Holonomy corrected Schwarzschild black hole lensing
A. R. Soares, C. F. S. Pereira, R. L. L. Vitória, Erick Melo Rocha
Abstract
In the present work, we theoretically investigate gravitational lensing in the spacetime of a holonomy corrected Schwarzschild black hole. Analytical expressions for the light deflection angle are obtained in both the weak field limit and the strong field limit. Furthermore, we analyze observables, such as relativistic images and magnifications, and compare the results with those expected in a Schwarzschild spacetime. We discuss the possibilities and difficulties of investigating such a solution in practice.
Topics & Concepts
Schwarzschild radiusPhysicsPhoton sphereSchwarzschild metricHolonomySpacetimeSchwarzschild geodesicsDeriving the Schwarzschild solutionBlack hole (networking)Classical mechanicsKerr metricCharged black holeGravitational lensLimit (mathematics)Gravitational fieldStrong gravitational lensingQuantum mechanicsGeneral relativityMathematical physicsRedshiftGalaxyMathematical analysisComputer networkRouting protocolComputer scienceRouting (electronic design automation)MathematicsLink-state routing protocolAstrophysical Phenomena and ObservationsPulsars and Gravitational Waves ResearchCosmology and Gravitation Theories