Hairy magnetic and dyonic black holes in the Standard Model

被引:20
作者
Bai, Yang [1 ]
Korwar, Mrunal [1 ]
机构
[1] Univ Wisconsin, Dept Phys, Madison, WI 53706 USA
关键词
Black Holes; Beyond Standard Model; PARTICLE; MONOPOLE; FIELD; STABILITY; EMISSION;
D O I
10.1007/JHEP04(2021)119
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
Spherically symmetric magnetic and dyonic black holes with a magnetic charge Q = 2 are studied in the Standard Model and general relativity. A magnetically charged black hole with mass below 9.3 x 10(35) GeV has a "hairy" cloud of electroweak gauge and Higgs fields outside the event horizon with 1/m(W) in size. An extremal magnetic black hole has a hair mass of 3.6 TeV, while an extremal dyonic black hole has an additional mass of q(2) x 1.6 GeV for a small electric charge q << 2 pi /e(2). A hairy dyonic black hole with an integer charge is not stable and can decay into a magnetic one plus charged fermions. On the other hand, a hairy magnetic black hole can evolve via Hawking radiation into a nearly extremal one that is cosmologically stable and an interesting object to be searched for.
引用
收藏
页数:21
相关论文
共 49 条
[41]  
Shovkovy I. A., 2013, Strongly interacting matter in magnetic fields, V871, P13, DOI 10.1007/978-3-642-37305-32
[42]   DECAY OF A DYON [J].
SONODA, H .
NUCLEAR PHYSICS B, 1984, 238 (02) :259-276
[43]   NON-ABELIAN BLACK-HOLES AND CATASTROPHE-THEORY .2. CHARGED TYPE [J].
TACHIZAWA, T ;
MAEDA, K ;
TORII, T .
PHYSICAL REVIEW D, 1995, 51 (08) :4054-4066
[44]  
THOOFT G, 1974, NUCL PHYS B, VB 79, P276
[45]   REGULAR SOLUTION OF THOOFTS MAGNETIC MONOPOLE MODEL IN CURVED SPACE [J].
VANNIEUWENHUIZEN, P ;
WILKINSON, D .
PHYSICAL REVIEW D, 1976, 13 (04) :778-784
[46]  
Wald RM., 1984, General Relativity
[47]   A YANG-MILLS-HIGGS MONOPOLE OF CHARGE-2 [J].
WARD, RS .
COMMUNICATIONS IN MATHEMATICAL PHYSICS, 1981, 79 (03) :317-325
[48]  
Weinberg E.J, 1994, 13 S THEOR PHYS FIEL
[49]   DYONS OF CHARGE E-THETA/2-PI [J].
WITTEN, E .
PHYSICS LETTERS B, 1979, 86 (3-4) :283-287