Energy of a stringy charged black hole in the teleparallel gravity


Creative Commons License

Salti M.

ASTROPHYSICS AND SPACE SCIENCE, cilt.306, ss.201-204, 2006 (SCI İndekslerine Giren Dergi) identifier identifier

  • Cilt numarası: 306 Konu: 4
  • Basım Tarihi: 2006
  • Doi Numarası: 10.1007/s10509-006-9208-7
  • Dergi Adı: ASTROPHYSICS AND SPACE SCIENCE
  • Sayfa Sayıları: ss.201-204

Özet

We use the teleparallel geometry analog of the Moller energy-momentum complex to calculate the energy distribution (due to matter plus field including gravity) of a charged black hole solution in heterotic string theory. We find the same energy distribution as obtained by Gad who investigated the same problem by using the Moller energy-momentum complex in general relativity. The total energy depends on the black hole mass M and charge Q. The energy obtained is also independent of the teleparallel dimensionless coupling constant, which means that it is valid not only in the teleparallel equivalent of general relativity, but also in any teleparallel model. Furthermore, our results also sustains (a) the importance of the energy-momentum definitions in the evaluation of the energy distribution of a given spacetime and (b) the viewpoint of Lessner that the Moller energy-momentum complex is a powerful concept of energy and momentum.