Relativistic equilibrium velocity distribution to improve standard solar models

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dc.creatorLiu, Jian-Miin
dc.date2001-12-09
dc.date.accessioned2026-07-07T02:43:46Z
dc.date.available2026-07-07T02:43:46Z
dc.descriptionThe current standard solar models can be improved by substituting the relativistic equilibrium velocity distribution for the Maxwellian velocity distribution. The relativistic equilibrium velocity distribution is close- fitting to the Maxwellian velocity distribution in the low-velocity part and substantially different from the Maxwellian velocity distribution in the high-velocity part, and vanishes at the velocity of light. If adopted in standard solar models, it will lower solar neutrino fluxes, change solar neutrino energy spectra but maintain solar sound speeds.
dc.description5 pages with no figure
dc.identifierhttps://arxiv.org/abs/cond-mat/0112146
dc.identifierhttp://arxiv.org/abs/cond-mat/0112146
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/18634
dc.subjectStatistical Mechanics
dc.subjectAstrophysics
dc.titleRelativistic equilibrium velocity distribution to improve standard solar models
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