Black holes with a charged quantum dust core

被引:0
作者
Casadio, R. [1 ,2 ]
Rocha, R. da [3 ]
Giusti, A. [4 ]
Meert, P. [5 ]
机构
[1] Univ Bologna, Dipartimento Fis & Astron, Via Irnerio 46, I-40126 Bologna, Italy
[2] INFN, Sez Bologna, IS FLAG Viale Berti Pichat 6-2, I-40127 Bologna, Italy
[3] Fed Univ ABC, Ctr Math Santo Andre, BR-09210580 Santo Andre, Brazil
[4] Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, England
[5] Univ Estadual Paulista, Inst Fis Teor, BR-01140070 Sao Paulo, Brazil
基金
巴西圣保罗研究基金会; 英国科学技术设施理事会;
关键词
CAUCHY-HORIZON; INSTABILITY; SPACETIME; ENERGY; MODEL;
D O I
10.1103/PhysRevD.110.104067
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
To understand the nature of the black holes that exist in the Universe, it is also necessary to study what happens to the (quantum) matter that collapses and forms such objects. In this work, we consider a dust ball with an electrically charged central core and study its quantum spectrum by quantizing the geodesic equation for individual dust particles in the corresponding Reissner-Nordstr & ouml;m spacetime. As in the neutral case investigated previously, we find a ground state of the dust ball with the size of a fraction of the outer horizon. Moreover, we determine a self-consistent configuration of layers in the ground state corresponding to an effective mass function that increases linearly with the areal radius and has no inner Cauchy horizon. We then briefly speculate on the possible phenomenological consequences for the endpoint of the gravitational collapse.
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页数:10
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