Generalized statistics and solar neutrinos

被引：251

作者：

Kaniadakis, G

Lavagno, A

Quarati, P

机构：

[1] POLITECN TORINO, INFM, I-10129 TURIN, ITALY

[2] IST NAZL FIS NUCL, CAGLIARI, ITALY

[3] IST NAZL FIS NUCL, I-10125 TURIN, ITALY

来源：

PHYSICS LETTERS B | 1996年 / 369卷 / 3-4期

关键词：

solar neutrinos; stellar polytropes; generalized statistics;

D O I：

10.1016/0370-2693(95)01535-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The generalized Tsallis statistics produces a distribution function appropriate to describe the interior solar plasma, thought as a stellar polytrope, showing a tail depleted with respect to the Maxwell-Boltzmann distribution and reduces to zero at energies greater than about 20k(B)T. The Tsallis statistics can theoretically support the distribution suggested in the past by Clayton and collaborators, which shows also a depleted tail, to explain the solar neutrino counting rate.

引用

页码：308 / 312

页数：5

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