Interior solutions of relativistic stars with anisotropic matter in scale-dependent gravity
Interior solutions of relativistic stars with anisotropic matter in scale-dependent gravity
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Berlin/Heidelberg: Springer Berlin Heidelberg
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English
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Berlin/Heidelberg: Springer Berlin Heidelberg
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We obtain well behaved interior solutions describing hydrostatic equilibrium of anisotropic relativistic stars in scale-dependent gravity, where Newton’s constant is allowed to vary with the radial coordinate throughout the star. Assuming (1) a linear equation-of-state in the MIT bag model for quark matter, and (2) a certain profile for the energy...
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Interior solutions of relativistic stars with anisotropic matter in scale-dependent gravity
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TN_cdi_doaj_primary_oai_doaj_org_article_94b8fcf1a40b4547814086097b87ad8b
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_94b8fcf1a40b4547814086097b87ad8b
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ISSN
1434-6044
E-ISSN
1434-6052
DOI
10.1140/epjc/s10052-021-08881-8
