Search results for "absorption."

showing 10 items of 2682 documents

The Computer Code for Calculations of the Positron Distribution in a Layered Stack Systems

2014

In this paper we present experimental and theoretical studies of the implantation pro le of positrons emitted fromNa radionuclide into layered sample. The measured pro le for the nonsymmetrical, around the positron emitter, stack of aluminium and silver foils was measured using the depth scanning of implantation pro le technique. For the description of the obtained results two theoretical approaches were applied. The rst one was the Monte Carlo simulation using the GEANT4 tool kit. The generated pro le does not reproduce accurately the experimental pro le. We proposed the multiple scattering model based on the fact that a positron due to backscattering can travel as an energetic particle se…

PhysicsSource codeScatteringmedia_common.quotation_subjectMonte Carlo methodGeneral Physics and AstronomySample (graphics)Computational physicsPositronStack (abstract data type)Physics::Accelerator PhysicsParticleAbsorption (electromagnetic radiation)media_commonActa Physica Polonica A
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GRB 050410 and GRB 050412: are they really dark gamma-ray bursts?

2007

We present a detailed analysis of the prompt and afterglow emission of GRB 050410 and GRB 050412 detected by Swift for which no optical counterpart was observed. The 15-150 keV energy distribution of the GRB 050410 prompt emission shows a peak energy at 53 keV. The XRT light curve of this GRB decays as a power law with a slope of alpha=1.06+/-0.04. The spectrum is well reproduced by an absorbed power law with a spectral index Gamma_x=2.4+/-0.4 and a low energy absorption N_H=4(+3;-2)x10^21 cm^(-2) which is higher than the Galactic value. The 15-150 keV prompt emission in GRB 050412 is modelled with a hard (Gamma=0.7+/-0.2) power law. The XRT light curve follows a broken power law with the f…

PhysicsSpectral indexAstrophysics::High Energy Astrophysical PhenomenaExtrapolationAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curvePower lawAfterglowInterstellar mediumSpace and Planetary ScienceGamma-ray burstAbsorption (electromagnetic radiation)Astrophysics::Galaxy Astrophysics
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Total absorption γ -ray spectroscopy of the β -delayed neutron emitters I137 and Rb95

2019

The decays of the β-delayed neutron emitters I137 and Rb95 have been studied with the total absorption γ-ray spectroscopy technique. The purity of the beams provided by the JYFLTRAP Penning trap at the ion guide isotope separator on-line facility in Jyvaskyla allowed us to carry out a campaign of isotopically pure measurements with the decay total absorption γ-ray spectrometer, a segmented detector composed of 18 NaI(Tl) modules. The contamination coming from the interaction of neutrons with the spectrometer has been carefully studied, and we have tested the use of time differences between prompt γ rays and delayed neutron interactions to eliminate this source of contamination. Due to the s…

PhysicsSpectrometer010308 nuclear & particles physicsNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaPenning trap01 natural sciencesNuclear physics13. Climate action0103 physical sciencesNeutronGamma spectroscopyNuclear Experiment010306 general physicsSpectroscopyAbsorption (electromagnetic radiation)Delayed neutronPhysical Review C
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Combination of 3 Different Measurements: Branching Fractions, Radiative Lifetimes, and Absorption Oscillator Strengths- a Good Opportunity for the An…

2021

We present the method and setup for determination and self-testing of atomic radiative constants: transition probabilities, oscillator strengths and natural lifetimes. We describe how it works in simple 4 level scheme, present our experimental setup, and preliminary results for As I branching fractions, and discuss some aspects of future development. This method can be valuable for analyzing the results from different experiments performed by various authors and methods without directly re-measuring them. For example, in astrophysics is very important to select correct oscillator strengths for evaluation element abundances in stars and interstellar media since inaccurate data lead to uncert…

PhysicsStarsRadiative transferBranching (polymer chemistry)Absorption (electromagnetic radiation)Computational physics2021 13th International Conference on Measurement
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Spectral broadening by incomplete thermalization of the energy in X-ray microcalorimeters with superconducting absorber and NTD-Ge thermal sensor

2004

Abstract We present a model of the response of a cryogenic microcalorimeter with superconducting absorber and phonon sensitive thermal sensor to the absorption of X-ray photons. The model is based on the main microscopic processes responsible for the thermalization of the deposited energy. We use a system of rate equations to describe the energy downconversion in the superconductor and transport to the thermal sensor. The model is a tool to investigate the thermalization efficiency with respect to the device characteristics (i.e. absorber material, geometry), in order to optimize the performances of these detectors. As a first case study, we report results of simulations for a microcalorime…

PhysicsSuperconductivityquasi-particleNuclear and High Energy PhysicsPhotonbusiness.industryPhononx-ray spectroscopymicrocalorimeterParticle detectorgermaniumThermalisationOpticsCondensed Matter::Superconductivitynumerical simulationNeutronAtomic physicsAbsorption (electromagnetic radiation)businessInstrumentationDoppler broadening
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Determination of the high-pressure crystal structure ofBaWO4andPbWO4

2006

We report the results of both angle-dispersive x-ray diffraction and x-ray absorption near-edge structure studies in $\mathrm{Ba}\mathrm{W}{\mathrm{O}}_{4}$ and $\mathrm{Pb}\mathrm{W}{\mathrm{O}}_{4}$ at pressures of up to $56\phantom{\rule{0.3em}{0ex}}\mathrm{GPa}$ and $24\phantom{\rule{0.3em}{0ex}}\mathrm{GPa}$, respectively. $\mathrm{Ba}\mathrm{W}{\mathrm{O}}_{4}$ is found to undergo a pressure-driven phase transition at $7.1\phantom{\rule{0.3em}{0ex}}\mathrm{GPa}$ from the tetragonal scheelite structure (which is stable under normal conditions) to the monoclinic fergusonite structure whereas the same transition takes place in $\mathrm{Pb}\mathrm{W}{\mathrm{O}}_{4}$ at $9\phantom{\rule{0…

PhysicsTetragonal crystal systemX-ray spectroscopyCrystallographyCondensed matter physicsX-ray crystallographyAbsorption (logic)Crystal structureIsostructuralCondensed Matter PhysicsFergusoniteElectronic Optical and Magnetic MaterialsMonoclinic crystal systemPhysical Review B
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Basic Physical Concepts

2010

Mossbauer spectroscopy is based on recoilless emission and resonant absorption of γ-radiation by atomic nuclei. The aim of this chapter is to familiarize the reader with the concepts of nuclear γ-resonance and the Mossbauer effect, before we describe the experiments and relevant electric and magnetic hyperfine interactions in Chaps. 3 and 4. We prefer doing this by collecting formulae without deriving them; comprehensive and instructive descriptions have already been given at length in a number of introductory books ([7–39] in Chap. 1). Readers who are primarily interested in understanding their Mossbauer spectra without too much physical ballast may skip this chapter at first reading and p…

PhysicsTheoretical physicsPhysical ConceptsReading (process)media_common.quotation_subjectMossbauer spectraResonant absorptionRecoil energymedia_common
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Enhancedγ-Ray Emission from Neutron Unbound States Populated inβDecay

2015

Total absorption spectroscopy is used to investigate the β-decay intensity to states above the neutron separation energy followed by γ-ray emission in (87,88)Br and (94)Rb. Accurate results are obtained thanks to a careful control of systematic errors. An unexpectedly large γ intensity is observed in all three cases extending well beyond the excitation energy region where neutron penetration is hindered by low neutron energy. The γ branching as a function of excitation energy is compared to Hauser-Feshbach model calculations. For (87)Br and (88)Br the γ branching reaches 57% and 20%, respectively, and could be explained as a nuclear structure effect. Some of the states populated in the daug…

PhysicsTotal absorption spectroscopy010308 nuclear & particles physicsNeutron stimulated emission computed tomographyGeneral Physics and Astronomy01 natural sciencesNeutron temperature0103 physical sciencesr-processNeutronAtomic physicsNuclear Experiment010306 general physicsSpectroscopys-processExcitationPhysical Review Letters
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Carbon coatings for soft-x-ray reflectivity enhancement

2007

In X-ray astronomical telescopes, the focalization of the radiation is achieved by means of grazing incidence Wolter I (parabola + hyperbola) optics in total reflection regime. In general, high density materials (e.g. Au, Pt, Ir, W) are used as reflecting coatings, in order to increase as much as possible the cut-off angles and energies for total reflection. However these materials present an important reduction of the reflectivity between 0.2 and 5 keV, due to the photoabsorption, and this phenomenon is particularly enhanced in correspondence of the M absorption edges (between 2 and 3.5 keV). In general, this determines a strong decrease of the telescope effective area. To overcome the pro…

PhysicsTotal internal reflectionbusiness.industrychemistry.chemical_elementSynchrotronlaw.inventionTelescopeOptical coatingReflection (mathematics)OpticschemistryAbsorption edgelawX-ray astronomical mirrors carbon overcoatings enhancement of the X-ray reflectivityAbsorption (electromagnetic radiation)businessCarbon
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X-ray absorption spectra at the CaL2,3edge calculated within multichannel multiple scattering theory

2004

We report a theoretical method for x-ray absorption spectroscopy (XAS) in condensed matter which is based on the multichannel multiple scattering theory of Natoli et al. and the eigen-channel $R$-matrix method. While the highly flexible real-space multiple scattering (RSMS) method guarantees a precise description of the single-electron part of the problem, multiplet-like electron correlation effects between the photoelectron and localized electrons can be taken account for in a configuration interaction scheme. For the case where correlation effects are limited to the absorber atom, a technique for the solution of the equations is devised, which requires only little more computation time th…

PhysicsX-ray absorption spectroscopyAbsorption spectroscopyElectronic correlationScatteringAtomElectronScattering theoryConfiguration interactionAtomic physicsCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsPhysical Review B
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