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三维爱因斯坦-标量引力的黑洞解

杨星宇

北京师范大学学报(自然科学版)2018,Vol.54Issue(2):175-178,4.
北京师范大学学报(自然科学版)2018,Vol.54Issue(2):175-178,4.DOI:10.16360/j.cnki.jbnuns.2018.02.005

三维爱因斯坦-标量引力的黑洞解

Black hole solution of three-dimensional Einstein-scalar gravity

杨星宇1

作者信息

  • 1. 北京师范大学物理学系,100875,北京
  • 折叠

摘要

Abstract

Simple three-dimensional Einstein-scalar gravity is constructed in the present work,its black hole solution is found on condition of ()=2aφ(a is a constant). Further analysis reveals some similarities of this black hole to Reissner -Nordstrom black hole, but the mass of this black hole could be negative with α>2e. Further, the Hawking temperature and Bekenstein-Hawking entropy of this black hole satisfy the laws of thermodynamics, and defines the internal energy of this black hole with a well-defined zero temperature limit. A comparison of the metric of this black solution with Reissner -Nordstrom metric reveals that a2 and l/l correspond to the mass and charge of the Reissner -Nordstrom black hole respectively.

关键词

三维时空/引力/标量场/黑洞热力学/RN黑洞

Key words

three-dimensional spacetime/gravity/scalar field/black hole thermodynamics/RN black hole

分类

数理科学

引用本文复制引用

杨星宇..三维爱因斯坦-标量引力的黑洞解[J].北京师范大学学报(自然科学版),2018,54(2):175-178,4.

北京师范大学学报(自然科学版)

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