TL;DR
This paper investigates how Gravity's Rainbow, a Planck-scale modification of space-time, affects the equilibrium and possible existence of different types of compact stars like white dwarfs and neutron stars.
Contribution
It introduces a novel analysis of the TOV equation under Gravity's Rainbow, exploring its implications for the structure of compact astrophysical objects.
Findings
Gravity's Rainbow alters the TOV equilibrium configurations.
Potential support for different types of compact stars due to Planck-scale effects.
Insights into quantum gravity effects on astrophysical objects.
Abstract
In recent years, a growing interest on the equilibrium of compact astrophysical objects like white dwarf and neutron stars has been manifested. In particular, various modifications due to Planck scale energy effects have been considered. In this paper we analyze the modification induced by Gravity's Rainbow on the equilibrium configurations described by the Tolman-Oppenheimer-Volkoff (TOV) equation. Our purpose is to explore the possibility that the Rainbow Planck-scale deformation of space-time could support the existence of different compact stars.
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