Slide 1

Mike Lisa - ISMD, Berkeley - August 20071 A menu of expectations for femtoscopy* 1.0 at LHC/ALICE Mike Lisa Ohio State University *femtoscopy (fem-ta-sk-pee) noun The measurement of spatial scales at the fermi level. Non-trivially related to the HBT effect invented to measure stellar scales Slide 2 Mike Lisa - ISMD, Berkeley - August 20072 Outline Brief motivation / review Model expectations for H.I. collisions [ mostly] The importance of femtoscopy in p+p collisions A menu Slide 3 Mike Lisa - ISMD, Berkeley - August 20073 MicroexplosionsFemtoexplosions ss0.1 J 1 J 10 17 J/m 3 5 GeV/fm 3 = 10 36 J/m 3 T10 6 K200 MeV = 10 12 K rate10 18 K/sec10 35 K/s fast energy deposition plasma hydro expansion cooling to original phase do geometric postmortem & infer momentum Slide 4 Mike Lisa - ISMD, Berkeley - August 20074 MicroexplosionsFemtoexplosions ss0.1 J 1 J 10 17 J/m 3 5 GeV/fm 3 = 10 36 J/m 3 T10 6 K200 MeV = 10 12 K rate10 18 K/sec10 35 K/s fast energy deposition plasma hydro expansion cooling to original phase do geometric postmortem & infer momentum Slide 5 Mike Lisa - ISMD, Berkeley - August 20075 MicroexplosionsFemtoexplosions ss0.1 J 1 J 10 17 J/m 3 5 GeV/fm 3 = 10 36 J/m 3 T10 6 K200 MeV = 10 12 K rate10 18 K/sec10 35 K/s fast energy deposition plasma hydro expansion cooling to original phase do geometric postmortem & infer momentum measure explosive pattern of the thermalized bulk matter (low-pT) B2B jets? access to bulk properties (EoS) driving dynamics Slide 6 Mike Lisa - ISMD, Berkeley - August 20076 Spectra v2v2 HBT measure explosive pattern of the thermalized bulk matter (low-pT) hydro expectation (off-center collision) collective p T component: m*v T Slide 7 Mike Lisa - ISMD, Berkeley - August 20077 Spectra v2v2 HBT measure explosive pattern of the thermalized bulk matter (low-pT) elliptic flow Slide 8 Mike Lisa - ISMD, Berkeley - August 20078 Spectra v2v2 HBT measure explosive pattern of the thermalized bulk matter (low-pT) femtoscopy probes x-p substructure Slide 9 Mike Lisa - ISMD, Berkeley - August 20079 hydro ideal fluid dynamics At RHIC: Explosive signature sensitive to physics in models cascade Boltzmann models - collisions between particles 3 talks later What might we expect at LHC? Slide 10 Mike Lisa - ISMD, Berkeley - August 200710 All soft-physics observables at RHIC (& often SPS/AGS) are multiplicity-driven S. Manly (PHOBOS) QM05 H. Caines (STAR) QM05 NA57 (open) STAR (filled) NA57 (open) STAR (filled) G. Westfall, WPCF 2007 E-by-E fluctuation in K/ MAL,Pratt Soltz,Wiedemann nucl-ex/0505014 Entropy dominance? Slide 11 Mike Lisa - ISMD, Berkeley - August 200711 PHOBOS White Paper: NPA 757, 28 1000 5.5 TeV 5 6 6.4 = RHICx1.6 Slide 12 Mike Lisa - ISMD, Berkeley - August 200712 NNUS*: Multiplicity sets scale: all else fixed PHOBOS-based extrapolation: R LHC / R RHIC = (1.6) 1/3 = 1.17 PHOBOS White Paper: NPA 757, 28 1000 5.5 TeV 5 6 6.4 = RHICx1.6 * NNUS = Nothing New Under the Sun Slide 13 Mike Lisa - ISMD, Berkeley - August 200713 NNUS*: Multiplicity sets scale: all else fixed PHOBOS-based extrapolation: R LHC / R RHIC = (1.6) 1/3 = 1.17 CGC prediction of multiplicity R LHC / R RHIC = (11/3.6) 1/3 = 3 1/3 = 1.45 Kharzeev, Levin & Nardi NPA747 609 (2005) Slide 14 Mike Lisa - ISMD, Berkeley - August 200714 NNUS*: Multiplicity sets scale: all else fixed PHOBOS-based extrapolation: R LHC / R RHIC = (1.6) 1/3 = 1.17 CGC prediction of multiplicity R LHC / R RHIC = (11/3.6) 1/3 = 3 1/3 = 1.45 R Mike Lisa - ISMD, Berkeley - August 200715 STAR PRC71 044906 (2005) NNUS*: Multiplicity sets scale: all else fixed PHOBOS-based extrapolation: R LHC / R RHIC = (1.6) 1/3 = 1.17 CGC prediction of multiplicity R LHC / R RHIC = (11/3.6) 1/3 = 3 1/3 = 1.45 Rhigh R Slide 16 Mike Lisa - ISMD, Berkeley - August 200716 Access to long-range non-Gaussian tail Generalized imaging* fit probes long-R / low-q access to resonance tail small below s ~ 10 GeV LHC should be ~RHIC (... and/or other tails...) details beyond gross size Brown, Soltz, Newby, Kisiel nucl-th/0705.1337 PHENIX, PRL 98, 132301 (2007), * c.f. talks of P. Danielewicz & P. Chung Slide 17 Mike Lisa - ISMD, Berkeley - August 200717 Physics from (Gaussian) scales - dynamic models Boltzmann models particle rescattering thermalization not assumed typically hard EoS softening must be put in by hand (string melting etc) Hydrodynamic models thermalization / perfect fluid EoS varied. Typically a soft point used Slide 18 Mike Lisa - ISMD, Berkeley - August 200718 Boltzmann-type models Humanic/Hadron Rescattering Model real model predicting flow & HBT (dN/d [LHC] / dN/d [RHIC] ) 1/3 ~ 1.9 dN/d T. Humanic, Int.J.Mod.Phys.E15197(2006) Slide 19 Mike Lisa - ISMD, Berkeley - August 200719 Boltzmann-type models R long (fm) dN/dt Humanic/Hadron Rescattering Model real model predicting flow & HBT (dN/d [LHC] / dN/d [RHIC] ) 1/3 ~ 1.9 LHC / RHIC = 2 :: (recall R long~ ~ ) dynamic effect R long [LHC] / R long [RHIC] ~ 2 all are connected?? T. Humanic, Int.J.Mod.Phys.E15197(2006) Slide 20 Mike Lisa - ISMD, Berkeley - August 200720 Boltzmann-type models Humanic/Hadron Rescattering Model real model predicting flow & HBT (dN/d [LHC] / dN/d [RHIC] ) 1/3 ~ 1.9 LHC / RHIC = 2 :: (recall R long~ ~ ) dynamic effect R long [LHC] / R long [RHIC] ~ 2 all are connected? R S, R O larger, but not a simple factor T. Humanic, Int.J.Mod.Phys.E15197(2006) Slide 21 Mike Lisa - ISMD, Berkeley - August 200721 Boltzmann-type models Humanic/Hadron Rescattering Model real model predicting flow & HBT (dN/d [LHC] / dN/d [RHIC] ) 1/3 ~ 1.9 LHC / RHIC = 2 :: (recall R long~ ~ ) dynamic effect R long [LHC] / R long [RHIC] ~ 2 all are connected? R S, R O larger, but not a simple factor steeper p T -dep due to more flow? dynamic effect Hard EoS rescattering models: dynamic effects superimposed on chemistry similar for AMPD C.M. Ko; WPCF06 T. Humanic, Int.J.Mod.Phys.E15197(2006) Slide 22 Mike Lisa - ISMD, Berkeley - August 200722 Hydro predictions I: Scales Neglecting flow, to cool to C [QGP] : C = 0 ( C / 0 ) 3/4 C no flow [RHIC] = 6 fm/c C no flow [LHC] = 20 fm/c Eskola et al PRC72044904 (2005) initial conditions from pQCD+saturation Slide 23 Mike Lisa - ISMD, Berkeley - August 200723 Neglecting flow, to cool to C [QGP] : C = 0 ( C / 0 ) 3/4 C no flow [RHIC] = 6 fm/c C no flow [LHC] = 20 fm/c Much larger flow @LHC signif. reduction of timescale @ LHC [similar to RHIC] larger transverse size @ FO Eskola et al PRC72044904 (2005) Hydro predictions I: Scales Slide 24 Mike Lisa - ISMD, Berkeley - August 200724 Neglecting flow, to cool to C [QGP] : C = 0 ( C / 0 ) 3/4 C no flow [RHIC] = 6 fm/c C no flow [LHC] = 20 fm/c Much larger flow @LHC signif. reduction of timescale @ LHC [similar to RHIC] larger transverse size @ FO No HBT prediction per se, but... R L [LHC] / R L [RHIC] ~ 1.1 1.2 R S [LHC] / R S [RHIC] ~ 1.5 2 (different than HRM) steeper p T -dependence Eskola et al PRC72044904 (2005) Hydro predictions I: Scales Slide 25 Mike Lisa - ISMD, Berkeley - August 200725 Neglecting flow, to cool to C [QGP] : C = 0 ( C / 0 ) 3/4 C no flow [RHIC] = 6 fm/c C no flow [LHC] = 20 fm/c Much larger flow @LHC signif. reduction of timescale @ LHC [similar to RHIC] larger transverse size @ FO No HBT prediction per se, but... R L [LHC] / R L [RHIC] ~ 1.1 1.2 R S [LHC] / R S [RHIC] ~ 1.5 2 (different than HRM) steeper p T -dependence Consistent w/ independent hydro for non-central collisions Eskola et al PRC72044904 (2005) Hydro predictions I: Scales Heinz&Kolb, PLB542 216 (2002) (LHC) Slide 26 Mike Lisa - ISMD, Berkeley - August 200726 easy prediction: importance of -dep measurements will continue @ LHC RP resolution at least as good as STAR asHBT measures source shape at freezeout Hydro predictions II: Shapes STAR 200 GeV PRL93 012301 (04) ALICE PPR (vol 2): J. Phys G. Part. Nucl. Phys. 32 1295 (2006) Slide 27 Mike Lisa - ISMD, Berkeley - August 200727 easy prediction: importance of -dep measurements will continue @ LHC RP resolution at least as good as STAR asHBT measures source shape at freezeout probes timescale & dynamics non-trivial (& incomplete!) excitation fctn Hydro predictions II: Shapes E895 2 GeV PLB496 1 (2000) STAR 200 GeV PRL93 012301 (04) OHara, et al, Science 298 2179 (2002) Slide 28 Mike Lisa - ISMD, Berkeley - August 200728 easy prediction: importance of -dep measurements will continue @ LHC RP resolution at least as good as STAR asHBT measures source shape at freezeout probes timescale & dynamics non-trivial (& incomplete!) excitation fctn hydro @ RHIC misses scale (well-known) impressive agreement on -dep Hydro predictions II: Shapes STAR PRL93 012301 (2004) Heinz&Kolb, PLB542 216 (2002) RHIC Slide 29 Mike Lisa - ISMD, Berkeley - August 200729 easy prediction: importance of -dep measurements will continue @ LHC RP resolution at least as good as STAR asHBT measures source shape at freezeout probes timescale & dynamics non-trivial (& incomplete!) excitation fctn hydro @ RHIC misses scale (well-known) impressive agreement on -dep prediction @ LHC sign change in shape & oscillations Hydro predictions II: Shapes Heinz&Kolb, PLB542 216 (2002) RHIC Heinz&Kolb, PLB542 216 (2002) IPES (LHC) Sign flip in oscillations reflects transition to in-plane geometry (more flow, more time) Slide 30 Mike Lisa - ISMD, Berkeley - August 200730 p+p: A clear reference system? Slide 31 Mike Lisa - ISMD, Berkeley - August 200731 e+e- (and p+p, +p...) -- similar HBT radii high-quality/stats data sparse diversity of methods corrections coordinate systems jet axis in e+e-... mixing... physics? OPAL e+e- -> Z July 2007 CERN-PH-EP/2007-025 Slide 32 Mike Lisa - ISMD, Berkeley - August 200732 e+e- (and p+p, +p...) -- similar HBT radii high-quality/stats data sparse diversity of methods corrections coordinate systems jet axis in e+e-... mixing... physics of x-p correlations in very small systems? strings? jets? pythia + rescattering? else? i-th particle Initial disk of radius r talk by T. Humanic L. Lonnblad - WPCF2007 Paic and Skowronski J. Phys. G31 1045 (2005) see also Csorgo & Zajc hep-ph/0412243 (ISMD04) pT signal? Slide 33 Mike Lisa - ISMD, Berkeley - August 200733 STAR preliminary m T (GeV) Z. Chajecki WPCF05 Caution: femtoscopy in p+p @ STAR p+p and A+A measured in same experiment with same method great opportunity to compare physics what causes p T -dependence in p+p? same cause as in A+A?? Slide 34 Mike Lisa - ISMD, Berkeley - August 200734 Surprising (puzzling) scaling HBT radii scale with pp Scary coincidence or something deeper? pp, dAu, CuCu - STAR preliminary Ratio of (AuAu, CuCu, dAu) HBT radii by pp p+p and A+A measured in same experiment with same method great opportunity to compare physics what causes p T -dependence in p+p? same cause as in A+A? !! But !! significant issues with nontrivial interplay non-femtoscopic correlations (restricted phasespace) - should be less of a problem at LHC - [see talk of T. Humanic] A. Biaasz (ISMD): I personally feel that its solution may provide new insight into the hadronization process of QCD Slide 35 Mike Lisa - ISMD, Berkeley - August 200735 5 as before (same p T dep etc) but scale by ~17% as before (same p T dep etc) but scale by ~45% NNUS: naive extrapolation HRM and AMPT R L (50-100% 30%increase) [dynamics / chemistry / both ??] R O,S smaller increase (~30% 10%) higher flow steeper p T dep plats principaux boissonsentres le menu des esprances au LHC hydro R L small increase (~30%) [huge flow rapid cooling short ] R O,S : huge flow larger increase (~60%) steeper p T dep shape inversion; oscillation sign flip large tilt for central region? p+p p p jet signif p T dep R increase w/ mult other details?? very large R O in high mult?? p+p = A+A ??? Slide 36 Mike Lisa - ISMD, Berkeley - August 200736 Slide 37 Mike Lisa - ISMD, Berkeley - August 200737 ++ -- K+K+ K-K- K0SK0S p pp ++ -- - K+K+ K-K- --K0SK0S p pp R(S NN, b, N part, A, B, m T, y, , PID 1, PID 2 ) Does lock pattern break? extract phaseshifts (inversion of K-P paradigm) p+p in multiplicity classes [esp very low multiplicity] HBT relative to jets in p+p and A+A excitation function - (direct yield) Slide 38 Mike Lisa - ISMD, Berkeley - August 200738 The end (...finally...) Slide 39 Mike Lisa - ISMD, Berkeley - August 200739 ALICE PPR2 plots Slide 40 Mike Lisa - ISMD, Berkeley - August 200740 Relative momentum resolution ITS+TPC tracks 2 MeV/c (-> 100 fm, for scale only...) del-qside small since azim. angle well-known qout probes sagitta resolution heavier particles less bending -> smaller sagitta -> worse resolution but due to mT scaling, worse resolution is OK :-) ALICE PPR (vol 2): J. Phys G. Part. Nucl. Phys. 32 1295 (2006) Slide 41 Mike Lisa - ISMD, Berkeley - August 200741 Track merging effects in the TPC merging -> ~0.3 fm bias in HBT radius determination for 8 fm source less impt for smaller sources less impt if Coulomb FSI included (?) impact on imaging (non-Gaussian shapes) (?) merging correlated in qo-qs (can mimic tilted source) requiring separation in TPC helps remove effect, but convergence is slow ALICE PPR (vol 2): J. Phys G. Part. Nucl. Phys. 32 1295 (2006) Slide 42 Mike Lisa - ISMD, Berkeley - August 200742 The ITS helps remove merging effects Ros = 0 as figure of merit Cutting on ITS separation reduces bias to ~0.1-0.2 fm ALICE PPR (vol 2): J. Phys G. Part. Nucl. Phys. 32 1295 (2006) similar triangles : qmin/pT = separationMin/radius Slide 43 Mike Lisa - ISMD, Berkeley - August 200743 Momentum resolution correction Triple-ratio correction first (?) used by NA44 uses single-particle resolution (assumed known) to smear ideal CF rapid convergence ALICE PPR (vol 2): J. Phys G. Part. Nucl. Phys. 32 1295 (2006) method of NA44/E895/STAR/... Slide 44 Mike Lisa - ISMD, Berkeley - August 200744 HBT radii : out versus in good to ~15 fm ALICE PPR (vol 2): J. Phys G. Part. Nucl. Phys. 32 1295 (2006) Slide 45 Mike Lisa - ISMD, Berkeley - August 200745 Event-by-event femtoscopy in Pb+Pb ALICE PPR (vol 2): J. Phys G. Part. Nucl. Phys. 32 1295 (2006) Slide 46 Mike Lisa - ISMD, Berkeley - August 200746 reactionplane resolution At least as good as RHIC/STAR ALICE PPR (vol 2): J. Phys G. Part. Nucl. Phys. 32 1295 (2006) Plot from T. Hirano 2005