Abstract
A detailed description of the temporal evolution of the thermodynamic fields in heavy ion collisions is presented within a hydrodynamic framework. Particular attention is devoted to the evolution of the collective flow fields and their space-time gradients.
Article PDF
Similar content being viewed by others
Avoid common mistakes on your manuscript.
References
Proc. of the 15th and 16th Int. Conf. on Ultrarelativistic Nucleus-Nucleus Collisions, Nucl. Phys.A698 (2002) 1c; ibid. A715 (2003) 1c.
P.F. Kolb and U. Heinz, nucl-ex/0305084.
B. Tomasik and U. Wiedemann, nucl-th/0207074.
P.F. Kolb, J. Sollfrank and U. Heinz, Phys. Rev. C 62 (2000) 054909.
P.F. Kolb, U. Heinz, P. Huovinen, K.J. Eskola and K. Tuominen, Nucl. Phys. A696 (2001) 197.
P.F. Kolb and R. Rapp, Phys. Rev. C 67 (2003) 044903.
E. Schnedermann, J. Sollfrank and U. Heinz, Phys. Rev. C 48 (1993) 2462.
P.F. Kolb et al. Phys. Lett. B500 (2001) 232; P. Huovinen et al., Phys. Lett. B503 (2001) 58; D. Teaney et al., Phys. Rev. Lett. 86 (2001) 4783; T. Hirano, Phys. Rev. C 65 (2001) 011901 (R).
J.-Y. Ollitrault, Phys. Rev. D 46 (1992) 229.
G.E. Brown and E.V. Shuryak, Nucl. Phys. A717 (2003) 322; P.F. Kolb and M. Prakash, Phys. Rev. C 67 (2003) 044902.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Kolb, P.F. Expansion Rates at RHIC. Acta Phys. Hung. A 21, 243–248 (2004). https://doi.org/10.1556/APH.21.2004.2-4.22
Received:
Issue Date:
DOI: https://doi.org/10.1556/APH.21.2004.2-4.22