Quantum Opacity, RHIC HBT Puzzle, and the Chiral Phase Transition RHIC Physics, HBT and RHIC HBT Puzzle Quantum mech. treatment of optical potential, U.

Slides:



Advertisements
Similar presentations
Zi-Wei Lin (ECU) 28th WWND, Puerto Rico April 10, Update of Initial Conditions in A Multiple Phase Transport (AMPT) Model Zi-Wei Lin Department.
Advertisements

Mass, Quark-number, Energy Dependence of v 2 and v 4 in Relativistic Nucleus- Nucleus Collisions Yan Lu University of Science and Technology of China Many.
Elliptic flow of thermal photons in Au+Au collisions at 200GeV QNP2009 Beijing, Sep , 2009 F.M. Liu Central China Normal University, China T. Hirano.
TJH: ISMD 2005, 8/9-15 Kromeriz, Czech Republic TJH: 1 Experimental Results at RHIC T. Hallman Brookhaven National Laboratory ISMD Kromeriz, Czech Republic.
The RHIC HBT Puzzle, Chiral Symmetry Restoration, and Pion Opacity John G. Cramer (with Gerald A. Miller) University of Washington Seattle, Washington,
K*(892) Resonance Production in Au+Au and Cu+Cu Collisions at  s NN = 200 GeV & 62.4 GeV Motivation Analysis and Results Summary 1 Sadhana Dash Institute.
In relativistic heavy ion collisions a high energy density matter Quark-Gluon Plasma (QGP) may be formed. Various signals have been proposed which probe.
ICPAQGP, Kolkata, February 2-6, 2015 Itzhak Tserruya PHENIX highlights.
CERN May Heavy Ion Collisions at the LHC Last Call for Predictions Initial conditions and space-time scales in relativistic heavy ion collisions.
Relativistic Heavy-Ion Collisions: Recent Results from RHIC David Hardtke LBNL.
DNP03, Tucson, Oct 29, Kai Schweda Lawrence Berkeley National Laboratory for the STAR collaboration Hadron Yields, Hadrochemistry, and Hadronization.
STAR Patricia Fachini 1 Brookhaven National Laboratory Motivation Data Analysis Results Conclusions Resonance Production in Au+Au and p+p Collisions at.
The DWEF Model: Refractive Distortions of HBT John G. Cramer (with Gerald A. Miller) University of Washington Seattle, Washington, USA John G. Cramer (with.
A. ISMD 2003, Cracow Indication for RHIC M. Csanád, T. Csörgő, B. Lörstad and A. Ster (Budapest & Lund) Buda-Lund hydro fits to.
We distinguish two hadronization mechanisms:  Fragmentation Fragmentation builds on the idea of a single quark in the vacuum, it doesn’t consider many.
Addition of a potential to the Klein-Gordon equation to determine ‘fireball’ size HBT Pion Correlations Laniece Miller – Clarkson University Dr. Ralf Rapp.
STAR Looking Through the “Veil of Hadronization”: Pion Entropy & PSD at RHIC John G. Cramer Department of Physics University of Washington, Seattle, WA,
Resonance Dynamics in Heavy Ion Collisions 22nd Winter Workshop on Nuclear Dynamics , La Jolla, California Sascha Vogel, Marcus Bleicher UrQMD.
Helen Caines Yale University SQM – L.A.– March 2006 Using strange hadron yields as probes of dense matter. Outline Can we use thermal models to describe.
DPG spring meeting, Tübingen, March Kai Schweda Lawrence Berkeley National Laboratory for the STAR collaboration Recent results from STAR at RHIC.
STAR Pion Entropy and Phase Space Density at RHIC John G. Cramer Department of Physics University of Washington, Seattle, WA, USA Second Warsaw Meeting.
Hadronic Resonances in Heavy-Ion Collisions at ALICE A.G. Knospe for the ALICE Collaboration The University of Texas at Austin 25 July 2013.
ISMD31 / Sept. 4, 2001 Toru Sugitate / Hiroshima Univ. The 31 st International Symposium on Multiparticle Dynamics on 1-7, Sept in Datong, China.
Particle Spectra at AGS, SPS and RHIC Dieter Röhrich Fysisk institutt, Universitetet i Bergen Similarities and differences Rapidity distributions –net.
Masashi Kaneta, LBNL Masashi Kaneta for the STAR collaboration Lawrence Berkeley National Lab. First results from STAR experiment at RHIC - Soft hadron.
Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)
In collaboration with Rupa Chatterjee. Direct photons are penetrating probes for the bulk matter produced in nuclear collisions, as they do not interact.
KROMĚŘĺŽ, August 2005WPCF Evolution of observables in hydro- and kinetic models of A+A collisions Yu. Sinyukov, BITP, Kiev.
Spectra Physics at RHIC : Highlights from 200 GeV data Manuel Calderón de la Barca Sánchez ISMD ‘02, Alushta, Ukraine Sep 9, 2002.
S C O T T PRATTPRATT M I C H I G A N STATESTATE U N I V E R S I Y T S U N A M I THETHE B T PUZZLEPUZZLE ANDAND T H E R H I C.
Matter System Size and Energy Dependence of Strangeness Production Sevil Salur Yale University for the STAR Collaboration.
Jaipur February 2008 Quark Matter 2008 Initial conditions and space-time scales in relativistic heavy ion collisions Yu. Sinyukov, BITP, Kiev (with participation.
EXPERIMENTAL EVIDENCE FOR HADRONIC DECONFINEMENT In p-p Collisions at 1.8 TeV * L. Gutay - 1 * Phys. Lett. B528(2002)43-48 (FNAL, E-735 Collaboration Purdue,
Roy A. Lacey (SUNY Stony Brook ) C ompressed B aryonic at the AGS: A Review !! C ompressed B aryonic M atter at the AGS: A Review !!
Solving the RHIC HBT Puzzle John G. Cramer and Gerald A. Miller University of Washington Seattle, Washington John G. Cramer and Gerald A. Miller University.
1 Jeffery T. Mitchell – Quark Matter /17/12 The RHIC Beam Energy Scan Program: Results from the PHENIX Experiment Jeffery T. Mitchell Brookhaven.
Helen Caines Yale University Soft Physics at the LHC - Catania - Sept Questions for the LHC resulting from RHIC Strangeness Outline Chemistry Yields.
Hadron Collider Physics 2012, 12/Nov/2012, KyotoShinIchi Esumi, Univ. of Tsukuba1 Heavy Ion results from RHIC-BNL ShinIchi Esumi Univ. of Tsukuba Contents.
Does HBT interferometry probe thermalization? Clément Gombeaud, Tuomas Lappi and J-Y Ollitrault IPhT Saclay WPCF 2009, CERN, October 16, 2009.
Masashi Kaneta, First joint Meeting of the Nuclear Physics Divisions of APS and JPS 1 / Masashi Kaneta LBNL
Two freeze-out model for the hadrons produced in the Relativistic Heavy-Ion Collisions. New Frontiers in QCD 28 Oct, 2011, Yonsei Univ., Seoul, Korea Suk.
Heavy-Ion Physics - Hydrodynamic Approach Introduction Hydrodynamic aspect Observables explained Recombination model Summary 전남대 이강석 HIM
Inha Nuclear Physics Group Quantum Opacity and Refractivity in HBT Puzzle Jin-Hee Yoon Dept. of Physics, Inha University, Korea John G. Cramer,
School of Collective Dynamics in High-Energy CollisionsLevente Molnar, Purdue University 1 Effect of resonance decays on the extracted kinetic freeze-out.
R. Lednicky: Joint Institute for Nuclear Research, Dubna, Russia I.P. Lokhtin, A.M. Snigirev, L.V. Malinina: Moscow State University, Institute of Nuclear.
Scott PrattMichigan State University Femtoscopy: Theory ____________________________________________________ Scott Pratt, Michigan State University.
Roy A. Lacey, Stony Brook, ISMD, Kromĕříž, Roy A. Lacey What do we learn from Correlation measurements at RHIC.
Budapest, 4-9 August 2005Quark Matter 2005 HBT search for new states of matter in A+A collisions Yu. Sinyukov, BITP, Kiev Based on the paper S.V. Akkelin,
Itzhak Tserruya Initial Conditions at RHIC: an Experimental Perspective RHIC-INT Workshop LBNL, May31 – June 2, 2001 Itzhak Tserruya Weizmann.
1 Probing dense matter at extremely high temperature Rudolph C. Hwa University of Oregon Jiao Tong University, Shanghai, China April 20, 2009.
Understanding the rapidity dependence of v 2 and HBT at RHIC M. Csanád (Eötvös University, Budapest) WPCF 2005 August 15-17, Kromeriz.
Andras. Ster, RMKI, Hungary ZIMANYI-SCHOOL’09, Budapest, 01/12/ Azimuthally Sensitive Buda-Lund Hydrodynamic Model and Fits to Spectra, Elliptic.
Measurement of Azimuthal Anisotropy for High p T Charged Hadrons at RHIC-PHENIX The azimuthal anisotropy of particle production in non-central collisions.
Bulk properties at RHIC Olga Barannikova (Purdue University) Motivation Freeze-out properties at RHIC STAR perspective STAR  PHENIX, PHOBOS Time-span.
Christina MarkertHirschegg, Jan 16-22, Resonance Production in Heavy Ion Collisions Christina Markert, Kent State University Resonances in Medium.
24 June 2007 Strangeness in Quark Matter 2007 STAR 2S0Q0M72S0Q0M7 Strangeness and bulk freeze- out properties at RHIC Aneta Iordanova.
Helen Caines Yale University Strasbourg - May 2006 Strangeness and entropy.
PHENIX Results from the RHIC Beam Energy Scan Brett Fadem for the PHENIX Collaboration Winter Workshop on Nuclear Dynamics 2016.
Hadron Spectra and Yields Experimental Overview Julia Velkovska INT/RHIC Winter Workshop, Dec 13-15, 2002.
A generalized Buda-Lund model M. Csanád, T. Csörgő and B. Lörstad (Budapest & Lund) Buda-Lund model for ellipsoidally symmetric systems and it’s comparison.
Soft physics in PbPb at the LHC Hadron Collider Physics 2011 P. Kuijer ALICECMSATLAS Necessarily incomplete.
What do the scaling characteristics of elliptic flow reveal about the properties of the matter at RHIC ? Michael Issah Stony Brook University for the PHENIX.
Duke University 野中 千穂 Hadron production in heavy ion collision: Fragmentation and recombination in Collaboration with R. J. Fries (Duke), B. Muller (Duke),
HBT results from a rescattering model Tom Humanic Ohio State University WPCF 2005 August 17, 2005.
Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Femtoscopy in relativistic heavy-ion collisions as a probe of system collectivity Adam Kisiel CERN.
Pion Opacity, Chiral Symmetry Restoration, and RHIC HBT John G. Cramer (with Gerald A. Miller) University of Washington Seattle, Washington, USA John G.
Hydro + Cascade Model at RHIC
Experimental Studies of Quark Gluon Plasma at RHIC
Outline First of all, there’s too much data!! BRAHMS PHOBOS PHENIX
Masahiro Konno (Univ. of Tsukuba) for the PHENIX Collaboration Contact
Presentation transcript:

Quantum Opacity, RHIC HBT Puzzle, and the Chiral Phase Transition RHIC Physics, HBT and RHIC HBT Puzzle Quantum mech. treatment of optical potential, U (Chiral symmetry), DWEF Reproducing π data Summary, future plans Phys.Rev.Lett.94:102302,2005 and J.Phys.G34: ,2007 Gerald Miller and John Cramer, UW

The RHIC HBT Puzzle Pratt’s talk- can’t fit entropy and HBT radii with same model Hydrodynamics works BUT NOT FOR HBT

q out q side q long R side R long R out p1p1 p2p2 p2p2 + p2p2 p1p1 q Quantum mechanical interference-space time separation of source q=p 1 -p 2 K=(p 1 +p 2 )/2 C(q,K)   p 1,p 2 )   p 1  p 2 ))-1 ~ λ(1-q 2 L R 2 L -q 2 S R 2 S –q 2 O R 2 O ) HBT- 2 particle interferometry Hydrodynamics predicts big R O /R S, Data R O /R S about 1 HBT puzzle

Old Formalism  source current density =J  Chaotic sources, Shuryak ‘74 S 0 ~ σ(p 1 )

Source Properties “Hydro- Inspired” Emission Function (Bose-Einstein thermal function) (medium density) (Space-time function) includes radial flow

Formalism Pions interact U with dense medium  is distorted (not plane) wave Gyulassy et al ‘79 DWEF- distorted wave emission function U -  self energy U :phenomenological-not from equil. thermo, J

Wave Equation Solutions Matter is infinitely long Bjorken tube and azimuthal symmetry, wave functions factorize: 3D  2D(distorted)  1D(plane) We solve the reduced Klein-Gordon wave equation for  p : U time independent, cylindrical, Partial wave expansion ! ordinary diff eq

Meaning of U Im (U) : Opacity, Re (U) :Refraction pions lose energy and flux Re(U) must exist. Next: very strong attraction chiral phase transition

Chiral Symmetry, Son & Stephanov 2002 v 2, v 2 m 2   approach  near T = T c Both terms of U are negative (attractive) =ω 2 -m 2 π

Overview Pions emitted anywhere, any time, not only at freeze- out surface Pions interact with the surroundings during escape. These interactions not included in the source function S- No relation between U and S Quarks, gluons are the dominant source of the pions, but not the cause of U Im [U] accounts for opacity Re[U] must exist, causes refraction, acts as mass-change of pions due to chiral-symmetry breaking as they pass from the hot, dense collision medium [m(  )  0]) to the outside vacuum [m(  )  140 MeV]. Relativistic quantum mechanics, solve pion wave equation with partial wave expansion.

Time-Independence, Resonances, and Freeze-Out Use of a time-independent phenomenological optical potential does not invoke the mean field approximation and represents an average over a duration  The effects of the optical potential disappear as the system decays. The optical potential also includes the effects of resonances, including the heavy ones. Heavy resonances decay into π’s outside of the plasma. We account for this by computing only that part of the spectra that is related to the pions in the HBT correlation function λ parameter accounts for these

Recent Corrections 1.We discovered in November a convergence vs. integration step size problem in our calculation of optical model wave functions. This had no effect on the HBT radii, but had a strong effect on the slope of the spectrum. This problem was corrected by changing from Runge-Kutta to Numerov wave function solutions. 2.We discovered in March that the effects of the strong chemical potential was being applied to the spectrum, but not to the HBT radii. This error was corrected. M. Luzum (UW) 3.The net result, after refitting, is that the “ambiguities” mentioned previously are gone, and the emission temperature of the model has dropped from T=193 MeV to T=161 MeV. The need for a very deep and absorptive optical potential remains. 4.Result: The New Improved DWEF Model (DWEF v.2.1).

Fit STAR Data 6 source, 3 optical potential parameters Fit central STAR data at  s NN =200 GeV T=160 MeV, μ π =pion mass reproduce R o, R s, R l reproduce dN   dy (both magnitude and shape) 8 momentum values (i.e., 32 data points) Correct spectrum for contribution of resonances decaying outside the target

DWEF Fits to STAR 200 GeV Pion HBT Radii K T (MeV/c) R O (fm) R S (fm) K T (MeV/c) R L (fm) R O /R S K T (MeV/c) Temperature is about 160 MeV

Components of DWEF Calculations Red Solid - Full DWEF Yellow Dots - Plane wave (U=0, no flow) Green Short Dash - Re( p^2 term) only, no flow Aqua Long Dash - Im(p^2 term) only, no flow Cyan Dot Dash - Re(Const term) only, no flow Blue 2-Dot Dash - Flow only, U=0 Violet 3-Dot Dash - DWEF with no BE correction K T (MeV/c) R O (fm) R S (fm) K T (MeV/c) Spectrum dN  2 /2  M T dM T dy

DWEF Fit to STAR 200 GeV Pion Spectrum Note: accurate prediction of spectrum slope involves subtle cancellations among wave functions K T (MeV/c) Spectrum dN  2 /2  M T dM T dy

Meaning of the Parameters Temperature: 160 MeV Transverse flow rapidity: 1.2  v max =0.83 c, v av =0.6 c Pion emission between 6.2 fm/c and 11 fm/c  soft EOS. WS radius: 12 fm = R (Au) fm > SPS Re(U): p 2   deep well  strong attraction size consistent with chiral phase transition ( p 2 ). Im(U): 0.13 p 2  mfp  8 K T =1 fm -1  strong absorption  high density Pion chemical potential:   = mass(  )

Optical Wave Functions [|  | 2  (b)] K T = 250 MeV/c K T = 600 MeV/c K T = 100 MeV/c Eikonal Approx. Observer DWEF

Centrality: 200 GeV Au+Au R O (fm) Au+Au Fit Au+Au Predictions R L (fm) Au+Au Fit Au+Au Predictions R S (fm) Au+Au Fit Au+Au Predictions Space-time parameters R WS, a WS,   are scaled by participant number. Emission duration  is constant. Red: Central Collisions... Indigo: Peripheral Collisions K T (MeV/c)

Centrality: 200 GeV Cu+Cu Cu+Cu Predictions Space-time parameters R WS, a WS,   are scaled by participant number. Emission duration  is scaled as A 1/3. Red: Central Collisions... Indigo: Peripheral Collisions R O (fm) Au+Au Fit R S (fm) Au+Au Fit R L (fm) Au+Au Fit K T (MeV/c)

Low p T Behavior: Ramsauer Resonances in Well K T (MeV/c) Phobos 0-6% K T (MeV/c) R O (fm)R S (fm) R L (fm) Spectrum dN  2 /2  M T dM T dy

Summary and Plans Quantum mechanical treatment of opacity and refraction Excellent fits- many parameters Parameters of U consistent with chiral phase transition, but no relation between U and S implemented Other tests needed- lower energy data –John v 2 Matt Luzum, UW