New Mathematical Models of Compact Stars with Charge Distributions
International Journal of Systems Science and Applied Mathematics
Volume 2, Issue 5, September 2017, Pages: 93-98
Received: Aug. 23, 2017; Accepted: Sep. 19, 2017; Published: Oct. 23, 2017
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Manuel Malaver, Department of Basic Sciences, Maritime University of the Caribbean, Catia la Mar, Venezuela
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In this paper, have been found new class of solutions to the Einstein-Maxwell system for charged anisotropic matter which are relevant in the description of highly compact stellar objects. The equation of state is barotropic with a linear relation between the radial pressure and the energy density and we have considered a prescribed form for the gravitational potential Z. Variables as the energy density, radial pressure and the metric coefficients are written in terms of elementary and polynomial functions. The obtained models not admit singularities in the matter and the charge density.
Einstein-Maxwell System, Charged Anisotropic Matter, Compact Stellar Objects, Energy Density, Metric Coefficients
To cite this article
Manuel Malaver, New Mathematical Models of Compact Stars with Charge Distributions, International Journal of Systems Science and Applied Mathematics. Vol. 2, No. 5, 2017, pp. 93-98. doi: 10.11648/j.ijssam.20170205.13
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