Particle physics models of inflation and curvaton scenarios

被引:267
作者
Mazumdara, Anupam [1 ,2 ]
Rocher, Jonathan [3 ]
机构
[1] Univ Lancaster, Dept Phys, Lancaster LA1 4YB, England
[2] Niels Bohr Inst, DK-2100 Copenhagen, Denmark
[3] Univ Libre Bruxelles, Serv Phys Theor, B-1050 Brussels, Belgium
来源
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2011年 / 497卷 / 4-5期
关键词
D-TERM INFLATION; COSMOLOGICAL MODULI PROBLEM; GRAND UNIFIED THEORIES; PRE-BIG-BANG; DYNAMICAL SUPERSYMMETRY BREAKING; BARYON-NUMBER NONCONSERVATION; 3-POINT CORRELATION-FUNCTION; SCALAR FIELD FLUCTUATIONS; TO-CLASSICAL TRANSITION; FAYET-ILIOPOULOS TERMS;
D O I
10.1016/j.physrep.2010.08.001
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We review the particle theory origin of inflation and curvaton mechanisms for generating large scale structures and the observed temperature anisotropy in the cosmic microwave background (CMB) radiation. Since inflaton or curvaton energy density creates all matter, it is important to understand the process of reheating and preheating into the relevant degrees of freedom required for the success of Big Bang Nucleosynthesis. We discuss two distinct classes of models, one where inflaton and curvaton belong to the hidden sector, which are coupled to the Standard Model gauge sector very weakly. There is another class of models of inflaton and curvaton, which are embedded within Minimal Supersymmetric Standard Model (MSSM) gauge group and beyond, and whose origins lie within gauge invariant combinations of supersymmetric quarks and leptons. Their masses and couplings are all well motivated from low energy physics, therefore such models provide us with a unique opportunity that they can be verified/falsified by the CMB data and also by the future collider and non-collider based experiments. We then briefly discuss the stringy origin of inflation, alternative cosmological scenarios, and bouncing universes. (C) 2010 Elsevier B.V. All rights reserved.
引用
收藏
页码:85 / 215
页数:131
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