Revisiting the Rhoades-Ruffini bound

Fuente: arXiv
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Main Authors: Blaschke, David, Wojcik, Adrian
Format: Preprint
Published: 2026
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author Blaschke, David
Wojcik, Adrian
author_facet Blaschke, David
Wojcik, Adrian
contents We revisit the derivation of the Rhoades-Ruffini bound on the upper limit for the maximum mass of neutron stars and find that the assumption made there for the onset of an ultimately stiff phase of high-density matter is not stringent. Relaxing this assumption and allowing for an onset of stiff non-nucleonic matter under neutron star constraints at the saturation density or below boost the upper limit of the theoretically possible maximum mass to $4~M_\odot$ or higher, in the mass-gap region between neutron stars and stellar-mass black holes. We provide a fit formula for the dependence of this upper limit on the speed of sound and the onset density of the deconfinement transition.
format Preprint
id arxiv_https___arxiv_org_abs_2604_03204
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Revisiting the Rhoades-Ruffini bound
Blaschke, David
Wojcik, Adrian
Nuclear Theory
High Energy Astrophysical Phenomena
We revisit the derivation of the Rhoades-Ruffini bound on the upper limit for the maximum mass of neutron stars and find that the assumption made there for the onset of an ultimately stiff phase of high-density matter is not stringent. Relaxing this assumption and allowing for an onset of stiff non-nucleonic matter under neutron star constraints at the saturation density or below boost the upper limit of the theoretically possible maximum mass to $4~M_\odot$ or higher, in the mass-gap region between neutron stars and stellar-mass black holes. We provide a fit formula for the dependence of this upper limit on the speed of sound and the onset density of the deconfinement transition.
title Revisiting the Rhoades-Ruffini bound
topic Nuclear Theory
High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2604.03204