Neutron star cooling in seven of eight transient outbursts from LMXBs is matched by thermonuclear heating leakage via an updated nscool boundary condition without ad hoc shallow heating.
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Bayesian analysis of generic hybrid EOS with first-order deconfinement shows mass-gap hybrids require early transition and stiff quark matter, but data favor twins at 1.4 M_sun that exclude them.
citing papers explorer
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On a re-examination of neutron star cooling in transient sources -- No shallow heating required?
Neutron star cooling in seven of eight transient outbursts from LMXBs is matched by thermonuclear heating leakage via an updated nscool boundary condition without ad hoc shallow heating.
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Hybrid stars among mass gap objects are excluded by twin stars at $1.4\,M_\odot$
Bayesian analysis of generic hybrid EOS with first-order deconfinement shows mass-gap hybrids require early transition and stiff quark matter, but data favor twins at 1.4 M_sun that exclude them.