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2+1 Relativistic hydrodynamics for heavy-ion collisions

2+1 Relativistic hydrodynamics for heavy-ion collisions. Mikołaj Chojnacki IFJ PAN NZ41. Outline. Angular asymmetry in non-central collisions 2+1 Hydrodynamic equations Boundary and initial conditions Results Conclusions. Angular asymmetry in non-central collisions. y. x.

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2+1 Relativistic hydrodynamics for heavy-ion collisions

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  1. 2+1 Relativistic hydrodynamics for heavy-ion collisions Mikołaj Chojnacki IFJ PAN NZ41

  2. Outline • Angular asymmetry in non-central collisions • 2+1 Hydrodynamic equations • Boundary and initial conditions • Results • Conclusions 2+1 Relativistic hydrodynamics for heavy-ion collisions

  3. Angular asymmetry in non-central collisions y x Space asymmetries transform to momentum space asymmetries Indirect proof that particle interactions take place 2+1 Relativistic hydrodynamics for heavy-ion collisions

  4. Equations of relativistic hydrodynamics • Energy and momentum conservation law: • energy-momentum tensor • at midrapidity (y=0) for RHIC energies temperature is the only thermodynamic parameter • thermodynamic relations 2+1 Relativistic hydrodynamics for heavy-ion collisions

  5. y v vR vT  z = 0 r  x Lorentz factor : System geometry Cylindrical coordinates ( r,  ) Boost – invariant symmetry Values of physical quantities at z ≠ 0 may be calculated by Lorentz transformation 2+1 Relativistic hydrodynamics for heavy-ion collisions

  6. Equations in covariant form Non-covariant notation Dyrek + Florkowski, Acta Phys.Polon.B15 (1984) 653 2+1 Relativistic hydrodynamics for heavy-ion collisions

  7. inverse function of Temperature dependent sound velocity cs(T) • Relation between T and s needed to close the set of three equations. TC = 170 [MeV] • Potential Φ Lattice QCD model by Mohanty and Alam Phys. Rev. C68 (2003) 064903 • Potential Φ dependent of T • Temperature T dependent of Φ 2+1 Relativistic hydrodynamics for heavy-ion collisions

  8. where transverse rapidity Semifinal form of 2 + 1 hydrodynamic equations in the transverse direction • auxiliary functions: 2+1 Relativistic hydrodynamics for heavy-ion collisions

  9. Generalization of 1+1 hydrodynamic equations by Baym, Friman, Blaizot, Soyeur, Czyz Nucl. Phys. A407 (1983) 541 2 + 1 hydrodynamic equations reduce to 1+1 case • angular isotropy in initial conditions • potential Φ independent of  2+1 Relativistic hydrodynamics for heavy-ion collisions

  10. Observables as functions of a± and  • solutions • velocity • potential Φ • sound velocity • temperature 2+1 Relativistic hydrodynamics for heavy-ion collisions

  11. Boundary conditions • Single function a to describe a± a±, a,  a(r,,t) a+(r,,t) a-(r,,t) (r,,t) • Function  symmetrically extended to negative values of r (-r,,t) • Equal values at  = 0 and  = 2π r • Automatically fulfilled boundary conditions at r = 0 2+1 Relativistic hydrodynamics for heavy-ion collisions

  12. Initial conditions - Temperature y • Initial temperature is connected with the number of participating nucleons A B b x Teaney,Lauret and Shuryak nucl-th/0110037 • Values of parameters 2+1 Relativistic hydrodynamics for heavy-ion collisions

  13. Initial conditions – velocity field • Isotropic Hubble-like flow • Final form of the a± initial conditions 2+1 Relativistic hydrodynamics for heavy-ion collisions

  14. Results • Impact parameter b and centrality classes • hydrodynamic evolution initial time t0 = 1 [fm] • sound velocity based on Lattice QCD calculations • initial central temperature T0 = 2 TC = 340 [MeV] • initial flow H0 = 0.01 [fm-1] 2+1 Relativistic hydrodynamics for heavy-ion collisions

  15. Centrality class 0 - 20% b = 3.9 [fm] 2+1 Relativistic hydrodynamics for heavy-ion collisions

  16. Centrality class 0 - 20% b = 3.9 [fm] 2+1 Relativistic hydrodynamics for heavy-ion collisions

  17. Centrality class 20 - 40% b = 7.1 [fm] 2+1 Relativistic hydrodynamics for heavy-ion collisions

  18. Centrality class 20 - 40% b = 7.1 [fm] 2+1 Relativistic hydrodynamics for heavy-ion collisions

  19. Centrality class 40 - 60% b = 9.2 [fm] 2+1 Relativistic hydrodynamics for heavy-ion collisions

  20. Centrality class 40 - 60% b = 9.2 [fm] 2+1 Relativistic hydrodynamics for heavy-ion collisions

  21. Conclusions • New and elegant approach to old problem: we have generalized the equations of 1+1 hydrodynamics to the case of angular asymmetry using the method of Baym et al. (this is possible for the crossover phase transition, recently suggested by the lattice simulations of QCD, only 2 equations in the extended r-space, automatically fulfilled boundary conditions at r=0) • Velocity field is developed that tends to transform the initial almond shape to a cylindrically symmetric shape. As expected, the magnitude of the flow is greater in the in-plane direction than in the out-of-plane direction. The direction of the flow changes in time and helps the system to restore a cylindrically symmetric shape. • For most peripheral collisions the flow changes the central hot region to a pumpkin-like form – as the system cools down this effect vanishes. • Edge of the system preserves the almond shape but the relative asymmetry is decreasing with time as the system grows. • Presented results may be used to calculate the particle spectra and the v2 parameter when supplemented with the freeze-out model (THERMINATOR). 2+1 Relativistic hydrodynamics for heavy-ion collisions

  22. centrality class 0 - 100%, sound velocity: lattice QCD, H0 = 0.01, 2+1 Relativistic hydrodynamics for heavy-ion collisions

  23. centrality class 0 - 100%, sound velocity: lattice QCD, H0 = 0.01, 2+1 Relativistic hydrodynamics for heavy-ion collisions

  24. centrality class 40 - 60%, sound velocity: analytic, H0 = 0.01, 2+1 Relativistic hydrodynamics for heavy-ion collisions

  25. centrality class 40 - 60%, sound velocity: analytic, H0 = 0.01, 2+1 Relativistic hydrodynamics for heavy-ion collisions

  26. centrality class 40 - 60%, sound velocity: constant 3-1/2, H0 = 0.01, 2+1 Relativistic hydrodynamics for heavy-ion collisions

  27. centrality class 40 - 60%, sound velocity: constant 3-1/2, H0 = 0.01, 2+1 Relativistic hydrodynamics for heavy-ion collisions

  28. centrality class 40 - 60%, sound velocity: analytic, H0 = 0.25, 2+1 Relativistic hydrodynamics for heavy-ion collisions

  29. centrality class 40 - 60%, sound velocity: analytic, H0 = 0.25, 2+1 Relativistic hydrodynamics for heavy-ion collisions

  30. 2+1 Relativistic hydrodynamics for heavy-ion collisions

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