Structure of Relativistic Stars Composed of Incompressible Matter in the Absence of Strict Electroneutrality
The structure of a star composed of locally non-electroneutral incompressible three-component matter is considered within the framework of general relativity. For thermodynamic quantities like the pressure, the solution can be represented as a series in the small parameter , where the first approxim...
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Published in: | Astronomy letters Vol. 47; no. 9; pp. 618 - 627 |
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Main Authors: | , |
Format: | Journal Article |
Language: | English |
Published: |
Moscow
Pleiades Publishing
01-09-2021
Springer Nature B.V |
Subjects: | |
Online Access: | Get full text |
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Summary: | The structure of a star composed of locally non-electroneutral incompressible three-component matter is considered within the framework of general relativity. For thermodynamic quantities like the pressure, the solution can be represented as a series in the small parameter
, where the first approximation is the well-known electroneutral solution. However, the equilibrium equations for the chemical potentials of the matter components, as it turns out, contain finite contributions from non-electroneutrality effects even in the zeroth order. Analytical solutions have been obtained for all of the parameters of the problem under consideration, which are illustrated by numerical examples. |
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ISSN: | 1063-7737 1562-6873 |
DOI: | 10.1134/S106377372109005X |