Search results for "Electromagnetic radiation"

showing 10 items of 755 documents

Baryon transition form factors at the pole

2016

Electromagnetic resonance properties are uniquely defined at the pole and do not depend on the separation of the resonance from background or the decay channel. Photon-nucleon branching ratios are nowadays often quoted at the pole, and we generalize the considerations to the case of virtual photons. We derive and compare relations for nucleon to baryon transition form factors both for the Breit-Wigner and the pole positions. Using the MAID2007 and SAID SM08 partial wave analyses of pion electroproduction data, we compare the $G_M$, $G_E$, and $G_C$ form factors for the $\Delta(1232)$ resonance excitation at the Breit-Wigner resonance and pole positions up to $Q^2=5$ GeV$^2$. We also explore…

PhysicsNuclear reactionParticle physicsNuclear Theory010308 nuclear & particles physicsBranching fractionNuclear TheoryVirtual particleFOS: Physical sciences01 natural sciencesElectromagnetic radiationtransition form factors Delta resonance L+P expansionBaryonNuclear Theory (nucl-th)PionExcited state0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment (nucl-ex)010306 general physicsNucleonNuclear ExperimentNuclear Experiment
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Test of the generation of High-Frequency Gravitational Waves by irradiating a dielectric film in a resonant cavity

2004

A recent proposal for generating High Frequency Gravitational Waves (HFGW) is based on the conversion of electromagnetic waves into gravitational waves by irradiating a dielectric film in the extreme conditions of a high vacuum and a strong magnetic field. These HFGWs can be tested using an electron paramagnetic resonant spectrometer (EPRS). This device contains all the necessary ingredients: a vacuum chamber, microwave generator, a strong magnetic field, and a resonant cavity where the substance to be analysed is introduced. The EPR spectrum of a very small paramagnetic core in a substance is the graph of the absorption of the paramagnetic core as a function of the strong magnetic field B.…

PhysicsOpticsSpectrometerGravitational wavebusiness.industryVacuum chamberElectronbusinessElectromagnetic radiationMicrowaveMagnetic fieldElectromagnetic induction
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From Measurement to Control of Electromagnetic Waves using a Near‐field Scanning Optical Microscope

2013

PhysicsOpticsbusiness.industryOptoelectronicsNear-field scanning optical microscopeNear and far fieldbusinessElectromagnetic radiationMeasurements using Optic and RF Waves
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Periodic Motion for an Imperfect Solar Sail Near an Asteroid

2014

In this paper we consider the Hill 3-body problem with the extra effect of the solar radiation pressure as a model for the motion of a solar sail close to an asteroid. To model the sail’s acceleration, we include both reflectivity and absorption of the sail’s material. We describe the most relevant dynamical properties of the system for different reflectivity and absorption coefficients as well as different fixed sail orientations. We show families of periodic orbits, describe how they relate to the parameters of the sail and discuss their stability.

PhysicsOrbital planeAstronomySolar sailMechanicsQuantitative Biology::OtherStability (probability)Periodic functionPhysics::Popular PhysicsAccelerationRadiation pressureAsteroidPhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsAbsorption (electromagnetic radiation)
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Diffusion of neutrons by a slab of moderating material: an application of the Monte Carlo Method

2004

An application of the Monte Carlo method to the diffusion of neutrons passing through a slab of a moderating material is presented. This method can be used as a tool to improve the student's comprehension of the statistical properties of many particle systems, showing the necessity of simulation procedures to obtain information on the expected results of real experiments. We have chosen a very simple example to illustrate it: the evaluation of the transmission, reflection and absorption probabilities of a monochromatic beam of neutrons diffusing through a slab of a moderator material. After a collision with a nucleus of the moderator the neutron may be either elastically scattered or captur…

PhysicsParticle systembusiness.industryMonte Carlo methodGeneral Physics and AstronomyComputational physicsOpticsTransmission (telecommunications)SIMULATIONReflection (physics)SlabNeutronDiffusion (business)Nuclear ExperimentAbsorption (electromagnetic radiation)business
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Quantum chemical study of electron‐phonon interaction in crystals

2013

Study of the interaction of the electromagnetic radiation with nonlocal potentials and the electron-phonon interaction is motivated by its key role in non-classical phenomena in dielectrics and semiconductors. Actual in second quantization is decoupling of the undesirable mixture of electronic and phonon birth/annihilation operators and obtaining the effect of radiation in presence of the nonlocal potentials. Here we transform an arbitrary effective electron- phonon Hamiltonian in two matrices – the matrix of a new interaction Hamiltonian and the matrix of the transformation. For a particular effective Hamiltonian formulated in second quantization these two matrices outline a starting point…

PhysicsPhononElectronCondensed Matter PhysicsElectromagnetic radiationSecond quantizationMatrix (mathematics)symbols.namesakeAtomic orbitalQuantum electrodynamicsQuantum mechanicssymbolsHamiltonian (quantum mechanics)Wave functionphysica status solidi c
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Gravity and handedness of photons

2017

Vacuum fluctuations of quantum fields are altered in presence of a strong gravitational background, with important physical consequences. We argue that a non-trivial spacetime geometry can act as an optically active medium for quantum electromagnetic radiation, in such a way that the state of polarization of radiation changes in time, even in the absence of electromagnetic sources. This is a quantum effect, and is a consequence of an anomaly related to the classical invariance under electric-magnetic duality rotations in Maxwell theory.

PhysicsPhoton010308 nuclear & particles physicsFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)RadiationQuantum Hall effectPolarization (waves)01 natural sciencesElectromagnetic radiationGeneral Relativity and Quantum CosmologyGravitationSpace and Planetary ScienceQuantum electrodynamics0103 physical sciences010306 general physicsQuantumMathematical PhysicsQuantum fluctuation
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Strong-field high-frequency approximation to the multiphoton ionization of hydrogen

1990

The strong-field multiphoton ionization of atoms is considered and a theoretical approach dealing nonperturbatively with the radiation field formulated. The general computational scheme is the conventional perturbation theory, but the intermediate states are dressed by the field. We present in detail a method to dress the continuum states and to study the dipole transitions within the continuum. In the high-frequency domain, the proposed procedure rapidly converges over a wide range of field intensity and offers an interesting framework for calculating ionization rates for arbitrary numbers of absorbed (above-threshold) photons and field polarization.

PhysicsPhotonAbove threshold ionizationStatistical and Nonlinear PhysicsPhotoionizationElectromagnetic radiationAtomic and Molecular Physics and OpticsDipoleElectric fieldQuantum electrodynamicsIonizationPhysics::Atomic PhysicsAtomic physicsCircular polarizationJournal of the Optical Society of America B
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Discovery of a Hard X‐Ray Source, SAX J0635+0533, in the Error Box of the Gamma‐Ray Source 2EG 0635+0521

1999

We have discovered an x-ray source, SAX J0635+0533, with a hard spectrum within the error box of the GeV gamma-ray source in Monoceros, 2EG J0635+0521. The unabsorbed x-ray flux is 1.2*10^-11 erg cm^-2 s^-1 in the 2-10 keV band. The x-ray spectrum is consistent with a simple powerlaw model with absorption. The photon index is 1.50 +/- 0.08 and we detect emission out to 40 keV. Optical observations identify a counterpart with a V-magnitude of 12.8. The counterpart has broad emission lines and the colors of an early B type star. If the identification of the x-ray/optical source with the gamma-ray source is correct, then the source would be a gamma-ray emitting x-ray binary.

PhysicsPhotonAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)X-rayGamma rayFOS: Physical sciencesFluxBinary numberAstronomy and AstrophysicsAstrophysicsAstrophysicsSpace and Planetary ScienceEmission spectrumAbsorption (electromagnetic radiation)Astrophysics::Galaxy AstrophysicsThe Astrophysical Journal
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Photoelectric effect from a metal surface: a revisited theoretical model

1992

The Sommerfeld model extended to include radiation–electron interaction in the regime of highly intense fields is taken as the basis for studying theoretically the laser multiphoton photoelectric effect from a metal surface. Numerical analysis is carried out without approximations other than those inherent in the model itself; the study of the multiphoton aspect of the problem is based on a scheme that is nonperturbative in an essential way. The numerical analysis facilitates insight into the potential and the limits of the model in the interpretation of recent experiments and into the similarities and differences between the metal multiphoton effect and atomic multiphoton ionization. The r…

PhysicsPhotonBasis (linear algebra)Numerical analysisStatistical and Nonlinear PhysicsElectronPhotoelectric effectElectromagnetic radiationAtomic and Molecular Physics and OpticsComputational physicsIonizationQuantum mechanicsPhysics::Atomic and Molecular ClustersPhysics::Atomic PhysicsTransmission coefficientJournal of the Optical Society of America B
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