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Using Higher Moments of Fluctuations and their Ratios in the Search for the QCD Critical Point

Using Higher Moments of Fluctuations and their Ratios in the Search for the QCD Critical Point. Christiana Athanasiou , MIT 4 work with: Krishna Rajagopal (MIT) Misha Stephanov (University of Illinois). Outline. Introduction. Critical Contribution to Particle Multiplicity Fluctuations

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Using Higher Moments of Fluctuations and their Ratios in the Search for the QCD Critical Point

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  1. Using Higher Moments of Fluctuations and their Ratios in the Search for the QCD Critical Point Christiana Athanasiou, MIT 4 work with: Krishna Rajagopal (MIT) MishaStephanov (University of Illinois)

  2. Outline • Introduction • Critical Contribution to Particle Multiplicity Fluctuations • Ratios of Fluctuation Observables • Summary

  3. QCD Phase Diagram T / MeV Quark-Gluon Plasma Lattice simulations ~ 170 crossover Models Critical point Hadron gas Color Superconductor nuclear matter vacuum 0 ~ 940 μB / MeV

  4. Heavy-Ion Collision Experiments • Locating the critical point from first-principles – hard • Heavy-Ion Collision Experiments • RHIC: Au-Au collisions at • Momentum asymmetry collective flow • strongly-coupled QGP

  5. QCD Phase Diagram T / MeV RHIC energy scan Quark-Gluon Plasma crossover ~ 170 Critical point Hadron gas Color Superconductor nuclear matter vacuum 0 ~ 940 μB / MeV

  6. Heavy-Ion Collision Experiments - continued • As QGP expands and cools, it follows trajectories with approx.

  7. QCD Phase Diagram T / MeV RHIC energy scan Quark-Gluon Plasma crossover ~ 170 Critical point Hadron gas Color Superconductor nuclear matter vacuum 0 ~ 940 μB / MeV

  8. Heavy-Ion Collision Experiments 2 • As QGP expands and cools, it follows trajectories with approx. • Chemical freeze-out: system dilute enough that particle numbers freeze • Detector “sees” particle multiplicities from freeze-out conditions • To maximize critical point (CP) effects vary to get freeze-out point near CP • Find observables that are sensitive to proximity to the CP Event-by-Event fluctuations

  9. Outline • Introduction • Critical Contribution to Particle Multiplicity Fluctuations • Ratios of Fluctuation Observables • Summary

  10. Critical Mode Fluctuations Critical Mode • Critical mode - σ : order parameter of the chiral phase transition • Develops long wavelength correlations at the CP • Effective action • Near the CP: with • dimensionless and known in the Ising universality class • Correlation length diverges at the CP

  11. Critical Mode Fluctuations • σ couples to pions and protons: • Critical mode fluctuations affect • Particle multiplicity fluctuations • Momentum distributions • Ratios, etc… • at CP in the thermodynamic limit • Finite system lifetime compared to away from the CP (Berdnikov,Rajagopal 00) • of these particles.

  12. Measuring fluctuations in particle multiplicities measure the mean, variance, skewness, etc… • Can repeat these calculations for pions, net protons, etc • Want to obtain the critical contribution to these quantities • We will use cumulants, e.g.:

  13. Critical contribution to pion/proton correlators ξ2 ξ9/2 + … ξ7 (Rajagopal, Shuryak, Stephanov 99, Stephanov 08)

  14. Net protons and mixed correlators • Net protons: • Adaptprevious expressions by replacing: • Can also calculate mixed correlators, e.g. 2 pion – 2 proton: • Note: correlators depend on 5 parameters: • which have large uncertainties

  15. Calculating multiplicity cumulants • Second cumulant – variance: • Normalizing: • For mixed cumulants with iprotons and jpions: ignore • Non-critical contribution to ωipjπ= δi,i+j+ δj,i+j+ (few %) Poisson • Bose-Einstein effects • Other interactions • Etc..

  16. Multiplicity cumulants – critical point signature • Higher cumulants depend stronger on ξ: • As we approach the CP ξ increases and then decreases as we move away from it • CP signature: Non-monotonic behavior, as a function of collision energy, of multiplicity cumulants • E.g. toy example

  17. Multiplicity cumulants – example plots Parametrization(Cleymans et al 05): and using

  18. Data on net proton cumulants (STAR Collaboration 2010) where

  19. Critical contribution to proton ω4

  20. Multiplicity cumulants – movie Changing the critical μB – the location of the CP:

  21. Outline • Introduction • Critical Contribution to Particle Multiplicity Fluctuations • Ratios of Fluctuation Observables • Summary

  22. Uncertainties of parameters • Cumulants depend on 5 non-universal parameters: • have large uncertainties hard to predict the critical contribution to cumulants • By taking ratios of cumulants can cancel some parameter dependence minimize observable uncertainties

  23. Ratios of multiplicity cumulants No parameter dependence Ratios taken after subtracting Poisson and defined

  24. Parameter independent ratios • Parameter and energy independent ratios: • where • All equal to 1 if CP contribution dominates • Poisson contribution: • How to use these ratios: • If one sees peaks in the measured cumulants at some μB • Calculate these ratios around the peak • If equal to 1 Parameter independent way of verifying that the fluctuations you see are due to the CP

  25. Constraining parameters • If CP found, can constrain parameters by measuring cumulant ratios near the CP • Parameters appear in certain combinations in the cumulants can only constraint 4 independent (but not unique) combinations • For example, some choices are: using or using or using using

  26. Outline • Introduction • Critical Contribution to Particle Multiplicity Fluctuations • Ratios of Fluctuation Observables • Summary

  27. Summary • We used particle multiplicity fluctuations as a probe to the location of the CP • Higher cumulants of event-by-event distributions are more sensitive to critical fluctuations • CP signature: Non-monotonic behavior, as a function of collision energy, of multiplicity cumulants • Constructed cumulant ratios to identify the CP location with reduced parameter uncertainties • If CP is found, showed how to use cumulant ratios to constraint the values of the non-universal parameters

  28. Thank you!

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