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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

Total Cross Section Color Exchange String Model Classical String String Action 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. [1]
    Proc. of “Quark Matter 1991”, Gatlinburg, USA, Nov. 1991, Nucl. Phys. A544 (1992)Google Scholar
  2. [2]
    K. Werner, Phys. Rep. 232 (1993) 87ADSCrossRefGoogle Scholar
  3. [3]
    A. Capella, U. Sukhatme, Chung-I Tan and J. Tran Thanh Van, preprint LPTHE 92–38, to appear in Physics ReportsGoogle Scholar
  4. [4]
    H. J. Möhring, A. Capella, J. Ranft, J. Tran Thanh Van, C. Merino, Nucl. Phys. A525 (1991) 493cADSGoogle Scholar
  5. [5]
    A. Kaidalov, Nucl. Phys. A525 (1991)39cADSGoogle Scholar
  6. V. D. Toneev, A. S. Amelin and K. K. Gudima preprint GSI-89–52, 1989Google Scholar
  7. [7]
    B. Andersen, G. Gustafson and B. Nielsson-Almqvist, Nucl. Phys. B281 (1987) 289ADSCrossRefGoogle Scholar
  8. [8]
    H. Sorge, H. Stöcker and W. Greiner, Nucl. Phys. A498 (1989) 567cADSGoogle Scholar
  9. [9]
    Y. Nambu, Proc. Intl. Conf. on Symmetries and Quark Models, Wayne State Univ., 1969Google Scholar
  10. [10]
    J. Scherk, Rev. Mod. Phys. 47 (1975) 123MathSciNetADSCrossRefGoogle Scholar
  11. [11]
    C. Rebbi, Phys. Rep. 12 (1974) 1MathSciNetADSCrossRefGoogle Scholar
  12. [12]
    X. Artru and G. Mennessier, Nucl. Phys. B70 (1974) 93ADSCrossRefGoogle Scholar
  13. [13]
    X. Artru, Phys. Rep. 97 (1983) 147ADSCrossRefGoogle Scholar
  14. [14]
    D. Gottschalk and D.A. Morris, Nucl. Phys. B288 (1987) 729ADSCrossRefGoogle Scholar
  15. [15]
    K. Werner and P. Koch, Z. Phys. C47 (1990) 215, preprint CERN-TH-5575/89Google Scholar
  16. [16]
    R.D. Field and R.P. Feynman, Nucl. Phys. B136 (1978) 1ADSCrossRefGoogle Scholar
  17. [17]
    B. Andersson, G. Gustafson, G. Ingelman and T. Sjöstrand, Phys. Rep. 97 (1983) 31ADSCrossRefGoogle Scholar
  18. [18]
    V. N. Gribov, Sov. Phys. JETP 26 (1968) 414ADSGoogle Scholar
  19. [19]
    K. A. Ter-Martirosyan, Nucl. Phys. B36 (1972) 566ADSCrossRefGoogle Scholar
  20. [20]
    V. A. Abramovskii, V. N. Gribov, O. V. Kancheli, Sov. J. Nucl. Phys. 18 (1974) 308Google Scholar
  21. [21]
    M. Ciafaloni, G. Marchesini, G. Veneziano, Nucl. Phys. B98 (1975) 472, 493ADSCrossRefGoogle Scholar

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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