Search results for "Atomic and Molecular Collisions"

showing 2 items of 2 documents

Temperature dependence of sodium and ionized calcium resonance lines perturbed by helium

2014

International audience; Traces of heavy metals in cool DZ white dwarf stars may be attributed to the accretion of circumstellar dust thought to originate from tidal disruption of rocky parent bodies. Spectra of such stars therefore provide a unique opportunity to study the composition of extrasolar planetary systems. The determination of metal abundances from stellar spectra depends on stellar atmospheric parameters and an accurate prior knowledge of the collision broadening of the line profiles by the most common constituents of the stellar atmosphere. For this purpose, we present theoretical absorption spectra of Na and Ca+ broadened by He for the conditions prevailing in cool white dwarf…

HistoryAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsHelium01 natural sciencesAstronomical spectroscopySpectral lineEducation0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics[PHYS]Physics [physics][PHYS.PHYS.PHYS-ATOM-PH]Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]ChemistryStellar atmosphereWhite dwarfAstronomyPlanetary system[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Accretion (astrophysics)Computer Science ApplicationsStars13. Climate actionCircumstellar dustAtomic and molecular collisions[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Astrophysics::Earth and Planetary AstrophysicsMolecular physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Journal of Physics: Conference Series
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Energy-loss straggling of 2-10 MeV/u Kr ions in gases

2013

Measurements have been performed on a time-of-flight setup at the Jyväskylä K130 cyclotron, aiming at energy-loss straggling of heavy ions in gases. Theoretical predictions based on recently developed theory as well as an empirical interpolation formula predict that straggling can be more than ten times higher than Bohr straggling in the MeV/u regime. Our measurements with up to 9.3 MeV/u Kr ions on He, N2, Ne and Kr targets confirm this feature. Our calculations show the relative contributions of linear straggling, bunching including packing, and charge exchange. Our results for stopping cross sections are compatible with values from the literature. Funding Agencies|EU||Academy of Finland …

PhysicsEnergy lossCyclotronPhysics::Medical Physics7. Clean energy01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmaslaw.inventionIonBohr modelNuclear physicssymbols.namesakelawAtomic and Molecular CollisionsTeknik och teknologier0103 physical sciencessymbolsEngineering and TechnologyAtomic physics010306 general physicsAtomien ja molekyylien törmäyksetCharge exchange
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