preprint · arXiv (Cornell University) · 2012
Charged Ball Static Star Model
А. М. Baranov, Zakhar V. Vlasov
Cited by 0Open access
Abstract
Within the framework of General Relativity a model approach to a description of spherical gravitating static fluid balls with an electric charge is considered. The metric interval is written in Bondi's radiation coordinates. The total energy-momentum tensor as a direct sum of the perfect Pascal fluid energy-momentum tensor and the energy-momentum tensor of an electromagnetic field is chosen. The exact solution of the Einstein-Maxwell equations as an extension of similar solution with parabolic distribution of mass density is found.
Cite this paper
Baranov, А. М., & Vlasov, Z. V. (2012). Charged Ball Static Star Model. arXiv (Cornell University). https://doi.org/10.48550/arxiv.1201.4673
Baranov, А. М., and Zakhar V. Vlasov. “Charged Ball Static Star Model.” arXiv (Cornell University), 2012, https://doi.org/10.48550/arxiv.1201.4673.
Baranov, А. М., and Zakhar V. Vlasov. 2012. “Charged Ball Static Star Model.” arXiv (Cornell University). https://doi.org/10.48550/arxiv.1201.4673.
Baranov, А.М. and Vlasov, Z.V. (2012) ‘Charged Ball Static Star Model’, arXiv (Cornell University). Available at: https://doi.org/10.48550/arxiv.1201.4673.
@misc{baranov2012charged,
title = {{Charged Ball Static Star Model}},
author = {Baranov, А. М. and Vlasov, Zakhar V.},
journal = {arXiv (Cornell University)},
year = {2012},
doi = {10.48550/arxiv.1201.4673}
}Made from the index record. Check names, capitalisation and page numbers against the paper. Need another style? AI for Research has over 10,000.