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

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

2000-10-23

arxiv.org/abs/astro-ph/0010452v1

Astronomy and Astrophysics

Astrophysics

4 pages, reply to Bahcall et al. astro-ph/0010055

Scientific paper

We 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).

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