'40 agev' diaporamas de présentation

SPS ????????????? Mean-Field effects at SPS energies @ ???? RCNP, 4 Nov. 2004

SPS ????????????? Mean-Field effects at SPS energies @ ???? RCNP, 4 Nov. 2004. ???? ?? ?? ( M. Isse) ????? ?? ?? ?? ( N. Otuka) IOP ?????? ( P.K. Sahu) Frankfurt U. ?? ? ( Y. Nara) ??? ?? ? ( A. Ohnishi). ???????. ???? ??????(?????) ??????????????????? ????? ???????? JAM

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or little Big Bang

370 views • 28 slides

Results from an Integrated Boltzmann+Hydrodynamics Approach

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Freeze-Out in a Hybrid Model

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or little Big Bang

Equilibration of Matter Near QCD Critical Point Larissa Bravina / Konrad Tywoniuk, University of Oslo. or little Big Bang. Content. Motivation. Why 40 AGeV? Conditions of thermal and chemical equilibrium Statistical model of ideal hadron gas Relaxation to equilibrium in central cell

337 views • 22 slides

Simulation of energy depositions in PSD for 7 Be+ 9 Be reaction

Simulation of energy depositions in PSD for 7 Be+ 9 Be reaction. Problem with SHIELD code. Identification of spectators. Use of Dpmjet model. Energy depositions in PSD from spectators and nonspectators. Discussion on PSD trigger. 1. 158 GeV/c SHIELD model. Energy deposition in PSD for:.

287 views • 19 slides

Nucleus-nucleus collisions at the future facility in Darmstadt -

Nucleus-nucleus collisions at the future facility in Darmstadt - Compressed Baryonic Matter at GSI. Peter Senger. Outline: ? Dense baryonic matter: fundamental physics ? Experimental observables ? Technical challenges and (possible) solutions.

288 views • 17 slides

- Onset of deconfinement

NA60+. Measuring dimuons at different energies in the range 20-160 AGeV and with different collision systems :. - Onset of deconfinement. - Existence (or non existence ) of QCD critical point. - C hiral symmetry restoration.

281 views • 14 slides