Magnetogenesis with gravitational waves and primordial black hole dark matter

被引:4
作者
Balaji, Shyam [1 ]
Fairbairn, Malcolm [1 ]
Olea-Romacho, Marfa Olalla [2 ]
机构
[1] Kings Coll London, Dept Phys, London WC2R 2LS, England
[2] Univ Paris Cite, Sorbonne Univ, Univ PSL, Lab Phys Ecole Normale Super,ENS, F-75005 Paris, France
基金
欧盟地平线“2020”;
关键词
MAGNETIC-FIELDS; CONSTRAINTS; RADIATION;
D O I
10.1103/PhysRevD.109.075048
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Strongly supercooled first-order phase transitions (FOPTs) can produce primordial black hole (PBH) dark matter (DM) along with observable gravitational waves (GWs) from bubble collisions. Such FOPTs may also produce coherent magnetic fields generated by bubble collisions and by turbulence in the primordial plasma. Here we find that the requirement for PBH DM can produce large primordial magnetic fields which subsequently yield intergalactic magnetic fields in the present Universe (with magnitude less than or similar to 20 pG across coherence length scales of similar or equal to 0.001-0.01 Mpc, assuming maximally helical magnetic fields) that easily exceed lower bounds from blazar observations. We follow a largely model-independent approach and highlight the possibility of producing DM and observable multimessenger magnetic fields and GW signals visible in next generation experiments.
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页数:8
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