The 21cm line from neutral hydrogen can be used to study cosmology during the first billion years of the universe. This includes the Dark Ages when no structures formed, the Cosmic Dawn when the first luminous objects formed, and the Epoch of Reionization when these objects reionized the intergalactic medium. Current and future 21cm experiments like LOFAR, MWA, PAPER, and HERA aim to detect the signal from these eras but face challenges in calibrating the instruments and subtracting bright foreground sources. Some progress has been made in placing upper limits on the signal and constraining the heating of the intergalactic medium by X-rays, but a clear detection of the signal is still needed
Using an ideal Lagrangian relaxation scheme for magnetic fields we investigate the formation of current concentrations for various magnetic field configurations. For sufficiently braided fields Parker (1972) hypothesizes the formation of singular current structures and subsequent reconnection. Here we find that even for highly braided fields current concentrations are well resolved and of finite magnitude. In presence of magnetic nulls, however, we confirm previous results of singular current structures at the nulls.
This document summarizes a presentation about exploring the early universe using the neutral hydrogen 21cm line. It discusses:
1. The history of the universe from the dark ages to the epoch of reionization, when the first stars and galaxies formed.
2. Current observations of the epoch of reionization provide constraints on the global neutral hydrogen fraction over time but do not reveal detailed spatial information.
3. Observing the 21cm line from neutral hydrogen in the intergalactic medium could directly probe the epoch of reionization and reveal information about ionized bubble morphology, the first luminous objects, and galaxy formation.
1) The document discusses challenging the assumption of an isotropic cosmos by analyzing patterns in the cosmic microwave background (CMB).
2) It summarizes past CMB space missions from 1991-2010 and upcoming missions from 2020 onward that aim to better measure the CMB anisotropy and polarization.
3) Non-parametric methods are presented to analyze the CMB angular power spectrum without assuming a particular cosmological model, allowing estimation of cosmological parameters in a model-independent way.
The document discusses using artificial neural networks (ANNs) to analyze 21cm cosmology data. Specifically, it discusses using ANNs to:
1) Emulate and speed up computation of 21cm power spectra from EoR parameters by 3 orders of magnitude.
2) Reconstruct EoR parameters like the mean free path and virial temperature from 21cm power spectra.
3) Recover the ionized bubble size distribution from 21cm power spectra to learn about the EoR source properties.
4) Generate 21cm distributions from Lyman-alpha emitter galaxy distributions using generative adversarial networks.
- The document discusses using 21cm forest observations to constrain properties of ultra-light dark matter particles like axions.
- 21cm forest observations can probe particle masses up to 10^-19 eV, 3 orders of magnitude higher than Lyman-alpha forest observations.
- Fisher forecast analysis suggests 21cm forest observations could probe ultra-light particle masses around 10^-20 eV and particle fraction values around 0.3.
- Ongoing work is studying effects of isocurvature fluctuations from breaking the Peccei-Quinn symmetry on 21cm forest observations.
- Ray theory explains many optical phenomena by considering light to travel in narrow paths called rays. Rays obey simple rules like reflection and Snell's laws.
- Optical resonators like Fabry-Perot cavities allow only certain resonant wavelengths/frequencies to propagate through interference of reflected waves. The modes are separated by the free spectral range and have a spectral width that depends on the finesse.
- Diffraction occurs when light passes through an aperture or obstruction, causing the beam to diverge and form an intensity pattern due to interference between wavelets from each point in the aperture. This pattern is explained by Huygens' principle and diffraction theory.
The 21cm line from neutral hydrogen can be used to study cosmology during the first billion years of the universe. This includes the Dark Ages when no structures formed, the Cosmic Dawn when the first luminous objects formed, and the Epoch of Reionization when these objects reionized the intergalactic medium. Current and future 21cm experiments like LOFAR, MWA, PAPER, and HERA aim to detect the signal from these eras but face challenges in calibrating the instruments and subtracting bright foreground sources. Some progress has been made in placing upper limits on the signal and constraining the heating of the intergalactic medium by X-rays, but a clear detection of the signal is still needed
Using an ideal Lagrangian relaxation scheme for magnetic fields we investigate the formation of current concentrations for various magnetic field configurations. For sufficiently braided fields Parker (1972) hypothesizes the formation of singular current structures and subsequent reconnection. Here we find that even for highly braided fields current concentrations are well resolved and of finite magnitude. In presence of magnetic nulls, however, we confirm previous results of singular current structures at the nulls.
This document summarizes a presentation about exploring the early universe using the neutral hydrogen 21cm line. It discusses:
1. The history of the universe from the dark ages to the epoch of reionization, when the first stars and galaxies formed.
2. Current observations of the epoch of reionization provide constraints on the global neutral hydrogen fraction over time but do not reveal detailed spatial information.
3. Observing the 21cm line from neutral hydrogen in the intergalactic medium could directly probe the epoch of reionization and reveal information about ionized bubble morphology, the first luminous objects, and galaxy formation.
1) The document discusses challenging the assumption of an isotropic cosmos by analyzing patterns in the cosmic microwave background (CMB).
2) It summarizes past CMB space missions from 1991-2010 and upcoming missions from 2020 onward that aim to better measure the CMB anisotropy and polarization.
3) Non-parametric methods are presented to analyze the CMB angular power spectrum without assuming a particular cosmological model, allowing estimation of cosmological parameters in a model-independent way.
The document discusses using artificial neural networks (ANNs) to analyze 21cm cosmology data. Specifically, it discusses using ANNs to:
1) Emulate and speed up computation of 21cm power spectra from EoR parameters by 3 orders of magnitude.
2) Reconstruct EoR parameters like the mean free path and virial temperature from 21cm power spectra.
3) Recover the ionized bubble size distribution from 21cm power spectra to learn about the EoR source properties.
4) Generate 21cm distributions from Lyman-alpha emitter galaxy distributions using generative adversarial networks.
- The document discusses using 21cm forest observations to constrain properties of ultra-light dark matter particles like axions.
- 21cm forest observations can probe particle masses up to 10^-19 eV, 3 orders of magnitude higher than Lyman-alpha forest observations.
- Fisher forecast analysis suggests 21cm forest observations could probe ultra-light particle masses around 10^-20 eV and particle fraction values around 0.3.
- Ongoing work is studying effects of isocurvature fluctuations from breaking the Peccei-Quinn symmetry on 21cm forest observations.
- Ray theory explains many optical phenomena by considering light to travel in narrow paths called rays. Rays obey simple rules like reflection and Snell's laws.
- Optical resonators like Fabry-Perot cavities allow only certain resonant wavelengths/frequencies to propagate through interference of reflected waves. The modes are separated by the free spectral range and have a spectral width that depends on the finesse.
- Diffraction occurs when light passes through an aperture or obstruction, causing the beam to diverge and form an intensity pattern due to interference between wavelets from each point in the aperture. This pattern is explained by Huygens' principle and diffraction theory.
This document discusses using 21cm forest probes to study axion dark matter. It finds that if Peccei-Quinn symmetry breaks after inflation, isocurvature perturbations would enhance matter fluctuations and the number of 21cm absorption lines in the forest. The document models this effect on 21cm forest for different axion oscillation scales corresponding to axion masses. It finds the most enhanced absorption lines would be at oscillation scales around 20,000 Mpc-1. Observing these absorption lines could constrain the axion mass scale. However, this technique requires bright background radio sources exist at high redshifts, which remains uncertain. The intergalactic medium temperature also impacts the number of observable absorption lines.
This document provides an introduction to 21cm cosmology and the study of the epoch of reionization (EoR) using the 21cm hydrogen line signal. It discusses how 21cm observations can map out the distribution of neutral hydrogen during the EoR and help answer questions about early galaxy and structure formation. Current telescopes like MWA and LOFAR are placing upper limits on the 21cm power spectrum but upcoming instruments like SKA aim to directly detect the signal through its high sensitivity and resolution. A key challenge is removing bright foreground signals to isolate the faint cosmological 21cm signal.
The document discusses using 21cm forest probes to explore axion dark matter. It summarizes that if Peccei-Quinn symmetry breaks after inflation, isocurvature perturbations would be generated, enhancing matter fluctuations detectable through the 21cm forest. The analysis suggests 21cm forest could explore axion mass scales between 530-5x10^5 Mpc^-1, complementary to other probes. Key uncertainties are the existence of bright background radio sources at high redshift needed to detect the 21cm forest, and how IGM temperature impacts the number of absorption lines.
Magnetic field line braiding in the solar atmosphereSimon Candelaresi
We study the effect of the magnetic field line braiding in the solar atmosphere using topological methods. By measuring the topological entropy of the magnetic field line mapping we show that footpoint motions are capable of inducing highly non-trivial braided structures, which has a fundamental effect on the formation of current layers. Those braids can reach further up in the solar atmosphere, through which energy is transported.
Depending on the structure of the field close to the photosphere, such energy transport can be very efficient.
Speaker: Michael Hippke
Affiliation: Sonneberg Observatory
Title: ''Interstellar communication: What works (not so) well and why? "
Abstract: Our nearest neighbor star, Alpha Centauri C, has a planet in the habitable zone. The Russian billionaire Yuri Milnor funds research to send an exploration probe there. Obtaining remote observational data from such a probe is not trivial because of minimal instrumentation (gram scale) and large distances (pc). Together, we follow the long journey of a photon from the transmitter beam through the interstellar dust and gas, atmospheric turbulence, and other obstacles, before finally arriving in the receiver on Earth. We discuss wavelength/frequency choices, gravitational lensing, and particles other than photons, such as Neutrinos. We conclude by asking the "big picture" question: Only when we understand how to communicate efficiently over interstellar communications, we can hope to learn how to receive such communications from other civilizations, if they exist. Are radio waves the best choice?
This document discusses the discovery of the accelerating expansion of the universe through observations of distant supernovae, for which the 2011 Nobel Prize in Physics was awarded. It provides background on assumptions in cosmology like the cosmological principle, homogeneous and isotropic universe, and using general relativity and the Friedmann-Robertson-Walker metric to derive equations describing the expansion. The document also summarizes how type Ia supernovae serve as standardizable candles and helped establish the Hubble diagram showing the accelerating expansion.
This document discusses several phenomena that demonstrate the wave-like properties of light, including diffraction, interference, polarization, and the photoelectric effect. It describes key experiments such as Young's double slit experiment and explains concepts such as Huygens' principle, Brewster's angle, and how diffraction patterns are formed. It also defines important terms for waves like wavelength, frequency, and the relationship between them given by the speed of light.
Light has several properties that make it useful for information processing and optical communication systems. It can be transmitted without interference from electrical signals or other light beams crossing its path. Optical signals also allow high parallelism and bandwidth exceeding 1013 bits per second. Radiation sources can be classified by their flux output and spectrum. Light behaves as an electromagnetic wave that propagates through space as oscillating electric and magnetic fields. In a material medium, the light's phase velocity decreases and is characterized by the medium's refractive index. Crystalline materials exhibit anisotropic refractive indices depending on the propagation and polarization directions.
This document summarizes a study on using 21cm forest probes to explore axion dark matter scenarios where Peccei-Quinn symmetry breaks after inflation. The enhanced matter power spectrum from axion-generated isocurvature fluctuations would increase the number of 21cm absorption lines, probing axion masses from 10^-18 eV to 10^-12 eV. The optimal range to see effects is for oscillation scales around 2x10^4 Mpc^-1. However, detecting the 21cm forest requires bright background radio sources at high redshifts, which remain uncertain.
This document provides an overview of laser fundamentals, including:
- The key elements of a laser are an amplifying medium, resonator, and pumping mechanism. Population inversion in the amplifying medium is required.
- Lasers produce light via stimulated emission. Pumping excites the medium, then spontaneous and stimulated emission occur within an optical cavity to produce coherent, directional light.
- Absorption, spontaneous emission, and stimulated emission are governed by Einstein coefficients. Lasing occurs when gain exceeds losses within the optical cavity.
The document discusses exploring the early universe using the neutral hydrogen 21cm line. It provides an overview of Hayato Shimabukuro's background and research interests, which include 21cm cosmology and analyzing 21cm signals with machine learning. The presentation outlines the basics of the 21cm line, the current status of 21cm cosmology experiments, and challenges in the field. It also describes work using artificial neural networks to estimate reionization parameters from 21cm power spectra and recover bubble size distributions from 21cm observations.
Galaxy Cluster Gas Motions with X-ray Surveyor: Probing the Small ScalesJohn ZuHone
This document discusses using X-ray telescopes to study gas motions in galaxy clusters. It argues that while Astro-H will provide some insights into cluster gas kinematics on large scales, an X-ray Surveyor telescope with higher spatial resolution (<1") and effective area would allow researchers to probe gas motions on smaller scales, such as measuring the dissipation scale in the Coma Cluster and precisely characterizing velocity fields in sloshing cores.
The document discusses key concepts related to the speed of light and distances in the universe. It defines important units like the gigameter, nanometer, light-year and explains how they relate to distances at different scales in the observable universe. For example, it notes that the filling of space by matter is incomplete at both small (atom) and large (cosmos) scales, with essentially void spaces around objects. It also discusses how light-years are used to convey the gigantic distances encountered in astronomy and how the finite speed of light means we see astronomical objects as they were in the past, not the present.
Laser trapped mirrors could enable the construction of large, lightweight optical systems in space. A laser traps microscopic particles at the interference fringes created by its reflection between two deflectors, arranging the particles into a reflective mirror surface. Key challenges include maintaining the trap against particle evaporation from infrared background photons and understanding optical binding forces between particles. Further experiments and simulations are needed to evaluate particle design, collective behavior, trap loading and damping mechanisms to develop this technology.
Binary pulsars provide an excellent tool to test theories of gravity. The document describes several binary pulsar systems and how measurements of their orbital parameters over time have allowed for high-precision tests of general relativity in strong gravitational fields. Specifically, the double pulsar system PSR J0737-3039A/B has enabled measurements that agree with general relativity predictions to within 0.05% precision by measuring parameters like periastron advance and gravitational redshift effects.
This document discusses orders of magnitude in size from atoms to the universe. It notes that while matter fills space at small scales like atoms, at both very small and very large cosmic scales, space is essentially empty. It also discusses the speed of light as a physical constant, how light speed depends on the medium, and defines the light-year as the distance light travels in one year which is used to measure vast cosmic distances.
This document discusses concepts for using lightsails propelled by solar radiation or laser beams for interstellar space travel. It proposes that refractory dielectric materials, like sapphire, could allow lightsails to withstand higher temperatures and accelerations compared to metal films. A demonstration experiment is proposed to test a carbon filmsail accelerated by a 1 MW, 95 GHz gyrotron beam over 8 meters, reaching 2 Gs and 3000 K to validate analytical models. Dielectric filmsails could enable faster outer planet and Kuiper Belt missions compared to traditional propulsion.
This document provides an overview of the principles of laser operation. It discusses:
- Laser cavities consisting of an amplifying medium between two mirrors that provide feedback.
- Fabry-Perot resonators and the standing wave patterns that form from interference between waves moving in opposite directions within the cavity.
- Population inversion being necessary for stimulated emission to exceed absorption, allowing amplification of light passing through the active medium.
- Optical pumping being used to invert the population by exciting atoms to a long-lived excited state, building up a population there.
- Stimulated emission causing photons to be emitted in phase with the stimulating photon, allowing amplification through an avalanche effect within the inverted medium.
The document discusses the electromagnetic spectrum, which spans over 140 octaves from low frequencies like microwaves up to a theoretical maximum frequency called the Planck frequency of 2.95 x 1042 Hz. It follows a logarithmic spiral pattern with wavelength inversely proportional to frequency. The visible light spectrum detectable by the human eye ranges from 430-770 THz. The highest measured gamma cosmic ray had a frequency of around 1023 Hz.
Optical antennas are devices designed to efficiently convert between propagating optical radiation and localized energy. Like radio frequency antennas, optical antennas can increase the interaction area of local absorbers or emitters with free radiation. Key aspects of optical antennas include their operation based on plasmonics and impedance matching. They can be fabricated using electron beam lithography or focused ion beam milling at the nanoscale. Applications include imaging, photovoltaics, and coherent control. Optical antennas provide opportunities for new optoelectronic architectures and devices by controlling light-matter interactions at the nanoscale.
p-i-n Solar Cell Modeling with Graphene as ElectrodeWahiduzzaman Khan
Graphene is a 2-D atomic layer of carbon atoms with unique electronic properties like outstanding carrier mobility, high carrier saturation velocity, excellent thermal conductivity, high mechanical strength, transparency, thinness, and flexibility which make graphene an excellent choice of material for advanced applications in future solar cell design. We modeled a solar cell using graphene as the front electrode to study its performance and compare the performance with that of other possible contenders- indium tin oxide (ITO), widely used material at present and carbon nanotube (CNT), another promising material in this regard. Numerical solutions of the electrostatic and transport equations were obtained using the finite-element method. It was found that solar cell with graphene electrode can outperform the others. We also studied its performance as a function of various parameters. The developed model and obtained results are important for the design of solar cell with graphene as electrode.
This document discusses using 21cm forest probes to study axion dark matter. It finds that if Peccei-Quinn symmetry breaks after inflation, isocurvature perturbations would enhance matter fluctuations and the number of 21cm absorption lines in the forest. The document models this effect on 21cm forest for different axion oscillation scales corresponding to axion masses. It finds the most enhanced absorption lines would be at oscillation scales around 20,000 Mpc-1. Observing these absorption lines could constrain the axion mass scale. However, this technique requires bright background radio sources exist at high redshifts, which remains uncertain. The intergalactic medium temperature also impacts the number of observable absorption lines.
This document provides an introduction to 21cm cosmology and the study of the epoch of reionization (EoR) using the 21cm hydrogen line signal. It discusses how 21cm observations can map out the distribution of neutral hydrogen during the EoR and help answer questions about early galaxy and structure formation. Current telescopes like MWA and LOFAR are placing upper limits on the 21cm power spectrum but upcoming instruments like SKA aim to directly detect the signal through its high sensitivity and resolution. A key challenge is removing bright foreground signals to isolate the faint cosmological 21cm signal.
The document discusses using 21cm forest probes to explore axion dark matter. It summarizes that if Peccei-Quinn symmetry breaks after inflation, isocurvature perturbations would be generated, enhancing matter fluctuations detectable through the 21cm forest. The analysis suggests 21cm forest could explore axion mass scales between 530-5x10^5 Mpc^-1, complementary to other probes. Key uncertainties are the existence of bright background radio sources at high redshift needed to detect the 21cm forest, and how IGM temperature impacts the number of absorption lines.
Magnetic field line braiding in the solar atmosphereSimon Candelaresi
We study the effect of the magnetic field line braiding in the solar atmosphere using topological methods. By measuring the topological entropy of the magnetic field line mapping we show that footpoint motions are capable of inducing highly non-trivial braided structures, which has a fundamental effect on the formation of current layers. Those braids can reach further up in the solar atmosphere, through which energy is transported.
Depending on the structure of the field close to the photosphere, such energy transport can be very efficient.
Speaker: Michael Hippke
Affiliation: Sonneberg Observatory
Title: ''Interstellar communication: What works (not so) well and why? "
Abstract: Our nearest neighbor star, Alpha Centauri C, has a planet in the habitable zone. The Russian billionaire Yuri Milnor funds research to send an exploration probe there. Obtaining remote observational data from such a probe is not trivial because of minimal instrumentation (gram scale) and large distances (pc). Together, we follow the long journey of a photon from the transmitter beam through the interstellar dust and gas, atmospheric turbulence, and other obstacles, before finally arriving in the receiver on Earth. We discuss wavelength/frequency choices, gravitational lensing, and particles other than photons, such as Neutrinos. We conclude by asking the "big picture" question: Only when we understand how to communicate efficiently over interstellar communications, we can hope to learn how to receive such communications from other civilizations, if they exist. Are radio waves the best choice?
This document discusses the discovery of the accelerating expansion of the universe through observations of distant supernovae, for which the 2011 Nobel Prize in Physics was awarded. It provides background on assumptions in cosmology like the cosmological principle, homogeneous and isotropic universe, and using general relativity and the Friedmann-Robertson-Walker metric to derive equations describing the expansion. The document also summarizes how type Ia supernovae serve as standardizable candles and helped establish the Hubble diagram showing the accelerating expansion.
This document discusses several phenomena that demonstrate the wave-like properties of light, including diffraction, interference, polarization, and the photoelectric effect. It describes key experiments such as Young's double slit experiment and explains concepts such as Huygens' principle, Brewster's angle, and how diffraction patterns are formed. It also defines important terms for waves like wavelength, frequency, and the relationship between them given by the speed of light.
Light has several properties that make it useful for information processing and optical communication systems. It can be transmitted without interference from electrical signals or other light beams crossing its path. Optical signals also allow high parallelism and bandwidth exceeding 1013 bits per second. Radiation sources can be classified by their flux output and spectrum. Light behaves as an electromagnetic wave that propagates through space as oscillating electric and magnetic fields. In a material medium, the light's phase velocity decreases and is characterized by the medium's refractive index. Crystalline materials exhibit anisotropic refractive indices depending on the propagation and polarization directions.
This document summarizes a study on using 21cm forest probes to explore axion dark matter scenarios where Peccei-Quinn symmetry breaks after inflation. The enhanced matter power spectrum from axion-generated isocurvature fluctuations would increase the number of 21cm absorption lines, probing axion masses from 10^-18 eV to 10^-12 eV. The optimal range to see effects is for oscillation scales around 2x10^4 Mpc^-1. However, detecting the 21cm forest requires bright background radio sources at high redshifts, which remain uncertain.
This document provides an overview of laser fundamentals, including:
- The key elements of a laser are an amplifying medium, resonator, and pumping mechanism. Population inversion in the amplifying medium is required.
- Lasers produce light via stimulated emission. Pumping excites the medium, then spontaneous and stimulated emission occur within an optical cavity to produce coherent, directional light.
- Absorption, spontaneous emission, and stimulated emission are governed by Einstein coefficients. Lasing occurs when gain exceeds losses within the optical cavity.
The document discusses exploring the early universe using the neutral hydrogen 21cm line. It provides an overview of Hayato Shimabukuro's background and research interests, which include 21cm cosmology and analyzing 21cm signals with machine learning. The presentation outlines the basics of the 21cm line, the current status of 21cm cosmology experiments, and challenges in the field. It also describes work using artificial neural networks to estimate reionization parameters from 21cm power spectra and recover bubble size distributions from 21cm observations.
Galaxy Cluster Gas Motions with X-ray Surveyor: Probing the Small ScalesJohn ZuHone
This document discusses using X-ray telescopes to study gas motions in galaxy clusters. It argues that while Astro-H will provide some insights into cluster gas kinematics on large scales, an X-ray Surveyor telescope with higher spatial resolution (<1") and effective area would allow researchers to probe gas motions on smaller scales, such as measuring the dissipation scale in the Coma Cluster and precisely characterizing velocity fields in sloshing cores.
The document discusses key concepts related to the speed of light and distances in the universe. It defines important units like the gigameter, nanometer, light-year and explains how they relate to distances at different scales in the observable universe. For example, it notes that the filling of space by matter is incomplete at both small (atom) and large (cosmos) scales, with essentially void spaces around objects. It also discusses how light-years are used to convey the gigantic distances encountered in astronomy and how the finite speed of light means we see astronomical objects as they were in the past, not the present.
Laser trapped mirrors could enable the construction of large, lightweight optical systems in space. A laser traps microscopic particles at the interference fringes created by its reflection between two deflectors, arranging the particles into a reflective mirror surface. Key challenges include maintaining the trap against particle evaporation from infrared background photons and understanding optical binding forces between particles. Further experiments and simulations are needed to evaluate particle design, collective behavior, trap loading and damping mechanisms to develop this technology.
Binary pulsars provide an excellent tool to test theories of gravity. The document describes several binary pulsar systems and how measurements of their orbital parameters over time have allowed for high-precision tests of general relativity in strong gravitational fields. Specifically, the double pulsar system PSR J0737-3039A/B has enabled measurements that agree with general relativity predictions to within 0.05% precision by measuring parameters like periastron advance and gravitational redshift effects.
This document discusses orders of magnitude in size from atoms to the universe. It notes that while matter fills space at small scales like atoms, at both very small and very large cosmic scales, space is essentially empty. It also discusses the speed of light as a physical constant, how light speed depends on the medium, and defines the light-year as the distance light travels in one year which is used to measure vast cosmic distances.
This document discusses concepts for using lightsails propelled by solar radiation or laser beams for interstellar space travel. It proposes that refractory dielectric materials, like sapphire, could allow lightsails to withstand higher temperatures and accelerations compared to metal films. A demonstration experiment is proposed to test a carbon filmsail accelerated by a 1 MW, 95 GHz gyrotron beam over 8 meters, reaching 2 Gs and 3000 K to validate analytical models. Dielectric filmsails could enable faster outer planet and Kuiper Belt missions compared to traditional propulsion.
This document provides an overview of the principles of laser operation. It discusses:
- Laser cavities consisting of an amplifying medium between two mirrors that provide feedback.
- Fabry-Perot resonators and the standing wave patterns that form from interference between waves moving in opposite directions within the cavity.
- Population inversion being necessary for stimulated emission to exceed absorption, allowing amplification of light passing through the active medium.
- Optical pumping being used to invert the population by exciting atoms to a long-lived excited state, building up a population there.
- Stimulated emission causing photons to be emitted in phase with the stimulating photon, allowing amplification through an avalanche effect within the inverted medium.
The document discusses the electromagnetic spectrum, which spans over 140 octaves from low frequencies like microwaves up to a theoretical maximum frequency called the Planck frequency of 2.95 x 1042 Hz. It follows a logarithmic spiral pattern with wavelength inversely proportional to frequency. The visible light spectrum detectable by the human eye ranges from 430-770 THz. The highest measured gamma cosmic ray had a frequency of around 1023 Hz.
Optical antennas are devices designed to efficiently convert between propagating optical radiation and localized energy. Like radio frequency antennas, optical antennas can increase the interaction area of local absorbers or emitters with free radiation. Key aspects of optical antennas include their operation based on plasmonics and impedance matching. They can be fabricated using electron beam lithography or focused ion beam milling at the nanoscale. Applications include imaging, photovoltaics, and coherent control. Optical antennas provide opportunities for new optoelectronic architectures and devices by controlling light-matter interactions at the nanoscale.
p-i-n Solar Cell Modeling with Graphene as ElectrodeWahiduzzaman Khan
Graphene is a 2-D atomic layer of carbon atoms with unique electronic properties like outstanding carrier mobility, high carrier saturation velocity, excellent thermal conductivity, high mechanical strength, transparency, thinness, and flexibility which make graphene an excellent choice of material for advanced applications in future solar cell design. We modeled a solar cell using graphene as the front electrode to study its performance and compare the performance with that of other possible contenders- indium tin oxide (ITO), widely used material at present and carbon nanotube (CNT), another promising material in this regard. Numerical solutions of the electrostatic and transport equations were obtained using the finite-element method. It was found that solar cell with graphene electrode can outperform the others. We also studied its performance as a function of various parameters. The developed model and obtained results are important for the design of solar cell with graphene as electrode.
This document provides an overview of the Institute of Nanoscience and its research activities related to semiconductor nanostructures and their applications. The institute has over 250 researchers studying the fundamental properties and manipulation of nanoscale systems through synthesis, fabrication, experimental and theoretical studies of nanostructures and devices. Key areas of research include semiconductor nanowires for applications in electronics, optoelectronics and spintronics. Heterostructured nanowires of InAs, InSb and InP are investigated for high mobility transistors and terahertz detectors. Strain-driven self-assembly is used to create 3D nanostructures for applications in sensing, energy harvesting and photonics.
This document discusses using tailored force fields for space-based construction. It proposes using radiation pressure from coherent beams of light or sound to manipulate particles and assemble large structures in space. Near term, acoustic standing waves could position particles to form walls. In the far future, electromagnetic fields may reconstruct asteroids by repositioning pulverized material. A middle term example looked at using magnetic fields to construct a radiation shield for a proposed O'Neill habitat. The document outlines the physics of radiation pressure and relevant parameters. It also discusses prior acoustic applications and simulations of wall formation. Overall the document argues that tailored force fields could enable large scale, automatic construction in space and support a space-based economy.
Angular and position stability of a nanorod trapped in an optical tweezersAmélia Moreira
The document summarizes the analysis of angular and position stability of a nanorod trapped in an optical tweezers. It computes the optical trapping forces and torques on a nano-cylinder using T-matrix and radiation stress integration approaches. The results show that lateral forces are several times stronger than axial forces, and lateral torques are 1-2 orders stronger than end-face torques. Torques due to surface stress are much stronger than spin torques. The analysis explains why low aspect ratio nanorods are stably trapped normal to the beam axis.
The document describes an analysis of using an electrostatic shield concept to protect a lunar base from radiation. It discusses the radiation environment, types of radiation and their energy spectra. It then examines passive and active shielding solutions, focusing on electrostatic shields. The document outlines an electrostatic shield design using charged spheres to generate an electric field, and models this using a Lunar Electrostatic Shield Model (LESM) simulation to analyze particle trajectories with and without an applied field. The simulation results suggest the shield design can effectively deflect energetic particles and protect a region near the lunar surface.
Neutron reflectometry can be used to study oxide interfaces. It provides a non-destructive technique to determine the structure and magnetism of surfaces and buried interfaces with angstrom-level resolution. Examples of systems studied include ferromagnet-superconductor heterostructures where competing interactions at the interface can be observed, and cuprate-manganite interfaces where charge transfer and magnetic reconstruction occur within a few nanometers of the boundary. Neutron reflectometry is a powerful "interface toolbox" for understanding complex oxide materials.
The document reports on an ARPES microscopy study of free-standing bilayer graphene. Key findings include:
1) Bilayer graphene samples were prepared by mechanical exfoliation on 5μm wells and studied using ARPES microscopy between 110-300K.
2) Analysis of ARPES data using a tight-binding model found the Fermi velocity to be 1.003-1.042×106 m/s, interlayer asymmetry Δ/2 = 48-56 meV, and interlayer coupling γ1 = 0.6-0.611 eV.
3) Additional trilayer graphene was studied at room temperature using a 74eV photon energy, showing a doped sample with a 350
This document discusses plasmonic chain waveguides. Plasmonic chain waveguides use linear chains of plasmonic nanoparticles to concentrate optical beams below the diffraction limit and guide electromagnetic energy. Each nanoparticle acts as a dipole that interacts with the nearest neighboring nanoparticles. This coupling supports localized surface plasmons and guided wave propagation along the chain. Both the particle size and distance between particles impact the coupling strength and guided modes. Plasmonic chain waveguides have applications in nanophotonics due to their ability to squeeze optical signals into subwavelength confinement.
1) Ion beam irradiation was used to nanopattern a Co-Si binary mixture, producing nanoripples that transitioned to mounds at higher fluence. Swinging the substrate during irradiation led to the formation of cauliflower-like structures.
2) Current-voltage measurements on the patterns showed diode-like behavior. Resistance increased with pattern ordering and decreased with larger macro roughness at higher fluence.
3) Swinging speed was found to have an optimum value that roughened the surface more than no swinging or very slow/fast swinging, due to anisotropic mass transport induced by the swinging motion.
This document provides an overview of optical nano antennas. It begins by defining nano antennas and their role in transmitting and receiving optical signals at the nanoscale. Next, it discusses the characteristics of metallic and dielectric nano antennas, including their directivity, radiation efficiency, gain, and ability to enhance localized electric fields. Applications mentioned include medicine, photovoltaics, spectroscopy, and near-field microscopy. The document concludes by introducing seebeck nano antennas for solar energy harvesting and discusses limitations of current photovoltaic technology.
Ion implantation allows for precise introduction of dopants into semiconductors. It involves ionizing and accelerating ions before injecting them into the target wafer. This creates a dopant profile under the surface. The profile characteristics like peak concentration and depth depend on implantation energy and dose. Implantation causes lattice damage but annealing restores the crystal structure and activates dopants. Implantation offers advantages over diffusion like independent control of concentration and depth with low temperature processing.
The document discusses nantennas, which are nanoscopic antennas that can efficiently convert solar radiation to electricity. Nantennas can absorb a wide range of wavelengths, unlike traditional solar cells, and provide alternating current without the efficiency limitations of photovoltaics. They work by using the oscillating electric field of light to induce a back-and-forth current in the nantenna, which is then rectified into direct current. While promising for scalable solar energy collection, challenges remain in developing high frequency rectifiers and optimizing mass manufacturing techniques.
- Surface plasmon polaritons are electromagnetic waves that propagate along the interface between a metal and a dielectric material. They arise from the coupling of incident light to oscillations of surface electrons known as surface plasmons.
- Surface plasmon polaritons can be excited through techniques like prism coupling using either the Otto or Kretschmann configurations, which use evanescent waves to overcome the momentum mismatch between incident light and surface plasmons.
- Applications of surface plasmon resonance include ultrasensitive biosensing, fluorescence imaging, catalysis, and phototherapy due to the ability of surface plasmons to concentrate electromagnetic fields at subwavelength scales.
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3. Plasmonic trapping
• Trapping nanoparticles using very strong gradient forces that are produced in the
near-field of plasmonic nanostructures.
b) Focused by a strong lens c) Far-field d) Near-field
Raziman TV et al. , Faraday Discuss., 2015, 178,
D >> wavelength D << wavelength and
strong gradient field
a) Homogenous
field
D < wavelength and
limited focused field
D > wavelength and
focused field
• The optical force is directly
proportional to the gradient of
intensity of light illuminated.
F = −𝛻 𝐼
4. ?
• Strong coupling between the LSPs of the nanostructures.
• Hence, a stronger field enhancement.
Raziman TV et. al , Faraday Discuss., 2015, 178,
5. Shell structure
• Initially , a golden shell of inner radius 25nm and outer 35nm was created and x-
plane polarized light was illuminated in the z-direction.
Top View3D View
25nm
35nm
Px
ǩ
Gold
Water
6. Resonance in the shell with an opening
[1] In work Plane : Cross section of the shell was drawn.
[2] It was revolved about z-axis
[3] Edges were made smooth by using fillet.
Work plane Shell obtained after
revolving and applying
fillet
Shift in resonance Peak after
making an opening
7. Full structure
Fig. (a) Fig. (b) Fig. (c)
a) The outermost layer of the structure : PML (Perfectly matched
layer)
b) A cubical block enclosing the shell and particle for a finer mesh.
c) The particle and shell system.
8. Geometry of the structure and parameters
Top View
Parameters
Gold
The wavelength of light was swept from 500 nm to 800
nm and the
• Force
• Charge Distribution (Power outflow)
• Electric field
on the nanoparticle were calculated.
Radius of Core 25 nm
Radius of Shell 35 nm
Initial wavelength 500 nm
Final wavelength 800 nm
Wavelength step size 10 nm
Opening Angle (theta) 45 °
9. Shift in resonance peak on trapping
A change in the resonance position of the reflectivity spectrum was observed due to
introduction of gold nanoparticle.
Legend
with np
without np
Field Gradient
xy plane
yz plane
10. Effect of position on force
Forces which the nanoparticle experiences when it is placed at different positions in the z-
direction:
11. Effect of Position on Force
Forces which the nanoparticle experiences when it is offset in x-direction:
FX FZ
Offset x
x = 14 nm
x = 0 nm
0
4x10-24
0
-10x10-25
12. Effect of Position on Force
Forces which the nanoparticle experiences when it is offset in y-direction:
FY
FZ
Offset y
y = 14 nm
y = 0 nm
6x10-25
0 -2.2x10-25
0
14. Electric Field
The particle is made offset along x-axis by 8nm
XY – Plane (Top View) XZ – Plane
We can observe that the field enhancement is maximum when it is near the
periphery. So, coupling between the nanoparticle and antenna takes place.
10
70
15. Electric Field
The particle is made offset along y-axis by 8nm
XY – Plane (Top View) XZ – Plane (Top View)
50
5
16. Applications & scope in future
• Optical tweezers
• Bio sensors
• Nanofactories
• Color engineering
• Plasmonic solar cells
Alexander S. Urban, Nanoscale, 2014, 6, 4458-447
17. Conclusion
• Shifting of the resonance peak on trapping a NP.
• The optical forces were maximum at the resonance.
• Magnitude of these forces change when the particle in displaced in x, y, z
directions.
• The forces push the NP towards periphery (at fixed height).
18. References
[1] Raziman TV et al. , Faraday Discuss., 2015, 178, 421
[2] Alexander S. Urban, Nanoscale, 2014, 6, 4458-4474
[3] Onofrio M. Maragò1, Nat Nanotechnol. 2013 Nov;8(11):807-19
19. Acknowledgement
I am very much thankful to
Dr. Shourya Dutta Gupta,
Pravallika Bandaru and Lavanya Devi for guidance and support during
the project.
Noble metal nanoparticles support surface plasmons (oscillations of the conduction electrons at the nanoparticle surface) that result in extraordinary optical properties that are not exhibited by any other class of material.
The basis for the effect is the plasmon resonance of the free electrons in the metal nanoparticle, which can be understood by studying the polarizability (the ease with which charges, such as the conduction electrons on the metal nanoparticle surface, undergo charge distribution and form partial dipoles).
--
What is a Surface Plasmon Resonance?
The remarkable optical properties of plasmonic materials occurs because the conduction electrons on the nanoparticle surface undergo a collective oscillation when excited by light at specific wavelengths (shown below). This oscillation, which is known as a surface plasmon resonance (SPR), results in the unusually strong scattering and absorption of light. When these resonances are excited, absorption and scattering intensities can be up to 40x higher than identically sized particles that are not plasmonic.
--
What are surface plasmons:
Surface plasmons (SPs) are coherent electron oscillations that exist at the interface between any two materials where the real part of the dielectric function changes sign across the interface . In our case, gold has negative permittivity. And water has positive value.
.
A localized surface plasmon (LSP) is the result of the confinement of a surface plasmon in a nanoparticle of size comparable to or smaller than the wavelength of light used to excite the plasmon.
The LSP has two important effects:
electric fields near the particle’s surface are greatly enhanced and the particle’s optical absorption is maximum at the plasmon resonant frequency.
Biomedical – Plasmonic nanoparticles are photostable and thus can be used as bio-nanoprobes. Plasmonic nanoparticles scatter light vigorously, and hence can be identified easily under dark-field illumination and other sensing techniques. Thus they can be utilized in various in vitro biological applications.
Color engineering – The unique optical properties of metal nanoparticles are very useful in color engineering. Here customized nanoparticle formulations are created for the purpose of absorbing and scattering specific wavelengths of light to generate a color. Plasmonic nanoparticles can concurrently absorb and scatter light to offer a bichromic color result.
Plasmonic solar cells – Plasmonic nanoparticles possess low absorption property as well as the ability to scatter light back into a photovoltaic structure. Researchers are keen on exploiting these aspects to enhance solar cell efficiency by forcing more light to be absorbed by solar cells