001552198 001__ 1552198
001552198 003__ SzGeCERN
001552198 005__ 20151106233117.0
001552198 0247_ $$2DOI$$a10.1140/epjc/s10052-013-2524-5
001552198 0248_ $$aoai:cds.cern.ch:1552198$$pcerncds:CERN
001552198 035__ $$9arXiv$$aoai:arXiv.org:1305.7052$$d2013-08-29$$h2013-08-29T02:00:20Z$$marXiv$$ttrue$$uhttp://export.arxiv.org/oai2
001552198 035__ $$9Inspire$$a1236252
001552198 037__ $$aarXiv:1305.7052
001552198 041__ $$aeng
001552198 100__ $$aDel Zanna, L$$uFlorence U.$$uINFN, Florence$$uArcetri Observ.
001552198 245__ $$aRelativistic viscous hydrodynamics for heavy-ion collisions with ECHO-QGP
001552198 269__ $$c30 May 2013
001552198 260__ $$c2013
001552198 300__ $$a22 p
001552198 500__ $$aComments: 22 pages, 23 figures
001552198 520__ $$aWe present ECHO-QGP, a numerical code for $(3+1)$-dimensional relativistic viscous hydrodynamics designed for the modeling of the space-time evolution of the matter created in high energy nuclear collisions. The code has been built on top of the \emph{Eulerian Conservative High-Order} astrophysical code for general relativistic magneto-hydrodynamics [\emph{Del Zanna et al., Astron. Astrophys. 473, 11, 2007}] and here it has been upgraded to handle the physics of the Quark-Gluon Plasma. ECHO-QGP features second-order treatment of causal relativistic viscosity effects in both Minkowskian or Bjorken coordinates; partial or complete chemical equilibrium of hadronic species before kinetic freeze-out; initial conditions based on the optical Glauber model, including a Monte-Carlo routine for event-by-event fluctuating initial conditions; a freeze-out procedure based on the Cooper-Frye prescription. The code is extensively validated against several test problems and results always appear accurate, as guaranteed by the combination of the conservative (shock-capturing) approach and the high-order methods employed. ECHO-QGP can be extended to include evolution of the electromagnetic fields coupled to the plasma.
001552198 595__ $$aLANL EDS
001552198 65017 $$2arXiv$$aNuclear Physics - Theory
001552198 690C_ $$aARTICLE
001552198 690C_ $$aCERN
001552198 695__ $$9LANL EDS$$anucl-th
001552198 700__ $$aChandra, V$$uINFN, Florence
001552198 700__ $$aInghirami, G$$uINFN, Florence$$uFlorence U.
001552198 700__ $$aRolando, V$$uFerrara U.$$uINFN, Ferrara
001552198 700__ $$aBeraudo, A$$uCERN
001552198 700__ $$aDe Pace, A$$uINFN, Turin
001552198 700__ $$aPagliara, G$$uFerrara U.$$uINFN, Ferrara
001552198 700__ $$aDrago, A$$uFerrara U.$$uINFN, Ferrara
001552198 700__ $$aBecattini, F$$uFlorence U.$$uINFN, Florence$$uFrankfurt U., FIAS
001552198 773__ $$c73$$oEur. Phys. J. C (2013) 73: 2524$$pEur. Phys. J. C$$y2013
001552198 8564_ $$uhttp://arxiv.org/pdf/1305.7052.pdf$$yPreprint
001552198 916__ $$sn$$w201321
001552198 960__ $$a13
001552198 980__ $$aARTICLE