On the use of a non-extensive distribution in the solar plasma

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dc.creatorLavagno, A.
dc.creatorQuarati, P.
dc.date2000-10-23
dc.date.accessioned2026-07-25T11:25:10Z
dc.descriptionWe describe the physical motivations why we are urged to look for an ionic equilibrium distribution function slightly different from the Maxwellian to calculate nuclear reaction rates in the solar core plasma answering, at the same time, to a recent paper by Bahcall et al. (astro-ph/0010055).
dc.description4 pages, reply to Bahcall et al. astro-ph/0010055
dc.identifierhttps://arxiv.org/abs/astro-ph/0010452
dc.identifierhttp://arxiv.org/abs/astro-ph/0010452
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/2541
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleOn the use of a non-extensive distribution in the solar plasma
dc.typetext

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