Entropy Production of Main-Sequence Stars

被引：6

作者：

Martyushev, Leonid M. ^{[1
,2
]}

Zubarev, Sergey N. ^{[1
]}

机构：

[1] Ural Fed Univ, Ekaterinburg 620002, Russia

[2] Inst Ind Ecol, Ekaterinburg 620219, Russia

来源：

ENTROPY | 2015年 / 17卷 / 02期

关键词：

BOLOMETRIC CORRECTIONS; PRINCIPLE; COLOR;

D O I：

10.3390/e17020658

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The entropy production (inside the volume bounded by a photosphere) of main-sequence stars is calculated based on B-V photometry data. The entropy-production distribution function and the dependences of entropy production on temperature and luminosity are obtained for these stars for the first time. A very small range of variation of specific (per volume) entropy production discovered for main-sequence stars (only 0.5 to 1.8 solar magnitudes) is an interesting result that can be crucial for understanding thermodynamic processes of stars.

引用

页码：658 / 668

页数：11

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