arXiv · gr-qc/0410045
Entropy in the NUT-Kerr-Newman Black Holes Due to an Arbitrary Spin Field
Abstract
Membrane method is used to compute the entropy of the NUT-Kerr-Newman black holes. It is found that even though the Euler characteristic is greater than two, the Bekenstein-Hawking area law is still satisfied. The formula $S=χA/8$ relating the entropy and the Euler characteristic becomes inapplicable for non-extreme four dimensional NUT-Kerr-Newman black holes.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Xian-Hui Ge, You-Gen Shen. 2004-10-09. Entropy in the NUT-Kerr-Newman Black Holes Due to an Arbitrary Spin Field. https://doi.org/10.1088/0264-9381%2F20%2F16%2F305
Cite the original work for its findings. Save a collection to share your selection of sources.