Photons from dark photon solitons via parametric resonance

被引:8
|
作者
Amin, Mustafa A. [1 ]
Long, Andrew J. [1 ]
Schiappacasse, Enrico D. [1 ]
机构
[1] Rice Univ, Dept Phys & Astron, 6100 Main St, Houston, TX 77005 USA
基金
美国国家科学基金会; 芬兰科学院;
关键词
absorption and radiation processes; particle physics-cosmology connection; axions; dark matter theory; MATTER; STARS;
D O I
10.1088/1475-7516/2023/05/015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Wave-like dark matter made of spin-1 particles (dark photons) is expected to form ground state clumps called "vector solitons", which can have different polarizations. In this work, we consider the interaction of dark photons with photons, expressed as dimension-6 operators, and study the electromagnetic radiation that arises from an isolated vector soliton due to parametric resonant amplification of the ambient electromagnetic field. We characterize the directional dependence and polarization of the outgoing radiation, which depends on the operator as well as the polarization state of the underlying vector soliton. We discuss the implications of this radiation for the stability of solitons and as a possible channel for detecting mergers of vector solitons through astrophysical observations.
引用
收藏
页数:33
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