Quark mass effects on the stability of hybrid stars

  • We perform a study of the possible existence of hybrid stars with color superconducting quark cores using a specific hadronic model in a combination with an NJL-type quark model. It is shown that the constituent mass of the non-strange quarks in vacuum is a very important parameter that controls the beginning of the hadron–quark phase transition. At relatively small values of the mass, the first quark phase that appears is the two-flavor color superconducting (2SC) phase which, at larger densities, is replaced by the color-flavor locked (CFL) phase. At large values of the mass, on the other hand, the phase transition goes from the hadronic phase directly into the CFL phase avoiding the 2SC phase. It appears, however, that the only stable hybrid stars obtained are those with the 2SC quark cores.

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Metadaten
Author:Michael BuballaORCiDGND, Frederik Neumann, Micaela OertelORCiDGND, Ihor Andrijovyč ŠovkovyjORCiDGND
URN:urn:nbn:de:hebis:30:3-761571
DOI:https://doi.org/10.1016/j.physletb.2004.05.064
ISSN:0370-2693
Parent Title (English):Physics Letters B
Publisher:Elsevier
Place of publication:Amsterdam
Document Type:Article
Language:English
Date of Publication (online):2004/06/22
Date of first Publication:2004/06/22
Publishing Institution:Universitätsbibliothek Johann Christian Senckenberg
Release Date:2023/10/19
Volume:595
Issue:1
Page Number:8
First Page:36
Last Page:43
Institutes:Physik
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 53 Physik / 530 Physik
Sammlungen:Universitätspublikationen
Licence (German):License LogoCreative Commons - Namensnennung 3.0