Correlations in hot and dense quark matter

H. J. Weber (Virginia U.); Inst. Tech. Aeronautics); M. Beyer (Rostock U); S. Mattiello; T. Frederico (Sao Paulo

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Correlations in hot and dense quark matter

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arxiv hep-ph/0110368 v1 pith:SSQENQT3 submitted 2001-10-29 hep-ph

Correlations in hot and dense quark matter

S. Mattiello , M. Beyer (Rostock U) , T. Frederico (Sao Paulo , Inst. Tech. Aeronautics) , H. J. Weber (Virginia U.) This is my paper

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We present a relativistic three-body equation to investigate three-quark clusters in hot and dense quark matter. To derive such an equation we use the Dyson equation approach. The equation systematically includes the Pauli blocking factors as well as the self energy corrections of quarks. Special relativity is realized through the light front form. Presently we use a zero-range force and investigate the Mott transition.

Correlations in hot and dense quark matter

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