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arXiv 0904.2746gr-qcastro-ph.COquant-ph
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标量场宇宙学:非线性薛定谔型表述

Scalar field cosmology: its non-linear Schrödinger-type formulation

Burin Gumjudpai

摘要:

标量场宇宙学是暗能量和暴胀的模型。最近发现,标准的弗里德曼公式的标量场宇宙学可以表示为一个非线性薛定谔方程。新的数学公式因此被称为非线性薛定谔(NLS)公式,它适用于具有不可忽略正压流体密度的FRLW宇宙学系统。它的主要特点在这里进行审查。

英文摘要:

Scalar field cosmology is a model for dark energy and inflation. It has been recently found that the standard Friedmann formulation of the scalar field cosmology can be expressed in a non-linear Schrödinger-type equation. The new mathematical formulation is hence called non-linear Schrödinger (NLS) formulation which is suitable for a FRLW cosmological system with non-negligible barotropic fluid density. Its major features are reviewed here.

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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