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What can we extract from Thermal EM Radiation in Heavy-Ion Collisions?

This presentation explores the use of thermal electromagnetic (EM) radiation in heavy-ion collisions to gather information about the fireball, degrees of freedom, chiral symmetry restoration, transport properties, and more. The talk discusses the use of the EM spectral function and its connection to the quark-to-hadron transition, chiral symmetry restoration, and electric conductivity. It also explores the application of dilepton rates and the lifetime and temperature of the fireball. The presentation concludes with the progress made in understanding these phenomena and the potential for using dilepton radiation as a precision tool.

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What can we extract from Thermal EM Radiation in Heavy-Ion Collisions?

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  1. What can we extract fromThermal EM Radiation in Heavy-Ion Collisions? Ralf Rapp Cyclotron Institute + Dept of Phys & Astro Texas A&M University College Station, USA International School on Nuclear Physics, 38th Course Erice (Sicily, Italy), 16.-24.09.16

  2. 1.) Intro: EM Spectral Function to Probe Fireball • Thermal Dilepton Rate ImΠem(M,q;mB,T) e+e-→ hadrons r Im Pem(M) / M2 e+ e- e+ e- M [GeV] • Hadronic Resonances - change in degrees of freedom? - restoration of chiral symmetry? • Continuum - temperature? • Low-q0,q limit: transport coefficient (charge)? • Total yields: fireball lifetime?

  3. 1.2 30 Years of Dileptons in Heavy-Ion Collisions <Nch>=120 • Robust understanding across QCD phase diagram: QGP + hadronic radiation with meltingr resonance

  4. Outline 1.) Introduction 2.) Degrees of Freedom of the Medium  Quark-to-Hadron Transition 3.) Chiral Symmery Restoration  QCD +Weinberg Sum Rules  Other Multiplets 4.) Transport Properties  Electric Conductivity 5.) Phenomenological Tool  Fireball Lifetime + Temperature (Excitation Fct.)  Fireball in pA? 6.) Conclusions

  5. 2.) Dilepton Rates and Degrees of FreedomdRee /dM2 ~ ∫d3q f B(q0;T) ImPem • r-meson resonance “melts” • spectral function merges into QGP description • Direct evidence for transition hadrons → quarks + gluons - [qq→ee] [HTL] dRee/d4q 1.4Tc (quenched) q=0 [Ding et al ’10] [RR,Wambach et al ’99]

  6. Outline 1.) Introduction 2.) Degrees of Freedom of the Medium  Quark-to-Hadron Transition 3.) Chiral Symmery Restoration  QCD +Weinberg Sum Rules  Other Multiplets 4.) Transport Properties  Electric Conductivity 5.) Phenomenological Tool  Fireball Lifetime + Temperature (Excitation Fct.)  Fireball in pA? 6.) Conclusions

  7. 3.1 QCD + Weinberg Sum Rules [Hatsuda+Lee’91, Asakawa+Ko ’93, Leupold et al ’98, …] r a1 [Weinberg ’67, Das et al ’67; Kapusta+Shuryak ‘94] Dr = rV -rA • accurately satisfied in vacuum • In Medium: condensates from hadron resonance gas, constrained by lattice-QCD T [GeV]

  8. 3.1.2 QCD + Weinberg Sum Rules in Medium → Search for solution for axial-vector spectral function [Hohler +RR ‘13] • quantitatively compatible with (approach to) chiral restoration • strong constraints by combining SRs • Chiral mass splitting “burns off”, resonances melt

  9. 3.2 Lattice-QCD Results for N(940)-N*(1535) Euclidean Correlator Ratios Exponential Mass Extraction “N*(1535)” “Nucleon” R=∫(G+-G-)/(G++G-) [Aarts et al ‘15] • also indicates MN*(T) → MN (T) ≈ MNvac • see also talk by R.-A. Tripolt

  10. Outline 1.) Introduction 2.) Degrees of Freedom of the Medium  Quark-to-Hadron Transition 3.) Chiral Symmery Restoration  QCD +Weinberg Sum Rules  Other Multiplets 4.) Transport Properties  Electric Conductivity 5.) Phenomenological Tool  Fireball Lifetime + Temperature (Excitation Fct.)  Fireball in pA? 6.) Conclusions

  11. 4.) Electric Conductivity • Similar behavior for different transport? h/s ~ (2pT) DsHF ~ sEM/T • Probes soft limit of EM spectral function sEM(T) = - e2 limq0→0 [ ∂/∂q0 Im PEM(q0,q=0;T) ] • Need density-squared contributions • Non-trivial for vertex corrections (usually evaluated with vacuum propagators) • Start out with pion gas: dress pions in r-cloud + vertex corrections [Atchison+RR in prog.]

  12. 4.2 Low-Energy Limit of Spectral Function Pion Gas Perturbative QGP T=150MeV ar = 0.7 ar = 1.2 ar = 2.7 0 2 4 6 8 10 q0 [MeV] [Moore+Robert ‘06] • conductivity peak strongly smeared out • suggestive for strongly coupled system

  13. 4.3 Conductivity: Comparison to other Approaches in-med.pgas → [Greif et al ‘16] • in-medium pion gas well above SYM limit • interactions with anti-/baryons likely to reduce it

  14. Outline 1.) Introduction 2.) Degrees of Freedom of the Medium  Quark-to-Hadron Transition 3.) Chiral Symmery Restoration  QCD +Weinberg Sum Rules  Other Mutiplets 4.) Transport Properties  Electric Conductivity 5.) Phenomenological Tool  Fireball Lifetime + Temperature (Excitation Fct.)  Fireball in pA? 6.) Conclusions

  15. 5.1 Fireball Lifetime Excitation Function of Low-Mass Dilepton Excess Yield 1000 [STAR ‘15] [RR+vanHees ‘14] • Low-mass excess tracks lifetime well (medium effects!) • Tool for critical point search?

  16. 5.2 Fireball Temperature Slope of Intermediate-Mass Excess Dileptons • unique ``early” temperature measurement (no blue-shift!) • Ts approaches Ti toward lower energies • first-order “plateau” at BES-II/CBM?

  17. 5.3 Low-Mass Dileptons in p-Pb (5.02GeV) • Thermal radiation at ~10% of cocktail • follows excess-lifetime systematics • photons [Shen et al ‘15]

  18. 6.) Conclusions • Explicit evidence for parton-hadron transition (rmelting) • Progress in understanding mechanisms of chiral restoration - evaporation of chiral mass r-a1 splitting (sum rules, MYM) • Electric conductivity suggests strongly coupled medium • Dilepton radiation as a precision tool to measure - fireball lifetime (low mass), including pA - early temperature (intermediate mass; no blue-shift)

  19. 4.3 Comparison to Data: RHIC Ideal Hydro Viscous Hydro [van Hees et al, ‘11, ’14] [Paquet et al ’16] • same rates + intial flow  similar results from various evolution models

  20. 3.2 Massive Yang-Mills in Hot Pion Gas Temperature progression of vector + axialvector spectral functions • supports “burning” of chiral-mass splitting as mechanism for chiral restoration [as found in sum rule analysis]

  21. 4.1 Initial Flow + Thermal Photon-v2 Bulk-Flow Evolution Direct-Photon v2 Ideal Hydro 0-20% Au-Au • initial radial flow: - accelerates bulk v2 - harder radiation spectra (pheno.: coalescence, multi-strange f.o.) • much enhances thermal-photon v2 [He et al ’14]

  22. 4.2 Thermal Photon Rates • ``Cocktail” of hadronic sources (available in parameterized form) • Sizable new hadronic sources: pr → gw , pw → gr , rw → gp [Heffernan et al ‘15] [Holt,Hohler+RR in prep] • Hadronic emission rate close to QGP-AMY • semi-QGP much more suppressed [Pisarski et al ‘14]

  23. 3.2 Massive Yang-Mills Approach in Vaccum • Gauge r + a1 into chiral pion lagrangian: • problems with vacuum phenomenology → global gauge? • Recent progress: - full rpropagator in a1 selfenergy - vertex corrections to preserve PCAC: [Urban et al ‘02, Rischke et al ‘10] [Hohler +RR ‘14] • enables fit to t-decay data! • local-gauge approach viable • starting point for addressing chiral restoration in medium

  24. 4.3.2 Photon Puzzle!? • Tslopeexcess ~240 MeV • blue-shift: Tslope ~ T √(1+b)/(1-b) T ~ 240/1.4 ~170 MeV

  25. 4.1.2 Sensitivity to Spectral Function In-Medium r-Meson Width • avg. Gr(T~150MeV)~370MeVGr (T~Tc) ≈ 600 MeV → mr • driven by (anti-) baryons Mmm [GeV]

  26. 4.2 Low-Mass Dileptons: Chronometer In-In Nch>30 • first “explicit” measurement of interacting-fireball lifetime: tFB≈ (7±1) fm/c

  27. 4.1 Prospects I: Spectral Shape at mB ~ 0 STAR Excess Dileptons [STAR ‘14] • rather different spectral shapes compatible with data • QGP contribution?

  28. 4.5 QGP Barometer: Blue Shift vs. Temperature SPS RHIC • QGP-flow driven increase of Teff ~ T + M (bflow)2 at RHIC • high pt: high T wins over high-flow r’s → minimum (opposite to SPS!) • saturates at “true” early temperature T0 (no flow)

  29. 2.3 Low-Mass e+e- Excitation Function: 20-200 GeV P. Huck et al. [STAR], QM14 • compatible with predictions from melting r meson • “universal” source around Tpc

  30. 3.3.2 Effective Slopes of Thermal Photons Thermal Fireball Viscous Hydro [van Hees,Gale+RR ’11] [S.Chen et al ‘13] • thermal slope can only arise from T ≤ Tc(constrained by • closely confirmed by hydro hadron data) • exotic mechanisms: glasma BE? Magnetic fields+ UA(1)? [Liao at al ’12, Skokov et al ’12, F. Liu ’13,…]

  31. 2.2 Transverse-Momentum Dependence pT -Sliced Mass Spectra mT -Slopes x100 • spectral shape as function of pair-pT • entangled with transverse flow (barometer)

  32. 3.1.2 Transverse-Momentum Spectra: Baro-meter Effective Slope Parameters RHIC SPS QGP HG [Deng,Wang, Xu+Zhuang ‘11] • qualitative change from SPS to RHIC: flowing QGP • true temperature “shines” at large mT

  33. 2.2 Chiral Condensate + r-Meson Broadening > Sp effective hadronic theory > - Sp • h = mq h|qq|h > 0 contains quark core + pion cloud = Shcore + Shcloud ~ ++ • matches spectral medium effects: resonances + pion cloud • resonances + chiral mixing drive r-SF toward chiral restoration r - - qq / qq0

  34. 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-) pt cuts

  35. 4.4 Elliptic Flow of Dileptons at RHIC • maximum structure due to late r decays [He et al ‘12] [Chatterjee et al ‘07, Zhuang et al ‘09]

  36. 3.3.2 Fireball vs. Viscous Hydro Evolution [van Hees, Gale+RR ’11] [S.Chen et al ‘13] • very similar!

  37. 4.7.2 Light Vector Mesons at RHIC + LHC • baryon effects important even at rB,tot= 0 : sensitive to rBtot= rB + rB (r-N and r-N interactions identical) • w also melts, f more robust ↔ OZI - -

  38. 4.1 Nuclear Photoproduction: rMeson in Cold Matter g + A → e+e- X • extracted “in-med” r-width Gr≈ 220 MeV e+ e- Eg≈1.5-3 GeV g r [CLAS+GiBUU ‘08] • Microscopic Approach: + in-med. r spectral fct. product. amplitude full calculation fix density 0.4r0 Fe-Ti r g N [Riek et al ’08, ‘10] M[GeV] • r-broadening reduced at high 3-momentum; need low momentum cut!

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