Diffusion and local deconfinement in relativistic systems
The evolution of net-proton rapidity spectra with sNN is heavy relativistic systems is proposed as an indicator for local equilibration, longitudinal expansion, and deconfinement. Bell-shaped distributions in central collisions at AGS energies and double-humped nonequilibrium spectra at SPS ishow su...
Gespeichert in:
| 1. Verfasser: | |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
25 March 2005
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| In: |
Nuclear physics. A, Nuclear and hadronic physics
Year: 2005, Jahrgang: 752, Pages: 484-488 |
| ISSN: | 1873-1554 |
| DOI: | 10.1016/j.nuclphysa.2005.02.053 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1016/j.nuclphysa.2005.02.053 Verlag, Volltext: http://www.sciencedirect.com/science/article/pii/S0375947405002046 
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| Verfasserangaben: | Georg Wolschin |
MARC
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| 520 | |a The evolution of net-proton rapidity spectra with sNN is heavy relativistic systems is proposed as an indicator for local equilibration, longitudinal expansion, and deconfinement. Bell-shaped distributions in central collisions at AGS energies and double-humped nonequilibrium spectra at SPS ishow substantial collective expansion. The broad midrapidity valley appearing at RHIC indicates longitudinal collective expansion of a locally equilibrated subsystem. In central Au-Au collisions at sNN=200 GeV, fast local equilibration which is most likely due to deconfinement is estimated in a Relativistic Diffusion Model to occur for 14 per cent of the incoming baryons. | ||
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