2021
DOI: 10.3390/sym13091598
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Gravitational Decoupling in Higher Order Theories

Abstract: Gravitational decoupling via the Minimal Geometric Deformation (MGD) approach has been used extensively in General Relativity (GR), mainly as a simple method for generating exact anisotropic solutions from perfect fluid seed solutions. Recently this method has also been used to generate exact spherically symmetric solutions of the Einstein-scalar system from the Schwarzschild vacuum metric. This was then used to investigate the effect of scalar fields on the Schwarzschild black hole solution. We show that this… Show more

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Cited by 25 publications
(9 citation statements)
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References 70 publications
(100 reference statements)
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“…[32][33][34][35][36][37][38][39][40][41][42][43][44][45][46][47][48][49]). Even this framework has been used widely in several scenarios such as 2 + 1 space-times [50][51][52][53][54][55], higher dimensions [56,57], asymptotically (A-)dS space-times [58], for axially symmetric systems and rotating black holes [59], hairy black holes [60][61][62], Cosmology [63,64], solutions in the background of Reissner-Nordström space-time [65][66][67], modified gravity theories [68][69][70][71][72][73][74][75][76][77][78], as well in braneworld gravity [79][80]…”
Section: Introductionmentioning
confidence: 99%
“…[32][33][34][35][36][37][38][39][40][41][42][43][44][45][46][47][48][49]). Even this framework has been used widely in several scenarios such as 2 + 1 space-times [50][51][52][53][54][55], higher dimensions [56,57], asymptotically (A-)dS space-times [58], for axially symmetric systems and rotating black holes [59], hairy black holes [60][61][62], Cosmology [63,64], solutions in the background of Reissner-Nordström space-time [65][66][67], modified gravity theories [68][69][70][71][72][73][74][75][76][77][78], as well in braneworld gravity [79][80]…”
Section: Introductionmentioning
confidence: 99%
“…We see that the effects are greater for the innermost layers, and are always proportional to K and 1/n. The same total effective pressure (73) is displayed in Figs. 2 and 3, now showing the effects of polytropes on stellar spheres explicitly.…”
Section: Coexistence Of Polytropes and Perfect Fluidsmentioning
confidence: 99%
“…Recently, Contreras and Fuenmayor [39] analyzed the stability of static spheres via gravitational cracking in the background of decoupling. Sultana [40] showed the applicability of decoupling through MGD in higher order theories as well.…”
Section: Introductionmentioning
confidence: 99%