论暴涨理论中宇宙的初始状态

IF 0.2 Q4 PHYSICS, MULTIDISCIPLINARY
Natalia N. Gorobey, Alexander S. Lukyanenko, Mikhail V. Svintsov
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引用次数: 0

摘要

我们考虑了暴胀宇宙的一个玩具量子模型,其中宇宙时间的作用是由暴胀标量场(它的对数)扮演的。基于广义相对论中正能量定理在封闭宇宙情况下的一个变体,引入了空间的严格正能量。提出了空间能量最小原理,该原理决定了量子宇宙学中宇宙的基态和激发态。根据这一原理,宇宙的开端确实以空间能量的最小激发状态存在。宇宙的初始原暴胀量子态被定义为一种空间能量的最小激发状态,前提是暴胀标量场在开始时的势能很大。同时,引入了空间能量激发的量子,宇宙的膨胀可以看作是这些量子的诞生。当膨胀标量场的势能降至零时,普通物质的量子诞生变得重要。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
On the initial state of the universe in the theory of inflation

A toy quantum model of the inflationary universe is considered in which the role of cosmic time is played by the inflaton scalar field (its logarithm). Based on a variant of the positive energy theorem in General Relativity for the case of a closed universe, a strictly positive energy of space is introduced. The principle of minimum of the energy of space is proposed which determines a ground state as well as the excited states of the universe in quantum cosmology. According to this principle, the Beginning of the universe does exist as a state of minimal excitation of the energy of space. The initial proto-inflation quantum state of the universe is defined as a state of minimal excitation of the energy of space provided that the potential energy of the inflaton scalar field is large at the Beginning. Simultaneously, quanta of space energy excitation are introduced and the expansion of the universe can be considered as the birth of these quanta. Quantum birth of the ordinary matter becomes significant when the potential energy of the inflaton scalar field comes down to zero value.

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