Status of the TECHQM ‘brick problem’ Marco van Leeuwen, Utrecht University.

Slides:



Advertisements
Similar presentations
Why soft interaction approximations are not strong enough for jets in the QGP Simon Wicks Work done with Miklos Gyulassy With thanks to Azfar Adil, William.
Advertisements

W. A. Horowitz Quark Matter 2005 A Promising Solution to the Elliptic Quench Puzzle at RHIC William A. Horowitz Columbia University August 4-5, 2005.
Effects of minijet degradation on hadron observables in heavy-ion collisions Lilin Zhu Sichuan University QPT2013, Chengdu.
A common description of jet-quenching and elliptic flow within a pQCD transport model Oliver Fochler H-QM Graduate Day arXiv:
High-p T spectra and correlations from Cu+Cu and Au+Au collisions in STAR Marco van Leeuwen, LBNL for the STAR collaboration.
Andrej Ficnar Columbia University INT 10-2A June 25, 2010 High order DGLV Monte Carlo and q models of jet quenching ^
#: 1... and your jet energy loss calculation? What drives you? aka Perturbative jet energy loss mechanisms: Learning from RHIC, extrapolating to LHC Simon.
Luan Cheng (Institute of Particle Physics, Huazhong Normal University) I. Introduction II. Interaction Potential with Flow III. Flow Effects on Light Quark.
Single & Dihadron Suppression at RHIC and LHC Xin-Nian Wang Lawrence Berkeley National Laboratory Last call for prediction for LHC, CERN, May 29-June 2,2007.
Centrality-dependent pt spectra of Direct photons at RHIC F.M. Liu 刘复明 Central China Normal University, China T. Hirano University of Tokyo, Japan K.Werner.
1 Heavy Quark Energy Loss Tatia Engelmore Journal Club 7/21.
Collective Flow Effects and Energy Loss in ultrarelativistic Heavy Ion Collisions Zhe Xu USTC, Hefei, July 11, 2008 with A. El, O. Fochler, C. Greiner.
Radiative energy loss Marco van Leeuwen, Utrecht University.
Photons and Dileptons at LHC Rainer Fries Texas A&M University & RIKEN BNL Heavy Ion Collisions at the LHC: Last Call for Predictions CERN, June 1, 2007.
Comparative Study of Jet-Quenching Schemes Working towards a unified approach in Jet-modification A. Majumder, Duke University Thanks to: N. Armesto, S.
M. Djordjevic 1 Effect of dynamical QCD medium on radiative heavy quark energy loss Magdalena Djordjevic The Ohio State University.
M. Djordjevic 1 Heavy quark energy loss in a dynamical QCD medium Magdalena Djordjevic The Ohio State University M. Djordjevic and U. Heinz, arXiv:
Marco van Leeuwen, Marta Verweij, Utrecht University Energy loss in a realistic geometry.
Enke Wang (Institute of Particle Physics, Huazhong Normal University) with A. Majumder, X.-N. Wang I. Introduction II.Quark Recombination and Parton Fragmentation.
A NLO Analysis on Fragility of Dihadron Tomography in High Energy AA Collisions I.Introduction II.Numerical analysis on single hadron and dihadron production.
What can we learn from/about QCD energy loss? (From an experimentalists point of view) Marco van Leeuwen, Utrecht University TECHQM meeting, 6-10 July.
Precision Probes for Hot QCD Matter Rainer Fries Texas A&M University & RIKEN BNL QCD Workshop, Washington DC December 15, 2006.
7/7/09 William Horowitz WHDG Brick and Comparing WHDG to ASW-SH William Horowitz The Ohio State University July 7, 2009 With many thanks to Brian Cole,
11/15/06 William Horowitz 1 LHC Predictions 1 from an extended theory 2 with Elastic, Inelastic, and Path Length Fluctuating Jet Energy Loss William Horowitz.
6/6/06William Horowitz Hard Probes Overcoming Fragility William Horowitz Columbia University June 14, 2006 With many thanks to Simon Wicks, Azfar.
Jet quenching and direct photon production F.M. Liu 刘复明 Central China Normal University, China T. Hirano 平野哲文 University of Tokyo, Japan K.Werner University.
1 Search for the Effects of the QCD Color Factor in High-Energy Collisions at RHIC Bedanga Mohanty LBNL  Motivation  Color Factors  Search for Color.
Luan Cheng (Institute of Particle Physics, Huazhong Normal University) I.Introduction II. Potential Model with Flow III.Flow Effects on Parton Energy Loss.
Jet energy loss at RHIC and LHC including collisional and radiative and geometric fluctuations Simon Wicks, QM2006 Work done with Miklos Gyulassy, William.
Hard probes of the Quark Gluon Plasma Part 1: Introduction, R AA Marco van Leeuwen, Nikhef & Utrecht University Lectures at: Quark Gluon Plasma and Heavy.
Comparing energy loss models Marco van Leeuwen Utrecht University What have we learned from the TECHQM brick problem? With many contributions from TEHCQM.
Jet Physics in ALICE Mercedes López Noriega - CERN for the ALICE Collaboration Hot Quarks 2006 Villasimius, Sardinia - Italy.
1 Jet quenching, Nov hep-ph/ ; CERN-TH
M. Djordjevic 1 Theoretical predictions of jet suppression: a systematic comparison with RHIC and LHC data Magdalena Djordjevic Institute of Physics Belgrade,
Ralf Averbeck Stony Brook University Hot Quarks 2004 Taos, New Mexico, July 19-24, 2004 for the Collaboration Open Heavy Flavor Measurements with PHENIX.
Cheng LuanInstitute of Particle Physics,CCNU1 Jet Quenching in 1+1 Dimension Expanding Medium with Chemical Nonequilibrium Inst. of Particle Phys., CCNU.
Radiative heavy quark energy loss in QCD matter Magdalena Djordjevic and Miklos Gyulassy Columbia University.
Third TECHQM Collaboration Meeting, CERN July 6-10, 2009 Xin-Nian Wang Lawrence Berkeley National Laboratory The Brick Problem in High-Twist Approximation.
Jet Jet Tomography of Hot & Dense Matter Xin-Nian Wang LBNL, June 25, 2003.
Parton energy loss Marco van Leeuwen. 2 Hard probes of QCD matter Use ‘quasi-free’ partons from hard scatterings to probe ‘quasi-thermal’ QCD matter Interactions.
Comparing energy loss phenomenology Marco van Leeuwen Utrecht University.
Comparison of energy loss formalisms Marco van Leeuwen, UU TECHQM meeting LBNL, Dec 2008.
Heavy Quark Energy Loss with Twist Expansion Approach Ben-Wei Zhang Institute of Particle Physics Central China Normal Univeristy CCAST, Beijing --- Augest.
Elastic, Inelastic and Path Length Fluctuations in Jet Tomography Simon Wicks Hard Probes 2006 Work done with William Horowitz, Magdalena Djordjevic and.
Enke Wang (Institute of Particle Physics, Huazhong Normal University) I. Introduction II. Ineraction Potential with Flow III.Flow Effects on Light Quark.
L. Apolinário, N. Armesto, J. G. Milhano, C. Salgado TOWARDS JET CALCULUS IN A QCD MEDIUM.
Enke Wang (Institute of Particle Physics, Huazhong Normal University) I.Jet Quenching in QCD-based Model II.Jet Quenching in High-Twist pQCD III.Jet Tomography.
12/16/08 William Horowitz TECHQM 2 nd Workshop, LBNL 1 DGLV : M. Djordjevic and M. Gyulassy, Nucl.Phys.A733, 265 (2004) [nucl-th/ ] WHDG : S. Wicks,
Heavy quark energy loss in hot and dense nuclear matter Shanshan Cao In Collaboration with G.Y. Qin, S.A. Bass and B. Mueller Duke University.
M. Djordjevic 1 Heavy quark energy loss in a dynamical QCD medium Magdalena Djordjevic The Ohio State University M. Djordjevic and U. Heinz, arXiv:
M. Djordjevic 1 Hard probes at RHIC and LHC Magdalena Djordjevic Ohio State University.
M. Djordjevic 1 Light and heavy flavor phenomenology at RHIC and LHC Magdalena Djordjevic Institute of Physics Belgrade, University of Belgrade.
M. Djordjevic 1 Suppression and energy loss in Quark-Gluon Plasma Magdalena Djordjevic Institute of Physics Belgrade, University of Belgrade.
Parton showers as a source of energy-momentum deposition and the implications for jet observables Bryon Neufeld, LANL 1Neufeld Based on the preprint R.B.
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),
Jet Quenching of Massive Quark in Nuclear Medium Ben-Wei Zhang Institute of Particle Physics Central China Normal Univeristy ICHEP, Beijing --- Augest.
Prospects for understanding energy loss in hot nuclear matter
Probing QGP-medium interactions
F. Dominguez, CM, A. Mueller, B. Xiao and B. Wu, arXiv:
High-pT results from ALICE
Status of the TECHQM ‘brick problem’
Energy loss in a realistic geometry
Theory Update on Energy Loss
Comparing energy loss models
Lawrence Berkeley National Laboratory
of Hadronization in Nuclei
Energy Loss in the Hot QCD Brick I
Uncertainties and Consistency (?) in pQCD and AdS/CFT Jet Physics
W. A. Horowitz The Ohio State University June 19, 2010
Modified Fragmentation Function in Strong Interaction Matter
Presentation transcript:

Status of the TECHQM ‘brick problem’ Marco van Leeuwen, Utrecht University

2 TECHQM Forum to discuss comparison between theory and experiment in areas where there is a potential significant quantitative understanding Two subgroups: –Parton energy loss –Elliptic flow/Hydro Workshops/meetings: –BNL May 2008 –LBL Dec 2008 –CERN July 2009 –BNL (with CATHIE) Dec Theory-Experiment Collaboration on Hot Quark Matter This talk is about Parton Energy loss

3 Energy loss formalisms I PHENIX, arXiv: , J. Nagle WWND08 PQM = 13.2 GeV 2 /fm ^ WHDG dN g /dy = ZOWW  0 = 1.9 GeV/fm AMY  s = GLV, AMY: T = MeV BDMPS: T ~ 1000 MeV Large difference in medium density: Different calculations use different geometries – not clear what dominates

4 Energy loss formalisms II Bass et al, PRC79, ASW: HT: AMY: AMY: T ~ 400 MeV Compare 3 formalisms with `same’ Hydro geometry: Different formalisms give different energy loss at given density, path length Why: Different physics implemented? Or `technical’ differences? What are the main uncertainties?

5 The Brick Problem Gluon(s) Plot: outgoing gluon, quark distributions Two types of comparison: - Same density - Same suppression Compare energy-loss in a well-defined model system: Fixed-length L (2, 5 fm) Density T, q Quark, E = 10, 20 GeV

6 Four formalisms Hard Thermal Loops (AMY) –Dynamical (HTL) medium –Single gluon spectrum: BDMPS-Z like path integral –No vacuum radiation Multiple soft scattering (BDMPS-Z, ASW) –Static scattering centers –Gaussian approximation for momentum kicks –Full LPM interference and vacuum radiation Opacity expansion ((D)GLV, ASW-OE) –Static scattering centers, Yukawa potential –Expansion in opacity L/ (N=1, interference between two centers default) –Interference with vacuum radiation Higher Twist (Guo, Wang, Majumder) –Medium characterised by higher twist matrix elements –Radiation kernel similar to GLV –Vacuum radiation in DGLAP evolution Multiple gluon emission Fokker-Planck rate equations Poisson ansatz (independent emission) DGLAP evolution

7 Large differences in medium density for R 7 = 0.25 Some brick results Outgoing quark spectrum T=300 MeV R AA > P 0  Difference between formalisms sizable even in simple geometry

8 Limitations of soft collinear approach Soft: Collinear: Need to extend results to full phase space to calculate observables (especially at RHIC) Soft approximation not problematic: For large E, most radiation is soft Also:  > E  full absorption Cannot enforce collinear limit: Small ,   k T always a part of phase space with large angles Calculations are done in soft collinear approximation:

9 Opacity expansions GLV and ASW-SH Expressions dN/dxdk ASW-OE and GLV are the same However, GLV use x = x+, while ASW use x=xE x + ~ x E in soft collinear limit, but not at large angles Different large angle cut-offs: k T <  = x E E k T <  = 2x + E Blue: k Tmax = xE Red: k Tmax = 2x(1-x)E Blue: m g = 0 Red: m g =  /√2 Horowitz and Cole, PRC81, Single-gluon spectrum Different definitions of x: ASW: GLV: Factor ~2 uncertainty from large-angle cut-off

10 Opacity expansion vs multiple soft Salgado, Wiedemann, PRD68, Different limits: SH (N=1 OE): interference between neighboring scattering centers MS: ‘all orders in opacity’, gaussian scattering approximation Quantitative differences sizable OE and MS related via path integral formalism So far, not clear which difference dominates. Would like: OE with gaussian and/or all orders (Wicks)

11 AMY and BDMPS Single-gluon kernel from AMY based on scattering rate: BMPS-Z use harmonic oscillator: BDMPS-Z: Salgado, Wiedemann, PRD68, Finite-L effects: Vacuum-medium interference + large-angle cut-off

12 AMY and BDMPS Large difference between AMY and ASW at L=2 fm?

13 HT and GLV Single-gluon kernel GLV and HT ‘similar’ L = 5 fm, T = 300 MeV HT:  √(E/L) kernel diverges for k T  0 GLV: HT: OE: Large uncertainty from k Tmax

14 Single gluon spectra Same temperatureSame suppression (Not suppression: OE (AMY?) peaked at low  ASW-MS not so temperature: AMY > OE > ASW-MS

15 Outgoing quark spectra Same temperatureSame suppression ASW-MS less suppression than OE at T=300 MeV At R 7 = 0.25 P 0 small for ASW-MS P 0 = 0 for AMY by definition

16 L=2 fm, T=250, 350 MeV GLV, HT, ASW-MS similar AMY: large suppression L=2 fm, T=250, 350 MeV AMY, HT larger suppression than OE, MS Fragmentation function Majumder, van Leeuwen, arXIv:

17 Conclusion Tentative summary: –AMY shows strongest suppression Lack of vacuum radiation? –ASW-MS: smallest suppression Soft scattering or interference or both? –OE, HT similar, between MS and AMY Large uncertainties associated with large angle radiation in all formalisms Differences between formalisms large at single-gluon level R AA probably not sensitive to details of multi-gluon treatment Thanks to all in TECHQM who contributed ! In preparation: TECHQM publication with more detailed report

18 Extra slides

19 X+ vs xE