Hidden photon and axion dark matter from symmetry breaking

被引:40
作者
Nakayama, Kazunori [1 ,2 ]
Yin, Wen [1 ,3 ]
机构
[1] Univ Tokyo, Dept Phys, Fac Sci, Tokyo 1130033, Japan
[2] Univ Tokyo, Kavli Inst Phys & Math Univ WPI, Kashiwa, Chiba 2778583, Japan
[3] Tohoku Univ, Dept Phys, Sendai, Miyagi 9808578, Japan
关键词
Beyond Standard Model; Cosmology of Theories beyond the SM; Spontaneous Symmetry Breaking; PARTICLE-PRODUCTION; CP CONSERVATION; SCALAR FIELDS; INFLATION; UNIVERSE; CONSTRAINTS; QCD; TEMPERATURE; INVARIANCE; COSMOLOGY;
D O I
10.1007/JHEP10(2021)026
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
A light hidden photon or axion-like particle is a good dark matter candidate and they are often associated with the spontaneous breaking of dark global or gauged U(1) symmetry. We consider the dark Higgs dynamics around the phase transition in detail taking account of the portal coupling between the dark Higgs and the Standard Model Higgs as well as various thermal effects. We show that the (would-be) Nambu-Goldstone bosons are efficiently produced via a parametric resonance with the resonance parameter q similar to 1 at the hidden symmetry breaking. In the simplest setup, which predicts a second order phase transition, this can explain the dark matter abundance for the axion or hidden photon as light as sub eV. Even lighter mass, as predicted by the QCD axion model, can be consistent with dark matter abundance in the case of first order phase transition, in which case the gravitational wave signals may be detectable by future experiments such as LISA and DECIGO.
引用
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页数:33
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