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arXiv 0910.1972hep-phastro-ph.HEastro-ph.SRgr-qcnucl-th
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玻色子星:化学势和夸克凝聚

Boson stars: Chemical potential and quark condensates

Jitesh R. Bhatt, V. Sreekanth

摘要:

我们在平均场近似下研究了由自引力玻色子气体构成的恒星的性质。在广义相对论框架下,考虑化学势的影响,导出了一组广义的TOV方程。化学势的度规依赖性给出了玻色子星的一类新的解。结果表明,当考虑有限化学势的影响时,恒星的最大质量和最大半径发生了显著的变化。我们还讨论了由夸克凝聚体构成的玻色子星的情况。研究发现,当凝聚体之间的自相互作用相对于它们的质量来说很小时,典型的密度太高而不能形成双夸克玻色子星。我们的结果表明,夸克凝聚星可能形成于低密度和高压区。

英文摘要:

We study the properties of a star made of self-gravitating bosons gas in a mean-field approximation. A generalized set of Tolman-Oppenheimer-Volkov(TOV) equations is derived to incorporate the effect of chemical-potential in the general relativistic frame work. The metric-dependence of the chemical-potential gives a new class of solutions for the boson stars. It is demonstrated that the maximum mass and radius of the star change in a significant way when the effect of finite chemical-potential is considered. We also discuss the case of a boson star made of quark-condensates. It is found that when the self-interaction between the condensates is small as compared to their mass, the typical density is too high to form a diquark-boson star. Our results indicate that the star of quark-condensate may be formed in a low-density and high-pressure regime.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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