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The Astrophysical journal, 2024-05, Vol.966 (1), p.3
2024

Details

Autor(en) / Beteiligte
Titel
Two-flavor Color Superconducting Quark Stars May Not Exist
Ist Teil von
  • The Astrophysical journal, 2024-05, Vol.966 (1), p.3
Ort / Verlag
Philadelphia: IOP Publishing
Erscheinungsjahr
2024
Link zum Volltext
Quelle
EZB Free E-Journals
Beschreibungen/Notizen
  • Large uncertainties in the determinations of the equation of state of dense stellar matter allow for the intriguing possibility that the bulk quark matter in beta equilibrium might be the true ground state of the matter at zero pressure. Also, quarks will form Cooper pairs very readily since the dominant interaction between quarks is attractive in some channels. As a result, quark matter will generically exhibit color superconductivity, with the favored pairing pattern at intermediately high densities being two-flavor pairing. In the light of several possible candidates for such self-bound quark stars, including the very low-mass central compact object in supernova remnant HESS J1731-347 reported recently, we carry out a one-field theoretic model, the Nambu–Jona–Lasinio model, to investigate the stability of the beta-stable two-flavor color superconducting (2SC) phase of quark matter, but find no physically allowed parameter space for the existence of 2SC quark stars.
Sprache
Englisch
Identifikatoren
ISSN: 0004-637X
eISSN: 1538-4357
DOI: 10.3847/1538-4357/ad354f
Titel-ID: cdi_doaj_primary_oai_doaj_org_article_6559592274ec4b11a63c9415f3218552

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