Do massive neutron stars end as invisible dark energy objects?
A.A. Hujeirat

TL;DR
This paper proposes that massive neutron stars undergo a phase transition into invisible dark energy objects due to a scalar field interaction, potentially explaining the absence of certain stellar remnants and linking to dark matter and dark energy.
Contribution
It introduces a modified TOV equation with a scalar field to model neutron star collapse into dark energy objects, a novel phase transition mechanism at high densities.
Findings
Massive neutron stars likely become invisible dark energy objects.
A phase transition occurs at about three times nuclear density.
Dark energy objects may connect to dark matter and dark energy in cosmology.
Abstract
Astronomical observations reveal a gap in the mass spectrum of relativistic objects: neither black holes nor neutron stars having masses in the range of 2 - 5 have ever been observed. Based on the solution of the TOV equation modified to include a universal scalar field we argue that all moderate and massive neutron stars should end invisible dark energy objects (DEOs). Triggered by the baryonic matter interaction, a phase transition from normal compressible nuclear matter into an incompressible quark-superfluid is shown to occur at roughly times the nuclear density. At the transition front, the scalar field is set to inject energy at the maximum possible rate via a non-local interaction potential This energy creates a global confining bag, inside which a sea of freely moving quarks is formed in line with the asymptotic freedom…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Cosmology and Gravitation Theories · Gamma-ray bursts and supernovae
