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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

Einstein-Klein-Gordon system by gravitational decoupling

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Author(s):
Ovalle, J. [1, 2, 3] ; Casadi, R. [4, 5] ; da Rocha, R. [6] ; Sotomayor, A. [7] ; Stuchlik, Z. [2, 3]
Total Authors: 5
Affiliation:
[1] Univ Simon Bolivar, Dept Fis, AP 89000, Caracas 1080A - Venezuela
[2] Silesian Univ Opava, Fac Philosophy & Sci, Inst Phys, CZ-74601 Opava - Czech Republic
[3] Silesian Univ Opava, Fac Philosophy & Sci, Res Ctr Theoret Phys & Astrophys, CZ-74601 Opava - Czech Republic
[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
Total Affiliations: 7
Document type: Journal article
Source: EPL; v. 124, n. 2 OCT 2018.
Web of Science Citations: 15
Abstract

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 (AU)

FAPESP's process: 17/18897-8 - Fluid/gravity correspondence, fermionic sectors and its ramifications
Grantee:Roldão da Rocha
Support Opportunities: Regular Research Grants