearity 0 4
Backgrounds: δ(fi ) δ(Ai )
Aluminum (b1) -58 4 8
Beamline (b2) 11 3 23
Neutrals (b3) 0 1 1
Inelastic (b4) 1 1 1
APV = Rtotal
Amsr
P − fi Ai
1 − fi
33
45. Helicity-Correlated Beam Properties Are Understood
Measured asymmetry depends on beam position, angle, energy
• Well-known and expected effect for PVES experiments
• “Driven” beam to check sensitivities from “natural” jitter
34
46. Helicity-Correlated Beam Properties Are Understood
Sensitivities are used to correct measured asymmetry
• Acorr = i
∂A
∂xi
∆xi with beam parameters i = x, y, x , y , E
• Sensitivities (derivatives) from simultaneous regression fits
Excellent agreement between natural and driven beam motion
• Figure includes about
50% of total dataset for
QWeak experiment
• No other corrections
applied to this data
35
47. However, Some Beamline Background Correlations Remain
After regression, correlation with background detectors
• Luminosity monitors & spare detector in super-elastic region
• Background asymmetries of up to 20 ppm (that’s huge!)
36
48. However, Some Beamline Background Correlations Remain
Hard work by grad students: now understood, under control
• Partially cancels with slow helicity reversal (half-wave plate)
• Likely caused by large asymmetry in small beam halo or tails
• Scattering off the beamline and/or “tungsten plug”
Qualitatively new background for PVES experiments at JLab
• Second regression using asymmetry in background detectors
• Measurements with blocked octants to determine dilution
factor (f MD
b2
= 0.19%)
37
50. Sensitivity to New Physics
New parity-violating physics
• Consider effective contact interaction
• Coupling constant g, mass scale Λ
• Effective charges hu
V = cos θh and hd
V = sin θh
Effective Lagrangian (Erler et al., PRD 68, 016006 (2003))
LPV
e−q = LPV
SM + LPV
New
= −
GF
√
2
eγµγ5e
q
C1qqγµ
q +
g2
4Λ2
eγµγ5e
q
hV
q qγµ
q
39
51. Sensitivity to New Physics
Determination of weak charge of the proton
• Assume agreement with Standard Model within ∆Qp
W
• What are the limits on Λ
g ?
Limits on new physics energy scale
Λ
g
=
1
2
√
2GF ∆Qp
W
−1/2
• Limits from ∆Qp
W = 0.005: Λ
g > 1.7 TeV at 1 σ
• For comparison with LHC results: g2 = 4π
• Lower limit Λ > 5.4 TeV at 95% C.L.
40
52. Progress on QWeak Data Analysis
A lot of progress has been made already
• Completed data-taking in May 2012
• Published first determination of proton’s weak charge and
global analysis in PRL in October 2013
• Qp
W (PVES + APV ) = 0.063 ± 0.012 with only 4% of the data
Unprecedented precision come with inevitable surprises
• Blind analysis precludes “incremental” preliminary results
• Discovered qualitatively new “beamline background” noise
• Discovered another qualitatively new systematic (non-noise)
background
41
53. Progress on QWeak Data Analysis
A lot of progress has been made already
• Discovered another qualitatively new systematic (non-noise)
background
• Various microscopic explanations consistent with effect
• Geant4 simulations & detector post-mortems on-going
• Confident that we can understand this effect better
42
54. The QWeak Experiment: Timeline
• Double-scattering effect studies were our last hangup
• Unblinding: March 31, 2017
• Publication and release during the summer/fall (DNP
meeting)
• Stay tuned!
43
55. The QWeak Experiment: Projections
Reduced parity-violating asymmetry
• This was all with only 4% of total data!
• Projected result with full data set (25 times more data)
44
56. The QWeak Experiment: Projections
Reduced parity-violating asymmetry
• This was all with only 4% of total data!
• Projected result with full data set (25 times more data)
44
59. The MOLLER Experiment
Measurement of the electroweak mixing angle at low energy
• Elastic scattering of electrons on electrons in hydrogen
• Precision measurement of the weak charge of the electron
Qe
W ≈ 0 at 11 GeV
• Asymmetry APV ≈ 35.6 ppb, with precision δAPV = ±0.7 ppb
• Precision δQe
W ≈ ±2.1%, δ sin2
θW = ±0.1%
Pushing the envelope of intensity (more events)
• Even higher luminosity: 85 µA on 1.5 m long cryo-target
• Event rates up to 150 GHz (integrated, of course)
Pushing the envelope of precision
• Electron beam polarization precision of 0.4% at 11 GeV
47
60. The MOLLER Experiment
Experimental Layout
• Long, narrow hybrid toroidal spectrometer system to select
very forward events
• Focusing of ee and ep on segmented quartz detector rings
48
61. The MOLLER Experiment
Experimental Layout
• Long, narrow hybrid toroidal spectrometer system to select
very forward events
• Focusing of ee and ep on segmented quartz detector rings
48
63. PV-DIS and SoLID Experiments
Analogy with Deep Inelastic Scattering
d2σ
dΩdE
=
α2
4E2 sin4 θ
2
2
M
F1(x) sin2 θ
2
+
1
ν
F2(x) cos2 θ
2
Quark structure through DIS
• F2(x) = x q e2
q(q + ¯q) ≈ 2xF1(x) (Callan-Gross)
Quark structure through PV-DIS: interference of γZ
• FγZ
2 (x) = x q eqgV
q (q + ¯q) → a1(x) ∼ q eqC1q (q + ¯q)
• FγZ
3 (x) = x q eqgA
q (q − ¯q) → a3(x) ∼ q eqC2q (q − ¯q)
50
64. PV-DIS and SoLID Experiments
Recent Results from PV-DIS at 6 GeV
• Published in Nature 506,
p67 (February 2014)
• First evidence at 95% C.L.
that the weak axial quark
couplings C2q are non-zero
(as predicted by the
Standard Model)
• Exclusion limits for contact
interactions Λ− > 4.8 TeV
and Λ+ > 5.8 TeV
51
65. PV-DIS and SoLID Experiments
Solenoidal Large Intensity Device
• 2 GeV < p < 8 GeV
• 2 GeV2
< Q2 < 10 GeV2
• 0.2 < x < 1
• 40% azimuthal acceptance
• L ≈ 5 · 1035 s−1cm−2
Experimental design
• Counting mode at rate > 200 kHz, 30 independent sectors
• Baffles filter low energy and neutral particles (no line of sight)
• Light gas Čerenkov for 1000–200 : 1 rejection of low-E π−
• Electromagnetic calorimeter for 50 : 1 π− rejection
52
66. PV-DIS and SoLID Experiments: Weak Axial Couplings
Projected Precision on C1q and C2q Couplings
53
68. Summary
The QWeak experiment
• Elastic e-p scattering on liquid hydrogen target
• Precision measurement of a proton weak charge Qp
W ≈ 0,
quantity suppressed by fundamental symmetries
• First determination of the weak charge of the proton
• With only 4% of the full data set
• Qp
W (PVES + APV ) = 0.063 ± 0.012
• Weak charge is in agreement with Standard Model
• Results from full data set anticipated in fall 2014
Broad program of electroweak precision measurements
• PV-DIS: weak axial quark couplings are non-zero at 95% C.L.
• MOLLER, SoLID: precision measurements of mixing angle and
weak quark couplings
55
71. Ancillary Measurements: Aluminum Target Walls
Aluminum asymmetry
(preliminary)
• Asymmetry consistent with
order of magnitude expected
• Asymmetry: few ppm
• Dilution f of 3%
• Correction ≈ 20%
Dilution measurement
(preliminary)
3
72. Ancillary Measurements: Inelastic Transitions
N → ∆ asymmetry (projected)
• In analysis, no result yet
• Expected precision 1 ppm
• Q2 = 0.025 GeV2
• Asymmetry: few ppm
• Dilution f of 0.1%
• Correction ≈ 1%
Simulation benchmark
(preliminary)
4
73. Ancillary Measurements: Inelastic Transitions
N → ∆ asymmetry (projected)
• In analysis, no result yet
• Expected precision 1 ppm
• Q2 = 0.025 GeV2
• Asymmetry: few ppm
• Dilution f of 0.1%
• Correction ≈ 1%
Simulation benchmark
(preliminary)
4
74. Ancillary Measurements: Transverse Asymmetry
• In main measurement, not 100% longitudinal polarization
• Transversely polarized beam (H or V) on unpolarized target
• Parity-conserving, T-odd transverse asymmetry of order ppm
Bn =
2 (T∗
1γ · T2γ)
|T1γ|2
• Access to imaginary part of 2-photon exchange amplitude T2γ
• Extensive transverse spin program:
• elastic ep in H, C, Al at E = 1.165 GeV
• inelastic ep → ∆ in H, C, Al at E = 0.877 GeV and 1.165 GeV
• elastic ee in H at E = 0.877 GeV
• deep inelastic ep in H at W = 2.5 GeV
• pion electro-production in H at E = 3.3 GeV
5
75. Ancillary Measurements: Transverse Asymmetry on H
• Vertical and horizontal polarization: 90◦ phase shift
• Observe the expected cancellation with slow helicity reversal
6
76. Ancillary Measurements: Transverse Asymmetry on H
• Vertical and horizontal polarization: 90◦ phase shift
• Observe the expected cancellation with slow helicity reversal
6
77. Ancillary Measurements: Transverse Asymmetry on H
• Shown asymmetries not corrected for backgrounds or
polarization
• Preliminary transverse asymmetry in ep in hydrogen:
Bn = −5.35 ± 0.07(stat) ± 0.15(syst) ppm
• More precise than any other measurement by a factor 5
• Theory: Pasquini & Vanderhaeghen, Afanasev & Merenkov,
Gorchtein
7
78. Ancillary Measurements: Transverse Asymmetry on H
Theoretical interpretation
• Theory: Pasquini & Vanderhaeghen, Afanasev & Merenkov,
Gorchtein
8
79. Ancillary Measurements: Transverse Asymmetry on C, Al
Aluminum: non-zero transverse asymmetry (uncorrected data)
• Aluminum target was alloy with 10% contamination
• Needs corrections for quasielastic and inelastic scattering, and
for nuclear excited states(?)
9
80. Ancillary Measurements: Transverse Asymmetry on C, Al
Projected uncertainties for C and Al transverse asymmetries
• Theory from Phys. Rev. C77, 044606 (2008)
• Pb data from PRL 109, 192501 (2012)
10
81. Data Quality: Understanding the Width
Asymmetry width
Battery width
Measurement
• 240 Hz helicity quartets
(+ − −+ or − + +−)
• Uncertainty = RMS/
√
N
• 200 ppm in 4 milliseconds
• < 1 ppm in 5 minutes
Asymmetry width
• Pure counting statistics ≈ 200 ppm
• + detector resolution ≈ 90 ppm
• + current monitor ≈ 50 ppm
• + target boiling ≈ 57 ppm
• = observed width ≈ 233 ppm
11
82. Data Quality: Helicity-Correlated Beam Properties
Natural beam motion
• Measured
asymmetry
correlated with
beam position and
angles
• False asymmetries
• Linear regression
removes effect:
Ac = i
∂A
∂xi
∆xi
i = x, y, x , y , E
12
83. Data Quality: Helicity-Correlated Beam Properties
Driven beam motion
• Deliberate motion
• i = x, y, x , y , E
• Sensitivity slopes ∂A
∂xi
determined
from natural beam motion or from
beam modulation → results
consistent between methods
• Actual regression corrections
smaller than specifications
13
85. Ancillary Measurements: Transverse Asymmetry
• Transversely polarized beam on unpolarized target
• Parity-conserving (T-odd) transverse asymmetry of order ppm
Bn =
2 (T∗
1γ · T2γ)
|T1γ|2
• Access to imaginary part of 2-photon exchange amplitude T2γ
• False asymmetry for parity-violating asymmetry APV due to
residual transverse polarization and broken azimuthal
symmetry
15
86. Ancillary Measurements: Transverse Asymmetry
• Vertical polarization: cancellation with helicity reversal
• Horizontal polarization: 90◦ phase shift from vertical
• Shown asymmetries not corrected for backgrounds or
polarization
• Preliminary transverse asymmetry:
Bn = −5.27 ± 0.07(stat) ± 0.14(syst) ppm
• Transverse asymmetry leakage in APV < 2 ppb
16
87. Ancillary Measurements: Transverse Asymmetry
• Vertical polarization: cancellation with helicity reversal
• Horizontal polarization: 90◦ phase shift from vertical
• Shown asymmetries not corrected for backgrounds or
polarization
• Preliminary transverse asymmetry:
Bn = −5.27 ± 0.07(stat) ± 0.14(syst) ppm
• Transverse asymmetry leakage in APV < 2 ppb
16
88. Ancillary Measurements: Transverse Asymmetry
• Vertical polarization: cancellation with helicity reversal
• Horizontal polarization: 90◦ phase shift from vertical
• Shown asymmetries not corrected for backgrounds or
polarization
• Preliminary transverse asymmetry:
Bn = −5.27 ± 0.07(stat) ± 0.14(syst) ppm
• Transverse asymmetry leakage in APV < 2 ppb
16
89. Ancillary Measurements: Transverse Asymmetry
• Pasquini & Vanderhaeghen: proton and πN, resonance region
with MAID, asymmetry dominated by inelastic contribution
• Afanasev & Merenkov: forward Compton amplitudes from real
photo-production
• E = 1.160 GeV, θ = 7.8◦, Q2 = 0.026 GeV2
• Other measurements: 0.877 GeV and 3.36 GeV, on Al and C
17
90. Ancillary Measurements: Transverse Asymmetry
• Pasquini & Vanderhaeghen: proton and πN, resonance region
with MAID, asymmetry dominated by inelastic contribution
• Afanasev & Merenkov: forward Compton amplitudes from real
photo-production
• E = 1.160 GeV, θ = 7.8◦, Q2 = 0.026 GeV2
• Other measurements: 0.877 GeV and 3.36 GeV, on Al and C
17
91. Ancillary Measurements: Transverse Asymmetry
• Pasquini & Vanderhaeghen: proton and πN, resonance region
with MAID, asymmetry dominated by inelastic contribution
• Afanasev & Merenkov: forward Compton amplitudes from real
photo-production
• E = 1.160 GeV, θ = 7.8◦, Q2 = 0.026 GeV2
• Other measurements: 0.877 GeV and 3.36 GeV, on Al and C
17
92. First Determination of the Weak Charge of the Proton
First results
• Publication in Phys. Rev. Lett. 111, 141803 (2013)
• Based on only 4% of the total data set: first experiment with
direct access to proton’s weak charge
• 25 times more data available: projected release in fall 2014
Global analysis method by Young, Roche, Carlini, Thomas
• Fit of parity-violating asymmetry data on H, D, 4He, up to
Q2 = 0.63 GeV2, and rotated to zero forward angle
• Free parameters were C1u, C1d , strange charge radius ρs and
magnetic moment µs, and isoscalar axial form factor (zero at
tree level)
18
93. Determination of the Weak Charge of the Proton
Reduced parity-violating asymmetry
APV = APV
A0
= Qp
W + Q2 · B(Q2, θ = 0) with A0 = − GF Q2
4πα
√
2
▲
▲
▲
0.0 0.1 0.2 0.3 0.4 0.5 0.6
0.0
0.1
0.2
0.3
0.4
■
■
■
✖
■
◆ This Experiment
■ HAPPEX
✖ SAMPLE
▲ PVA4
● G0
SM (prediction)
◆
Data Rotated to the Forward-Angle Limit
[GeV/c]Q
22
ç
ç
WA/A=Q+B(,θ=0)
p
0Q
2
Q
2
ep
19
96. Data Quality: Understanding the Width
Asymmetry width
Battery width
Measurement
• 240 Hz helicity quartets
(+ − −+ or − + +−)
• Uncertainty = RMS/
√
N
• 200 ppm in 4 milliseconds
• < 1 ppm in 5 minutes
Asymmetry width
• Pure counting statistics ≈ 200 ppm
• + detector resolution ≈ 90 ppm
• + current monitor ≈ 50 ppm
• + target boiling ≈ 57 ppm
• = observed width ≈ 233 ppm
22
97. The QWeak Experiment: Tracking Mode
Horizontal drift chambers
• 32 wires in 0.5 m wide planes
• 12 planes per octant
• 2 instrumented octants
• Constructed at Va Tech
Vertical drift chambers
• 181 wires in 2 m long planes
• 4 planes per octant (65◦ tilt)
• 2 instrumented octants
• Constructed at W&M
23
98. The QWeak Experiment: Tracking Mode
Horizontal drift chambers
• 32 wires in 0.5 m wide planes
• 12 planes per octant
• 2 instrumented octants
• Constructed at Va Tech
Vertical drift chambers
• 181 wires in 2 m long planes
• 4 planes per octant (65◦ tilt)
• 2 instrumented octants
• Constructed at W&M
23
99. The QWeak Experiment: Tracking Mode
Reconstruction of angle θ
(preliminary)
Reconstruction of momentum
transfer Q2
(preliminary)
• Periodic tracking runs at 50 pA (HDC/VDC) to few nA (VDC)
• VDC track resolution of 250 µm meets design goal
• HDC track resolution of 350 µm (work ongoing)
• Required precision of 0.5% on value of Q2 achievable
24
100. The QWeak Experiment: Tracking Mode
Simulation of electrons hitting main detector bar
Projection of reconstructed tracks to detector bar
Focal plane scanner detector (1 cm square quartz)
25
101. Data Quality: Helicity-Correlated Beam Properties
Natural beam motion
• Measured
asymmetry
correlated with
beam position and
angles
• False asymmetries
• Linear regression
removes effect:
Ac = i
∂A
∂xi
∆xi
i = x, y, x , y , E
26
102. Data Quality: Helicity-Correlated Beam Properties
Driven beam motion
• Deliberate motion
• i = x, y, x , y , E
• Sensitivity slopes ∂A
∂xi
determined
from natural beam motion or from
beam modulation → results
consistent between methods
• Actual regression corrections
smaller than specifications
27
103. Sensitivity to New Physics
Lower bound on new physics (95% CL)
Figure: Young, Carlini, Thomas, Roche (2007)
Constraints from
• Atomic PV:
Λ
g > 0.4 TeV
• PV electron
scattering:
Λ
g > 0.9 TeV
Projection QWeak
• Λ
g > 2 TeV
• 4% precision
28
104. Sensitivity to New Physics
Lower bound on new physics (95% CL)
Figure: Young, Carlini, Thomas, Roche (2007)
Constraints from
• Atomic PV:
Λ
g > 0.4 TeV
• PV electron
scattering:
Λ
g > 0.9 TeV
Projection QWeak
• Λ
g > 2 TeV
• 4% precision
28
105. Sensitivity to New Physics
Lower bound on new physics (95% CL)
Figure: Young, Carlini, Thomas, Roche (2007)
Constraints from
• Atomic PV:
Λ
g > 0.4 TeV
• PV electron
scattering:
Λ
g > 0.9 TeV
Projection QWeak
• Λ
g > 2 TeV
• 4% precision
28
111. Precision Electroweak Experiments: JLab 12 GeV
MOLLER Experiment
Source ∆APV
Mom. transfer Q2 0.5%
Beam polarization 0.4%
2nd order beam 0.4%
Inelastic ep 0.4%
Elastic ep 0.3%
SoLID PV-DIS Experiment
Source ∆APV
Beam polarization 0.4%
Rad. corrections 0.3%
Mom. transfer Q2 0.5%
Inelastic ep 0.2%
Statistics 0.3%
Precision beam polarimetry is crucial to these experiments.
32
112. Precision Electroweak Experiments: Polarimetry
Compton Polarimetry
• eγ → eγ (polarized laser)
• Detection e and/or γ
• Only when beam energy
above few hundred MeV
• High photon polarization
but low asymmetry
• Total systematics ∼ 1%
• laser polarization
• detector linearity
Møller Polarimetry
• ee → ee (magnetized Fe)
• Low current because
temperature induces
demagnetization
• High asymmetry but low
target polarization
• Levchuk effect: scattering
off internal shell electrons
• Intermittent measurements
at different beam conditions
• Total systematics ∼ 1%
33
113. Atomic Hydrogen Polarimetry
Møller polarimetry
• 300 mK cold atomic H
• 8 T solenoid trap
• 3 · 1016 atoms/cm2
• 3 · 1015−17 atoms/cm3
• 100% polarization of e in
the atomic hydrogen
Advantages
• High beam currents
• No Levchuk effect
• Non-invasive, continuous
Reference: E. Chudakov, V. Luppov, IEEE Trans. on Nucl. Sc.
51, 1533 (2004).
34
114. Atomic Hydrogen Polarimetry: 100% e Polarization
Hyperfine Splitting in Magnetic Field
• Force (−µ · B) will pull
|a and |b into field
• Energy splitting of ∆E = 2µB:
↑ / ↓= exp(−∆E/kT) ≈ 10−14
• Low energy states with |sesp :
• |d = |↑⇑
• |c = cos θ |↑⇓ + sin θ |↓⇑
• |b = |↓⇓
• |a = cos θ |↓⇑ − sin θ |↑⇓
• with sin θ ≈ 0.00035
• Pe(↓) ≈ 1 with only 105 dilution
from |↑⇓ in |a at B = 8 T
• Pp(⇑) ≈ 0.06 because 53% |a
and 47% |b
35
115. Atomic Hydrogen Polarimetry: Expected Contaminations
Without beam
• Recombined molecular hydrogen suppressed by coating of cell
with superfluid He, ∼ 10−5
• Residual gasses, can be measured with beam to < 0.1%
With 100 µA beam
• 497 MHz RF depolarization for 200 GHz |a → |c transition,
tuning of field to avoid resonances, uncertainty ∼ 2 · 10−4
• Ion-electron contamination: builds up at 20%/s in beam
region, cleaning with E field of ∼ 1 V/cm, uncertainty ∼ 10−5
36
117. Atomic Hydrogen Polarimetry: Collaboration with Mainz
P2 Experiment in Mainz: Weak Charge of the Proton
• “QWeak experiment” with improved statistical precision
• Dedicated 200 MeV accelerator MESA under construction
• Required precision of electron beam polarimetry < 0.5%
• Strong motivation for collaboration on a short timescale
(installation in 2017)
38
118. Ancillary Measurements: Background Processes
Aluminum asymmetry
(preliminary)
• Asymmetry consistent with
order of magnitude expected
• Asymmetry: few ppm
• Dilution f of 3%
• Correction ≈ 20%
Dilution measurement
(preliminary)
39
119. Radiative Corrections
Modified expression, Qp
W = 1 − 4 sin2
θW only at tree level
• Qp
W = (ρNC +∆e)(1−4 sin2
θW (0)+∆e)+BWW +BZZ +BγZ
• ∆ sin2
θW (MZ ), WW , ZZ box diagrams: uncertainty small
• γZ box: 8% correction with ≈ 1% uncertainty
Corrections to Qp
W ≈ 0.07
• Verification in “DIS” region, calculation by Melnitchouk
40
120. Radiative Corrections
Modified expression, Qp
W = 1 − 4 sin2
θW only at tree level
• Qp
W = (ρNC +∆e)(1−4 sin2
θW (0)+∆e)+BWW +BZZ +BγZ
• ∆ sin2
θW (MZ ), WW , ZZ box diagrams: uncertainty small
• γZ box: 8% correction with ≈ 1% uncertainty
Corrections to Qp
W ≈ 0.07
• Verification in “DIS” region, calculation by Melnitchouk
40
121. Radiative Corrections
Modified expression, Qp
W = 1 − 4 sin2
θW only at tree level
• Qp
W = (ρNC +∆e)(1−4 sin2
θW (0)+∆e)+BWW +BZZ +BγZ
• ∆ sin2
θW (MZ ), WW , ZZ box diagrams: uncertainty small
• γZ box: 8% correction with ≈ 1% uncertainty
Corrections to Qp
W ≈ 0.07
• Verification in “DIS” region, calculation by Melnitchouk
40
123. The QWeak Experiment: Main Detector
Event mode characterization
• Larger signal in + or - end
depending on proximity
• Number of photo-electrons
≈ 85 per track
Integrating data chain noise
• Current source (battery)
• Width ≈ 2.3 ppm
• Actual data with beam
• Width ≈ 240 ppm
• Not limited by electronic
noise
42
124. The QWeak Experiment: Main Detector
Event mode characterization
• Larger signal in + or - end
depending on proximity
• Number of photo-electrons
≈ 85 per track
Integrating data chain noise
• Current source (battery)
• Width ≈ 2.3 ppm
• Actual data with beam
• Width ≈ 240 ppm
• Not limited by electronic
noise
42
125. The QWeak Experiment: Systematic Uncertainties
Projected uncertainties on Ameas and Qp
W
Source of Contribution to Contribution to
uncertainty ∆Ameas/Ameas ∆Qp
W /Qp
W
Statistics 2.1% 3.2%
Hadronic structure – 1.5%
Beam polarimetry 1.0% 1.5%
Measurement Q2 0.5% 1.0%
Backgrounds 0.5% 0.7%
Helicity-correlated
beam properties 0.5% 0.7%
Total 2.5% 4.1%
43
132. The QWeak Experiment: Toroidal Magnet (QTOR)
QTOR installed in Hall C
• Full assembly and power supply tests
• Mapped at half field, within tolerances
QTOR properties
• Warm coils
• 10000 A
• 6 m high
Large coils aligned
to 1 mm
At MIT/Bates
49
133. The QWeak Experiment: Main Detector
Low noise electronics
• Event rate: 800 MHz/PMT
• Asymmetry of only 0.2 ppm
• Low noise electronics
(custom design, TRIUMF)
I-V Preamplifier 18-bit 500 kHz sampling ADC
Delivered, tested: noise is 3 times lower than counting statistics
50
134. The QWeak Experiment: Systematic Uncertainties
Reminder: weak vector charges
• Proton weak charge
Qp
W ≈ −0.072
• Neutron weak charge Qn
W = −1
Sources of neutron scattering
• Al target windows
• Secondary collimator events
• Small number of events, but
huge false PV asymmetry
Al target windows
51
135. The QWeak Experiment: Systematic Uncertainties
Largest projected uncertainties on Qp
W
• Total uncertainty on Qp
W : 4.1%
• Statistical uncertainty: 3.2%
• Hadronic structure: 1.5%
• Beam polarimetry: 1.5%
• Measurement of Q2: 1.0%
• Background events: 0.7%
• Helicity-correlated beam properties: 0.7%
Responsibilities of MIT group
• Track reconstruction/momentum determination software
• Construction of Compton polarimeter
52
136. The QWeak Experiment: Systematic Uncertainties
Largest projected uncertainties on Qp
W
• Total uncertainty on Qp
W : 4.1%
• Statistical uncertainty: 3.2%
• Hadronic structure: 1.5%
• Beam polarimetry: 1.5%
• Measurement of Q2: 1.0%
• Background events: 0.7%
• Helicity-correlated beam properties: 0.7%
Responsibilities of MIT group
• Track reconstruction/momentum determination software
• Construction of Compton polarimeter
52
137. The QWeak Experiment: Systematic Uncertainties
Largest projected uncertainties on Qp
W
• Total uncertainty on Qp
W : 4.1%
• Statistical uncertainty: 3.2%
• Hadronic structure: 1.5%
• Beam polarimetry: 1.5%
• Measurement of Q2: 1.0%
• Background events: 0.7%
• Helicity-correlated beam properties: 0.7%
Responsibilities of MIT group
• Track reconstruction/momentum determination software
• Construction of Compton polarimeter
52
138. The QWeak Experiment: Systematic Uncertainties
Largest projected uncertainties on Qp
W
• Total uncertainty on Qp
W : 4.1%
• Statistical uncertainty: 3.2%
• Hadronic structure: 1.5%
• Beam polarimetry: 1.5%
• Measurement of Q2: 1.0%
• Background events: 0.7%
• Helicity-correlated beam properties: 0.7%
Responsibilities of MIT group
• Track reconstruction/momentum determination software
• Construction of Compton polarimeter
52
139. The QWeak Experiment: Tracking Mode
Gas-electron multiplier (GEM)
• Very close to target, very high dose
• GEMs have high radiation hardness
• Several days of radcon cool-down in GEM bunker
• Remotely controlled rotator mounted on collimator
53
140. The QWeak Experiment: Tracking Mode
Horizontal drift chambers (HDC)
• 12 planes per octant
• u, v, x, u, v, x planes per assembly
• 4 + 1 constructed, tested
• Residuals from cosmic events
• Ready for installation
HDC rotator system
54
141. The QWeak Experiment: Tracking Mode
Vertical drift chambers (VDC)
• 181 wires in 2 m wide planes
• u, v, u, v planes per assembly
• Multiplexed read-out on delay lines
Principle of operation
VDC rotator system
55
142. Electroweak Interaction: Running of sin2
θW
Atomic parity-violation on 133
Cs
• New calculation in many-body atomic theory
• Porsev, Beloy, Derevianko; arXiv:0902.0335 [hep-ph]
• Experiment: QW (133Cs) = −73.25 ± 0.29 ± 0.20
• Standard Model: QW (133Cs) = −73.16 ± 0.03
NuTeV anomaly explained
• Originally, 3 σ deviation from Standard Model
• Erler, Langacker: strange quark PDFs
• Londergan, Thomas: charge symmetry violation, mu = md
• Cloet, Bentz, Thomas: in-medium modifications to PDFs,
isovector EMC-type effect
• Entire anomaly accounted for (everybody stops looking. . . )
56
143. Electroweak Interaction
Running of sin2
θW
• Higher order loop diagrams
• sin2
θW varies with Q2
APV(Cs)
SLAC E158
ν-DIS
Z-pole
CDF
D0
Møller [JLab]
Qweak [JLab]
PV-DIS [JLab]
0.225
0.230
0.235
0.240
0.245
0.250
sin2
θMS
W
0.001 0.01 0.1 1 10 100 1000 10000
Q (GeV)
Standard Model
Completed Experiments
Future Experiments
57
144. Electroweak Interaction
Running of sin2
θW
• Higher order loop diagrams
• sin2
θW varies with Q2
APV(Cs)
SLAC E158
Z-pole
CDF
D0
Møller [JLab]
Qweak [JLab]
PV-DIS [JLab]
0.225
0.230
0.235
0.240
0.245
0.250
sin2
θMS
W
0.001 0.01 0.1 1 10 100 1000 10000
Q (GeV)
Standard Model
Completed Experiments
Future Experiments
ν-DIS
57
145. Sensitivity to New Physics
New physics
• Consider effective contact interaction
• Coupling constant g, mass scale Λ
• Effective charges hu
V and hd
V
Effective Lagrangian
LPV
e−q = LPV
SM + LPV
New
= −
GF
√
2
eγµγ5e
q
C1qqγµ
q +
g2
4Λ2
eγµγ5e
q
hV
q qγµ
q
58