String cosmology: From the early universe to today

被引:66
作者
Cicoli, Michele [1 ,2 ]
Conlon, Joseph P. [3 ]
Maharana, Anshuman [4 ]
Parameswaran, Susha [5 ]
Quevedo, Fernando [6 ]
Zavala, Ivonne [7 ]
机构
[1] Univ Bologna, Dipartimento Fis & Astron, Via Irnerio 46, I-40126 Bologna, Italy
[2] INFN, Sez Bologna, Viale Berti Pichat 6-2, I-40127 Bologna, Italy
[3] Univ Oxford, Rudolf Peierls Ctr Theoret Phys, Clarendon Lab, Beecroft Bldg,Parks Rd, Oxford OX1 3PU, England
[4] CI Homi Bhabha Natl Inst, Harish Chandra Res Inst, Chattnag Rd, Allahabad 211019, India
[5] Univ Liverpool, Dept Math Sci, Liverpool L69 7ZL, England
[6] Univ Cambridge, DAMTP, Wilberforce Rd, Cambridge CB3 0WA, England
[7] Swansea Univ, Dept Phys, Swansea SA2 8PP, Wales
来源
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2024年 / 1059卷
关键词
Early universe cosmology; String theory; Inflation; Dark energy; FLUX-SCALING SCENARIO; COLD DARK-MATTER; PRE-BIG-BANG; CALABI-YAU; SUPERSYMMETRY BREAKING; MODULI STABILIZATION; GRAVITINO-OVERPRODUCTION; ACCELERATING COSMOLOGIES; NATURAL INFLATION; AXION MONODROMY;
D O I
10.1016/j.physrep.2024.01.002
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We review applications of string theory to cosmology, from primordial times to the present -day accelerated expansion. Starting with a brief overview of cosmology and string compactifications, we discuss in detail moduli stabilisation, inflation in string theory, the impact of string theory on post-inflationary dynamics (reheating, moduli domination, kination), dark energy (the cosmological constant from a string landscape and models of quintessence) and various alternative scenarios (string/brane gases, the pre big-bang scenario, rolling tachyons, ekpyrotic/cyclic cosmologies, bubbles of nothing, S-brane and holographic cosmologies). The state of the art in string constructions is described in each topic and, where relevant, connections to swampland conjectures are made. The possibilities for novel particles and excitations (axions, moduli, cosmic strings, branes, solitons, oscillons and boson stars) are emphasised. Implications for the physics of the CMB, gravitational waves, dark matter and dark radiation are discussed along with potential observational signatures. (c) 2024 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).
引用
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页码:1 / 155
页数:155
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