Dark energy, chaotic fields, and fundamental constants
被引:0
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作者:
Beck, Christian
论文数: 0引用数: 0
h-index: 0
机构:
Queen Mary Univ London, Sch Math Sci, London E1 4NS, EnglandQueen Mary Univ London, Sch Math Sci, London E1 4NS, England
Beck, Christian
[1
]
机构:
[1] Queen Mary Univ London, Sch Math Sci, London E1 4NS, England
来源:
FRONTIERS OF FUNDAMENTAL PHYSICS
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2006年
关键词:
D O I:
10.1007/1-4020-4339-2_20
中图分类号:
O4 [物理学];
学科分类号:
0702 ;
摘要:
To explain the currently observed accelerated expansion of the universe, a large number of different theoretical models are presently being discussed. In one way or another, all of these contain 'new physics', though at different levels. The big question is how to select out of infinitely many possible models the right one. We here discuss a possibility that has so far been somewhat neglected, namely that the new physics underlying dark energy arises out of a gravitationally active amendment of the electroweak and strong sector of the standard model. This amendment basically consists of a rapidly fluctuating gravitationally active dynamics of vacuum fluctuations with a cutoff of the order of the neutrino mass scale. We consider a concrete model for this based on second-quantized self-interacting scalar fields, which evolve in a chaotic way. It is shown that expectations with respect to the chaotic dynamics yield statements on the observed numerical values of the electroweak coupling constants with amazing precision, thus providing evidence for the physical relevance of this model.
机构:
Univ Roma La Sapienza, Int Ctr Relativist Astrophys, Dept Phys, I-00185 Rome, ItalyUniv Roma La Sapienza, Int Ctr Relativist Astrophys, Dept Phys, I-00185 Rome, Italy