中国物理B ›› 1997, Vol. 6 ›› Issue (9): 666-670.doi: 10.1088/1004-423X/6/9/003

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SCHWARZSCHILD BLACK HOLE,VACUUM C METRIC WHEN m=0 AND RINDLER METRIC

王永成   

  1. Department of Physics,Beijing Normal University,Beijing 100875,China
  • 收稿日期:1997-02-19 出版日期:1997-09-20 发布日期:1997-09-20
  • 基金资助:
    Project supported by the National Natural Science Foundation of China.

SCHWARZSCHILD BLACK HOLE,VACUUM C METRIC WHEN m=0 AND RINDLER METRIC

WANG YONG-CHENG (王永成)   

  1. Department of Physics,Beijing Normal University,Beijing 100875,China
  • Received:1997-02-19 Online:1997-09-20 Published:1997-09-20
  • Supported by:
    Project supported by the National Natural Science Foundation of China.

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摘要： In this paper,vacuum C-metric when m=0 is derived from the metric of a Schwarzschild black hole if its mass and location approach to infinity in an appropriate way.Furthermore,by using coordinate transformation in which there is no acceleration,vacuum C-metric when m=0 is transformed to Rindler metric.The result shows that an infinitesimal neighborhood of the horizon of an infinite Schwarzschild black hole is a Rindler space-time,and the acceleration in the Rindler space-time can arise from the in finite Schwarzschild black hole.

Abstract: In this paper,vacuum C-metric when m=0 is derived from the metric of a Schwarzschild black hole if its mass and location approach to infinity in an appropriate way.Furthermore,by using coordinate transformation in which there is no acceleration,vacuum C-metric when m=0 is transformed to Rindler metric.The result shows that an infinitesimal neighborhood of the horizon of an infinite Schwarzschild black hole is a Rindler space-time,and the acceleration in the Rindler space-time can arise from the in finite Schwarzschild black hole.

中图分类号:  (Physics of black holes)

  • 04.70.-s
02.40.-k (Geometry, differential geometry, and topology) 04.20.-q (Classical general relativity)