Hypernuclei and dense matter in RMF model with chiral SU(3) potential

Details Hypernuclei and dense matter in RMF model with chiral SU(3) potential Hypernuclei and dense matter in RMF model with chiral SU(3) potential

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1016..288t&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From

Physics

Hypernuclei, Nuclear Matter, Quark-Gluon Plasma

Scientific paper

We present a RMF model including chiral SU(3) potential which is suggested form strong coupling limit of lattice QCD and we discuss nuclear star in this chiral SU(3) RMF model and show an effect to nuclear star maximum mass by introducing this potential. The calculation results in soft EOS which imcomressibility is as similar as empirical value. However, when we mind an appearance of hyperon, estimated nuclear star maximum mass underestimates the observable data. We suppose we have to investigate re-stiffen mechanism in high baryon density phase.

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