the challenge of discovering qcd critical point
play

The challenge of discovering QCD critical point M. Stephanov M. - PowerPoint PPT Presentation

The challenge of discovering QCD critical point M. Stephanov M. Stephanov QCD Critical Point ASU 2020 1 / 36 Outline 1 Introduction. Critical point. History. QCD Critical point Heavy-Ion Collisions 2 Equilibrium physics of the QCD


  1. The challenge of discovering QCD critical point M. Stephanov M. Stephanov QCD Critical Point ASU 2020 1 / 36

  2. Outline 1 Introduction. Critical point. History. QCD Critical point Heavy-Ion Collisions 2 Equilibrium physics of the QCD critical point Critical fluctuations Intriguing data from RHIC BES I 3 Non-equilibrium physics of the QCD critical point (work in progress) Hydrodynamics and fluctuations Hydro+ General formalism 4 Summary and Outlook M. Stephanov QCD Critical Point ASU 2020 2 / 36

  3. History Cagniard de la Tour (1822): discovered continuos transition from liquid to vapour by heating alcohol, water, etc. in a gun barrel, glass tubes. M. Stephanov QCD Critical Point ASU 2020 3 / 36

  4. Name Faraday (1844) – liquefying gases: “Cagniard de la Tour made an experiment some years ago which gave me occasion to want a new word.” Mendeleev (1860) – measured vanishing of liquid-vapour surface tension: “Absolute boiling temperature”. Andrews (1869) – systematic studies of many substances established continuity of vapour-liquid phases. Coined the name “critical point”. M. Stephanov QCD Critical Point ASU 2020 4 / 36

  5. Theory van der Waals (1879) – in “On the continuity of the gas and liquid state” (PhD thesis) wrote e.o.s. with a critical point. Smoluchowski, Einstein (1908,1910) – explained critical opalescence. Landau – classical theory of critical phenomena Fisher, Kadanoff, Wilson – scaling, full fluctuation theory based on RG. M. Stephanov QCD Critical Point ASU 2020 5 / 36

  6. Critical opalescence shining laser light through liquid M. Stephanov QCD Critical Point ASU 2020 6 / 36

  7. Critical point – end of phase coexistence – is a ubiquitous phenomenon Water: Is there one in QCD? M. Stephanov QCD Critical Point ASU 2020 7 / 36

  8. Physics of QCD Fundamental constituents – quarks and gluons – are (almost) massless. But hadrons (quasiparticles of QCD) are massive. m proton = E QCD /c 2 This is the origin of almost all of the visible mass in the Universe. Color charges and color forces are “confined” within hadrons. High-energy collisions expose color degrees of freedom and high T environment “liberates” color forces (gluons) and color charges. The resulting new form of matter is Quark-Gluon Plasma. M. Stephanov QCD Critical Point ASU 2020 8 / 36

  9. � μ Is there a CP between QGP and hadron gas phases? M. Stephanov QCD Critical Point ASU 2020 9 / 36

  10. � μ Is there a CP between QGP and hadron gas phases? Q1: Can the two phases continuously transform into each other? Yes. M. Stephanov QCD Critical Point ASU 2020 9 / 36

  11. Is there a CP between QGP and hadron gas phases? Q1: Can the two phases continuously transform into each other? Yes. Lattice QCD at µ B = 0 – a crossover. 300 The Phases of QCD 250 Quark-Gluon Plasma Temperature (MeV) 200 150 Crossover 1 s t O r d e r P h a s e T r a 100 n Critical s i t i o n Point? s a G Color n o r d a H 50 Superconductor Nuclear Vacuum Ma � er 0 0 200 400 600 800 1000 1200 1400 1600 Baryon Chemical Potential μ B (MeV) QCD in crossover region: no quasiparticles (not hadrons, not quarks/gluons). Strongly interacting matter (sQGP). More a liquid than a gas. M. Stephanov QCD Critical Point ASU 2020 9 / 36

  12. � μ Is there a CP between QGP and hadron gas phases? Q2: Is there phase coexistence, i.e., 1st order transition? Likely. M. Stephanov QCD Critical Point ASU 2020 10 / 36

  13. Is there a CP between QGP and hadron gas phases? Q2: Is there phase coexistence, i.e., 1st order transition? Likely. Unfortunately, lattice QCD cannot reach beyond µ B ∼ 2 T . 300 The Phases of QCD 250 Quark-Gluon Plasma Temperature (MeV) 200 150 Crossover 1 s t O r d e r P h a s e T r a 100 n Critical s i t i o n Point? s a G Color n o r d a H 50 Superconductor Nuclear Vacuum Ma � er 0 0 200 400 600 800 1000 1200 1400 1600 Baryon Chemical Potential μ B (MeV) M. Stephanov QCD Critical Point ASU 2020 10 / 36

  14. Is there a CP between QGP and hadron gas phases? Q2: Is there phase coexistence, i.e., 1st order transition? Likely. Unfortunately, lattice QCD cannot reach beyond µ B ∼ 2 T . 300 The Phases of QCD 250 Quark-Gluon Plasma Temperature (MeV) 200 150 Crossover 1 s t O r d e r P h a s e T r a 100 n Critical s i t i o n Point? s a G Color n o r d a H 50 Superconductor Nuclear Vacuum Ma � er 0 0 200 400 600 800 1000 1200 1400 1600 Baryon Chemical Potential μ B (MeV) But 1st order transition (and thus C.P .) is ubiquitous in models of QCD: NJL, RM, Holography, Strong coupl. Lattice QCD, . . . M. Stephanov QCD Critical Point ASU 2020 10 / 36

  15. How can one discover the QCD critical point? Essentially two approaches to discovering the QCD critical point. Each with its own challenges. Lattice simulations. The sign problem restricts reliable lattice calculations to µ B = 0 . Under different assumptions one can estimate the position of the critical point, assuming it exists, by extrapolation from µ = 0 . Heavy-ion collisions. Non-equilibrium. M. Stephanov QCD Critical Point ASU 2020 11 / 36

  16. Heavy-ion collisions vs the Big Bang Similarity: expanding and cooling Difference: One Event vs many events (cosmic variance vs e.b.e. fluctuations) M. Stephanov QCD Critical Point ASU 2020 12 / 36

  17. Similarity: Expansion accompanied by cooling, followed by freezeout. Difference: tunable parameter µ B via √ s . 300 2760 The Phases of QCD 200 √ s = 62.4 GeV 39 250 27 19.6 Quark-Gluon Plasma Temperature (MeV) 14.5 200 11.5 B E S - I I 9.1 150 7.7 1 s t O r d e r P h a s e T r a 100 n Critical s i t i o n Point s a Color G n o r d a H Superconductor 50 Nuclear Vacuum Ma � er 0 0 200 400 600 800 1000 1200 1400 1600 Baryon Chemical Potential μ B (MeV) M. Stephanov QCD Critical Point ASU 2020 13 / 36

  18. Assumption for the next part of this talk H.I.C. are sufficiently close to equilibrium that we can study thermodynamics at freezeout T and µ B — as a first approximation. M. Stephanov QCD Critical Point ASU 2020 14 / 36

  19. Assumption for the next part of this talk H.I.C. are sufficiently close to equilibrium that we can study thermodynamics at freezeout T and µ B — as a first approximation. NB: Event-by-event fluctuations: Heavy-ion collisions create systems which are large (thermody- namic limit), but not too large ( N ∼ 10 2 − 10 4 particles) √ EBE fluctuations are small ( 1 / N ), but measurable. M. Stephanov QCD Critical Point ASU 2020 14 / 36

  20. Outline 1 Introduction. Critical point. History. QCD Critical point Heavy-Ion Collisions 2 Equilibrium physics of the QCD critical point Critical fluctuations Intriguing data from RHIC BES I 3 Non-equilibrium physics of the QCD critical point (work in progress) Hydrodynamics and fluctuations Hydro+ General formalism 4 Summary and Outlook M. Stephanov QCD Critical Point ASU 2020 15 / 36

  21. What are the signatures of the critical point? EBE fluctuations vs √ s [PRL81(1998)4816] Equilibrium = maximum entropy. P ( σ ) ∼ e S ( σ ) (Einstein 1910) M. Stephanov QCD Critical Point ASU 2020 16 / 36

  22. What are the signatures of the critical point? EBE fluctuations vs √ s [PRL81(1998)4816] Equilibrium = maximum entropy. P ( σ ) ∼ e S ( σ ) (Einstein 1910) M. Stephanov QCD Critical Point ASU 2020 16 / 36

  23. What are the signatures of the critical point? EBE fluctuations vs √ s [PRL81(1998)4816] Equilibrium = maximum entropy. P ( σ ) ∼ e S ( σ ) (Einstein 1910) At the critical point S ( σ ) “flattens”. And χ ≡ � δσ 2 � V → ∞ . CLT? M. Stephanov QCD Critical Point ASU 2020 16 / 36

  24. What are the signatures of the critical point? EBE fluctuations vs √ s [PRL81(1998)4816] Equilibrium = maximum entropy. P ( σ ) ∼ e S ( σ ) (Einstein 1910) At the critical point S ( σ ) “flattens”. And χ ≡ � δσ 2 � V → ∞ . CLT? δσ is not an average of ∞ many uncorrelated contributions: ξ → ∞ In fact, � δσ 2 � ∼ ξ 2 /V . M. Stephanov QCD Critical Point ASU 2020 16 / 36

  25. Higher order cumulants n > 2 cumulants (shape of P ( σ ) ) depend stronger on ξ . E.g., � σ 2 � ∼ ξ 2 while κ 4 = � σ 4 � c ∼ ξ 7 [PRL102(2009)032301] For n > 2 , sign depends on which side of the CP we are. This dependence is also universal. [PRL107(2011)052301] Using Ising model variables: M. Stephanov QCD Critical Point ASU 2020 17 / 36

  26. Mapping Ising to QCD and observables near CP Equilibrium κ 4 vs µ B and T : In QCD ( t, H ) → ( µ − µ CP , T − T CP ) Pradeep-MS 1905.13247 M. Stephanov QCD Critical Point ASU 2020 18 / 36

  27. Mapping Ising to QCD and observables near CP Equilibrium κ 4 vs µ B and T : In QCD ( t, H ) → ( µ − µ CP , T − T CP ) Pradeep-MS 1905.13247 κ n ( N ) = N + O ( κ n ( σ )) 1104.1627 M. Stephanov QCD Critical Point ASU 2020 18 / 36

  28. Beam Energy Scan I: intriguing hints Equilibrium κ 4 vs µ B and T : M. Stephanov QCD Critical Point ASU 2020 19 / 36

  29. Beam Energy Scan I: intriguing hints Equilibrium κ 4 vs µ B and T : M. Stephanov QCD Critical Point ASU 2020 19 / 36

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend