@article{16d5fd4fdb4341fd8f9ba41e50f34233,
title = "Superradiance in the Kerr-de Sitter space-time",
abstract = "A Kerr-de Sitter black hole loses energy and angular momentum through both quantum superradiance and thermal emission. Our investigation of the former process indicates that a rapidly rotating black hole spins down faster as we increase Λ, but after spinning down takes longer to evaporate.",
author = "Takashi Tachizawa and Maeda, {Kei ichi}",
note = "Funding Information: We would like to thank Dr. Laurens D. Gunnarsen for his critical reading of our report. This work was supported partially by the Grant-in-Aid for Scientific Research Fund of the Ministry of Education, Science and Culture, nos. 04234211 and 0.4640312.",
year = "1993",
month = jan,
day = "11",
doi = "10.1016/0375-9601(93)90111-C",
language = "English",
volume = "172",
pages = "325--330",
journal = "Physics Letters A",
issn = "0375-9601",
publisher = "Elsevier",
number = "5",
}