中国物理B ›› 2012, Vol. 21 ›› Issue (6): 60401-060401.doi: 10.1088/1674-1056/21/6/060401

• GENERAL • 上一篇    下一篇

Gravitational collapse with standard and dark energy in the teleparallel equivalent of general relativity

Gamal G. L. Nasheda b c   

  1. a. Mathematics Department, Faculty of Science, King Faisal University, P. O. Box 380 Al-Ahsaa 31982,the Kingdom of Saudi Arabia;
    b. Mathematics Department, Faculty of Science, Ain Shams University, Cairo, 11566, Egypt;
    c. Center for Theoretical Physics, British University of Egypt, Sherouk City 11837, P. O. Box 43, Egypt
  • 收稿日期:2011-11-19 修回日期:2012-01-06 出版日期:2012-05-01 发布日期:2012-05-01

Gravitational collapse with standard and dark energy in the teleparallel equivalent of general relativity

Gamal G. L. Nasheda)b)c)†   

  1. a. Mathematics Department, Faculty of Science, King Faisal University, P. O. Box 380 Al-Ahsaa 31982,the Kingdom of Saudi Arabia;
    b. Mathematics Department, Faculty of Science, Ain Shams University, Cairo, 11566, Egypt;
    c. Center for Theoretical Physics, British University of Egypt, Sherouk City 11837, P. O. Box 43, Egypt
  • Received:2011-11-19 Revised:2012-01-06 Online:2012-05-01 Published:2012-05-01
  • Contact: Gamal G. L. Nashed E-mail:nashed@bue.edu.eg

摘要: A perfect fluid with self-similarity of the second kind is studied within the framework of the teleparallel equivalent of general relativity (TEGR). A spacetime which is not asymptotically flat is derived. The energy conditions of this spacetime are studied. It is shown that after some time the strong energy condition is not enough to satisfy showing a transition from standard matter to dark energy. The singularities of this solution are discussed.

关键词: perfect fluid with self-similarity of second kind, teleparallel equivalent of general relativity, asymptotically nonflat spacetime, energy conditions

Abstract: A perfect fluid with self-similarity of the second kind is studied within the framework of the teleparallel equivalent of general relativity (TEGR). A spacetime which is not asymptotically flat is derived. The energy conditions of this spacetime are studied. It is shown that after some time the strong energy condition is not enough to satisfy showing a transition from standard matter to dark energy. The singularities of this solution are discussed.

Key words: perfect fluid with self-similarity of second kind, teleparallel equivalent of general relativity, asymptotically nonflat spacetime, energy conditions

中图分类号:  (Exact solutions)

  • 04.20.Jb
04.50.Kd (Modified theories of gravity) 04.30.-w (Gravitational waves)