含有自相互作用玻色-爱因斯坦气体的宇宙的加速膨胀
Accelerated expansion of a universe containing a self-interacting Bose-Einstein gas
摘要：
宇宙的加速度是从一个非相对论性粒子模型中得到的，该模型具有短程吸引相互作用，在足够低的温度下产生玻色-爱因斯坦凝聚体。条件推导出负压行为。特别是，我们表明，幻影加速制度在宇宙的开始解决了视界问题，一致的核合成。
英文摘要：
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.
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。
