November 29, 2010Zimanyi Winter School 2010, Budapest11 3D Pion & Kaon Source Imaging from 200 AGeV Au+Au collisions Paul Chung (STAR Collaboration) NPI.

Slides:



Advertisements
Similar presentations
Anomalous Pion Production in High Energy Particle Collisions Alexander Bylinkin, Andrey Rostovtsev XV Moscow School of Physics XXXX ITEP Winter School.
Advertisements

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.
ISMD13, 09/19/2013M. Šumbera, STAR: Kaon Femtoscopy 1 Kaon Freeze-out Dynamics in √s NN =200 GeV Au+Au Collisions at RHIC * Kaon Freeze-out Dynamics in.
1 Roy Lacey & Paul Chung Nuclear Chemistry, SUNY, Stony Brook Evidence for a long-range pion emission source in Au+Au collisions at.
STAR Patricia Fachini 1 Brookhaven National Laboratory Motivation Data Analysis Results Conclusions Resonance Production in Au+Au and p+p Collisions at.
1 Systematic studies of freeze-out source size in relativistic heavy-ion collisions by RHIC-PHENIX Akitomo Enokizono Lawrence Livermore National Laboratory.
Pion correlations in hydro-inspired models with resonances A. Kisiel 1, W. Florkowski 2,3, W. Broniowski 2,3, J. Pluta 1 (based on nucl-th/ , to.
STAR Looking Through the “Veil of Hadronization”: Pion Entropy & PSD at RHIC John G. Cramer Department of Physics University of Washington, Seattle, WA,
Roy A. Lacey, Stony Brook; 24 th Winter Workshop on Nuclear Dynamics, April 5-12, Roy A. Lacey Prospects for locating the QCD Critical End Point.
Recent Results from STAR Rene Bellwied, Wayne State, for the STAR Collaboration  Thermalization & Timescales  High pt physics  Fluctuations  130 to.
5-12 April 2008 Winter Workshop on Nuclear Dynamics STAR Particle production at RHIC Aneta Iordanova for the STAR collaboration.
Collision system dependence of 3-D Gaussian source size measured by RHIC-PHENIX Akitomo Enokizono Lawrence Livermore National Laboratory 23 rd Winter Workshop.
WPCF07, Sonoma, California, August Observation of Extended Pion Sources in Relativistic Heavy Ion Collisions: extraction of source breakup time.
High p T identified hadron anisotropic flow and Deuteron production in 200 GeV Au+Au Collisions Shengli Huang Vanderbilt University for the PHENIX Collaboration.
1 Paul Chung ( for the PHENIX Collaboration ) Nuclear Chemistry, SUNY, Stony Brook Evidence for a long-range pion emission source in Au+Au collisions at.
1 P. Chung Nuclear Chemistry, SUNY, Stony Brook Evidence for a long-range pion emission source in Au+Au Collisions at.
12 th Zimányi Winter School on Heavy Ion Physics Kaon source imaging with the STAR experiment in 200 GeV Au+Au collisions at RHIC Róbert Vértesi (for the.
Zbigniew Chajęcki National Superconducting Cyclotron Laboratory Michigan State University Probing reaction dynamics with two-particle correlations.
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.
Measurements of the Charge Balance Function at RHIC from √s NN = 7.7 to 200 GeV Gary D. Westfall, for the STAR Collaboration (Michigan State University)
QM’05 Budapest, HungaryHiroshi Masui (Univ. of Tsukuba) 1 Anisotropic Flow in  s NN = 200 GeV Cu+Cu and Au+Au collisions at RHIC - PHENIX Hiroshi Masui.
Roy A. Lacey, Stony Brook; EDT-HIC, McGill, Montreal, Canada, July 16-19, Roy A. Lacey New Prospects for locating the Critical End Point (CEP) in.
BNL/ Tatsuya CHUJO CNS workshop, Tokyo Univ. Identified Charged Single Particle Spectra at RHIC-PHENIX Tatsuya Chujo (BNL) for the PHENIX.
1 Roy Lacey ( for the PHENIX Collaboration ) Nuclear Chemistry Group Stony Brook University PHENIX Measurements of 3D Emission Source Functions in Au+Au.
ISMD13, 09/19/2013M. Šumbera, STAR: Kaon Freeze-out Dynamics at RHIC 1 Kaon Freeze-out Dynamics in √s NN =200 GeV Au+Au Collisions at RHIC * Kaon Freeze-out.
July 21, 2011M.Š. EPS-HEP 2011, Grenoble11 Three-dimensional Kaon Source Extraction from STAR Experiment at RHIC Michal Šumbera NPI ASCR Prague (for the.
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,
QM06, Shanghai, China, Nov Evidence of non-Gaussian tail in Pion Emission SPS: Sensitivity to source formation & emission duration Paul.
November 6, 2012M.Š. STAR regional mtg., Warsaw11 Kaon Freeze-out Dynamics in √s NN =200GeV Au+Au Collisions at RHIC Michal Šumbera NPI ASCR, Prague (for.
Hadron emission source functions measured by PHENIX Workshop on Particle Correlations and Fluctuations The University of Tokyo, Hongo, Japan, September.
1 Jeffery T. Mitchell – Quark Matter /17/12 The RHIC Beam Energy Scan Program: Results from the PHENIX Experiment Jeffery T. Mitchell Brookhaven.
Sergey Panitkin Current Status of the RHIC HBT Puzzle Sergey Panitkin Brookhaven National Lab La Thuile, March 18, 2005.
M. Muniruzzaman University of California Riverside For PHENIX Collaboration Reconstruction of  Mesons in K + K - Channel for Au-Au Collisions at  s NN.
Masashi Kaneta, First joint Meeting of the Nuclear Physics Divisions of APS and JPS 1 / Masashi Kaneta LBNL
Peter Kolb, CIPANP03, May 22, 2003what we learn from hydro1 What did we learn, and what will we learn from Hydro CIPANP 2003 New York City, May 22, 2003.
Azimuthal HBT measurement of charged pions With respect to 3 rd event plane In Au+Au 200GeV collisions at RHIC-PHENIX Takafumi Niida for the PHENIX Collaboration.
Masashi Kaneta, LBL Hadron Spectra in Au+Au Collisions by STAR Experiment at RHIC Masashi Kaneta for the STAR collaboration LBNL.
1 Roy Lacey Nuclear Chemistry, SUNY, Stony Brook Proofing the Source Imaging Technique.
School of Collective Dynamics in High-Energy CollisionsLevente Molnar, Purdue University 1 Effect of resonance decays on the extracted kinetic freeze-out.
S. PrattNSCL/MSU Deciphering the Space-Time Evolution of Heavy-Ion Collisons with Correlation Measurements Scott Pratt Michigan State University.
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.
Charged and Neutral Kaon correlations in Au-Au Collisions at sqrt(s_NN) = 200 GeV using the solenoidal tracker at RHIC (STAR) Selemon Bekele The Ohio State.
BNL/ Tatsuya CHUJO JPS RHIC symposium, Chuo Univ., Tokyo Hadron Production at RHIC-PHENIX Tatsuya Chujo (BNL) for the PHENIX Collaboration.
Andras. Ster, RMKI, Hungary ZIMANYI-SCHOOL’09, Budapest, 01/12/ Azimuthally Sensitive Buda-Lund Hydrodynamic Model and Fits to Spectra, Elliptic.
Christina MarkertHirschegg, Jan 16-22, Resonance Production in Heavy Ion Collisions Christina Markert, Kent State University Resonances in Medium.
1 Space-time analysis of reactions at RHIC Fabrice Retière Lawrence Berkeley Lab STAR collaboration.
QGP-Meet’06, VECC, Kolkata. 6 th Feb-2006 RAGHUNATH SAHOO, INSTITUTE OF PHYSICS, BHUBANESWAR TRANSVERSE ENERGY PRODUCTION AT RHIC OUTLINE: Introduction.
T. Csörgő 1,2 for the PHENIX Collaboration Femtoscopic results in Au+Au & p+p from PHENIX at RHIC 1 MTA KFKI RMKI, Budapest,
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.
Paul Chung for the STAR Collaboration Nuclear Physics Institute ASCR Prague WPCF 2011, Tokyo 3D kaon source extraction from 200GeV Au+Au collisions.
SQM2003March 13Zi-wei Lin The Ohio State University ● Why transport model? ● Space-time (x-t) correlation: its effect on R out/ R side Extract radii from.
Analysis of the anomalous tail of pion production in Au+Au collisions as measured by the PHENIX experiment at RHIC M. Nagy 1, M. Csanád 1, T. Csörgő 2.
IOPB Dipak Mishra (IOPB), ICPAQGP5, Kolkata Feb 8 – 12 1 Measurement of  ++ Resonance Production in d+Au sqrt(s NN ) = 200 GeV Dipak Mishra.
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.
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.
Fall DNP Meeting,  meson production in Au-Au and d-Au collision at \ /s NN = 200 GeV Dipali Pal Vanderbilt University (for the PHENIX collaboration)
Adam Kisiel – CERN Hirschegg 2010 – 19 Jan Femtoscopy in relativistic heavy-ion collisions as a probe of system collectivity Adam Kisiel CERN.
EHS/NA22 Collaboration Na Li Institute of Particle Physics
Offline meeting Azimuthally sensitive Hanbury-Brown-Twiss (HBT) Interferometry Lukasz Graczykowski Warsaw University of Technology Johanna.
Example analysis of toy model
Takafumi Niida from Univ. of Tsukuba for the PHENIX Collaborations
Takafumi Niida from Univ. of Tsukuba for the PHENIX Collaborations
Two Particle Interferometry at RHIC
Hiroshi Masui for the PHENIX collaboration August 5, 2005
Dalian University of Technology, Dalian, China
Presentation transcript:

November 29, 2010Zimanyi Winter School 2010, Budapest11 3D Pion & Kaon Source Imaging from 200 AGeV Au+Au collisions Paul Chung (STAR Collaboration) NPI ASCR Prague

November 29, 2010 Zimanyi Winter School 2010, Budapest 2 initial state pre-equilibrium QGP and hydrodynamic expansion hadronization hadronic phase and freeze-out Conjecture of collisions at RHIC : Motivation Which observables & phenomena connect to the de-confined stage?

PHENIX 1D Source Imaging Phys.Rev.Lett.98:132301,2007 November 29, 2010 Zimanyi Winter School 2010, Budapest 3 Phys.Rev.Lett.103:142301,2009

November 29, 2010 Zimanyi Winter School 2010, Budapest 44 Outline Run 4 200AGeV: 3D pion correlation functions Overview of 3D source shape analysis : Cartesian Spherical Harmonic decomposition & Imaging Technique Correlation moments for low kT (0.25<kT<0.35 GeV) pion pairs from peripheral collisions (50<cen<80%). 3D source function extraction: Moment Imaging & Fitting Therminator comparison for extracting pion source lifetime & pion emission duration 3D Kaon correlation functions from Run 4 & Run 7 central Au+Au collisions Kaon source extraction & Therminator comparison

November 29, 2010 Zimanyi Winter School 2010, Budapest 55 Technique Devised by: D. Brown, P. Danielewicz, PLB 398:252 (1997). PRC 57:2474 (1998). Inversion of Linear integral equation to obtain source function Source function (Distribution of pair separations) Encodes FSI Correlationfunction Inversion of this integral equation ==  Source Function Emitting source 1D Koonin Pratt Eqn. Extracted S(r) in pair CM frame Hence Model-independent i.e Kernel independent of freeze-out conditions No Shape assumption for S(r) 1D Imaging Formulation

November 29, 2010 Zimanyi Winter School 2010, Budapest 66 Imaging : Inversion procedure Freeze-out occurs after last scattering Hence only Coulomb & BE effect included in kernel Expansion in B-spline basis

November 29, 2010 Zimanyi Winter School 2010, Budapest 77 1D Imaging ST STAR PRELIMINARY

November 29, 2010 Zimanyi Winter School 2010, Budapest 88 (3) 3D Koonin Pratt Plug in (1) and (2) into (3) Invert (1) Invert (2) Expansion of R(q) and S(r) in Cartesian Harmonic basis [Danielewicz and Pratt nucl-th/ (v1)] x=out-direction y=side-direction z=long-direction 3D Analysis Basics

November 29, 2010 Zimanyi Winter School 2010, Budapest 99 Monte Carlo Events: Phasemaker, Therminator CRAB3D C(q) Correlation Moments Source FITTING Source IMAGING Source Function Model calculation from space points SIMULATION PROCEDURE

November 29, 2010 Zimanyi Winter School 2010, Budapest 10 Fit Functions Ellipsoid Fit (3D Gaussian) : G = lambda exp[-{ (x/2r x ) 2 + (y/2r y ) 2 + (z/2r z ) 2 }] Hump Fit : H = exp[- F s { (x/2r xs ) 2 + (y/2r ys ) 2 + (z/2r zs ) 2 }] x exp[- F l { (x/2r xl ) 2 + (y/2r yl ) 2 + (z/2r zl ) 2 }] F s = 1/[1 + (r/r 0 ) 2 ] F l = 1 - F s

November 29, 2010 Zimanyi Winter School 2010, Budapest 11 Simulation – Therminator

November 29, 2010 Zimanyi Winter School 2010, Budapest 12 Comparison- C 0 moment vs 1D C(q) STAR PRELIM.STAR PRELIMINARY

L=2 & 4 moments November 29, 2010 Zimanyi Winter School 2010, Budapest 13 STAR PRELIMINARY

November 29, 2010 Zimanyi Winter School 2010, Budapest 14 L=6 moments STAR PRELIMINARY

November 29, 2010 Zimanyi Winter School 2010, Budapest 15 Imaging C 2 x2 & C 2 y2 STAR PRELIMINARY

November 29, 2010 Zimanyi Winter School 2010, Budapest 16 3D Imaging – S(r) & restored C(q) STAR PRELIMINARY

November 29, 2010 Zimanyi Winter School 2010, Budapest 17 Ellipsoid vs Hump Fit : l=0 & 2 mom. STAR PRELIMINARY

November 29, 2010 Zimanyi Winter School 2010, Budapest 18 Ellipsoid vs Hump Fit : l=4 moments STAR PRELIMINARY

November 29, 2010 Zimanyi Winter School 2010, Budapest 19 Ellipsoid vs Hump Fit : l=6 moments STAR PRELIMINARY

November 29, 2010 Zimanyi Winter School 2010, Budapest 20 Image vs Ellipsoid & Hump S(r) STAR PRELIMINARY

November 29, 2010 Zimanyi Winter School 2010, Budapest 21 3D C(q) : Ellipsoid vs Hump Fit STAR PRELIMINARY

November 29, 2010 Zimanyi Winter School 2010, Budapest 22 Therminator BW: Source lifetime & Pion emission duration extraction Therminator (Kisiel et al PRC 73, ) : Production of particles from thermalized and expanding system with Boost invariance & cylindrical symmetry BW mode: Freeze-out hypersurface defined by constant laboratory time independent of transverse radius

November 29, 2010 Zimanyi Winter School 2010, Budapest 23 STAR vs PHENIX comparison STAR PRELIMINARY

Source extraction – central collisions PRL100, (2008) (PHENIX) Transverse dimension = 8.9fm Source lifetime = 8.5fm/c Emission duration = 2fm/c Source parameters larger for central collisions than for peripheral collisions Full centrality dependence extraction underway November 29, 2010 Zimanyi Winter School 2010, Budapest 24

Extracted Pion Source Images from semi-central & peripheral collisions November 29, 2010 Zimanyi Winter School 2010, Budapest 25

November 29, 2010 Zimanyi Winter School 2010, Budapest 26 Run 7 & Run 4 KK : C 0 vs 1D C(q inv ) STAR PRELIMINARY

November 29, 2010 Zimanyi Winter School 2010, Budapest 27 Run 7 + Run 4 KK : C 0 vs 1D C(q inv ) STAR PRELIMINARY

Run 7 + Run 4 KK : l=2 & l=4 moments November 29, 2010 Zimanyi Winter School 2010, Budapest 28 STAR PRELIMINARY

KK: Ellipsoid Fit November 29, 2010 Zimanyi Winter School 2010, Budapest 29 STAR PRELIMINARY

THERMINATOR Model comparison November 29, 2010 Zimanyi Winter School 2010, Budapest 30

November 29, 2010 Zimanyi Winter School 2010, Budapest 31 Conclusion Correlation moments for low kT pion pairs from Run4 peripheral Au+Au collisions well described by the Hump Fit function. For low kT pion pairs from peripheral collisions, inferred pion source lifetime ~ 3.5 fm/c & pion emission duration ~ 1.5 fm/c < central collisions. Extracted Kaon source function essentially Gaussian – No significant non-Gaussian tail observed. Kaon source dimension & lifetime comparable to pion source; Kaon emission instantaneous (Therminator)