ROTATING RINDLER SPACE TIME WITH CONSTANT ANGULAR VELOCITY

doi:10.1088/1009-1963/9/5/003

中国物理B ›› 2000, Vol. 9 ›› Issue (5): 329-332.doi: 10.1088/1009-1963/9/5/003

ROTATING RINDLER SPACE TIME WITH CONSTANT ANGULAR VELOCITY

王永成

Department of Physics, Beijing Normal University, Beijing 100875, China

收稿日期:1999-10-27 出版日期:2005-06-12 发布日期:2005-06-12
基金资助:
Project supported by the National Natural Science Foundation of China (Grant No. 19773003).

ROTATING RINDLER SPACE TIME WITH CONSTANT ANGULAR VELOCITY

Wang Yong-cheng (王永成)

Department of Physics, Beijing Normal University, Beijing 100875, China

Received:1999-10-27 Online:2005-06-12 Published:2005-06-12
Supported by:
Project supported by the National Natural Science Foundation of China (Grant No. 19773003).

摘要/Abstract

摘要： A new space time metric is derived from Kerr metric if its mass and location approach to infinite in an appropriate way. The new space-time is an infinitesimal neighborhood nearby one of the two horizon poles of an infinite Kerr black hole. In other words, it is the second order infinitesimal neighborhood nearby one of the two horizon poles of a Kerr black hole. It is flat and has event horizon and infinite red shift surface. We prove that it is a rotating Rindler space time with constant angular velocity.

中图分类号: (Spacetime topology, causal structure, spinor structure)

04.20.Gz

04.70.-s (Physics of black holes)

王永成. ROTATING RINDLER SPACE TIME WITH CONSTANT ANGULAR VELOCITY[J]. 中国物理B, 2000, 9(5): 329-332.

Wang Yong-cheng (王永成). ROTATING RINDLER SPACE TIME WITH CONSTANT ANGULAR VELOCITY[J]. Chinese Physics, 2000, 9(5): 329-332.

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ROTATING RINDLER SPACE TIME WITH CONSTANT ANGULAR VELOCITY

ROTATING RINDLER SPACE TIME WITH CONSTANT ANGULAR VELOCITY

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