Quasi-Local Masses of Rotating Space-Times

• 来源期刊: 理论物理通讯（英文版）
• 年，卷（期）: 2017,（9）
• 页码范围: 342-346
• 页数: 5页
• 语种: 英文
• DOI: 10.1088/0253-6102/68/3/342

摘要

We derive the Misner-Sharp-like masses of the Reissner-Nordstr（o）m black hole and the Einstein-Maxwell Dilaton-Axion black hole by using the modified first law of thermodynamics.Their surface tensions are investigated.For the Reissner-Nordstr(o)m black hole,the outer horizon radius is treated as a variable and the effective temperature is introduced.For the Einstein-Maxwell-Dilaton-Axion black hole,the outer horizon radius,the angular momentum unit mass and the parameter b are seen as three independent variables,and the mass,the horizon area and the angular momentum are functions of them.