Minimal Geometric Deformation in a cloud of strings

Abstract

We find new exact analytical solutions in three-dimensional gravity applying the Minimal Geometric Deformation approach in a cloud of strings.

6 pages, 3 figures, accepted for publication in EPJC

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• The Gravitational decoupling method: the higher dimensional case to find new analytic solutions
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• A way of decoupling gravitational sources in pure Lovelock gravity
• Anisotropic Tolman V Solution by Minimal Gravitational Decoupling Approach
• Exploring physical properties of minimally deformed strange star model and constraints on maximum mass limit in $f(\mathcal{Q})$ gravity
• Decoupling gravitational sources by MGD approach in Rastall gravity
• Extended gravitational decoupling in $2+1$ dimensional space--times
• Stellar models with like--Tolman IV complexity factor
• A simple protocol to construct solutions with vanishing complexity by Gravitational Decoupling
• Ultracompact stars with polynomial complexity by gravitational decoupling
• Anisotropic Strange Star Model Beyond Standard Maximum Mass Limit by Gravitational Decoupling in $f(Q)$ Gravity
• Gravitational cracking and complexity in the framework of gravitational decoupling
• MGD Dirac stars
• The minimal of geometric deformation of Yang-Mills-Dirac stellar configurations
• Anisotropic 2+1 dimensional black holes by gravitational decoupling
• Gravitational decoupling in $2+1$ dimensional space--times with cosmological term
• Energy exchange between relativistic fluids: the polytropic case
• Role of gravitational decoupling on isotropization and complexity of self-gravitating system under complete geometric deformation approach
• Rotating hairy black holes and thermodynamics from gravitational decoupling
• Influence of three parameters on maximum mass and stability of strange star under linear $f(Q)-$action
• Probing hairy black holes caused by gravitational decoupling using quasinormal modes and greybody bounds
• Regularity condition on the anisotropy induced by gravitational decoupling in the framework of MGD
• Holographic entanglement entropy under the minimal geometric deformation and extensions
• Echoes of the gravitational decoupling: scalar perturbations and quasinormal modes of hairy black holes
• MGD-decoupled black holes, anisotropic fluids and holographic entanglement entropy
• Probing the minimal geometric deformation with trace and Weyl anomalies
• Effects of Charge on Gravitational Decoupled Anisotropic Solutions in f(R) Gravity
• Durgapal IV model in light of the minimal geometric deformation approach
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• Extra packing of mass of anisotropic interiors induced by MGD
• Gravitational decoupling, hairy black holes and conformal anomalies
• Gravitational decoupling of generalized Horndeski hybrid stars
• Braneworld Gravity under gravitational decoupling
• Quasi Normal Modes of hairy black holes at higher--order WKB approach
• Integration of the Lane-Emden equation for relativistic anisotropic polytropes through Gravitational Decoupling: a novel approach
• Rotating black hole mimicker surrounded by the string cloud
• Imprints of dark matter on the structural properties of minimally deformed compact stars
• A note of the first law of thermodynamics by gravitational decoupling
• Relativistic Polytropic Models of Charged Anisotropic Compact Object
• Complexity factor of spherically anisotropic polytropes from gravitational decoupling
• Axion stars in MGD background
• Gravitational Decoupling algorithm modifies the value of the conserved charges and thermodynamics properties in Lovelock Unique Vacuum theory
• Gravitational decoupling and aerodynamics: black holes and analog gravity in a jet propulsion lab
• Quasinormal modes of charged BTZ black holes
• When gravitational decoupling and quantum gravity (re)unite
• Minimally deformed wormholes inspired by noncommutative geometry
• 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
• Energy transfer between the sources in gravitational decoupling
• The Dirac oscillator in the curved spacetime of a cloud of strings