MSSM at direction inflation: slow roll, stability fine-tuning and reheating

被引:169
作者
Allahverdi, Rouzbeh [1 ]
Enqvist, Kari
Garcia-Bellido, Juan
Jokinen, Asko
Mazumdar, Anupam
机构
[1] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada
[2] Univ Helsinki, Dept Phys Sci, FIN-00014 Helsinki, Finland
[3] Univ Helsinki, Inst Phys, FIN-00014 Helsinki, Finland
[4] Univ Autonoma Madrid, Dept Fis Teor C11, E-28049 Madrid, Spain
[5] NORDITA, DK-2100 Copenhagen, Denmark
[6] CNRS, UMR 5207, Lab Phys Theor & Astroparticles, F-34095 Montpellier, France
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2007年 / 06期
关键词
cosmology of theories beyond the SM; physics of the early universe; SUPERSYMMETRIC STANDARD MODEL; FLAT DIRECTIONS; COSMOLOGICAL PROBLEMS; BREAKING; SUPERGRAVITY; DECAY;
D O I
10.1088/1475-7516/2007/06/019
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider low scale slow roll inflation driven by the gauge-invariant flat directions udd and LLe of the minimally supersymmetric standard model at the vicinity of a saddle point of the scalar potential. We study the stability of the saddle point and the slow roll regime by considering radiative and supergravity corrections. The latter are found to be harmless, but the former require a modest fine-tuning of the saddle point condition. We show that, while the inflaton decays almost instantly, full thermalization occurs late, typically at a temperature T approximate to 10(7) GeV, so that there is no gravitino problem. We also compute the renormalization group running of the inflaton mass and relate it to slepton masses that may be within the reach of the LHC and could be precisely determined in a future linear collider experiment.
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页数:26
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