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 |
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creator | 周康 岳瑞宏 杨战营 邹德成 |
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). |
doi_str_mv | 10.1088/1674-1056/21/7/079801 |
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language | eng |
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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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