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摘要:
The vacuum component of the Universe is investigated in both the quantum and the classical regimes of its evolution. The associated vacuum energy density was reduced by more than 78 orders of magnitude in 10-6 sec in the quantum regime and by nearly 45 orders of magnitude in 4 × 1017 sec in the classical regime. The vacuum energy was spent for the organization of new microstates during the expansion of the Universe. In the quantum regime, phase transitions were more effective in reducing the vacuum energy than in producing new microstates. Both of these phenomena have been recorded in the history of the Universe. Herein, the need for the evolution of the Universe’s vacuum component is discussed. Indeed, through this evolution, all 123 crisis orders of dark energy are reduced by conventional physical processes. A table of the vacuum energy’s evolution as the function of red shift and a short discussion about vacuum stability are presented.
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篇名 Dark Energy as a Vacuum Component of the Universe
来源期刊 现代物理(英文) 学科 地球科学
关键词 DARK Energy Early UNIVERSE Quantum REGIME Phase TRANSITIONS CLASSICAL REGIME
年,卷(期) 2013,(9) 所属期刊栏目
研究方向 页码范围 1185-1188
页数 4页 分类号 P1
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DARK
Energy
Early
UNIVERSE
Quantum
REGIME
Phase
TRANSITIONS
CLASSICAL
REGIME
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研究分支
研究去脉
引文网络交叉学科
相关学者/机构
期刊影响力
现代物理(英文)
月刊
2153-1196
武汉市江夏区汤逊湖北路38号光谷总部空间
出版文献量(篇)
1826
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0
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0
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