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We study the properties of two-flavor quark matter in the Dyson-Schwinger model and investigate the possible consequences for hybrid neutron stars, with particular regard to the two-solar-mass limit. We find… Click to show full abstract
We study the properties of two-flavor quark matter in the Dyson-Schwinger model and investigate the possible consequences for hybrid neutron stars, with particular regard to the two-solar-mass limit. We find that with some extreme values of the model parameters, the mass fraction of two-flavor quark matter in heavy neutron stars can be as high as 30 percent and the possible energy release during the conversion from nucleonic neutron stars to hybrid stars can reach $10^{52}\;$erg.
Keywords:
two flavor;
dyson schwinger;
flavor hybrid;
model;
hybrid stars;
neutron stars
Journal Title: Chinese Physics C
Year Published: 2017
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Journal Title: Chinese Physics C
Year Published: 2017
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!