Gravitationally decoupled non-Schwarzschild black holes and wormhole space–times
Francisco Tello‐Ortiz, Ángel Rincón, A. Alvarez, Saibal Ray
Abstract
Abstract In this article, using gravitational decoupling by means of minimal geometric deformation approach, we obtain a new spherically symmetric and static black hole solution. To progress, we close the system by assuming that the average pressure of the $$\theta $$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>θ</mml:mi> </mml:math> -sector is vanishing. Also, we tackle the problem regarding how, for a given minimally deformed black hole solution, one can connect it to a wormhole space–time.
Topics & Concepts
WormholeDecoupling (probability)Schwarzschild radiusSchwarzschild metricPhysicsGravitationBlack hole (networking)Space (punctuation)Classical mechanicsMathematical physicsTheoretical physicsComputer scienceGeneral relativityEngineeringOperating systemControl engineeringComputer networkRouting (electronic design automation)Link-state routing protocolRouting protocolBlack Holes and Theoretical PhysicsCosmology and Gravitation TheoriesPulsars and Gravitational Waves Research