The String Model of Nuclear Scattering: Theoretical Concepts

  • K. Werner
Part of the NATO ASI Series book series (NSSB, volume 333)

Abstract

The early universe was probably a hot and dense “fireball” of quarks and gluons, before, due to expansion and cooling, hadrons emerged. Presently, there are considerable efforts to create such a “quark-gluon plasma” (QGP) in nucleus-nucleus scattering at ultrarelativistic energies (≫1 GeV per nucleon)1.

Keywords

Covariance Convolution Summing Salami 

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Copyright information

© Springer Science+Business Media New York 1994

Authors and Affiliations

  • K. Werner
    • 1
  1. 1.Institut für Theoretische PhysikUniversität HeidelbergHeidelbergGermany

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