Abstract
We compute the energy and momentum of a regular black hole of type defined by Mars, Martin-Prats, and Senovilla using the Einstein and Papapetrou definitions for energy-momentum density. Some other definitions of energy-momentum density are shown to give mutually contradictory and less reasonable results. Results support the Cooperstock hypothesis.
| Original language | English |
|---|---|
| Pages (from-to) | 1607-1619 |
| Number of pages | 13 |
| Journal | International Journal of Modern Physics D |
| Volume | 14 |
| Issue number | 9 |
| DOIs | |
| Publication status | Published - Sept 2005 |
Bibliographical note
16 pages, 3 figures, LaTex2e; made minor corrections (in content and in references) at the behest of two anonymous referees. Paper to appear in IJMPDKeywords
- energy-momentum complex
- regular black hole
- general relativity
- Einstein
- Papapetrou
- Landau-Lifshitz
- moller
- cooperstock hypothesis
- CYLINDRICAL GRAVITATIONAL-WAVES
- GENERAL-RELATIVITY
- MAGNETIC UNIVERSE
- ANGULAR-MOMENTUM
- MOLLER ENERGY
- SPACE-TIME
- CONSERVATION
- MASS
- SYSTEM