Noncommutative Reissner-Nordstrøm Black hole
arXiv:1503.05469 · doi:10.1139/cjp-2017-0599
Abstract
A deformed embedding of the Reissner-Nordstrøm spacetime is constructed within the framework of a noncommutative Riemannian geometry. We find noncommutative corrections to the usual Riemannian expressions for the metric and curvature tensors, which, in the case of the metric, are valid to all orders in the deformation parameter. We calculate the area of the event horizon of the corresponding noncommutative R-N black-hole, obtaining corrections up to fourth order in the deformation parameter for the area of the black-hole. Finally we include some comments on the noncommutative version on one of the second order scalar invariants of the Riemann tensor, the so called Kretschmann invariant, a quantity regularly used in order to extend gravity to quantum level.
7 page
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Cited by in corpus (4)
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- Proton Decay and the Quantum Structure of Spacetime