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以太、暗能量与弦紧致化

Aether, dark energy and string compactifications.

作者信息

Townsend Paul K

机构信息

Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK.

出版信息

Philos Trans A Math Phys Eng Sci. 2022 Aug 22;380(2230):20210185. doi: 10.1098/rsta.2021.0185. Epub 2022 Jul 4.

Abstract

The nineteenth-century aether died with special relativity but was resurrected by general relativity in the form of dark energy; a tensile material with tension equal to its energy density. Such a material is provided by the D-branes of string-theory; these can support the fields of supersymmetric particle-physics, although their energy density is cancelled by orientifold singularities upon compactification. Dark energy can still arise from supersymmetry-breaking anti-D-branes but it is probably time-dependent. Recent results on time-dependent compactifications to an FLRW universe with late-time accelerated expansion are reviewed. This article is part of the theme issue 'The future of mathematical cosmology, Volume 2'.

摘要

19世纪的以太随狭义相对论一同消逝,但又以暗能量的形式在广义相对论中复活;暗能量是一种张力等于其能量密度的拉伸物质。弦理论中的D膜提供了这样一种物质;这些D膜能够支撑超对称粒子物理学的场,尽管在紧致化时它们的能量密度会被定向反演奇点抵消。暗能量仍可能源自超对称破缺的反D膜,但它可能是随时间变化的。本文回顾了关于紧致化为具有晚期加速膨胀的FLRW宇宙的随时间变化的紧致化的最新研究成果。本文是主题为“数学宇宙学的未来,第2卷”的一部分。

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引用本文的文献

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