Transcript Document
Energy dependence of anisotropic flow Raimond Snellings RHIC: the first 3 years RHIC Scientists Serve Up “Perfect” Liquid New state of matter more remarkable than predicted -- raising many new questions April 18, 2005 5 July 2006 [email protected] 2 Outline The perfect liquid at RHIC How do we approach the perfect liquid? What can we expect at the LHC? What can we learn from higher harmonics? 5 July 2006 [email protected] 3 Anisotropic Flow d3 N 1 d2 N E 3 1 2 v ( p , y ) cos n n t r d p 2 pt dpt dy n 1 Anisotropic flow ≡ azimuthal correlation with the reaction plane vn cosn r 5 July 2006 the cleanest signal of final-state reinteractions Unavoidable consequence of thermalization Natural description in hydrodynamic language, however when we talk about flow we do not necessary imply (ideal) hydrodynamic behavior Flow in cascade models: depends on constituent cross sections and densities, partonic and/or hadronic Non-flow ≡ contribution to vn from azimuthal correlations between particles not due to their correlation with the reaction plane (HBT, resonances, jets, etc) [email protected] 4 Measuring Anisotropic Flow vn cos n( r ) ein( ψ r ) ein (1 2 ) ein (1 r ) ein ( r 2 ) ein (1 r ) ein ( r 2 ) (vn {2}) 2 Assumption: all correlations between particles due to flow Non flow correlation contribute order (1/N), problem if vn≈1/√N v2 2 v22 ein (1 2 3 4 ) ein (1 2 ) ein (3 4 ) ein (1 4 ) ein (3 2 ) (vn {4}) 4 Non flow correlation contribute order (1/N3), problem if vn≈1/N¾ v2 4 2 v 2 2 2 1/ 4 v 4 2 Measuring the cumulants of different order provides constraints on both fluctuations and non-flow. Can be conveniently calculated using generating functions, extended to vn{∞} using Lee-Yang zeros, reliable vn>1/N N. Borghini, P.M. Dinh and J.-Y Ollitrault, Phys. Rev. C63 (2001) 054906 5 July 2006 [email protected] 5 The perfect liquid 5 July 2006 [email protected] 6 The “nearly perfect” liquid HYDRO: Kolb, Sollfrank, Heinz, PRC 62 (2000) 054909 STAR PRL 86, 402 (2001) P.F. Kolb et al., PLB 500 (2001) 0012137 v2{4} 130 GeV Zhixu Liu 5 July 2006 Magnitude and transverse momentum dependence of v2 A strongly interacting, more thermalized system which is for more central collisions behaves consistent with ideal fluid behavior! [email protected] 7 Viscosity and parton cascade D. Molnar and P. Huovinen, PRL94:012302,2005 D. Teaney PRC68:034913,2003 Viscosity needs to be small Parton cascades need huge opacities Partially solved by coalescence Microscopic picture responsible for large v2 still not understood (E. Shuryak sQGP is being understood) 5 July 2006 [email protected] 8 Strong Collective Motion, v2(m,pt) Particles flow with a common velocity The most compact representation of the strong radial flow and its azimuthal variation Best described by QGP EoS!? 5 July 2006 [email protected] 9 The QCD EoS and Cs F. Karsch and E. Laermann, arXiv:hep-lat/0305025 Test the effect of four different EoS; qp is lattice inspired, Q has first order phase transition, H is hadron gas with no phase transition and T a smooth parameterization between hadron and QGP phase Pasi Huovinen, arXiv:nucl-th/0505036 5 July 2006 [email protected] 10 v2(m,pt) and the softest point Pasi Huovinen, arXiv:nucl-th/0505036 5 July 2006 EoS Q and EoS T (both have significant softening) do provide the best description of the magnitude of the mass scaling in v2(pt) The lattice inspired EoS (EoS qp) in ideal hydro does as poorly as a hadron gas EoS! (opposite to conclusion Kämpfer) Elliptic flow as function of pt and mass very sensitive to EoS (particular the heavier particles) Before we can draw conclusions about the EoS much more work needed in theory (test different EoS, influence viscosity, hadronic phase) [email protected] 11 Energy dependence NA49, Phys. Rev. C(68), 034903 (2003) Kolb, Sollfrank, Heinz, PRC 62 (2000) 054909 Heiselberg and Levi PRC 59 D. Teaney, J. Lauret, E.V. Shuryak, arXiv:nuclth/0011058; Phys. Rev. Lett 86, 4783 (2001). v2 5 July 2006 S tr dN dy Energy dependence missed by ideal hydro Hydro + cascade describes v2 from SPS to RHIC At higher energies ideal hydro contribution dominates Hydro + cascade follows “low density limit”?? [email protected] 12 v2, eccentricity and fluctuations M. Miller and RS, arXiv:nucl-ex/0312008 y 2 x2 y 2 x2 v2 v2 {2} v22 2 2 2 v2 {4} 2 v v2 {6} v 1 4 5 July 2006 6 2 v 4 2 9 v24 1/ 4 2 3 2 v22 12 v 1/ 6 [email protected] 13 v2, eccentricity and fluctuations M. Miller and RS, arXiv:nucl-ex/0312008 “standard” v2{2} overestimates v2 by 10%, higher order cumulant underestimate v2 by 10% at intermediate centralities Measuring the cumulants of different order provides constraints on both fluctuations! and on non-flow contributions! 5 July 2006 [email protected] 14 PHOBOS eccentricity fluctuations y' x' 2 part 2 y' y x' y' x' 2 2 x S. Manly, QM2005 Large effect for small systems over whole centrality range 5 July 2006 [email protected] 15 v2/ revisited S. Voloshin CIPANP-’06 By using participant eccentricity Cu+Cu and Au+Au at two energies follow the v2/ scaling Although fluctuations in part are reduced to compared to ”standard” using {2} and v2{4}/{4} could be an improvement Why does it work that well? 5 July 2006 [email protected] 16 Rapidity dependence Hirano: Nucl Phys A715 821 824 2003 No boost invariance! 5 July 2006 [email protected] 17 Rapidity dependence PHOBOS nucl-ex/0509034 PHOBOS PRL 94, 122303 (2005) dN/dh scales versus h-ybeam v2/ ~ 1/S dN/dy Rapidity dependence no surprise? 5 July 2006 [email protected] 18 Rapidity dependence of eccentricity Is the /S independent of rapidity? 5 July 2006 [email protected] 19 LHC energies E. Simili v2 dNch dh Using dN/dy scaling of multiplicity and v2/eps extrapolation Values a bit above hydro predictions (from T. Hirano) 5 July 2006 [email protected] 20 Energy dependence T. Hirano D. Teaney, J. Lauret, E.V. Shuryak, arXiv:nuclth/0011058; Phys. Rev. Lett 86, 4783 (2001). The higher the beam energy the more dominant the QGP (here ideal hydro) contribution becomes 5 July 2006 [email protected] 21 Viscosity/entropy versus T Hirano and Gyulassy arXiv:nucl-th/0506049 Csernai, Kapusta and McLerran arXiv:nucl-th/0604032 Important to quantitatively calculate the effect of viscosity on v2 Would reduce further the elliptic flow 5 July 2006 [email protected] 22 Higher Harmonics Peter Kolb, PRC 68, 031902 STAR, Phys. Rev. Lett.(92), 062301 (2004) 5 July 2006 Higher harmonics are expected to be present, for smooth azimuthal distributions the higher harmonics will be small vn ~ v2n/2 v4 - a small, but sensitive observable for heavy ion collisions (Peter Kolb, PRC 68, 031902) v4 - magnitude sensitive to ideal hydro behavior (Borghini and Ollitrault, arXiv:nucl-th/0506045) Ideal hydro v4/v22 = 0.5 [email protected] 23 What do we learn from v4? Ratio v4/v22 is sensitive to degree of thermalization (Borghini and Ollitrault nuclth/0506045) v4(pt)/v2(pt)2 is 1/2 for ideal hydro (more accurate for increasing values of pt) Observed integrated ratio is larger than unity Do we have intuitive test if the ratio is related to the degree of thermalization? ratio v4/v22 expected to decrease as the collisions become more central ratio v4/v22 expected to increase as function of transverse momenta rapidity & energy dependence 5 July 2006 [email protected] 24 v2 and v4 at 200 GeV STAR preliminary Y. Bai, AGS users meeting 2006 5 July 2006 [email protected] 25 200 GeV v4{EP2}/v2{4}2 Y. Bai, AGS users meeting 2006 v4/v22 decreases with pt below 1 GeV/c after which is starts to increase again (expected) Magnitude and centrality dependence do not follow intuitive expectations 5 July 2006 [email protected] 26 62 GeV v4{EP2}/v2{4}2 Y. Bai, AGS users meeting 2006 Centrality and pt dependence similar to 200 GeV magnitude of v4/v22 even somewhat lower! Energy dependence does not follow intuitive expectations 5 July 2006 [email protected] 27 Rapidity dependence A. Tang Ratio increases towards midrapidity contrary to expectations 5 July 2006 [email protected] 28 Conclusions Strong collective motion at RHIC energies, consistent with perfect liquid behavior No microscopic picture available Constraining the EoS requires more detailed calculations Energy dependence No obvious horns, kinks or steps Collapse of the proton v2 at SPS (next talk) Measurements of v2{2}, v2{4}, v2{6} allow for estimates of the fluctuations and non flow as function of energy (detailed measurement still needs to be done, strong argument for energy scan) v2 measurement at LHC will provide critical test of our understanding of the almost perfect liquid, testing the “hydro limit” Au+Au and Cu+Cu follow v2/ scaling when using part Why does it work that well? v4 is promising new observable to test hydrodynamic behavior Detailed high statistics measurement available Are the non-flow and fluctuation contributions to v4 under control? Challenge to theory! 5 July 2006 [email protected] 29