The document summarizes key aspects of quantum field theory on de Sitter spacetime, including solutions to the Dirac, scalar, electromagnetic, and other field equations. It presents:
1) Fundamental solutions for the Dirac equation and orthonormalization relations for Dirac spinor modes.
2) Solutions to the Klein-Gordon equation for a scalar field and corresponding orthonormalization relations.
3) Quantization of electromagnetic vector potentials in the Coulomb gauge and orthonormalization relations for photon modes.
Dual Gravitons in AdS4/CFT3 and the Holographic Cotton TensorSebastian De Haro
This document summarizes research on dual gravitons in AdS4/CFT3 and the holographic Cotton tensor. Key points:
- In AdS4/CFT3, both modes of the graviton are normalizable, allowing duality to interchange the boundary metric g(0) and stress tensor T.
- The Cotton tensor C, which maps a metric to its stress tensor, plays a special role as the "holographic Cotton tensor".
- There is a duality symmetry of the bulk equations of motion under which the linearized metric fluctuations ḣ and Cotton tensor of the dual metric C(ḣ) are interchanged.
- This relates the
This document discusses unconditionally stable finite-difference time-domain (FDTD) methods for solving Maxwell's equations numerically. It outlines FDTD algorithms such as Yee's method from 1966 which discretize the equations on a staggered grid. It also discusses the von Neumann stability analysis and compares implicit Crank-Nicolson and alternating-direction implicit methods to conventional explicit FDTD methods. The document notes the advantages of unconditionally stable methods but also mentions potential disadvantages.
The document describes a Hamiltonian with terms including Ji,j|ωiωj| and Ei|ωiωi| that depends on parameters ∆/J and ω. It studies the behavior of the system as ∆/J increases from 0 to greater than 6, including plots of the momentum distribution |P(k)|2 that show it spreading out over more values of k/k1. The dependence of the system on other parameters like α, s1, and s2 is also examined through additional plots.
This document contains mathematical equations and definitions related to quantum mechanics and quantum operators. It defines operators such as momentum, position, angular momentum, and their commutation relations. It also provides equations for wave functions, energy levels, and harmonic oscillator states. Harmonic oscillator wave functions, energy eigenvalues, and operator relations are summarized.
1. The function f(x) is defined as 2 + x^2 and g(x) is defined as 1 + x^2.
2. It is given that f(g(x)) = 3 + 2(g(x) - 1) + (g(x) - 1)^2.
3. Substituting g(x) = 1 + x^2 into the equation for f(g(x)) yields f(x) = 2 + x^2.
This document discusses using Gaussian process models for change point detection in atmospheric dispersion problems. It proposes using multiple kernels in a Gaussian process to model different regimes indicated by change points. A two-stage process is used to first estimate the change point (release time) and then estimate the source location. Simulation results show the approach outperforms existing techniques in estimating change points and source locations from concentration sensor measurements. The approach is applied to model real concentration data to estimate a CBRN release scenario.
1. Gibbs sampling is a technique for drawing samples from probability distributions by iteratively sampling each variable conditioned on the current values of the other variables. It can be used to sample from Markov random fields and Bayesian networks.
2. An Ising model is a Markov random field with binary variables on a grid that are correlated with their neighbors. Gibbs sampling in an Ising model samples each variable based on its neighbors' current values.
3. Boltzmann machines generalize the Ising model to arbitrary graph structures between variables. Restricted Boltzmann machines and Hopfield networks are specific types of Boltzmann machines.
The document discusses Gauss-Seidel, Successive Over Relaxation (SOR), and block SOR methods for solving systems of linear equations. Gauss-Seidel converges faster than Jacobi iteration. SOR can further accelerate convergence by introducing a relaxation parameter ω between 0 and 2. Block SOR generalizes the approach to block-structured matrices by solving blocks simultaneously. Examples show how to apply these methods to finite difference discretizations in 2D and 3D.
Dual Gravitons in AdS4/CFT3 and the Holographic Cotton TensorSebastian De Haro
This document summarizes research on dual gravitons in AdS4/CFT3 and the holographic Cotton tensor. Key points:
- In AdS4/CFT3, both modes of the graviton are normalizable, allowing duality to interchange the boundary metric g(0) and stress tensor T.
- The Cotton tensor C, which maps a metric to its stress tensor, plays a special role as the "holographic Cotton tensor".
- There is a duality symmetry of the bulk equations of motion under which the linearized metric fluctuations ḣ and Cotton tensor of the dual metric C(ḣ) are interchanged.
- This relates the
This document discusses unconditionally stable finite-difference time-domain (FDTD) methods for solving Maxwell's equations numerically. It outlines FDTD algorithms such as Yee's method from 1966 which discretize the equations on a staggered grid. It also discusses the von Neumann stability analysis and compares implicit Crank-Nicolson and alternating-direction implicit methods to conventional explicit FDTD methods. The document notes the advantages of unconditionally stable methods but also mentions potential disadvantages.
The document describes a Hamiltonian with terms including Ji,j|ωiωj| and Ei|ωiωi| that depends on parameters ∆/J and ω. It studies the behavior of the system as ∆/J increases from 0 to greater than 6, including plots of the momentum distribution |P(k)|2 that show it spreading out over more values of k/k1. The dependence of the system on other parameters like α, s1, and s2 is also examined through additional plots.
This document contains mathematical equations and definitions related to quantum mechanics and quantum operators. It defines operators such as momentum, position, angular momentum, and their commutation relations. It also provides equations for wave functions, energy levels, and harmonic oscillator states. Harmonic oscillator wave functions, energy eigenvalues, and operator relations are summarized.
1. The function f(x) is defined as 2 + x^2 and g(x) is defined as 1 + x^2.
2. It is given that f(g(x)) = 3 + 2(g(x) - 1) + (g(x) - 1)^2.
3. Substituting g(x) = 1 + x^2 into the equation for f(g(x)) yields f(x) = 2 + x^2.
This document discusses using Gaussian process models for change point detection in atmospheric dispersion problems. It proposes using multiple kernels in a Gaussian process to model different regimes indicated by change points. A two-stage process is used to first estimate the change point (release time) and then estimate the source location. Simulation results show the approach outperforms existing techniques in estimating change points and source locations from concentration sensor measurements. The approach is applied to model real concentration data to estimate a CBRN release scenario.
1. Gibbs sampling is a technique for drawing samples from probability distributions by iteratively sampling each variable conditioned on the current values of the other variables. It can be used to sample from Markov random fields and Bayesian networks.
2. An Ising model is a Markov random field with binary variables on a grid that are correlated with their neighbors. Gibbs sampling in an Ising model samples each variable based on its neighbors' current values.
3. Boltzmann machines generalize the Ising model to arbitrary graph structures between variables. Restricted Boltzmann machines and Hopfield networks are specific types of Boltzmann machines.
The document discusses Gauss-Seidel, Successive Over Relaxation (SOR), and block SOR methods for solving systems of linear equations. Gauss-Seidel converges faster than Jacobi iteration. SOR can further accelerate convergence by introducing a relaxation parameter ω between 0 and 2. Block SOR generalizes the approach to block-structured matrices by solving blocks simultaneously. Examples show how to apply these methods to finite difference discretizations in 2D and 3D.
One way to see higher dimensional surfaceKenta Oono
The document defines and describes various matrix groups and their properties in 3 sentences:
It introduces common matrix groups such as GLn(R), SLn(R), On, and defines them as subsets of Mn(R) satisfying certain properties like determinant constraints. It also discusses low dimensional examples including SO(2), SO(3), and representations of groups like SU(2) acting on su(2) by adjoint representations. Finally, it briefly mentions homotopy groups πn and homology groups Hn as topological invariants that can distinguish spaces.
The document summarizes two models:
1. The Lo-Zivot Threshold Cointegration Model, which uses a threshold vector error correction model (TVECM) to analyze the dynamic adjustment of cointegrated time series variables to their long-run equilibrium. It allows for nonlinear and asymmetric adjustment speeds.
2. A bivariate vector error correction model (VECM) and band-threshold vector error correction model (BAND-TVECM) that extend the VECM to allow for nonlinear and discontinuous adjustments to long-run equilibrium across multiple regimes defined by thresholds on a variable. This captures asymmetric adjustment speeds and dynamic behavior.
The BAND-TVECM allows modeling of
The document discusses properties and applications of the Z-transform, which is used to analyze linear discrete-time signals. Some key points:
1) The Z-transform plays an important role in analyzing discrete-time signals and is defined as the sum of the signal samples multiplied by a complex variable z raised to the power of the sample's time index.
2) Important properties of the Z-transform include linearity, time-shifting, frequency-shifting, differentiation in the Z-domain, and the convolution theorem.
3) The Z-transform can be used to find the transform of basic sequences like the unit impulse, unit step, exponentials, polynomials, and derivatives of signals.
This document summarizes a talk on Lorentz surfaces in pseudo-Riemannian space forms with horizontal reflector lifts. It introduces examples of Lorentz surfaces with zero mean curvature in these spaces. It also discusses reflector spaces and horizontal reflector lifts, and presents a rigidity theorem stating that if two isometric immersions from a Lorentz surface to a pseudo-Riemannian space form both have horizontal reflector lifts and satisfy certain curvature conditions, then the immersions must differ by an isometry of the target space.
1) The document defines properties of exponential and logarithmic functions including: exponential functions follow exponent laws, logarithmic functions follow logarithmic laws, and the derivatives of exponentials and logarithms are the exponential/logarithmic functions themselves multiplied by the exponent/logarithm's argument.
2) Rules for limits of exponentials and logarithms as the argument approaches positive/negative infinity or zero are provided.
3) Graphs of the natural logarithm and logarithms with base a > 1 are similar shapes that increase without bound as the argument increases from 0 to infinity.
This document provides an introduction to inverse problems and their applications. It summarizes integral equations like Volterra and Fredholm equations of the first and second kind. It also describes inverse problems for partial differential equations, including inverse convection-diffusion, Poisson, and Laplace problems. Applications mentioned include medical imaging, non-destructive testing, and geophysics. Bibliographic references are provided.
This document provides summaries of common derivatives and integrals, including:
- Basic properties and formulas for derivatives and integrals of functions like polynomials, trig functions, inverse trig functions, exponentials/logarithms, and more.
- Standard integration techniques like u-substitution, integration by parts, and trig substitutions.
- How to evaluate integrals of products and quotients of trig functions using properties like angle addition formulas and half-angle identities.
- How to use partial fractions to decompose rational functions for the purpose of integration.
So in summary, this document outlines essential derivatives and integrals for many common functions, along with standard integration strategies and techniques.
This document provides a calculus cheat sheet covering key topics in limits, derivatives, and integrals. It defines limits, including one-sided limits and limits at infinity. Properties of limits are listed. Derivatives are defined and basic rules like the power, constant multiple, sum, difference, and chain rules are covered. Common derivatives are provided. Higher order derivatives and the second derivative are defined. Evaluation techniques like L'Hospital's rule, polynomials at infinity, and piecewise functions are summarized.
This calculus cheat sheet provides definitions and formulas for:
1) Integrals including definite integrals, anti-derivatives, and the Fundamental Theorem of Calculus.
2) Common integration techniques like u-substitution and integration by parts.
3) Standard integrals of common functions like polynomials, trigonometric functions, logarithms, and exponentials.
Proximal Splitting and Optimal TransportGabriel Peyré
This document summarizes proximal splitting and optimal transport methods. It begins with an overview of topics including optimal transport and imaging, convex analysis, and various proximal splitting algorithms. It then discusses measure-preserving maps between distributions and defines the optimal transport problem. Finally, it presents formulations for optimal transport including the convex Benamou-Brenier formulation and discrete formulations on centered and staggered grids. Numerical examples of optimal transport between distributions on 2D domains are also shown.
Cosmological Perturbations and Numerical SimulationsIan Huston
Talk given at Queen Mary, University of London in March 2010.
Cosmological perturbation theory is well established as a tool for
probing the inhomogeneities of the early universe.
In this talk I will motivate the use of perturbation theory and
outline the mathematical formalism. Perturbations beyond linear order
are especially interesting as non-Gaussian effects can be used to
constrain inflationary models.
I will show how the Klein-Gordon equation at second order, written in
terms of scalar field variations only, can be numerically solved.
The slow roll version of the second order source term is used and the
method is shown to be extendable to the full equation. This procedure
allows the evolution of second order perturbations in general and the
calculation of the non-Gaussianity parameter in cases where there is
no analytical solution available.
Low Complexity Regularization of Inverse ProblemsGabriel Peyré
This document discusses regularization techniques for inverse problems. It begins with an overview of compressed sensing and inverse problems, as well as convex regularization using gauges. It then discusses performance guarantees for regularization methods using dual certificates and L2 stability. Specific examples of regularization gauges are given for various models including sparsity, structured sparsity, low-rank, and anti-sparsity. Conditions for exact recovery using random measurements are provided for sparse vectors and low-rank matrices. The discussion concludes with the concept of a minimal-norm certificate for the dual problem.
The document outlines research on developing optimal finite difference grids for solving elliptic and parabolic partial differential equations (PDEs). It introduces the motivation to accurately compute Neumann-to-Dirichlet (NtD) maps. It then summarizes the formulation and discretization of model elliptic and parabolic PDE problems, including deriving the discrete NtD map. It presents results on optimal grid design and the spectral accuracy achieved. Future work is proposed on extending the NtD map approach to non-uniformly spaced boundary data.
This document provides definitions and formulas from theoretical computer science, including:
1. Big O, Omega, and Theta notation for analyzing algorithm complexity.
2. Common series like geometric and harmonic series.
3. Recurrence relations and methods for solving them like the master theorem.
4. Combinatorics topics like permutations, combinations, and binomial coefficients.
1) The volume of the solid region bounded by z = 9 - x^2 - y in the first octant is found using iterated integration.
2) The volume of the region bounded by z = x^2 + y^2, x^2 + y^2 = 25, and the xy-plane is found using polar coordinates.
3) The double integral of sin(x^2) over the region from 0 to 9 in x and y from 0 to x is evaluated.
Stuff You Must Know Cold for the AP Calculus BC Exam!A Jorge Garcia
This document provides a summary of key concepts from AP Calculus that students must know, including:
- Differentiation rules like product rule, quotient rule, and chain rule
- Integration techniques like Riemann sums, trapezoidal rule, and Simpson's rule
- Theorems related to derivatives and integrals like the Mean Value Theorem, Fundamental Theorem of Calculus, and Rolle's Theorem
- Common trigonometric derivatives and integrals
- Series approximations like Taylor series and Maclaurin series
- Calculus topics for polar coordinates, parametric equations, and vectors
Special second order non symmetric fitted method for singularAlexander Decker
The document presents a special second order non-symmetric fitted difference method for solving singularly perturbed two-point boundary value problems with boundary layers. The method introduces a fitting factor in the finite difference scheme to account for rapid changes in the boundary layer. The fitting factor is derived from singular perturbation theory. The method is applied to problems with left-end and right-end boundary layers. A tridiagonal system is obtained and solved using the discrete invariant embedding algorithm. Numerical results illustrate the accuracy of the proposed method.
The document provides information about Fourier transforms. It defines the Fourier integral transform using a kernel function k(s,x). It presents the Fourier integral theorem relating a function f(x) to its Fourier integral. It gives examples of using the Fourier integral formula to express functions as Fourier integrals and evaluates related integrals. It also defines the complex form of Fourier integrals and Fourier transforms, and presents the inversion formulas. It discusses Fourier sine and cosine transforms and their inversion formulas. It provides problems demonstrating the use of Fourier integral and transform formulas to represent functions and prove identities.
A. Lombardo, 25 Years of Central European Initiative: Contributing to Europea...SEENET-MTP
The Central European Initiative (CEI) is a regional intergovernmental forum that promotes cooperation across 18 Central European member states. For 25 years, the CEI has contributed to European integration in the region through multilateral diplomacy and project management. It provides funding and acts as both a donor and recipient on EU-funded projects, leveraging its resources to mobilize over 50 times their value in additional EU funding. Looking ahead, the CEI aims to strengthen scientific cooperation across the region and participate in the EU macro-regional strategies.
R. Jimenez: Fundamental Physics Beyond the Standard Model from Astronomical O...SEENET-MTP
This document discusses how future cosmological experiments can provide information about fundamental physics. It summarizes some key findings from the Planck experiment and discusses how measurements of the cosmic microwave background and large scale structure can constrain properties of neutrinos and test for new physics beyond the standard model, such as primordial non-Gaussianities and interactions between photons and axion-like particles. Future surveys like EUCLID are expected to dramatically improve constraints on these models and properties by providing a vast amount of high quality cosmological data.
B. Sazdović: Canonical Approach to Closed String Non-commutativitySEENET-MTP
This document discusses closed string noncommutativity in string theory. It begins by reviewing open string noncommutativity and T-duality. It then considers a weakly curved background with both constant and coordinate-dependent fields. A generalized Buscher transformation is used to derive T-duality along all directions, resulting in a doubled geometry description. This leads to noncommutativity of both winding and momentum modes of the closed string. Nongeometric fluxes are also introduced that contribute to closed string noncommutativity.
One way to see higher dimensional surfaceKenta Oono
The document defines and describes various matrix groups and their properties in 3 sentences:
It introduces common matrix groups such as GLn(R), SLn(R), On, and defines them as subsets of Mn(R) satisfying certain properties like determinant constraints. It also discusses low dimensional examples including SO(2), SO(3), and representations of groups like SU(2) acting on su(2) by adjoint representations. Finally, it briefly mentions homotopy groups πn and homology groups Hn as topological invariants that can distinguish spaces.
The document summarizes two models:
1. The Lo-Zivot Threshold Cointegration Model, which uses a threshold vector error correction model (TVECM) to analyze the dynamic adjustment of cointegrated time series variables to their long-run equilibrium. It allows for nonlinear and asymmetric adjustment speeds.
2. A bivariate vector error correction model (VECM) and band-threshold vector error correction model (BAND-TVECM) that extend the VECM to allow for nonlinear and discontinuous adjustments to long-run equilibrium across multiple regimes defined by thresholds on a variable. This captures asymmetric adjustment speeds and dynamic behavior.
The BAND-TVECM allows modeling of
The document discusses properties and applications of the Z-transform, which is used to analyze linear discrete-time signals. Some key points:
1) The Z-transform plays an important role in analyzing discrete-time signals and is defined as the sum of the signal samples multiplied by a complex variable z raised to the power of the sample's time index.
2) Important properties of the Z-transform include linearity, time-shifting, frequency-shifting, differentiation in the Z-domain, and the convolution theorem.
3) The Z-transform can be used to find the transform of basic sequences like the unit impulse, unit step, exponentials, polynomials, and derivatives of signals.
This document summarizes a talk on Lorentz surfaces in pseudo-Riemannian space forms with horizontal reflector lifts. It introduces examples of Lorentz surfaces with zero mean curvature in these spaces. It also discusses reflector spaces and horizontal reflector lifts, and presents a rigidity theorem stating that if two isometric immersions from a Lorentz surface to a pseudo-Riemannian space form both have horizontal reflector lifts and satisfy certain curvature conditions, then the immersions must differ by an isometry of the target space.
1) The document defines properties of exponential and logarithmic functions including: exponential functions follow exponent laws, logarithmic functions follow logarithmic laws, and the derivatives of exponentials and logarithms are the exponential/logarithmic functions themselves multiplied by the exponent/logarithm's argument.
2) Rules for limits of exponentials and logarithms as the argument approaches positive/negative infinity or zero are provided.
3) Graphs of the natural logarithm and logarithms with base a > 1 are similar shapes that increase without bound as the argument increases from 0 to infinity.
This document provides an introduction to inverse problems and their applications. It summarizes integral equations like Volterra and Fredholm equations of the first and second kind. It also describes inverse problems for partial differential equations, including inverse convection-diffusion, Poisson, and Laplace problems. Applications mentioned include medical imaging, non-destructive testing, and geophysics. Bibliographic references are provided.
This document provides summaries of common derivatives and integrals, including:
- Basic properties and formulas for derivatives and integrals of functions like polynomials, trig functions, inverse trig functions, exponentials/logarithms, and more.
- Standard integration techniques like u-substitution, integration by parts, and trig substitutions.
- How to evaluate integrals of products and quotients of trig functions using properties like angle addition formulas and half-angle identities.
- How to use partial fractions to decompose rational functions for the purpose of integration.
So in summary, this document outlines essential derivatives and integrals for many common functions, along with standard integration strategies and techniques.
This document provides a calculus cheat sheet covering key topics in limits, derivatives, and integrals. It defines limits, including one-sided limits and limits at infinity. Properties of limits are listed. Derivatives are defined and basic rules like the power, constant multiple, sum, difference, and chain rules are covered. Common derivatives are provided. Higher order derivatives and the second derivative are defined. Evaluation techniques like L'Hospital's rule, polynomials at infinity, and piecewise functions are summarized.
This calculus cheat sheet provides definitions and formulas for:
1) Integrals including definite integrals, anti-derivatives, and the Fundamental Theorem of Calculus.
2) Common integration techniques like u-substitution and integration by parts.
3) Standard integrals of common functions like polynomials, trigonometric functions, logarithms, and exponentials.
Proximal Splitting and Optimal TransportGabriel Peyré
This document summarizes proximal splitting and optimal transport methods. It begins with an overview of topics including optimal transport and imaging, convex analysis, and various proximal splitting algorithms. It then discusses measure-preserving maps between distributions and defines the optimal transport problem. Finally, it presents formulations for optimal transport including the convex Benamou-Brenier formulation and discrete formulations on centered and staggered grids. Numerical examples of optimal transport between distributions on 2D domains are also shown.
Cosmological Perturbations and Numerical SimulationsIan Huston
Talk given at Queen Mary, University of London in March 2010.
Cosmological perturbation theory is well established as a tool for
probing the inhomogeneities of the early universe.
In this talk I will motivate the use of perturbation theory and
outline the mathematical formalism. Perturbations beyond linear order
are especially interesting as non-Gaussian effects can be used to
constrain inflationary models.
I will show how the Klein-Gordon equation at second order, written in
terms of scalar field variations only, can be numerically solved.
The slow roll version of the second order source term is used and the
method is shown to be extendable to the full equation. This procedure
allows the evolution of second order perturbations in general and the
calculation of the non-Gaussianity parameter in cases where there is
no analytical solution available.
Low Complexity Regularization of Inverse ProblemsGabriel Peyré
This document discusses regularization techniques for inverse problems. It begins with an overview of compressed sensing and inverse problems, as well as convex regularization using gauges. It then discusses performance guarantees for regularization methods using dual certificates and L2 stability. Specific examples of regularization gauges are given for various models including sparsity, structured sparsity, low-rank, and anti-sparsity. Conditions for exact recovery using random measurements are provided for sparse vectors and low-rank matrices. The discussion concludes with the concept of a minimal-norm certificate for the dual problem.
The document outlines research on developing optimal finite difference grids for solving elliptic and parabolic partial differential equations (PDEs). It introduces the motivation to accurately compute Neumann-to-Dirichlet (NtD) maps. It then summarizes the formulation and discretization of model elliptic and parabolic PDE problems, including deriving the discrete NtD map. It presents results on optimal grid design and the spectral accuracy achieved. Future work is proposed on extending the NtD map approach to non-uniformly spaced boundary data.
This document provides definitions and formulas from theoretical computer science, including:
1. Big O, Omega, and Theta notation for analyzing algorithm complexity.
2. Common series like geometric and harmonic series.
3. Recurrence relations and methods for solving them like the master theorem.
4. Combinatorics topics like permutations, combinations, and binomial coefficients.
1) The volume of the solid region bounded by z = 9 - x^2 - y in the first octant is found using iterated integration.
2) The volume of the region bounded by z = x^2 + y^2, x^2 + y^2 = 25, and the xy-plane is found using polar coordinates.
3) The double integral of sin(x^2) over the region from 0 to 9 in x and y from 0 to x is evaluated.
Stuff You Must Know Cold for the AP Calculus BC Exam!A Jorge Garcia
This document provides a summary of key concepts from AP Calculus that students must know, including:
- Differentiation rules like product rule, quotient rule, and chain rule
- Integration techniques like Riemann sums, trapezoidal rule, and Simpson's rule
- Theorems related to derivatives and integrals like the Mean Value Theorem, Fundamental Theorem of Calculus, and Rolle's Theorem
- Common trigonometric derivatives and integrals
- Series approximations like Taylor series and Maclaurin series
- Calculus topics for polar coordinates, parametric equations, and vectors
Special second order non symmetric fitted method for singularAlexander Decker
The document presents a special second order non-symmetric fitted difference method for solving singularly perturbed two-point boundary value problems with boundary layers. The method introduces a fitting factor in the finite difference scheme to account for rapid changes in the boundary layer. The fitting factor is derived from singular perturbation theory. The method is applied to problems with left-end and right-end boundary layers. A tridiagonal system is obtained and solved using the discrete invariant embedding algorithm. Numerical results illustrate the accuracy of the proposed method.
The document provides information about Fourier transforms. It defines the Fourier integral transform using a kernel function k(s,x). It presents the Fourier integral theorem relating a function f(x) to its Fourier integral. It gives examples of using the Fourier integral formula to express functions as Fourier integrals and evaluates related integrals. It also defines the complex form of Fourier integrals and Fourier transforms, and presents the inversion formulas. It discusses Fourier sine and cosine transforms and their inversion formulas. It provides problems demonstrating the use of Fourier integral and transform formulas to represent functions and prove identities.
A. Lombardo, 25 Years of Central European Initiative: Contributing to Europea...SEENET-MTP
The Central European Initiative (CEI) is a regional intergovernmental forum that promotes cooperation across 18 Central European member states. For 25 years, the CEI has contributed to European integration in the region through multilateral diplomacy and project management. It provides funding and acts as both a donor and recipient on EU-funded projects, leveraging its resources to mobilize over 50 times their value in additional EU funding. Looking ahead, the CEI aims to strengthen scientific cooperation across the region and participate in the EU macro-regional strategies.
R. Jimenez: Fundamental Physics Beyond the Standard Model from Astronomical O...SEENET-MTP
This document discusses how future cosmological experiments can provide information about fundamental physics. It summarizes some key findings from the Planck experiment and discusses how measurements of the cosmic microwave background and large scale structure can constrain properties of neutrinos and test for new physics beyond the standard model, such as primordial non-Gaussianities and interactions between photons and axion-like particles. Future surveys like EUCLID are expected to dramatically improve constraints on these models and properties by providing a vast amount of high quality cosmological data.
B. Sazdović: Canonical Approach to Closed String Non-commutativitySEENET-MTP
This document discusses closed string noncommutativity in string theory. It begins by reviewing open string noncommutativity and T-duality. It then considers a weakly curved background with both constant and coordinate-dependent fields. A generalized Buscher transformation is used to derive T-duality along all directions, resulting in a doubled geometry description. This leads to noncommutativity of both winding and momentum modes of the closed string. Nongeometric fluxes are also introduced that contribute to closed string noncommutativity.
N. Kroo, On the changing world of scienceSEENET-MTP
The document discusses how science and education are changing in response to rapid technological, economic, social, and environmental changes. Some key points:
- The complexity of knowledge is increasing, requiring deeper specialization but also more interdisciplinary research to address complex problems. The costs of research are rising significantly.
- Globalization is influencing all aspects of science and education through increased internationalization, collaboration, and competition between universities.
- Education systems must adapt to better prepare students for an uncertain future with jobs that may not even exist yet. This requires teaching skills like critical thinking and leadership over just knowledge acquisition.
- Cooperation between countries can help build on shared experiences and increase critical mass in education and research to tackle
R. Doran, Galileo Teacher Training Program - Helping Teachers Build the Schoo...SEENET-MTP
This document discusses empowering educators with skills for innovative science teaching that involves doing science. It proposes establishing a community of stakeholders including trainers, teachers, students, scientists and education authorities. It also mentions using online labs for large-scale science education.
I. Doršner, Leptoquark Mass Limit in SU(5)SEENET-MTP
The document summarizes a talk given on leptoquark mass limits in the SU(5) model of particle physics. It discusses how the SU(5) model unifies fermions into representations and predicts their mass relations. It also addresses proton decay processes mediated by scalar leptoquarks and the resulting limits on the leptoquark mass from non-observation of proton decay. The talk outlines fermion masses in SU(5), proton decay operators, and predictions for proton lifetimes that constrain the minimal viable SU(5) scenario.
S. Ignjatović, On Some Models of the Exotic Hadron StatesSEENET-MTP
This document discusses models of exotic hadron states beyond conventional quark-antiquark mesons and three-quark baryons. It summarizes the tetraquark model where a tetraquark is composed of a diquark and antidiquark binding together. Other models discussed include uncorrelated quark models and meson-meson molecules. The document concludes that tetraquarks remain an active area of research, various models cannot be distinguished by spectroscopy alone, and diquarks are an important concept in non-perturbative quantum chromodynamics.
1) The composite Higgs paradigm proposes that the Higgs boson arises as a pseudo-Nambu-Goldstone boson from a strongly interacting sector that spontaneously breaks a global symmetry. This provides a natural explanation for the Higgs mass.
2) A 125 GeV Higgs mass implies the existence of new light fermion resonances below 1 TeV that mix with top quarks to generate the Higgs potential radiatively. Direct searches for top partners at the LHC are important to test this scenario.
3) A key open problem is constructing ultraviolet completions of composite Higgs models that address issues like Landau poles from introducing many new fermions to generate masses for all standard model fermions via partial compositeness.
G. Zaharijas, Indirect Searches for Dark Matter with the Fermi Large Area Tel...SEENET-MTP
The Fermi LAT provides a rich program for indirect dark matter searches across multiple scales. It can detect both gamma rays and electrons. Key targets include dwarf spheroidal galaxies, which are the smallest resolved halos with stellar components; galaxy clusters, which are the largest halos; and searches for gamma ray lines and diffuse emission from regions around the Galactic Center and at high Galactic latitudes. The Fermi LAT has a large field of view allowing it to monitor 20% of the sky at once. Its energy range from 20 MeV to over 300 GeV is well suited for WIMP searches. It has detected features such as the Fermi bubbles and provided precision measurements of the cosmic electron and positron spectra.
Likelihood is sometimes difficult to compute because of the complexity of the model. Approximate Bayesian computation (ABC) makes it easy to sample parameters generating approximation of observed data.
The document discusses dual gravitons in AdS4/CFT3 and proposes that the holographic Cotton tensor can play the role of the dual operator to the metric in the boundary CFT.
The Cotton tensor is a symmetric, traceless and conserved tensor that can be constructed from the linearized metric. It is the stress-energy tensor of gravitational Chern-Simons theory. The document proposes that the Cotton tensor and stress-energy tensor form a dual pair under the holographic duality, with the Cotton tensor acting as the operator corresponding to fluctuations of the metric in the bulk. This is motivated by properties of gravitational instantons and self-dual solutions in AdS.
The document provides 4 examples of calculating triple integrals over different regions. Example 1 calculates a triple integral over a region bounded by a paraboloid and plane in rectangular coordinates, then evaluates it in polar coordinates. Example 2 calculates a triple integral over a hemisphere in spherical coordinates. Example 3 finds the volume under a paraboloid and above a rectangle using a double integral. Example 4 calculates a triple integral over a tetrahedron bounded by 4 planes.
This document summarizes Hill's method for numerically approximating the eigenvalues and eigenfunctions of differential operators. Hill's method has two main steps:
1. Perform a Floquet-Bloch decomposition to reduce the problem from the real line to the interval [0,L] with periodic boundary conditions, parameterized by the Floquet exponent μ. This gives an operator with a compact resolvent.
2. Approximate the solutions by Fourier series, reducing the problem to a matrix eigenvalue problem that can be solved numerically.
The method is straightforward to implement and effective for various problems involving differential operators on the real line or with periodic boundary conditions. Convergence rates and error bounds for Hill's method are also presented.
The document provides 14 formulae across various topics:
- Algebra formulas for operations, exponents, logarithms
- Calculus formulas for derivatives, integrals, areas under curves
- Statistics formulas for means, standard deviations, probabilities
- Geometry formulas for distances, midpoints, areas of shapes
- Trigonometry formulas for trig functions, angles, triangles
- The symbols used in the formulas are explained.
The document provides 14 formulae across various topics:
- Algebra formulas for operations, exponents, logarithms
- Calculus formulas for derivatives, integrals, areas under curves
- Statistics formulas for means, standard deviations, probabilities
- Geometry formulas for distances, midpoints, areas of shapes
- Trigonometry formulas for trig functions, angles, triangles
- The symbols used in the formulas are explained.
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The document provides 14 formulae across 4 topics:
1) Algebra - includes formulae for roots of quadratic equations, logarithms, sequences, etc.
2) Calculus - includes formulae for derivatives, integrals, areas under curves, volumes of revolution.
3) Statistics - includes formulae for means, standard deviation, probability, binomial distribution.
4) Geometry - includes formulae for distances, midpoints, areas of triangles, circles, trigonometry ratios.
The document provides 14 formulae across 4 topics:
1) Algebra - includes formulae for roots of quadratic equations, logarithms, sequences, etc.
2) Calculus - includes formulae for derivatives, integrals, areas under curves, volumes of revolution.
3) Statistics - includes formulae for means, standard deviation, probability, binomial distribution.
4) Geometry - includes formulae for distances, midpoints, areas of triangles, circles, trigonometry ratios.
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A Szemeredi-type theorem for subsets of the unit cubeVjekoslavKovac1
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2) Estimating errors by pigeonholing scales, the difference between smooth and sharp progressions over various scales is bounded above by a sublinear function of scales.
3) For sufficiently nice subsets, the difference between measure and smoothed measure is arbitrarily small by choosing a small smoothing parameter.
Combining these propositions shows that for sufficiently nice subsets, gaps between progressions contain an interval
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The convenience yield implied by quadratic volatility smiles presentation [...yigalbt
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3) Tunneling probabilities between vacua can be computed from the instanton solutions, representing gravitational tunneling effects in the bulk and phase transitions in the boundary CFT.
Similar to Cosmin Crucean: Perturbative QED on de Sitter Universe. (20)
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Cosmin Crucean: Perturbative QED on de Sitter Universe.
1. PERTURBATIVE Q.E.D
ON DE SITTER UNIVERSE
WEST UNIVERSITY OF TIMISOARA
FACULTY OF PHYSICS
author: Crucean Cosmin
1
2. THE THEORY OF FREE FIELDS ON DE
SITTER UNIVERSE
Dirac field
• De Sitter metric:
1
ds2 = dt2 − e2ωtdx 2 = (dt2 − dx 2), ω > 0, ωtc = −e−ωt (1)
(ωtc)2 c
ˆ
gµν = ηαβ eαeβ
ˆ
ˆ
ˆ µ ν (2)
• In the Cartesian gauge the nonvanishing tetradic components are:
ˆ 1 ˆ ˆ 1
e0 = −ωtc, eˆ = −δˆωtc, e0 = − , ei = −δj .
ˆ
0
i
j
i
j 0 j
i
(3)
ωtc ωtc
2
3. • Action for Dirac field
√i ¯ α
S [e, ψ] = d x −g [ψγ ˆ Dαψ − (Dαψ)γ αψ]
4
ˆ ˆ
ˆ
2
¯
−mψψ , (4)
where
Dα = eµ Dµ = ∂α + Γα
ˆ α
ˆ ˆ ˆ (5)
• In this gauge the Dirac operator reads:
3iω 0
ED = iγ 0∂t + ie−ωtγ i∂i + γ
2
0 i 3iω 0
= −iωtc(γ ∂tc + γ ∂i) + γ (6)
2
• the Dirac equation
(ED − m)ψ = 0 (7)
• The fundamental solutions are:
1 πk/2 (1)
πp/ω e Hν− (qe−ωt)ξλ(p )
Up, λ(t, x ) = i 2
(1) eip·x−2ωt
(2π)3/2 λe−πk/2Hν+ (qe−ωt)ξλ(p )
(2)
πp/ω −λe−πk/2Hν− (qe−ωt)ηλ(p )
Vp, λ(t, x ) = i 1 πk/2 (2)
e−ip·x−2ωt , (8)
(2π)3/2 2 e Hν+ (qe−ωt)ηλ(p )
3
4. • Charge conjugation
¯
Up, λ(x) → Vp, λ(x) = iγ 2γ 0(Up, λ(x))T . (9)
• The orthonormalization relations :
¯
d3x(−g)1/2Up, λ(x)γ 0Up , λ (x) =
¯
d3x(−g)1/2Vp, λ(x)γ 0Vp , λ (x) = δλλ δ 3(p − p )
¯
d3x(−g)1/2Up,λ(x)γ 0Vp ,λ (x) = 0, (10)
d3p Up, λ(t, x )Up, λ(t, x ) + Vp, λ(t, x )Vp, λ(t, x ) = e−3ωtδ 3(x − x ).
+ +
(11)
λ
• The field operator
ψ(t, x ) = ψ (+)(t, x ) + ψ (−)(t, x )
= d3p Up, λ(t, x )a(p, λ) + Vp, λ(t, x )b+(p, λ) . (12)
λ
• Canonic cuantization
{a(p, λ), a+(p , λ )} = {b(p, λ), b+(p , λ )} = δλλ δ 3(p − p ) , (13)
4
5. {ψ(t, x ), ψ(t, x )} = e−3ωtγ 0δ 3(x − x ) , (14)
SF (t, t , x − x ) = i 0|T [ψ(x)ψ(x )]|0
= θ(t − t )S (+)(t, t , x − x )
−θ(t − t)S (−)(t, t , x − x ) . (15)
[ED (x) − m]SF (t, t , x − x ) = −e−3ωtδ 4(x − x ). (16)
• Conserved operators
Pi =: ψ, P iψ := d3p pi [a+(p, λ)a(p, λ) + b+(p, λ)b(p, λ)] (17)
λ
W =: ψ, W ψ := d3p pλ[a+(p, λ)a(p, λ) + b+(p, λ)b(p, λ)] . (18)
λ
iω 3 i +
↔
+
↔
H= d pp a (p, λ) ∂ pi a(p, λ) + b (p, λ) ∂ pi b(p, λ) . (19)
2
λ
5
6. •
[H, P i] = iωP i. (20)
Scalar field
• Action of the scalar field
∗ √ √
S[φ, φ ] = 4
d x −g L = d x −g ∂ µφ∗∂µφ − m2φ∗φ ,
4
(21)
• The Klein-Gordon equation:
1 √
√ ∂µ −g g µν ∂ν φ + m2φ = 0 . (22)
−g
∂t2 − e−2ωt∆ + 3ω∂t + m2 φ(x) = 0 . (23)
• Solutions of Klein-Gordon equation:
1 π e−3ωt/2 −πk/2 (1) p −ωt ip·x
fp (x) = 3/2
e Hik e e , (24)
2 ω (2π) ω
6
7. 9 m
k= µ2 − , 4 µ = , m > 3ω/2 (25)
ω
• The orthonormalization relations:
↔
3 1/2 ∗
i d x (−g) fp (x) ∂t fp (x) =
↔
3 1/2 ∗
−i d x (−g) fp (x) ∂t fp (x) = δ 3(p − p ) , (26)
↔
3 1/2
i d x (−g) fp (x) ∂t fp (x) = 0 , (27)
↔
∗
i 3
d p fp (t, x ) ∂t fp (t, x ) = e−3ωtδ 3(x − x ) . (28)
• Canonic cuantization
∗
φ(x) = φ(+)(x) + φ(−)(x) = d3p fp (x)a(p ) + fp (x)b+(p ) , (29)
[a(p ), a†(p )] = [b(p ), b†(p )] = δ 3(p − p ) . (30)
•
7
8. [φ(t, x ), ∂tφ†(t, x )] = ie−3ωtδ 3(x − x ) . (31)
• The commutator functions:
D(±)(x, x ) = i[φ(±)(x), φ(±)†(x )], (32)
∗
D(+)(x, x ) = i d3p fp (x)fp (x ),
∗
D(−)(x, x ) = −i d3p fp (x)fp (x ). (33)
• G(x, x ) is a Green function of the Klein-Gordon equation if:
∂t2 − e−2ωt∆x + 3ω∂t + m2 G(x, x ) = e−3ωtδ 4(x − x ) . (34)
DR(t, t , x − x ) = θ(t − t )D(t, t , x − x ) , (35)
DA(t, t , x − x ) = − θ(t − t)D(t, t , x − x ) , (36)
8
9. • The Feynman propagator,
DF (t, t , x − x ) = i 0|T [φ(x)φ†(x )] |0
= θ(t − t )D(+)(t, t , x − x ) − θ(t − t)D(−)(t, t , x − x ) ,
(37)
The electromagnetic field
• The action
√ 1 √
S[A] = d4x −g L = − d4x −g Fµν F µν , (38)
4
Fµν = ∂µAν − ∂ν Aµ
• Field equation √
∂ν ( −g g ναg µβ Fαβ ) = 0 , (39)
• In the Coulomb gauge A0 = 0, (Ai) ; i = 0 ,and chart {tc, x}
¸
(∂t2c − ∆)Ai = 0 (40)
9
10. • The field operator
(+) (−)
Ai(x) = Ai (x) + Ai (x)
= d3k ei(nk , λ)fk (x)a(k, λ) + [ei(nk , λ)fk (x)]∗a∗(k, λ)
λ
(41)
1 1
fk (x) = √ e−iktc+ik·x , (42)
(2π)3/2 2k
• the Hermitian form
↔ ↔
3 ∗
f, g = i d x f (tc, x ) ∂tc g(tc, x ) , f ∂ g = f (∂g) − g(∂f ) (43)
• The orthonormalization relations:
∗ ∗
fk , fk = − fk , fk = δ 3(k − k ) , (44)
∗
fk , fk = 0 , (45)
↔
3 ∗
i d k fk (tc, x) ∂tc fk (tc, x ) = δ 3(x − x ) , (46)
k · e (nk , λ) = 0 , (47)
10
11. e (nk , λ) · e (nk , λ )∗ = δλλ , (48)
∗ k ik j
ei(nk , λ) ej (nk , λ) = δij − 2 . (49)
k
λ
• In local frame
·
Aˆ (x) = e ˆj Aj =
i i·
d3k wˆ k,λ)(x)a(k, λ) + [wˆ k,λ)(x)]∗a∗(k, λ) .
i( i( (50)
λ
• Conformal transformation
gµν (x) = Ω(x)ηµν , (51)
g µν (x) = Ω−1(x)η µν , ds2 = Ω ds2,
c (52)
Aµ = Aµ ; Aµ = Ω−1A µ. (53)
• Quantization
[a(k, λ), a†(k , λ )] = δλλ δ 3(k − k ) . (54)
[Ai(tc, x ), π j (tc, x )] = [Ai(tc, x ), ∂tc Aj (tc, x )] = i δij (x − x ) ,
tr
(55)
11
12. • The momentum density
j √ δL
π = −g = ∂tc Aj (56)
δ(∂tc Aj )
tr 1 q iq j
δij (x ) = d3q δij − 2 eiq·x (57)
(2π)3 q
• Conserved operators
1
Pl = δij : Ai, (P l A)j := d3k k l a†(k, λ)a(k, λ) , (58)
2
λ
1
H= δij : Ai, (HA)j : (59)
2
1
W = δij : Ai, (W A)j : = d3k k λ a†(k, λ)a(k, λ) (60)
2
λ
12
13. [H, P i] = iωP i , [H, W] = iωW , [W, P i] = 0 , (61)
3 i
(Hfk ) (x) = −iω k ∂ki + f (x) (62)
2 k
iω 3 i †
↔
H= d kk a (k, λ) ∂ ki a(k, λ) , (63)
2
• The commutator functions
(±) (±) (±) †
Dij (x − x ) = i[Ai (x), Aj (x )] (64)
(+) 3 ∗ k ik j
Dij (x −x) = i d k fk (x)fk (x ) δij − 2 (65)
k
(+) i d3k k ik j )−ik(tc −tc )
Dij (x −x)= δij − 2 eik·(x−x (66)
(2π)3 2k k
13
14. • at equal times,
(+) 1 tr
∂tc Dij (tc − tc, x − x ) = δij (x − x ) . (67)
tc =tc 2
• The transversal Green functions
tr
∂t2c − ∆x Gij (x − x ) = δ(tc − tc)δij (x − x ) (68)
si ∂iGi· (x) = 0.
¸ ·j
R
Dij (x − x ) = θ(tc − tc)Dij (x − x ) , (69)
A
Dij (x − x ) = −θ(tc − tc)Dij (x − x ) , (70)
• The Feynman propagator ,
F
Dij (x − x ) = i 0|T [Ai(x)Aj (x )] |0
(+) (−)
= θ(tc − tc)Dij (x − x ) − θ(tc − tc)Dij (x − x ) , (71)
14
15. Interaction between Dirac field and
electromagnetic field
• The action for interacting fields:
√
i ¯ α
S [e, ψ, A] = 4
d x −g [ψγ ˆ Dαψ − (Dαψ)γ αψ]
ˆ ˆ
ˆ
2
¯ 1 ¯ ˆ ˆ
−mψψ − Fµν F µν − eψγ αAαψ , (72)
4
• Equations for fields in interaction
iγ αDαψ − mψ = eγ αAαψ,
ˆ
ˆ
ˆ
ˆ
1 ¯ ˆ
∂µ (−g)F µν = eeν ψγ αψ.
α
ˆ (73)
(−g)
15
16. Interaction between scalar field and
electromagnetic field
• The action
√ µ † 1
2 †
S[φ, A] = d x −g (∂ φ ∂µφ − m φ φ) − Fµν F µν
4
4
−ie[(∂µφ†)φ − (∂µφ)φ†]Aµ + e2φ†φAµAµ . (74)
• Equations for fields in interaction
1 √ √
√ ∂µ −g g ∂ν φ − ie −gφAµ + m2φ = ie(∂µφ)Aµ + e2φAµAµ,
µν
−g
1
∂µ (−g)F µν = −ie[(∂ ν φ†)φ − (∂ ν φ)φ†]
(−g)
+2e2φ†φAν . (75)
16
17. The in out fields
• The equation of the interaction fields in the Coulomb gauge
¯
(∂t2c − ∆x)A(x) = eψ(x)γψ(x) (76)
• Solution:
ˆ
A(x) = A(x) − e ¯
d3ydtc DG(x − y)ψ(y)γψ(y), (77)
ˆ
A(x) = A(R/A)(x) − e ¯
d3ydtc DR/A(x − y)ψ(y)γψ(y), (78)
ˆ
• the free fields , A(R/A)(x) satisfy:
ˆ
lim (A(x) − A(R/A)(x)) = 0. (79)
t→ ∞
• The fields in/out:
√ ¯
z3Ain/out(x) = A(x) + e d3ydtc DR/A(x − y)ψ(y)γψ(y). (80)
17
18. • The in/out fields, final expressions:
√
z3Ain/out(x) = A(x) + d3ydtc DR/A(x − y)(∂t2c − ∆y )A(y), (81)
↔
3
a(k, λ)in/out = i d xfk (x)e (nk , λ) ∂tc Ain/out(x) (82)
• The case of interaction with scalar field
ˆ + e d4y √−g G(x, y) √ i ∂µ[√−gφ(y)Aµ(y)]
φ(x) = φ(x)
−g
+i[∂µφ(y)]Aµ(y) + eφ(y)Aµ(y)Aµ(y) , (83)
ˆ √ i √
φ(x) = φR/A(x) + e d y −gDR/A(x, y) √ ∂µ[ −gφ(y)Aµ(y)]
4
−g
+i[∂µφ(y)]Aµ(y) + eφ(y)Aµ(y)Aµ(y) . (84)
18
19. • The in/out fields:
√ √
zφin/out(x) = φ(x) − d y −gDR/A(x, y)[EKG(y) + m2]φ(y).
4
(85)
•
↔
3 ∗
a(p )in/out = i d x(−g)1/2fp (x) ∂t φin/out(x)
↔
† 3 1/2
b (p )in/out = i d x(−g) fp (x) ∂t φin/out(x). (86)
19
20. Perturbation theory
• The expression of Green functions
1 ˆ ˆ ˆ
G(y1, y2, ..., yn) = 0|T [φ(y1)φ(y2)...φ(yn), S]|0 , (87)
0|S|0
∞
(x)d4 x (−i)n
S = T e−i LI
=1+ T [LI (x1)...LI (xn)]d4x1...d4xn, (88)
n=1
n!
• The interaction Lagrangian
√
LI (x) = −ie −g : [(∂µφ†)φ − (∂µφ)φ†]Aµ : (89)
(−i)n ˆ ˆ ˆ
0|T [φ(y1)φ(y2)...φ(yn), LI (x1)...LI (xn)]|0 d4x1...d4xn. (90)
n! 0|S|0
20
21. • the amplitude:
3 1 ∗
out, 1(p )|in, 1(p ) = δ (p − p ) − −g(y) −g(z)fp (y)[EKG(y) + m2]
z
× 0|T [φ(y)φ†(z)]|0 [EKG(z) + m2]fp (z)d4yd4z. (91)
• The scattering amplitude in the first order of perturbation theory
↔
∗
Ai→f = −e −g(x) fp (x) ∂µ fp (x) Aµ(x)d4x, (92)
Ai→f = −ie ¯
−g(x)Up ,λ (x)γµ A
µ
ˆ
(x)Up,λ (x)d4x, (93)
21
22. Coulomb scattering for the charged scalar field
• External field
ˆ
0 Ze −ωt
A = e (94)
|x|
• initial and final states are:
φf (x) = fpf (x), φi(x) = fpi (x). (95)
• Scattering amplitude
−αZ pi ∞ (2) (1) (2) (1)
Ai→f = − z Hik (pf z)Hik−1(piz) − Hik (pf z)Hik+1(piz) dz
8π|pf − pi|2 2 0
pf ∞ (2) (1) (2) (1)
+ z Hik−1(pf z)Hik (piz) − Hik+1(pf z)Hik (piz) dz , (96)
2 0
e−ωt
z= . (97)
ω
22