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ROTATING RINDLER SPACE TIME WITH CONSTANT ANGULAR VELOCITY

         

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 fiat and has event horizon and infinite red shift surface. We prove that it is a rotating Rindler space time with constant angular velocity.

著录项

  • 来源
    《中国物理:英文版》 |2000年第5期|329-332|共4页
  • 作者

    WANG YONG-CHENG;

  • 作者单位

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

  • 原文格式 PDF
  • 正文语种 chi
  • 中图分类
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