Physics Opportunities with e+A Collisions at an Electron Ion Collider A New Experimental Quest to Study the Glue That Binds us All Thomas Ullrich,
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Physics Opportunities with e+A Collisions at an Electron Ion Collider A New Experimental Quest to Study the Glue That Binds us All Thomas Ullrich, BNL Hall C Meeting, JLAB August 9, 2007 Theory of Strong Interactions: QCD LQCD a Asymptotic Freedom & Color Confinement In large part due to non-perturbative structure of QCD vacuum Gluons: mediator of the strong interactions “Emergent” Phenomena not evident from Lagrangian 1 a q (i m)q g ( q Ta q) A G Ga 4 Determine essential features of strong interactions Dominate structure of QCD vacuum (fluctuations in gluon fields) Responsible for > 98% of the visible mass in universe Hard to “see” the glue in the low-energy world Gluon degrees of freedom “missing” in hadronic spectrum but drive the structure of baryonic matter at low-x are crucial players at RHIC and LHC Requires fundamental investigation via experiment 2 What Do We Know About Glue in Matter? Deep Inelastic Scattering : 2 d 2 ep eX 4 e.m. y 2 y2 2 2 1 y F2 (x,Q ) FL (x,Q ) 2 4 dxdQ xQ 2 2 Scaling violation: dF2/dlnQ2 and linear DGLAP Evolution G(x,Q2) Gluons dominate low-x wave function xG ( 1 20 xu v ) xd v xS ( 1 20 ) 3 The Issue With Our Current Understanding Established Model: Linear DGLAP evolution scheme Weird behavior of xG and FL from HERA at small x and Q2 Could signal saturation, higher twist effects, need for more/better data? Unexpectedly large diffractive crosssection more severe: Linear Evolution has a built in high energy “catastrophe” xG rapid rise for decreasing x and violation of (Froissart) unitary bound must saturate What’s the underlying dynamics? Need new approach 4 Non-Linear QCD - Saturation BFKL Evolution in x proton linear explosion of color field? N partons any 2partons new partonsemitted can recombine as energy into increases one could be emitted off any of the N partons Regimes of QCD Wave Function New: BK/JIMWLK based models introduce non-linear effects saturation characterized by a scale Qs(x,A) arises naturally in the Color Glass Condensate (CGC) framework 5 e+A: Studying Non-Linear Effects Scattering of electrons off nuclei: Probes interact over distances L ~ (2mN x)-1 For L > 2 RA ~ A1/3 probe cannot distinguish between nucleons in front or back of nucleon Probe interacts coherently with all nucleons s xG(x,Qs2 ) Q ~ RA2 2 s 1 HERA : xG ~ 0.3 x Nuclear “Oomph” Factor Pocket Formula: A dependence : xGA ~ A 1/3 A 2 2 A (Qs ) cQ0 x Enhancement of QS with A non-linear QCD regime reached at significantly lower energy in A than in proton 6 Nuclear “Oomph” Factor Note : Q Q s s (Q ) Q2 Q s s (Qs2 ) 2 2 s 2 s 2 More sophisticated analyses more detailed picture even exceeding the Oomph from the pocket formula (e.g. Armesto et al., PRL 94:022002, Kowalski, Teaney, PRD 68:114005) 7 Universality & Geometric Scaling Crucial consequence of non-linear evolution towards saturation: Physics invariant along trajectories parallel to saturation regime (lines of constant gluon occupancy) Scale with Q2/Q2s(x) instead of x and Q2 separately Geometric Scaling Consequence of saturation which manifests itself up to kT > Qs x < 0.01 8 Qs a Scale that Binds them All Nuclear shadowing: Geometrical scaling proton 5 nuclei Freund et al., hep-ph/0210139 Are hadrons and nuclei wave function universal at low-x ? 9 A Truly Universal Regime ? Small x QCD evolution predicts: QS approaches universal behavior for all hadrons and nuclei Not only functional form f(Qs) “Research is what I'm doing when universal but Ieven Qs becomes the same don't know what I'm doing. “ ? A.H. Mueller, hep-ph/0301109 Wernher von Braun Radical View: Nuclei and all hadrons have a component of their wave function with the same behavior This is a conjecture! Needs to be tested 10 Understanding Glue in Matter Understanding the role of the glue in matter involves understanding its key properties which in turn define the required measurements: What is the momentum distribution of the gluons in matter? What is the space-time distributions of gluons in matter? e+p and e+A Unknown in e+A How do fast probes interact with the gluonic medium? e+p and e+A Exploration of saturation regime better in e+A (Oomph Factor) Strength of e+A Do strong gluon fields effect the role of color neutral excitations (Pomerons)? e+p and e+A Unknown in e+A 11 eA Landscape and a New Electron Ion Collider Well mapped in e+p Not so for ℓ+A (A) Electron Ion Collider (EIC): L(EIC) > 100 L(HERA) Different EIC Concepts: eRHIC ELIC Terra incognita: small-x, Q Qs high-x, large Q2 12 Electron Ion Collider Concepts eRHIC (BNL): Add Energy Recovery Linac to RHIC Ee = 10 (20) GeV EA = 100 GeV (up to U) seN = 63 (90) GeV LeAu (peak)/n ~ 2.9·1033 cm-2 s-1 eRHIC (Linac-Ring) PHENIX ELIC (JLAB): Add hadron beam facility to existing electron facility CEBAF Ee = 9 GeV EA = 90 GeV (up to Au) seN = 57 GeV LeAu (peak)/n ~ 1.6·1035 cm-2 s-1 e-cooling (RHIC II) Electron Cooling IR Snake Main ERL (2 GeV per pass) STAR Snake Four e-beam passes Both allow for polarized e+p collisions ! IR ELIC 13 What is the Momentum Distribution of Gluons? Gluon distribution G(x,Q2) Shown here: Scaling violation in F2: dF2/dlnQ2 FL ~ s G(x,Q2) Other Methods: 2+1 jet rates (needs jet algorithm and modeling of hadronization for inelastic hadron final states) inelastic vector meson production (e.g. J/) diffractive vector meson production ~ [G(x,Q2)]2 14 F2 : Sea (Anti)Quarks Generated by Glue at Low x F2 will be one of the first measurements at EIC nDS, EKS, FGS: pQCD based models with different amounts of shadowing Syst. studies of F2(A,x,Q2): G(x,Q2) with precision distinguish between models d 2 ep eX 4 2 y 2 y2 2 2 1 y F2 (x,Q ) FL (x,Q ) 2 4 dxdQ xQ 2 2 15 FL at EIC: Measuring the Glue Directly FL requires s scan Q2/xs = y Here: Ldt = 5/A fb-1 (10+100) GeV = 5/A fb-1 (10+50) GeV = 2/A fb-1 (5+50) GeV statistical error only G(x,Q2) with great precision d 2 ep eX 4 2 y 2 y2 2 2 1 y F2 (x,Q ) FL (x,Q ) 2 4 dxdQ xQ 2 2 16 The Gluon Space-Time Distribution What we know is mostly the momentum distribution of glue? How is the glue distributed spatially in nuclei? Gluon density profile: small clumps or uniform ? Various techniques & methods: Exclusive final states (e.g. vector meson production r, J/, DVCS) Deep Virtual Compton Scattering (DVCS) color transparency color opacity Integrated DVCS cross-section: DVCS ~ A4/3 Measurement of structure functions for various mass numbers A (shadowing, EMC effect) and its impact parameter dependence 17 Diffractive Physics in e+A ‘Standard Diffractive DISevent event’ ? Detector activity in proton direction HERA/ep: 15% of all events are hard diffractive Diffractive cross-section diff/tot in e+A ? Predictions: ~25-40%? Look inside the “Pomeron” Diffractive structure functions Diffractive vector meson production ~ [G(x,Q2)]2 18 Diffractive Structure Function F2D at EIC 2 d 4 eh eXh 4 e.m. y 2 D y 2 D 2 4 1 y F2 FL 2 dxdQ ddt Q 2 2 = x/xIP xIP = momentum fraction of the pomeron w.r.t the hadron Distinguish between linear evolution and saturation models Insight into the nature of pomeron Search for exotic objects (Odderon) Curves: Kugeratski, Goncalves, Navarra, EPJ C46, 413 19 Hadronization and Energy Loss nDIS: Suppression of high-pT hadrons analogous but weaker than at RHIC Clean measurement in ‘cold’ nuclear matter Fundamental question: When do colored partons get neutralized? Parton energy loss vs. (pre)hadron absorption Energy transfer in lab rest frame EIC: 10 < < 1600 GeV HERMES: 2-25 GeV EIC: can measure heavy flavor energy loss zh = Eh/ 20 Connection to p+A Physics F. Schilling, hex-ex/0209001 e+A and p+A provide excellent information on properties of gluons in the nuclear wave functions Both are complementary and offer the opportunity to perform stringent checks of factorization/universality Issues: p+A lacks the direct access to x, Q2 Breakdown of factorization (e+p HERA versus p+p Tevatron) seen for diffractive final states. 21 Connection to RHIC & LHC Physics Matter at RHIC: thermalizes fast (t0 ~ 0.6 fm/c) We don’t know why and how? Initial conditions? G(x, Q2) Role of saturation ? RHIC → forward region LHC → midrapidity bulk (low-pT matter) & semi-hard jets LHC RHIC Jet Quenching: Need Refererence: E-loss in cold matter No HERMES data for charm energy loss in LHC energy range EIC provides new essential input: • Precise handle on x, Q2 • Means to study exclusive effects 22 Experimental Aspects I. Abt, A. Caldwell, X. Liu, J. Sutiak, hep-ex 0407053 J. Pasukonis, B.Surrow, physics/0608290 Concepts: Focus on the rear/forward acceptance and thus on low-x / high-x physics compact system of tracking and central electromagnetic calorimetry inside a magnetic dipole field and calorimetric end-walls outside Focus on a wide acceptance detector system similar to HERA experiments allow for the maximum possible Q2 range. 23 EIC Timeline & Status NSAC Long Range Plan 2007 Goal for Next Long Range Plan 2012 Recommendation: $6M/year for 5 years for machine and detector R&D High-level (top) recommendation for construction EIC Roadmap (Technology Driven) Finalize Detector Requirements from Physics Revised/Initial Cost Estimates for eRHIC/ELIC Investigate Potential Cost Reductions Establish process for EIC design decision Conceptual detector designs R&D to guide EIC design decision EIC design decision High priority in Long Range Plan 2008 2008 2009 2010 2010 2011 2011 2012 24 Summary The EIC presents a unique opportunity in high energy nuclear physics and precision QCD physics e+A Study the Physics of Strong Color Fields Establish (or not) the existence of the saturation regime Explore non-linear QCD Measure momentum & space-time of glue Study the nature of color singlet excitations (Pomerons) Test and study the limits of universality (eA vs. pA) e+p (polarized) Precisely image the sea-quarks and gluons to determine the spin, flavor and spatial structure of the nucleon For more see: http://web.mit.edu/eicc/ 25 The EIC Collaboration 17C. Aidala, 28E. Aschenauer, 10J. Annand, 1J. Arrington, 26R. Averbeck, 3M. Baker, 26K. Boyle, 28W. Brooks, 28A. Bruell, 19A. Caldwell, 28J.P. Chen, 2R. Choudhury, 10E. Christy, 8B. Cole, 4D. De Florian, 3R. Debbe, 26,24-1A. Deshpande, 18K. Dow, 26A. Drees, 3J. Dunlop, 2D. Dutta, 7F. Ellinghaus, 28R. Ent, 18R. Fatemi, 18W. Franklin, 28D. Gaskell, 16G. Garvey, 12,241M. Grosse-Perdekamp, 1K. Hafidi, 18D. Hasell, 26T. Hemmick, 1R. Holt, 8E. Hughes, 22C. Hyde-Wright, 5G. Igo, 14K. Imai, 10D. Ireland, 26B. Jacak, 15P. Jacobs, 28M. Jones, 10R. Kaiser, 17D. Kawall, 11C. Keppel, 7E. Kinney, 18M. Kohl, 9H. Kowalski, 17K. Kumar, 2V. Kumar, 21G. Kyle, 13J. Lajoie, 3M. Lamont, 16M. Leitch, 27A. Levy, 27J. Lichtenstadt, 10K. Livingstone, 20W. Lorenzon, 145. Matis, 12N. Makins, 6G. Mallot, 18M. Miller, 18R. Milner, 2A. Mohanty, 3D. Morrison, 26Y. Ning, 15G. Odyniec, 13C. Ogilvie, 2L. Pant, 26V. Pantuyev, 21S. Pate, 26P. Paul, 12J.-C. Peng, 18R. Redwine, 1P. Reimer, 15H.-G. Ritter, 10G. Rosner, 25A. Sandacz, 7J. Seele, 12R. Seidl, 10B. Seitz, 2P. Shukla, 15E. Sichtermann, 18F. Simon, 3P. Sorensen, 3P. Steinberg, 24M. Stratmann, 22M. Strikman, 18B. Surrow, 18E. Tsentalovich, 11V. Tvaskis, 3T. Ullrich, 3R. Venugopalan, 3W. Vogelsang, 28C. Weiss, 15H. Wieman,15N. Xu,3Z. Xu, 8W. Zajc. 1Argonne National Laboratory, Argonne, IL; 2Bhabha Atomic Research Centre, Mumbai, India; 3Brookhaven National Laboratory, Upton, NY; 4University of Buenos Aires, Argentina; 5University of California, Los Angeles, CA; 6CERN, Geneva, Switzerland; 7University of Colorado, Boulder,CO; 8Columbia University, New York, NY; 9DESY, Hamburg, Germany; 10University of Glasgow, Scotland, United Kingdom; 11Hampton University, Hampton, VA; 12University of Illinois, UrbanaChampaign, IL; 13Iowa State University, Ames, IA; 14University of Kyoto, Japan; 15Lawrence Berkeley National Laboratory, Berkeley, CA; 16Los Alamos National Laboratory, Los Alamos, NM; 17University of Massachusetts, Amherst, MA; 18MIT, Cambridge, MA; 19Max Planck Institut für Physik, Munich, Germany; 20University of Michigan Ann Arbor, MI; 21New Mexico State University, Las Cruces, NM; 22Old Dominion University, Norfolk, VA; 23Penn State University, PA; 24RIKEN, Wako, Japan; 24-1RIKEN-BNL Research Center, BNL, Upton, NY; 25Soltan Institute for Nuclear Studies, Warsaw, Poland; 26SUNY, Stony Brook, NY; 27Tel Aviv University, Israel; 28Thomas Jefferson National Accelerator Facility, Newport News, VA 96 Scientists, 28 Institutions, 9 countries 26 Additional Slides 27 Regimes of QCD Wave Function in 3D 28 Spin Physics at the EIC - The Quest for G Spin Structure of the Proton ½ = ½ + G + Lq + Lg quark contribution ΔΣ ≈ 0.3 gluon contribution ΔG ≈ 1 ± 1 ? G: a “quotable” property of the proton (like mass, charge) Measure through scaling violation: dg1 2 g(x,Q ) 2 d log( Q ) G x1 g(x,Q )dx 2 x 0 Superb sensitivity to g at small x! 29 Charm at EIC in e+A Based on HVQDIS model, J. Smith EIC: allows multi-differential measurements of heavy flavor covers and extend energy range of SLAC, EMC, HERA, and JLAB allowing study of wide range of formation lengths 30 What Do We Know About Glue in Matter? Deep Inelastic Scattering : 2 d 2 ep eX 4 e.m. y 2 y2 2 2 1 y F2 (x,Q ) FL (x,Q ) 2 4 dxdQ xQ 2 2 Deep Inelastic Scattering: Scaling Measure of resolution violation: dF2power: /dlnQ2 and ~1/wavelength linear DGLAP Evolution G(x,Q2) Q 2 q 2 (k k ) 2 2 Measure of momentum fraction of struck quark x Gluons dominate 2 Qlow-x wave function 2 pqxG ( 1 20 xu v ) Measure of inelasticity xd v E E y Ee xS ( 1 ) ' e 20 e “Perfect” Tomography 31