A way of decoupling gravitational sources in pure Lovelock gravity

Abstract

We provide an algorithm that shows how to decouple gravitational sources in Pure Lovelock gravity. This method allows to obtain several new and known analytic solutions of physical interest in scenarios with extra dimensions and with presence of higher curvature terms. Furthermore, using our method, it is shown that applying the minimal geometric deformation to the Anti de Sitter space time it is possible to obtain regular black hole solutions.

arXiv commentAccepted for publication in Eur.Phys.J.C

References in corpus (39)

• Decoupling gravitational sources in general relativity: from perfect to anisotropic fluids
• Anisotropic solutions by gravitational decoupling
• Decoupling gravitational sources in general relativity: the extended case
• Planck stars
• Gravitational decoupled anisotropies in compact stars
• Black holes by gravitational decoupling
• Isotropization and change of complexity by gravitational decoupling
• A new family of analytical anisotropic solutions by gravitational decoupling
• Gravitational Decoupled Charged Anisotropic Spherical Solutions
• Black Holes in Pure Lovelock Gravities
• Minimal Geometric Deformation in a cloud of strings
• A causal Schwarzschild-de Sitter interior solution by gravitational decoupling
• Using MGD gravitational decoupling to extend the isotropic solutions of Einstein equations to the anisotropical domain
• Minimal geometric deformation decoupling in $2+1$ dimensional space-times
• Compact Anisotropic Models in General Relativity by Gravitational Decoupling
• Anisotropic ultracompact Schwarzschild star by gravitational decoupling
• A general interior anisotropic solution for a BTZ vacuum in the context of the Minimal Geometric Deformation decoupling approach
• Bardeen black hole chemistry
• Charged anisotropic compact objects by gravitational decoupling
• On the Effective Metric of a Planck Star
• The Gravitational decoupling method: the higher dimensional case to find new analytic solutions
• Einstein-Klein-Gordon by gravitational decoupling
• Gravitational Decoupled Anisotropic Solutions in $f(\mathcal{G})$ Gravity
• Minimal Geometric Deformation: the inverse problem
• $D$-dimensional Bardeen-AdS black holes in Einstein-Gauss-Bonnet theory
• Minimal Geometric Deformation in asymptotically (A-)dS space-times and the isotropic sector for a polytropic black hole
• Characterization of the Lovelock gravity by Bianchi derivative
• Gravitational decoupling in $2+1$ dimensional space--times with cosmological term
• Regular Stringy Black Holes?
• Buchdahl compactness limit for a pure Lovelock static fluid star
• Universality of isothermal fluid spheres in Lovelock gravity
• A discerning gravitational property for gravitational equation in higher dimensions
• Regular black holes and its thermodynamics in Lovelock gravity
• Compact objects in pure Lovelock theory
• On Lovelock analogues of the Riemann tensor
• Topological black holes in pure Gauss-Bonnet gravity and phase transitions
• Buchdahl-Vaidya-Tikekar model for stellar interior in pure Lovelock gravity - II
• Static pure Lovelock black hole solutions with horizon topology ${\mathbf{S}}^{(\mathbf{n})}\times {\mathbf{S}}^{(\mathbf{n})}$
• Regular black holes with $\Lambda >0$ and its evolution in Lovelock gravity

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• Hair imprints of the gravitational decoupling and hairy black hole spectroscopy
• Gravitational decoupling and regular hairy black holes: Geodesic stability, quasinormal modes, and thermodynamic properties
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