Abstract
Reissner–Nordstrom de Sitter spacetime with photon rest mass is studied. An iteration method is used to get the metric of this spacetime. In the case of μ → 0, the solution will return to the common Reissner–Nordstrom de Sitter spacetime.
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References
Bennett, C. L., Halpern, M., Hinshaw, G. et al. (2003). [astro-ph/0302207].
Carmeli, M. (2001) [astro-ph/0111259].
Ghosh, K. (2004) [gr-qc/0212060].
Goldhaber, A. S. and Nieto, M. M. (1971). Reviews of Modern Physics 43, 277.
Lakes, R. (1998). Physical Review Letters 80, 1826.
Luo, J., Tu, L. C., Hu, Z. K., and Luan, E. J. (2003). Physical Review Letters 90, 081801.
Obukov, Y. and Vlachynsky, E. J. (2000). Preprint gr-qc/0004081 28 April 2000.
Padmanahan, T. (2003). Physics Reports 380, 235–320.
Proca, A. (1936). Le Journal de Physique et le Radium 7, 347.
Kramer, D., Stephani, H., Herlt, E., and MacCallum, M. (1980). Exact Solutions of Einstein’s Field Equations, Cambridge University Press, Cambridge.
Salgado, M. (2003) [gr-qc/0304010].
Toussaint, M. (1999). Preprint gr-qc/991042, 12 October 1999.
Vuille, C., Ipser, J., and Gallag, J. (2002). General Relativity and Gravitation 34(5).
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Shi, C., Liu, Z. Proca Effect in Reissner–Nordstrom de Sitter Metric. Int J Theor Phys 44, 303–308 (2005). https://doi.org/10.1007/s10773-005-2992-y
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DOI: https://doi.org/10.1007/s10773-005-2992-y