Einstein-Klein-Gordon system by gravitational decoupling

被引:90
作者
Ovalle, J. [1 ,2 ,3 ]
Casadi, R. [4 ,5 ]
da Rocha, R. [6 ]
Sotomayor, A. [7 ]
Stuchlik, Z. [1 ,2 ]
机构
[1] Silesian Univ Opava, Fac Philosophy & Sci, Inst Phys, CZ-74601 Opava, Czech Republic
[2] Silesian Univ Opava, Fac Philosophy & Sci, Res Ctr Theoret Phys & Astrophys, CZ-74601 Opava, Czech Republic
[3] Univ Simon Bolivar, Dept Fis, AP 89000, Caracas 1080A, Venezuela
[4] Alma Mater Univ Bologna, Dipartimento Fis & Astron, Via Irnerio 46, I-40126 Bologna, Italy
[5] Ist Nazl Fis Nucl, Sez Bologna, IS FLAG, Viale Berti Pichat 6-2, I-40127 Bologna, Italy
[6] Univ Fed Abc, Ctr Matemat Comp & Cognicao, BR-09210580 Santo Andre, SP, Brazil
[7] Univ Antofagasta, Dept Matemat, Antofagasta, Chile
基金
巴西圣保罗研究基金会;
关键词
DILATONIC BLACK-HOLES; STARS;
D O I
10.1209/0295-5075/124/20004
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We investigate how a spherically symmetric scalar field can modify the Schwarzschild vacuum solution when there is no exchange of energy-momentum between the scalar field and the central source of the Schwarzschild metric. This system is described by means of the gravitational decoupling, by Minimal Geometric Deformation (MGD-decoupling), which allows us to show that, under the MGD paradigm, the Schwarzschild solution is modified in such a way that a naked singularity appears. Copyright (C) EPLA, 2018
引用
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页数:7
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