Spontaneous symmetry breaking vacuum energy in cosmology

The gravitational effect of spontaneous symmetry breaking vacuum energy density is investigated by subtracting the fiat space-time contribution from the energy in the curved space-time. We find that the remaining effective energy- momentum tensor is too small to cause the acceleration of the univers...

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Veröffentlicht in:Chinese physics B 2012-07, Vol.21 (7), p.617-622
1. Verfasser: 周康 岳瑞宏 杨战营 邹德成
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description The gravitational effect of spontaneous symmetry breaking vacuum energy density is investigated by subtracting the fiat space-time contribution from the energy in the curved space-time. We find that the remaining effective energy- momentum tensor is too small to cause the acceleration of the universe, although it satisfies the characteristics of dark energy. However, it could provide a promising explanation to the puzzle of why the gravitational effect produced by the huge symmetry breaking vacuum energy in the electroweak theory has not been observed, as it has a sufficiently small value (smaller than the observed cosmic energy density by a factor of 1032).
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source IOP Publishing Journals
subjects Broken symmetry
Cosmology
Dark energy
Energy density
Flats
Gravitational effects
Mathematical analysis
Spontaneous
Universe
宇宙学
对称性破缺
对称性自发破缺
引力效应
弯曲时空
有效能量
真空能量
能量密度
title Spontaneous symmetry breaking vacuum energy in cosmology
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