Nuclear reaction rates and energy in stellar plasmas : The effect of highly damped modes

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dc.creatorOpher, Merav
dc.creatorSilva, Luis O.
dc.creatorDauger, Dean E.
dc.creatorDecyk, Viktor K.
dc.creatorDawson, John M.
dc.date2001-05-09
dc.date.accessioned2026-07-07T11:45:58Z
dc.date.available2026-07-07T11:45:58Z
dc.descriptionThe effects of the highly damped modes in the energy and reaction rates in a plasma are discussed. These modes, with wavenumbers $k \gg k_{D}$, even being only weakly excited, with less than $k_{B}T$ per mode, make a significant contribution to the energy and screening in a plasma. When the de Broglie wavelength is much less than the distance of closest approach of thermal electrons, a classical analysis of the plasma can
dc.description42nd Annual Meeting of the APS Division of Plasma Physics, invited talk
dc.identifierhttps://arxiv.org/abs/astro-ph/0105153
dc.identifierhttp://arxiv.org/abs/astro-ph/0105153
dc.identifierPhys.Plasmas8:2454-2460,2001
dc.identifierdoi:10.1063/1.1362533
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202061
dc.subjectAstrophysics
dc.titleNuclear reaction rates and energy in stellar plasmas : The effect of highly damped modes
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