Bosons star at finite temperature

被引：25

作者：

Latifah, S. ^{[1
]}

Sulaksono, A. ^{[1
]}

Mart, T. ^{[1
]}

机构：

[1] Univ Indonesia, FMIPA, Dept Fis, Depok 16424, Indonesia

来源：

PHYSICAL REVIEW D | 2014年 / 90卷 / 12期

关键词：

SELF-GRAVITATING BOSONS; BOSE-GAS;

D O I：

10.1103/PhysRevD.90.127501

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

By using a simple thermodynamical method, we confirm the finding of Chavanis and Harko that stable Bose-Einstein condensate stars can form. However, by using a thermodynamically consistent boson equation of state, we obtain a less massive Bose-Einstein condensate star compared to the one predicted by Chavanis and Harko. We also obtain that the maximum mass of a boson star is insensitive to the change of matter temperature. However, the mass of a boson star with relatively large radius depends significantly on the temperature of the boson matter.

引用

页数：5

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