The RM31 project started in 2005-2006, following its precedessor FI31 which started in 2002. The research scope is wide, the main focus being on relativistic heavy ion physics and related theoretical problems as well as on QCD at finite temperature and density. There is an ongoing collaboration between Firenze (F. Becattini, L. Del Zanna, G. Inghirami), Ferrara (A. Drago, V. Rolando) and Torino (A. De Pace, A. Beraudo) aimed at providing the italian community working on heavy ion physics with a numerical hydrodynamical code in 3+1 dimensions endowed with dissipative corrections (ECHO-QGP project, see web page http://www.arcetri.astro.it/~gabriele/echo/) This is an important tool for the analysis of the data collected by LHC experiments; for this special purpose, we are taking advantage of the support of PRIN2009 project (involving Firenze, Catania, Torino).
Iniziativa Specifica dell'Istituto Nazionale di Fisica Nucleare denominata RM31
DRAGO, Alessandro
2012
Abstract
The RM31 project started in 2005-2006, following its precedessor FI31 which started in 2002. The research scope is wide, the main focus being on relativistic heavy ion physics and related theoretical problems as well as on QCD at finite temperature and density. There is an ongoing collaboration between Firenze (F. Becattini, L. Del Zanna, G. Inghirami), Ferrara (A. Drago, V. Rolando) and Torino (A. De Pace, A. Beraudo) aimed at providing the italian community working on heavy ion physics with a numerical hydrodynamical code in 3+1 dimensions endowed with dissipative corrections (ECHO-QGP project, see web page http://www.arcetri.astro.it/~gabriele/echo/) This is an important tool for the analysis of the data collected by LHC experiments; for this special purpose, we are taking advantage of the support of PRIN2009 project (involving Firenze, Catania, Torino).I documenti in SFERA sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
