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Cosmological window onto the string axiverse and the supersymmetry breaking scale

机译:弦轴和超对称断裂尺度上的宇宙学窗口

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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.
机译:在最简单的图中,填充轴的弦轴的质量取决于两个参数:超对称性破坏标度M susy和负责破坏轴对称性的弦子瞬子的作用S。在这项工作中,我们探索宇宙数据是否可以用来探测这两个参数。在对数为10 M的sussus和S上采用字符串启发式的平坦先验,并假设M sussy为Sub-Planckian,我们发现S = 198±28。这些界限表明,宇宙学数据与弦启发的先验相辅相成,在轴范围内选择了相当狭窄的轴突质量范围,log 10(m a / eV)=? 21. 5? 2.3 + 1.3。我们发现由于S的基本参数简并性,M susy仍然不受约束。我们探索了其他先验选择对结果的重大影响,并对近期文献中的类似发现进行了评论。

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