Cosmological window onto the string axiverse and the supersymmetry breaking scale

被引:84
|
作者
Visinelli, Luca [1 ,2 ,3 ,4 ]
Vagnozzi, Sunny [1 ,2 ,3 ]
机构
[1] Stockholm Univ, Oskar Klein Ctr Cosmoparticle Phys, Roslagstullsbacken 21A, SE-10691 Stockholm, Sweden
[2] KTH Royal Inst Technol, Nordita, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden
[3] Stockholm Univ, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden
[4] Uppsala Univ, Dept Phys & Astron, Lagerhyddsvagen 1, S-75120 Uppsala, Sweden
基金
瑞典研究理事会;
关键词
ISOTHERMAL DENSITY PERTURBATIONS; INFLATIONARY ENERGY DENSITY; TIME PHASE-TRANSITION; COLD DARK-MATTER; CP CONSERVATION; GALACTIC HALO; INVARIANCE; DETECTOR; DESIGN; AXIONS;
D O I
10.1103/PhysRevD.99.063517
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the simplest picture, the masses of string axions populating the axiverse depend on two parameters: the supersymmetry-breaking scale M-susy and the action S of the string instantons responsible for breaking the axion shift symmetry. In this work, we explore whether cosmological data can be used to probe these two parameters. Adopting string-inspired flat priors on log(10) M-susy and S and imposing that M-susy be sub-Planckian, we find S = 198 +/- 28. These bounds suggest that cosmological data complemented with string-inspired priors select a quite narrow axion mass range within the axiverse, log(10)(m(a)/eV) = -21.5(-2.3)(+1.3). We find that M-susy remains unconstrained due to a fundamental parameter degeneracy with S. We explore the significant impact of other choices of priors on the results, and we comment on similar findings in recent previous literature.
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页数:12
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