Neutrinos in dense quark matter and cooling of compact stars
D. Blaschke (Wroclaw, Dubna), J. Berdermann (Zeuthen)
TL;DR
This paper explores how observational data on neutrino cooling can limit the types of quark matter phases that exist inside compact stars, impacting our understanding of their internal composition.
Contribution
It introduces a framework linking neutrino cooling observations to constraints on quark matter phases in compact stars.
Findings
Neutrino cooling observations restrict quark matter phase models.
Certain quark matter phases are incompatible with observed cooling rates.
The study provides criteria for viable quark matter phases in stars.
Abstract
We discuss that observational constraints on neutrino cooling processes may restrict the spectrum of quark matter phases admissible for compact star interiors.
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