Holographic foam, dark energy and infinite statistics
Holographic foam, dark energy and infinite statistics
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DOI：
10.1016/j.physletb.2007.09.052
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发表时间：
2007-03
影响因子：
4.4
通讯作者：
Y. Ng
中科院分区：
文献类型：
--
作者：
Y. Ng
时空的量子涨落会产生量子泡沫，而黑洞物理学规定这种泡沫是全息类型的。应用于宇宙学，全息模型需要暗能量的存在，我们认为，是由大量的惰性“粒子”的极长的波长。这些“粒子”必然服从无限的统计，其中粒子置换群的所有表示都可以出现。在目前可观测的宇宙中，每一个玻色子或费米子都可能有1031个这样的“粒子”。我们还讨论了全息原理与无限统计之间的兼容性。
Quantum fluctuations of spacetime give rise to quantum foam, and black hole physics dictates that the foam is of holographic type. Applied to cosmology, the holographic model requires the existence of dark energy which, we argue, is composed of an enormous number of inert “particles” of extremely long wavelength. These “particles” necessarily obey infinite statistics in which all representations of the particle permutation group can occur. For every boson or fermion in the present observable universe there could be ∼1031such “particles”. We also discuss the compatibility between the holographic principle and infinite statistics.