arXiv · 2112.12865
Absorption by stringy black holes
Abstract
We investigate the absorption of planar massless scalar waves by a charged rotating stringy black hole, namely a Kerr--Sen black hole. We compute numerically the absorption cross section and compare our results with those of the Kerr-Newman black hole, a classical general relativity solution. In order to better compare both charged black holes, we define the ratio of the black hole charge to the extreme charge as $Q$. We conclude that Kerr--Sen and Kerr-Newman black holes have a similar absorption cross section, with the difference increasing for higher values of $Q$.
Explore related subjects
Keep this discovery
Sérgio Vinicius M. C. B. Xavier, Carolina L. Benone, Luís C. B. Crispino. 2021-12-23. Absorption by stringy black holes. https://doi.org/10.1140/epjc%2Fs10052-021-09933-9
Cite the original work for its findings. Save a collection to share your selection of sources.