Quark mass effects on the stability of hybrid stars

M. Buballa, F. Neumann, M. Oertel, I. Shovkovy

Research output: Contribution to journalArticle

46 Scopus citations

Abstract

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.

Original languageEnglish (US)
Pages (from-to)36-43
Number of pages8
JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume595
Issue number1-4
DOIs
StatePublished - Aug 12 2004
Externally publishedYes

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

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