eFTC-221001

High Density Stars in Einstein Real Gravity
14 October 2022

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Abstract

Making use of the Yilmaz-like exponential parametrization of General Relativity with the so-called tensor potentials describing the physical gravitational field (Einstein Real Gravity), we re-analyze the theory of spherical general relativistic polytropic fluids as well as the gravitational theory of dense compact objects (dense relativistic fluids) such as white dwarfs, neutron stars, supermassive stars and eternally collapsing objects (ECOs/MECOs). We present a generalization of the Lane-Emden equation in the full context of Einstein Real Gravity and construct an analytical solution in closed form for high density neutron stars. We finally derive the exponential decay law for the ECOs/MECOs mass. Black hole solutions do not exist in Einstein Real Gravity.

Copyright © 2022 Yvan Leblanc. All rights reserved

PACS: 4.60.+n, 11.17.+y, 97.60.Lf

Cite as: Leblanc, Y., "High Density Stars in Einstein Real Gravity", Report no. eFTC-221001 (2022). http://www.efieldtheory.com/abs/?eFTC-221001; doi:10.13140/RG.2.2.18110.36169.