Non-local gravitational corrections in black hole shadow images

Abstract

With the help of Newman-Janis method new spinning black hole (BH) solution for a non-local gravity model was obtained. We show how to account the quantum gravitational correction part in BH shadows modelling using spinning BH metrics with a model independent approach. It is confirmed that in the future to follow the increasing of the experimental accuracy and therefore to reproduce new results theoretically one could take into account different field correction terms instead of introducing of new fields and/or curvature expansions.

12 pages, 6 figures

References in corpus (5)

• Measurement of the Kerr Spin Parameter by Observation of a Compact Object's Shadow
• Janis-Newman algorithm: generating rotating and NUT charged black holes
• Quantum Gravitational Corrections to a Star Metric and the Black Hole Limit
• Gravity Induced Non-Local Effects in the Standard Model
• Extended Gravity Constraints at Different Scales