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(2002)
for the STAR collaboration
* Electronic address: kari.eskola, harri.niemi, vesa
I. Arsene, I. Bearden, D. Beavis, S. Bekele, C. Besliu, B. Budick, H. Boggild, C. Chasman, C. Christensen, P. Christiansen, H. Dalsgaard, R. Debbe, J. Gaardhøje, K. Hagel, H. Ito, A. Jipa, E. Johnson, C. Jørgensen, R. Karabowicz, N. Katryńska, E. Kim, T. Larsen, Jeong-Hun Lee, G. Løvhøiden, Z. Majka, A. Marcinek, M. Murray, J. Natowitz, B. Nielsen, C. Nygaard, D. Pal, A. Qviller, F. Rami, C. Ristea, O. Ristea, D. Røhrich, S. Sanders, P. Staszel, T. Tveter, F. Videbæk, R. Wada, Hongyan Yang, Z. Yin, I. Zgură, V. Zhukova (2009)
The BRAHMS CollaborationNuclear Physics, 830
(2000)
Particle Data Group Coll.
(1974)
arXiv:0709.0742 [nucl-th]. [13] F
We determine the decoupling surfaces for the hydrodynamic description of heavy ion collisions at RHIC and LHC by comparing the local hydrodynamic expansion rate with the microscopic pion-pion scattering rate. The pion p T spectra for nuclear collisions at BNL Relativistic Heavy Ion Collider (RHIC) and CERN Large Hadron Collider (LHC) are computed by applying the Cooper-Frye procedure on the dynamical-decoupling surfaces and compared with those obtained from the constant-temperature freeze-out surfaces. Comparison with RHIC data shows that the system indeed decouples when the expansion rate becomes comparable with the pion scattering rate. The dynamical decoupling based on the rates comparison also suggests that the effective decoupling temperature in central heavy ion collisions remains practically unchanged from RHIC to LHC.
Physical Review C – American Physical Society (APS)
Published: Apr 1, 2008
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