Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Femtoscopy in relativistic heavy-ion collisions as a probe of system collectivity Adam Kisiel CERN.

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Presentation transcript:

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Femtoscopy in relativistic heavy-ion collisions as a probe of system collectivity Adam Kisiel CERN

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Heavy Ion collision evolution time M. Chojnacki, W. Florkowski, PRC 74 (2006) Transverse plane ● HIC is expected to go through a QGP phase in its evolution ● In this phase matter is strongly interacting – resulting in the development of collective motion ● Radial flow dominates, with elliptic flow modifying the azimuthal behavior

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Which collectivity do we seek? ● A collective component is a “common” velocity for all particles emitted close to each other ● To that one adds “thermal” (random) velocity ● We expect specific “common” velocity – radial direction, pointing outwards from the center

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Quantifying collectivity ● Hydrodynamics produces collective flow: common velocity of all particles ● The process drives the space-time evolution of the system ● For non-central collisions differences between in-plane and out-of plane velocities arise Chojnacki M., Florkowski W. nucl-th/ , Phys. Rev. C74: (2006) Phys.Rev.C79:014902,2009

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Thermal emission from collective medium ● A particle emitted from a medium will have a collective velocity β f and a thermal (random) one β t ● As observed p T grows, the region from where such particles can be emitted gets smaller and shifted to the outside of the source velocity direction

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan m T dependence at RHIC ● A clear m T dependence is observed, for all femtoscopic radii and for all particle types: but is it hydrodynamic like? And can we tell? STAR, Phys. Rev. C 71 (2005) 44906

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Non-central collisions: azimuthal modulation of collectivity hydro evolutionlater hadronic stage? Kolb & Heinz anisotropic pressure gradients drives the emergence of elliptic flow (v 2 ) Space-time and momentum anisotropy connected: can they be described at the same time? Azimuthally sensitive femtoscopy measures the space-time asymmetry by measuring radii vs. reaction plane Specific oscillations are expected  p =0°  p =90° R.P. R s small R s big

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Emission from the source vs. time ● Azimuthal anisotropy is self-quenching – evolving towards a spherical shape ● Observed shape a multipicity-weighted average time slices of 1 fm/c Phys.Rev.C79: ,2009

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Radii vs. reaction plane orientation ● Separate CFs are constructed for each orientations of pair k T vs. reaction plane ● Radii are extracted vs this angle, total dependence can be characterized by: ● Experiment clearly sees an anisotropic source shape STAR, Phys. Rev. Lett. 93 (2004) e-Print Archives (nucl-ex/ )

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan RHIC Hydro-HBT puzzle ● First hydro calculations struggle to describe femtoscopic data: predicted too small R side, too large R out – too long emission duration ● No evidence of first order phase tr. U. Heinz, P. Kolb, hep-ph/ T. Hirano, K. Tsuda, nucl-th/ Phys.Rev.C66:054905,2002. Phys. Rev. Lett. 93, (2004) Phys. Rev. Lett. 93, (2004),

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan How about rescattering models? ● Rescattering models also struggle to describe the femtoscopic data ● Problems similar to hydro: R side too small (but with correct slope), R out too large Bleicher et al., nucl-th/

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Revisiting hydrodynamics assumptions ● Data in the momentum sector ( p T spectra, elliptic flow) well described by hydrodynamics, why not in space-time? ● Usually initial conditions do not have initial flow at the start of hydrodynamics (~1 fm/c) – they should. ● Femtoscopy data rules out first order phase transition – smooth cross-over is needed ● Resonance propagation and decay as well as particle rescattering after freeze-out need to be taken into account: similar in effects to viscosity S. Pratt, Phys. Rev. Lett. 102, (2009) Initial flow Cross-over EOS viscosity

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Lhyquid+Therminator at RHIC ● Dynamical model with hydrodynamical evolution, propagation of strong resonances ● Reproduces spectra, elliptic flow and HBT ● Initial flow, smooth cross- over phase transition, resonance treatment W.Broniowski, W.Florkowski, M.Chojnacki, AK nucl-th/ ; nucl-th/

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Full centrality dependence ● Full centrality vs. pair transverse momentum vs. reaction plane orientation dependence of HBT radii is reproduced. ● Collectivity at RHIC consistent with hydro-like behavior. ● But is it unique? Filled points: STAR data from: Phys. Rev. Lett. 93 (2004) e-Print Archives (nucl-ex/ ) Colors: different kt bins Open points: Lhyquid+Therminator Phys.Rev.C79:014902,2009. Phys.Rev.C78:014905,2008.

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Does femotscopy probe collectivity? ● Ideal hydrodynamics: strong assumptions about the system (zero mean free path, local thermalization, “large” system) ● Relaxing assumptions seems not to affect m T scaling of radii for massless particles – is femtoscopy really probing the collectivity (and hence thermalization) of the system? Gombeaud C., Lappi T., Ollitrault J., Phys.Rev.C79:054914,2009. arXiv: [nucl-th]

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Relaxing hydro assumptions – rescattering test ● Simple model: two types of particles (“pions” and “kaons”), rescattering with cross-section d 2. ● Initial state: no collectivity. Two scenarios: uniform temperature or temperature gradient. ● d increases: spectra evolve to thermal, collectivity develops Closed: pions Open: kaons d 0.1 fm 1.0 fm 2.0 fm 5.0 fm 10.0 fm AK, T.J. Humanic,

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Is “gradient” and “collectivity” the same? pionsfaster pions same velocity kaons Gradient case No interactions Size decreases No shift Gradient case With interactions Size decreases Mean emission point shifted ● m T scaling of radii can be produced both by temperature gradients and “collectivity” ● Additional effect of collectivity: the source is shifted arXiv:

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan m T scaling = collectivity? ● “Gradient” case with no interactions shows m T dependence – scenario alternative to collectivity? ● Kaons do not follow the trend ● Simulations with interactions also show m T dependence, but now kaons follow the same trend as pions ● Predictions from hydro (with resonance propagation) also show common m T scaling open: uniform closed: gradient pions kaons pions Therminator, nucl-th/ Phys.Rev.C73:064902,2006. kaons arXiv:

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan m T scaling for kaons and protons ● m T scaling, coming both from p T and from mass, is observed in data for pions, kaons, protons ● It is consistent with collective flow, inconsistent with temperature gradients with no collectivity PHENIX, Phys. Rev. Lett. 103, (2009),Phys. Rev. Lett. 103, (2009) 200 AGeV 200 AGeV pp 200 AGeV arXiv:

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Mean emission point difference: clean signal of collectivity ● Mean emission point difference between pions and kaons increases linearly with number of collisions per particle – clean and unambigous signature of collectivity ● Initial temperature gradients do not matter – asymmetry depends only on collectivity ● Can be measured by non- identical particle femtoscopy arXiv:

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Collectivity and emission asymmetry Pions Kaons Protons β = (0.6,0.8) ● As particle mass (or p T ) grows, average emission point moves more “outwards” - origin of the effect the same as m T scaling ● Average emission points for particles with same velocity but different mass: ● Similar asymmetry can come from time difference (e.g. from resonance products) but detailed simulation shows it is less than 1/3 of the total effect arXiV: Asymmetry :

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Predictions from Therminator+Lhyquid ● Expected centrality trend: size grows, asymmetry grows ● Expected size and asymmetry ordering for three pair types ● Sizeable asymmetry predicted for pion- kaon and pion-proton pairs, dominated by collectivity induced pion-kaon pion-proton kaon-proton arXiV: STAR 130 AGeV

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Pion – Kaon correlations at 130 AGeV ● Clear asymmetry in the “out” direction is seen for all pairs. ● Asymmetry direction consistent with hydrodynamic predictions: pions are emitted closer to the center and/or later than kaons with the same velocity Phys. Rev. Lett. 91 (2003)

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Pion-Kaon correlations at 200 AGeV system size asymmetry Therminator predictions STAR preliminary The correlation AuAu 200 GeV The asymmetry signal π + K + π - K - π + K - π - K + STAR preliminary Points: STAR preliminary data Lines: prediction from the Therminator model ● Data show clear asymmetry: pions are emitted closer to the center and/or later than kaons ● Consistent with hydrodynamic model predictions, strong evidence against competing explanations

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Pion-proton – STAR vs. Therminator STAR preliminary points: STAR data lines: calculations from Therminator model same sign opposite sign Correlation function Emission asymmetry signal

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Femtoscopy with exotic systems ● Pion-Xi correlations show robust asymmetry signal: the Xi is emitted earlier or more on the outside of the system – even the heavy and weakly interacting Xi flows Petr Chaloupka  Braz.J.Phys.37: ,2007 R = (6.7 ±1.0) fm ∆ out = (-5.6 ±1.0) fm STAR preliminary A00 - Correlation function A11 – asymmetry signal Petr Chaloupka

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Predictions for collectivity at LHC ● Specific predictions for LHC: steeper m T dependence from larger flow, longer evolution gives larger size and the reversal of the azimuthal anisotropy in space-time. The decrease of R out /R side ratio is even larger than at RHIC. LHC RHIC Phys.Rev.C79:014902,2009

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Azimuthal oscillations at the LHC ● At the LHC longer evolution makes the shape in-plane extended at the end. The averaged shape is still out-of- plane extended, but with smaller oscillations Phys.Rev.C79:014902,2009

Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Summary ● Collectivity is one of defining features differentiating elementary collisions and complicated systems created in heavy-ion collisions ● Hydrodynamic-like behavior, also seen in rescattering simulations, produces specific patterns in femtoscopic observables: m T scaling of radii for particles of all masses, oscillation of radii vs. reaction plane orientation and mean emission point differences ● All effects observed in data, but modifications in original assumptions of hydrodynamics needed to describe them exactly: femtoscopy provides important constraints on the physics assumptions