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2009

Nuclear matter to strange matter transition in holographic QCD

Kim, Youngman, Seo, Yunseok, Sin, Sang-Jin

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We construct a simple holographic QCD model to study nuclear matter to strange matter transition.

The interaction of dense medium and hadrons is taken care of by imposing the force balancing condition for stable D4/D6/D6 configuration.
By considering the intermediate and light flavor branes interacting with baryon vertex homogeneously distributed along R^3 space and requesting the energy minimization, we find that there is a well defined transition density as a function of current quark mass.
We also find that as density goes up very high, intermediate (or heavy) and light quarks populate equally as expected from the Pauli principle.

Nuclear matter to strange matter transition in holographic QCD · Around

Built on

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C. G. . Callan, A. Guijosa, K. G. Savvidy and O. Tafjord, Nucl. Phys. B 555
1999
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W. Weise, Hot and dense hadronic matter - selected topics -
2000
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Then

S. Lawley, W. Bentz, and A. W. Thomas, Nucleons, nuclear matter and quark matter: A Unified NJL approach
2005
Later among the works it cites.
K.-Y. Kim, S.-J. Sin and I. Zahed, ”Dense hadronic matter in holographic QCD,” hep-th/0608046; N. Horigome and Y. Tanii, JHEP 0701
2007
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J. Erdmenger, N. Evans, I. Kirsch and E. Threlfall, Mesons in Gauge/Gravity Duals - A Review
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2008
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Y. Seo and S. J. Sin, Baryon Mass in medium with Holographic QCD
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