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Correlations in Hot and Dense Quark Matter

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Abstract.

 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.

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Authors and Affiliations

  1.  Fachbereich Physik, Universität Rostock, D-18051 Rostock, Germany, , , , , , DE

    S. Mattiello & M. Beyer

  2.  Dep. de Física, Instituto Tecnológico de Aeronáutica, Centro Técnico Aeroespacial, 12.228-900 São José dos Campos, São Paulo, Brazil, , , , , , BR

    T. Frederico

  3.  Dept. of Physics, University of Virginia, Charlottesville, VA 22904, USA, , , , , , US

    H. J. Weber

Authors
  1. S. Mattiello
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  2. M. Beyer
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  3. T. Frederico
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  4. H. J. Weber
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Received October 29, 2001; accepted for publication November 12, 2001

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Mattiello, S., Beyer, M., Frederico, T. et al. Correlations in Hot and Dense Quark Matter. Few-Body Systems 31, 159–164 (2002). https://doi.org/10.1007/s006010200015

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  • DOI: https://doi.org/10.1007/s006010200015

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