Search results for "electromagnetic"

showing 10 items of 1595 documents

The emission time of harmonics emitted by a molecule

2003

The behaviour of a one-electron, one-dimensional, asymmetric molecule driven by a laser field of intermediate intensity is studied. At the laser intensity used, the electron bounces back and forth from one atom to another undergoing repeated collisions with the nuclei. The scattered electromagnetic spectrum shows even and odd harmonics of the pump frequency. By means of a wavelet transform it is seen that the harmonics are emitted at different instants of time, corresponding to different locations of the electron. It is suggested that the emission time can be used as a tool to determine the position of the electron.

PhysicsField (physics)Electromagnetic spectrumElectronCondensed Matter PhysicsLaserDiatomic moleculeAtomic and Molecular Physics and OpticsIntensity (physics)law.inventionlawHarmonicsAtomAtomic physicsJournal of Physics B: Atomic, Molecular and Optical Physics
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Space-time localization of the radiation emitted by an electromagnetically driven charge and the question of the position of an electron

2003

Abstract We study the electromagnetic spectrum emitted by a free charge driven by a strong laser field in the proximity of a stationary scattering centre that acts as an accelerating third body. We show that under the most general conditions the radiation is emitted close to the scatterer and during a welldefined time interval. Thus it should be possible, at least in principle, to determine the position of the electron by observing the radiation that it is emitting.

PhysicsField (physics)Electromagnetic spectrumScatteringbusiness.industrySpace timeCharge (physics)ElectronRadiationLaserAtomic and Molecular Physics and Opticslaw.inventionOpticslawAtomic physicsbusiness
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Magnetic shielding of soft protons in future X-ray telescopes: the case of the ATHENA Wide Field Imager

2018

Both the interplanetary space and the Earth magnetosphere are populated by low energy ($\leq300$ keV) protons that are potentially able to scatter on the reflecting surface of Wolter-I optics of X-ray focusing telescopes and reach the focal plane. This phenomenon, depending on the X-ray instrumentation, can dramatically increase the background level, reducing the sensitivity or, in the most extreme cases, compromising the observation itself. The use of a magnetic diverter, deflecting protons away from the field of view, requires a detailed characterization of their angular and energy distribution when exiting the mirror. We present the first end-to-end Geant4 simulation of proton scattering…

PhysicsField (physics)ProtonAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsMagnetosphereFOS: Physical sciencesAstronomy and AstrophysicsX-ray telescopeField of view01 natural sciencesComputational physicsMagnetic field010309 opticsCardinal pointSpace and Planetary Science0103 physical sciencesElectromagnetic shieldinginstrumentation: miscellaneous – telescopesAstrophysics - Instrumentation and Methods for Astrophysics010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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Finite difference time domain simulation of soil ionization in grounding systems under lightning surge conditions

2004

This paper proposes a Maxwell’s equations finite difference time domain (FDTD) approach for electromagnetic transients in ground electrodes in order to take into account the non linear effects due to soil ionization. A time variable soil resistivity method is used in order to simulate the soil breakdown, without the formulation of an initial hypothesis about the geometrical shape of the ionized zone around the electrodes. The model has been validated by comparing the computed results with available data found in technical literature referred to concentrated earths. Some application examples referred to complex grounding systems are reported to show the computational capability of the propos…

PhysicsFinite difference electromagnetic transient grounding systemsGroundSoil resistivityFinite differenceFinite-difference time-domain methodSoil ionizationOcean EngineeringMechanicsPhysics::Classical PhysicsNon-linear effectsSettore MAT/08 - Analisi NumericaSettore ING-IND/31 - ElettrotecnicaIonizationLightning surgesSimulation
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TAGS measurements of $^{100}$Nb ground and isomeric states and $^{140}$Cs for neutrino physics with the new DTAS detector

2016

V. Guadilla et al. -- 4 pags., 6 figs. -- Open Access funded by Creative Commons Atribution Licence 4.0

PhysicsFission productsta114Spectrometer010308 nuclear & particles physicsPhysicsQC1-999Detector[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences3. Good healthNuclear physicsnuclear masses0103 physical sciencesstructuredecay data measurementsNeutrino010306 general physicsSpectroscopyAbsorption (electromagnetic radiation)
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Analysis of high-harmonic generation in terms of complex Floquet spectral analysis

2017

Recent developments on intense laser sources is opening a new field of optical sciences. An intense coherent light beam strongly interacting with the matter causes a coherent motion of a particle, forming a strongly dressed excited particle. A photon emission from this dressed excited particle is a strong nonlinear process causing high-harmonic generation (HHG), where the perturbation analysis is broken down. In this work, we study a coherent photon emission from a strongly dressed excited atom in terms of complex spectral analysis in the extended Floquet-Hilbert-space. We have obtained the eigenstates of the total Hamiltonian with use of Feshbach-Brilloiun-Wigner projection method. In this…

PhysicsFloquet theoryQuantum PhysicsPhotonElectromagneticsFloquet spectral analysisTime evolutionFOS: Physical sciencesHigh harmonic generationsymbols.namesakeSingularityExcited statesymbolsHigh harmonic generationPhysics::Atomic PhysicsAtomic physicsHamiltonian (quantum mechanics)Quantum Physics (quant-ph)Physics - OpticsOptics (physics.optics)
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Sudden change in the nuclear charge distribution of very light gold isotopes

1987

4 pages, 3 tables, 2 figures.-- PACS nrs.: 21.10.Ft, 21.10.Ky, 27.70.+q.

PhysicsGeneral Physics and AstronomyCharge densityRadiusPhotoionizationEffective nuclear chargeTime of flight[PACS] Electromagnetic momentsIonization[PACS] Charge distribution150 ≤ A ≤ 189 [[PACS] Properties of specific nuclei listed by mass ranges]Nuclear Physics - ExperimentPhysics::Atomic PhysicsIsotopes of gold[PACS] Properties of specific nuclei listed by mass ranges:150 ≤ A ≤ 189Atomic physicsHyperfine structure
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Thermal density fluctuations in amorphous polymers as revealed by small angle X-ray diffraction

1973

In the case of equilibrium the mean square relative fluctuations of the thermodynamic parameters vanish asymptotically as the number of degrees of freedom approach infinity. There are various observable effects, however, which are related to local fluctuations of the thermodynamic quantities within small parts of the macroscopic system. In particular the scattering of electromagnetic waves by a one-component, one-phase system is due to thermal density fluctuations within small volumes V of the sample. Considering a grand canonical ensemble the phenomenological theory of local fluctuations (1) for a one component system shows that the fluctuation of the number of particles N in the volume V …

PhysicsGrand canonical ensembleCrystallographyNumber densityScatteringX-ray crystallographyDegrees of freedom (physics and chemistry)ObservableAtomic physicsElectromagnetic radiationBar (unit)
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IGR J17451-3022: a dipping and eclipsing low mass X-ray binary

2016

In this paper, we report on the available X-ray data collected by INTEGRAL, Swift, and XMM-Newton during the first outburst of the INTEGRAL transient IGR J17451-3022, discovered in 2014 August. The monitoring observations provided by the JEM-X instruments on-board INTEGRAL and the Swift/XRT showed that the event lasted for about 9 months and that the emission of the source remained soft for the entire period. The source emission is dominated by a thermal component (kT~1.2 keV), most likely produced by an accretion disk. The XMM-Newton observation carried out during the outburst revealed the presence of multiple absorption features in the soft X-ray emission that could be associated to the p…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesX-rays: individuals: IGR J17451-3022Astronomy and AstrophysicsAbsorption columnAstrophysicsAstronomy and AstrophysicOrbital periodX-rays: binarie01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaAccretion discSpace and Planetary ScienceIonization0103 physical sciencesThermalbinaries; X-rays: individuals: IGR J17451-3022; Astronomy and Astrophysics; Space and Planetary Science [X-rays]Astrophysics - High Energy Astrophysical PhenomenaLow MassAbsorption (electromagnetic radiation)010303 astronomy & astrophysics
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The nature of the extreme X-ray variability in the NLS1 1H 0707-495

2021

We examine archival XMM-Newton data on the extremely variable narrow-line Seyfert 1 (NLS1) active galactic nucleus (AGN) 1H 0707-495. We construct fractional excess variance (Fvar) spectra for each epoch, including the recent 2019 observation taken simultaneously with eROSITA. We explore both intrinsic and environmental absorption origins for the variability in different epochs, and examine the effect of the photoionised emission lines from outflowing gas. In particular, we show that the unusual soft variability first detected by eROSITA in 2019 is due to a combination of an obscuration event and strong suppression of the variance at 1 keV by photoionised emission, which makes the variance …

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Active galactic nucleusAccretion (meteorology)Astrophysics::High Energy Astrophysical PhenomenaX-rayFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLow frequencySpectral lineAmplitudeSpace and Planetary ScienceEmission spectrumAbsorption (electromagnetic radiation)Astrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
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