A-term inflation and the minimal supersymmetric standard model

被引:64
作者
Sanchez, Juan C. Bueno [1 ]
Dimopoulos, Konstantinos [1 ]
Lyth, David H. [1 ]
机构
[1] Univ Lancaster, Dept Phys, Lancaster LA1 4YB, England
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2007年 / 01期
关键词
inflation; cosmology of theories beyond the SM;
D O I
10.1088/1475-7516/2007/01/015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The parameter space for A-term inflation is explored with W = lambda(phi p)(p)/pM(P)(p-3) . With p = 6 and lambda(p)similar to 1, the observed spectrum and spectral tilt can be obtained with soft mass of order 10(2) GeV but not with a much higher mass. The case p = 3 requires lambda(p) similar to 10(-9) to 10(-12). The ratio m/A requires fine-tuning, which may be justified on environmental grounds. An extension of the minimal supersymmetric standard model to include non-renormalizable terms and/ or Dirac neutrino masses might support either A-term inflation or modular inflation.
引用
收藏
页数:10
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