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Update on Search for Chiral Symmetry Restoration in Heavy-Ion Collisions Ralf Rapp Cyclotron Institute + Dept of Phys & Astro Texas A&M University College.

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Presentation on theme: "Update on Search for Chiral Symmetry Restoration in Heavy-Ion Collisions Ralf Rapp Cyclotron Institute + Dept of Phys & Astro Texas A&M University College."— Presentation transcript:

1 Update on Search for Chiral Symmetry Restoration in Heavy-Ion Collisions Ralf Rapp Cyclotron Institute + Dept of Phys & Astro Texas A&M University College Station, USA 11 th Int. Conference on Nucleus-Nucleus Collisions San Antonio (Texas), 29.05.12

2 1.) Intro: EM Spectral Function + Fate of Resonances Electromagn. spectral function - √s < 2 GeV : non-perturbative - √s > 2 GeV : perturbative (“dual”) Vector resonances “prototypes” - representative for bulk hadrons: neither Goldstone nor heavy flavor Modifications of resonances ↔ phase structure: - hadron gas → Quark-Gluon Plasma - realization of transition? √s = M e + e  → hadrons Im Π em (M,q;  B,T) Im  em (M) in Vacuum

3 1.2 Phase Transition(s) in Lattice QCD cross-over(s) ↔ smooth e + e  rate chiral restoration in “hadronic phase”?! (low-mass dileptons!) hadron resonance gas “T c conf ” ~170MeV “T c chiral ”~155MeV ≈  qq  /  qq  - [Fodor et al ’10]

4 2.) Chiral Symmetry Breaking in Vacuum  “Higgs Mechanism”, Condensates + Mass Gap in QCD  Hadron Spectrum, Chiral Partners + Sum Rules 3.) EM Spectral Function in Medium  Hadronic Theory  QGP + Lattice QCD 4.) EM Probes in Heavy-Ion Collisions  Spectro-, Thermo-, Chrono- + Baro-meter  Thermal Photons  P t Spectra + Collectivity 5.) Conclusions Outline

5 “Higgs” Mechanism in Strong Interactions: qq attraction  condensate fills QCD vacuum! Spontaneous Chiral Symmetry Breaking 2.1 Chiral Symmetry + QCD Vacuum : flavor + “chiral” (left/right) invariant > > > > qLqL qRqR qLqL - qRqR - - Profound Consequences: effective quark mass: ↔ mass generation! near-massless Goldstone bosons  0,± “chiral partners” split:  M ≈ 0.5GeV J P =0 ± 1 ± 1/2 ±

6 2.2 Chiral (Weinberg) Sum Rules Quantify chiral symmetry breaking via observable spectral functions Vector (  ) - Axialvector (a 1 ) spectral splitting [Weinberg ’67, Das et al ’67]  →(2n+1)  pQCD Key features of updated “fit”: [Hohler+RR ‘12]  + a 1 resonance, excited states (  ’+ a 1 ’), universal continuum (pQCD!)  →(2n)  [ALEPH ‘98, OPAL ‘99]

7 2.2.2 Evaluation of Chiral Sum Rules in Vacuum vector-axialvector splitting (one of the) cleanest observable of spontaneous chiral symmetry breaking promising starting point to search for chiral restoration pion decay constants chiral quark condensates

8 2.3 QCD Sum Rules:  and a 1 in Vacuum dispersion relation: lhs: hadronic spectral fct. rhs: operator product expansion [Shifman,Vainshtein+Zakharov ’79] 4-quark + gluon condensate dominant vector axialvector

9 2.) Chiral Symmetry Breaking in Vacuum  “Higgs Mechanism”, Condensates + Mass Gap in QCD  Hadron Spectrum, Chiral Partners + Sum Rules 3.) EM Spectral Function in Medium  Hadronic Theory  QGP + Lattice QCD 4.) EM Probes in Heavy-Ion Collisions  Spectro-, Thermo-, Chrono- + Baro-meter  Thermal Photons  P t Spectra + Collectivity 5.) Conclusions Outline

10 > >    B *,a 1,K 1... N, ,K … 3.1 Vector Mesons in Hadronic Matter D  (M,q;  B,T) = [M 2 - m  2 -   -   B -   M ] -1  -Propagator: [Chanfray et al, Herrmann et al, Asakawa et al, RR et al, Koch et al, Klingl et al, Post et al, Eletsky et al, Harada et al …]   =   B,  M  = Selfenergies:  Constraints: decays: B,M→  N,  scattering:  N →  N,  A, …  B /  0 0 0.1 0.7 2.6 SPS RHIC/LHC

11 3.2 Axialvector in Medium: Dynamical a 1 (1260) + +... =           Vacuum: a 1 resonance In Medium: + +... [Cabrera,Jido, Roca+RR ’09] in-medium  +  propagators broadening of  -  scatt. Amplitude pion decay constant in medium:

12 3.3 Vector Correlator in Thermal Lattice QCD Euclidean Correlation fct. Hadronic Many-Body [RR ‘02] Lattice (quenched) [Ding et al ‘10] “Parton-Hadron Duality” of lattice and in-medium hadronic?!

13 3.3.2 Back to Spectral Function suggests approach to chiral restoration + deconfinement -Im  em /(C T q 0 )

14 3.4 Dilepton Rates: Hadronic - Lattice - Perturbative dR ee /dM 2 ~ ∫d 3 q f B (q 0 ;T) Im  V 3-fold “degeneracy” toward ~T c Quark-Hadron Duality at all M ?! (  degenerate axialvector SF) [qq→ee] - [HTL] [RR,Wambach et al ’99] [Ding et al ’10] dR ee /d 4 q 1.4T c (quenched) q=0

15 3.5 Summary: Criteria for Chiral Restoration Vector (  ) – Axialvector (a 1 ) degenerate [Weinberg ’67, Das et al ’67] pQCD QCD sum rules: medium modifications ↔ vanishing of condensates Agreement with thermal lattice-QCD Approach to perturbative rate (QGP)

16 2.) Chiral Symmetry Breaking in Vacuum  “Higgs Mechanism”, Condensates + Mass Gap in QCD  Hadron Spectrum, Chiral Partners + Sum Rules 3.) EM Spectral Function in Medium  Hadronic Theory  QGP + Lattice QCD 4.) EM Probes in Heavy-Ion Collisions  Spectro-, Thermo-, Chrono- + Baro-meter  Thermal Photons  P t Spectra + Collectivity 5.) Conclusions Outline

17 4.1 Dilepton Rates vs. Exp.: NA60 “Spectrometer” invariant-mass spectrum directly reflects thermal emission rate! Acc.-corrected  +   Excess Spectra In-In(158AGeV) [NA60 ‘09] M  [GeV] Thermal     Emission Rate Evolve rates over fireball expansion: [van Hees+RR ’08]

18 M  [GeV] 4.1.2 Sensitivity to Spectral Function avg.   (T~150MeV) ~ 370 MeV    (T~T c ) ≈ 600 MeV → m  driven by baryons In-Medium  -Meson Width

19 4.2 Low-Mass e + e  at RHIC: PHENIX vs. STAR “large” enhancement not accounted for by theory cannot be filled by QGP radiation… (very) low-mass region overpredicted… (SPS?!)

20 4.3 Direct Photons at RHIC v 2 ,dir comparable to pions! under-predicted by ealry QGP emission ← excess radiation T eff excess = (220±25) MeV QGP radiation? radial flow? Spectra Elliptic Flow [Holopainen et al ’11,…]

21 4.3.2 Revisit Ingredients multi-strange hadrons at “T c ” v 2 bulk fully built up at hadronization chemical potentials for , K, … Hadron - QGP continuity! Emission Rates Fireball Evolution [van Hees et al ’11] [Turbide et al ’04]

22 4.3.3 Thermal Photon Spectra + v 2 : PHENIX both spectral slope and v 2 point at blue-shifted hadronic source… to be tested in full hydro thermal + prim.  [van Hees,Gale+RR ’11]

23 4.4 QGP Barometer: Blue Shift vs. Temperature QGP-flow driven increase of T eff ~ T + M (  flow ) 2 at RHIC temperature overcomes flowing late  ’s → minimum (opposite to SPS!) expect to be more pronounced at LHC RHIC SPS

24 5.) Conclusions: Potential of Thermal EM Radiation Spectrometer: “prototype” in-medium spectral function, hadron-to-quark transition Chiral Restoration: Weinberg + QCD sum rules, lattice QCD (  B ~0!) + perturbative limit Quality control: rates (constraints, continuity), medium evolution, consistency SIS-SPS-RHIC-LHC, … Needed: high-quality data to determine spectral shape, then use with flow diagnostics (Non-) Redundancy of RHIC and LHC critical

25 4.7 Elliptic Flow Diagnostics (RHIC) maximum structure due to late  decays [Chatterjee et al ‘07, Zhuang et al ‘09] [He et al ‘12]

26 4.1.3 Mass Spectra as Thermometer Overall slope T~150-200MeV (true T, no blue shift!) [NA60, CERN Courier Nov. 2009] Emp. scatt. ampl. + T-  approximation Hadronic many-body Chiral virial expansion Thermometer

27 2.3.2 NA60 Mass Spectra: p t Dependence more involved at p T >1.5GeV: Drell-Yan, primordial/freezeout , … M  [GeV]

28 5.2 Chiral Restoration Window at LHC low-mass spectral shape in chiral restoration window: ~60% of thermal low-mass yield in “chiral transition region” (T=125-180MeV) enrich with (low-) p t cuts

29 4.3 Dimuon p t -Spectra and Slopes: Barometer theo. slopes originally too soft increase fireball acceleration, e.g. a ┴ = 0.085/fm → 0.1/fm insensitive to T c =160-190MeV Effective Slopes T eff

30 2.) Chiral Symmetry Breaking in Vacuum  “Higgs Mechanism”, Condensates + Mass Gap in QCD  Hadron Spectrum, Chiral Partners + Sum Rules 3.) EM Spectral Function in Medium  Hadronic Theory  QGP + Lattice QCD 4.) Highlights of EM Probes in Heavy-Ion Collisions  Spectro-, Thermo-, Chrono- + Baro-meter  Thermal Photons 5.) Low-Mass Dileptons at LHC  Mass Spectra + Collectivity 6.) Conclusions Outline

31 5.1 Thermal Dileptons at LHC charm comparable, accurate (in-medium) measurement critical low-mass spectral shape in chiral restoration window

32 2.2 EM Probes at SPS all calculated with the same e.m. spectral function! thermal source: T i ≈210MeV, HG-dominated,  -meson melting!

33 2.) Transport: Electric Conductivity hadronic theories (T~150MeV): - chiral pert. theory (pion gas):  em / T ~ 0.11 e 2 - hadronic many-body theory:  em / T ~ 0.09 e 2 [Fernandez-Fraile+ Gomez-Nicola ’07] lattice QCD (T ~ (1.5-3) T c ):  em /T ~ (0.26±0.02) e 2 [Gupta ’04, Aarts et al ’07, Ding et al. ‘11] soft-photon limit of thermal emission rate EM Susceptibility ( → charge fluctuations):  Q 2    Q  2 = χ em = Π em (q 0 =0,q→0)

34 5.2 Intermediate-Mass Dileptons: Thermometer use invariant continuum radiation (M>1GeV): no blue shift, T slope = T ! independent of partition HG vs QGP (dilepton rate continuous/dual) initial temperature T i ~ 190-220 MeV at CERN-SPS Thermometer

35 4.7.2 Light Vector Mesons at RHIC + LHC baryon effects important even at  B,tot = 0 : sensitive to  Btot =   +  B (  -N and  -N interactions identical)  also melts,  more robust ↔ OZI - 

36 5.3 Intermediate Mass Emission: “Chiral Mixing” = = low-energy pion interactions fixed by chiral symmetry mixing parameter [Dey, Eletsky +Ioffe ’90] 0 0 0 0 degeneracy with perturbative spectral fct. down to M~1GeV physical processes at M≥ 1GeV:  a 1 → e + e  etc. (“4  annihilation”)

37 3.2 Dimuon p t -Spectra and Slopes: Barometer modify fireball evolution: e.g. a ┴ = 0.085/fm → 0.1/fm both large and small T c compatible with excess dilepton slopes pions: T ch =175MeV a ┴ =0.085/fm pions: T ch =160MeV a ┴ =0.1/fm

38 2.3.2 Acceptance-Corrected NA60 Spectra more involved at p T >1.5GeV: Drell-Yan, primordial/freezeout , … M  [GeV]

39 4.4.3 Origin of the Low-Mass Excess in PHENIX? QGP radiation insufficient: space-time, lattice QGP rate + resum. pert. rates too small - “baked Alaska” ↔ small T - rapid quench+large domains ↔ central A-A -  therm +  DCC → e + e  ↔ M~0.3GeV, small p t must be of long-lived hadronic origin Disoriented Chiral Condensate (DCC)? Lumps of self-bound pion liquid? Challenge: consistency with hadronic data, NA60 spectra! [Bjorken et al ’93, Rajagopal+Wilczek ’93] [Z.Huang+X.N.Wang ’96 Kluger,Koch,Randrup ‘98]

40 2.3.3 Spectrometer III: Before Acceptance Correction Discrimination power much reduced can compensate spectral “deficit” by larger flow: lift pairs into acceptance hadr. many-body + fireball emp. ampl. + “hard” fireball schem. broad./drop. + HSD transport chiral virial + hydro

41 4.2 Improved Low-Mass QGP Emission LO pQCD spectral function:  V (q 0,q) = 6 ∕ 9 3M 2 /2  1+Q HTL (q 0 )] 3-momentum augmented lattice-QCD rate (finite  rate)

42 4.4.1 Variations in QGP Radiation improvements in QGP rate insufficient

43 4.4.2 Variations in Fireball Properties variations in space-time evolution only significant in (late) hadronic phase

44 4.1 Nuclear Photoproduction:  Meson in Cold Matter  + A → e + e  X [CLAS+GiBUU ‘08] E  ≈1.5-3 GeV  e+ee+e  extracted “in-med”  -width   ≈ 220 MeV Microscopic Approach: Fe - Ti  N  product. amplitude in-med.  spectral fct. + M [GeV] [Riek et al ’08, ‘10] full calculation fix density 0.4  0  -broadening reduced at high 3-momentum; need low momentum cut!

45 1.2 Intro-II: EoS and Particle Content Hadron Resonance Gas until close to T c - but far from non-interacting: short-lived resonances R: a + b → R → a + b,  R ≤ 1 fm/c Parton Quasi-Particles shortly above T c - but large interaction measure I(T) =  -3P  both “phases” strongly coupled (hydro!): - large interaction rates → large collisional widths - resonance broadening → melting → quarks - broad parton quasi-particles - “Feshbach” resonances around T c (coalescence!)

46 2.3.6 Hydrodynamics vs. Fireball Expansion very good agreement between original hydro [Dusling/Zahed] and fireball [Hees/Rapp]

47 2.1 Thermal Electromagnetic Emission EM Current-Current Correlation Function: e+ e-e+ e- γ Im Π em (M,q) Im Π em (q 0 =q) Thermal Dilepton and Photon Production Rates: Im  em ~ [ImD  + ImD  /10 + ImD  /5] Low Mass:   -meson dominated

48 4.2 Low-Mass Dileptons: Chronometer first “explicit” measurement of interacting-fireball lifetime:  FB ≈ (7±1) fm/c In-In N ch >30


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