Charged Einstein-aether black holes and Smarr formula
Chikun DingDepartment of Information Science and Technology, Hunan University of Humanities, Science and Technology, Loudi, Hunan 417000, People’s Republic of ChinaAnzhong WangDepartamento de Física Teórica, Instituto de Física, The State University of Rio de Janeiro, 20550-900 Rio de Janeiro, BrazilXinwen WangGCAP-CASPER, Physics Department, Baylor University, Waco, Texas 76798-7316, USA
2015en
ABI
Annotatsiya
In the framework of the Einstein-Maxwell-aether theory, we present two new classes of exact charged black hole solutions, which are asymptotically flat and possess the universal as well as Killing horizons. We also construct the Smarr formulas and calculate the temperatures of the horizons, using the Smarr mass-area relation. We find that, in contrast to the neutral case, a temperature obtained this way is not proportional to its surface gravity at either of the two types of horizons. Einstein-Maxwell-aether black holes with the cosmological constant and their topological cousins are also presented.
Hali tarjima qilinmagan
Identifikatorlar
Iqtiboslar va manbalar
7 ta iqtibos0 ta foydalanilgan manba