Dielectronic Recombination Rates In Astrophysical Plasmas

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dc.creatorBachari, Fatima
dc.creatorFerro, Fabrizio
dc.creatorMaero, Giancarlo
dc.creatorQuarati, Piero
dc.date2006-07-19
dc.date.accessioned2026-07-07T07:22:42Z
dc.date.available2026-07-07T07:22:42Z
dc.descriptionIn this work we introduce a new expression of the plasma Dielecronic Recombination (DR) rate as a function of the temperature, derived assuming a small deformation of the Maxwell-Boltzmann distribution and containing corrective factors, in addition to the usual exponential behaviour, caused by non-linear effects in slightly non ideal plasmas. We then compare the calculated DR rates with the experimental DR fits in the low temperature region.
dc.description6 pages, 1 figure, proceedings to the "International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX", 25-30 June 2006, CERN - Geneve
dc.identifierhttps://arxiv.org/abs/physics/0607172
dc.identifierhttp://arxiv.org/abs/physics/0607172
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/115756
dc.subjectAtomic Physics
dc.titleDielectronic Recombination Rates In Astrophysical Plasmas
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