Accelerated expansion of a universe containing a self-interacting Bose-Einstein gas

被引：4

作者：

Izquierdo, German ^{[1
]}

Besprosvany, Jaime ^{[1
]}

机构：

[1] Univ Nacl Autonoma Mexico, Inst Fis, Mexico City 04510, DF, Mexico

来源：

CLASSICAL AND QUANTUM GRAVITY | 2010年 / 27卷 / 06期

关键词：

DARK ENERGY; COSMOLOGICAL CONSEQUENCES;

D O I：

10.1088/0264-9381/27/6/065012

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Acceleration of the universe is obtained from a model of non-relativistic particles with a short-range attractive interaction, at low enough temperature to produce a Bose-Einstein condensate. Conditions are derived for negative-pressure behavior. In particular, we show that a phantom-accelerated regime at the beginning of the universe solves the horizon problem, consistently with nucleosynthesis.

引用

页数：16

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