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Local Thermal Equilibrium of Strange Hadrons at CBM Energies Somnath De Post-doctorate Fellow Institute of Physics, Bhubaneswar Collaborators: Sudipan De Universidade de São Paulo, Brazil Subhasish Chattopadhyay Variable Energy Cyclotron Centre, Kolkata, India The Compressed Baryonic Matter (CBM) experiment at FAIR / GSI Aim: To explore the QCD phase diagram at high baryonic density and moderate temperature, which is complementary to the heavy ion studies performed at RHIC and LHC experiment. The experiment is being designed to collide stable (and exotic) nuclei at fixed target mode with energies 5-45 GeV/ nucleon and designed reaction rate 107 / sec. It is expected rare probes like; Charmed Mesons (D, C), Multi-strange Hyperons , Dileptons (decaying from vector mesons) are copiously produced even at such low energies due to high beam luminosity. Our goal in the present study is to investigate the time scale for local thermal equilibriation of the matter created in such collisions; specially the newly breed strange particles . Brief tour to UrQMD model The Ultra Relativistic Quantum Molecular Dynamics (UrQMD) is a N-body transport model extensively used for describing heavy ion collisions of c.m. energy ranging from a few GeV/ nucleon to a few TeV/ nucleon. It includes 55 baryon species (up to mass 2.25 GeV) and 32 meson species (up to mass 1.9 GeV) and their isospin projected states and corresponding anti-particles. For Elab 4 GeV/ nucleon, the hadron-hadron collisions are performed stochastically in the spirit of Cascade model. The total cross-sections are fitted through experimental p-p or p- scattering wherever possible. Particles are generated in UrQMD via inelastic collisions and decay of resonances at lower energies and string fragmentation at higher energies. We are using UrQMD-3.3p2 (without hybrid mode) model to simulate most central Au+Au collisions (b=2fm) at laboratory energies 10, 20, 30, 40 GeV/ nucleon. Choice of volume in phase space: We have considered a cell (222 fm3 ) centered around the origin in c.m. frame of Au+Au system. There is no collective flow by symmetry. In addition, we are only interested in the rapidity window |ycm |< 1.0. vcm -vcm We have studied time evolution of Net particle density, Longitudinal-toTransverse Pressure ratio, Slope parameter of the energy spectra for Nonstrange baryon, Strange baryon and Kaon. The above physical quantities are statistically averaged over 60K events for each time step. Evolution of particle densities: Earlier studies for Au+Au collisions at AGS energies (Bravina et al., PLB, 434 (1998) ) has found the thermal equilibrium of hadronic matter for t 10 fm/c. Considering an ideal gas of relativistic particles; different components of microscopic pressure of hadrons are calculated in UrQMD as: P{ x, y , z} i PL Pz 2 i{ x , y , z } p 3V ( p m ) 2 i 2 i 1 2 1 PT ( Px Py ) 2 Thermal equilibrium is established when microscopic pressure is nearly isotropic inside the cell. Time evolution of PL / PT : We have parameterized the particle momentum spectra inside the cell as: dN E 3 C (1 (q 1) E / T ) d p 1 q 1 Tsallis distribution Slope parameter (Tslope ) : T + (q-1) E In the asymptotic limit (E 0); Tslope corresponds to M.B. temperature of the system We have studied the time evolution of Tslope (at E = 0.1 GeV) for Lamda and Proton at four collision energies. Time dependence of av. number of collisions: P+N + + + 0 Summary and Outlook: We have studied the density evolution, local pressure isotropization and local thermalization of strange hadrons for most central Au-Au collisions at CBM energies. We find the density of particles becomes maximum during the nuclear passage time at their rest frame, as expected. Total strangeness content of the created matter is found to be dominated by baryons for all energies. From the analysis of longitudinal-to-transverse pressure anisotropy, we conclude that Baryons (strange and non-strange ) achieve thermal equilibrium for t > 9 fm/c at 10A GeV and for t > 6fm/c at 40A GeV collision energies. An alternative analysis of time evolution of slope parameter of energy spectra of Baryons supports the earlier conclusion. A comparison of thermodynamic quantities with the statistical model is under way. Acknowledgement: We thank Grid Kolkata Tier-2 Center for providing computing resources. Proton Lamda Bravina et al., PLB 434 (1998) reported T= 128 MeV at 13 fm/c