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Extreme QCD at RHIC and LHC Jamal Jalilian-Marian Baruch College, - PowerPoint PPT Presentation

Extreme QCD at RHIC and LHC Jamal Jalilian-Marian Baruch College, New York, NY, USA OUTLINE QCD at high temperature Phase transition: hadrons to partons ( QGP ) QCD at high energy Unitarity: small to large ( CGC ) RHIC and LHC QCD at high T


  1. Extreme QCD at RHIC and LHC Jamal Jalilian-Marian Baruch College, New York, NY, USA

  2. OUTLINE QCD at high temperature Phase transition: hadrons to partons ( QGP ) QCD at high energy Unitarity: small to large ( CGC ) RHIC and LHC

  3. QCD at high T Hadrons vs. partons: energy density Hadronic Matter: quarks and gluons confined up to T ~ 200 MeV, 3 pions with spin=0 Quark Gluon Matter: 8 gluons; 2 quark flavors, antiquarks, 2 spins, 3 colors 37 >> 3

  4. QGP vs. Hadron Gas Lattice QCD ε /T 4 Transition values: T = 170 MeV ε _ c = 0.8 GeV/fm 3 Assumes thermal system hadrons ⇒ quark/gluon T/T c need to create ε >> ε c

  5. RHIC Center of mass energy: 20, 60, 130, 200 GeV Hot nuclear matter: Central: gold-gold, copper-copper maximum overlap Cold nuclear matter: deuteron-gold Baseline: proton-proton Peripheral: “Almond” of RHIC-II overlap region

  6. Colliding heavy ions at high energies B jorken: high p t par tp ns sca tu er fs om ti e medium an d “ lose energy ” ( radia tf gluons ) path length L λ

  7. QGP at RHIC * Note deuteron-gold control experiment with no suppression dAu d-Au Au-Au

  8. Probing the medium

  9. QGP at RHIC disappearance of 1/N trigger dN/d(Df) back to back jets away side near side

  10. From CGC to QGP: Space-Time History of a Heavy Ion Collision Initial conditions

  11. Degrees of Freedom in a Nucleus? It depends on the scales probed! A point particle λ >> 10 fm A collection of protons and neutrons λ ∼ 1 fm A dense system of quarks and gluons λ << 1 fm

  12. Deeply Inelastic Scattering (DIS) THE SIMPLEST WAY TO STUDY QCD IN A HADRON/NUCLEUS QED e p (A) ---> e X Kinematic Invariants: Center of mass energy squared S ≡ ( p + q ) 2 Momentum resolution squared Q 2 ≡ − q 2 Q 2 X bj ≡ QCD: Structure Functions F 1 , F 2 2 p · q

  13. The hadron at high energy Q 2 Q 2 , ν → ∞ ★ Bjorken: but fixed ν structure functions F 1 , F 2 depend only on x bj ★ Feynman: Parton constituents of proton are “quasi-free” on interaction time scale 1/Q << 1/ Λ (interaction time scale between partons) X F = fraction of hadron momentum carried by a parton = X bj

  14. The hadron at high energy Parton model QCD - bound quarks

  15. pQCD--RG evolution (radiation) “sea” quarks Valence quarks � 1 dx x [ xq ( x ) − x¯ q ( x )] = 3 # of valence quarks 0 � 1 dx x [ xq ( x ) + x¯ q ( x )] → ∞ # of quarks .... 0

  16. pQCD--RG evolution (radiation) evolution of distribution functions DGLAP Bj scaling

  17. pQCD--RG evolution (radiation) # of gluons grows rapidly at small x…

  18. Resolving the hadron: DGLAP evolution Radiated gluons have smaller and smaller sizes (~ 1/Q 2 ) as Q 2 grows The number of gluons increases but the phase space density decreases: hadron becomes more dilute

  19. QCD in the Regge-Gribov limit Q 2 fixed , S → ∞ X bj → 0 Regge Gribov

  20. BFKL evolution � The infrared sensitivity of bremsstrahlung favors the emission of ‘soft’ (= small– x ) gluons d k z d x d P ∝ α s = α s k z x � The ‘price’ of an additional gluon: � 1 d x 1 = α s ln 1 P (1) ∝ α s x 1 x x

  21. BFKL evolution: Unitarity violation � The ‘last’ gluon at small x can be emitted off any of the ‘fast’ gluons with x � > x radiated in the previous steps : ∂ n n ( Y ) ∝ e ωα s Y = ∂ Y � α s n ⇒ � Dipole scattering amplitude: T ∼ α s n � Unitarity bound : SS † = 1 = ⇒ T ≤ 1 — violated by BFKL !

  22. The hadron at high energy QCD Bremsstrahlung Non-linear evolution- Gluon recombination: Proton this is essential if proton is a dense object

  23. How to achieve high gluon density Increase the energy large x Radiated gluons have the same size (1/Q 2 ) - the number of partons increase due to the increased longitudinal phase space small x or/and large nuclei

  24. Parton saturation Competition between “attractive” bremsstrahlung and “repulsive” recombination effects maximal phase space density saturated for Q = Q s ( x ) � Λ QCD � 0 . 2 GeV

  25. Classical Effective Theory McLerran, Venugopalan Consider a large nucleus in the IMF frame One large component of the current-others suppressed by Wee partons see a large density of valence color charges at small transverse resolutions

  26. Born-Oppenheimer: separation of large x and small x modes Large X partons are static over small X parton life times

  27. The effective action coupling of color Yang-Mills charges to gluon fields weight function for color charge configurations where MV:

  28. Hadron/nucleus at high energy is a Color Glass Condensate dN k t d 2 k t k t Λ QCD Q s ( x ) ✤ Gluons are colored ✤ Random sources evolving on time scales much larger than natural time scales - very similar to spin glasses n ∼ 1 ✤ Bosons with a large occupation number α s ✤ Typical momentum of gluons is Q s ( x )

  29. QCD at High Energy: from classical to quantum ( α s Log 1/x ) Fields Sources 0 1 Integrate out small fluctuations => Increase color charge of B-JIMWLK

  30. B-JIMWLK equations describe evolution of all N-point correlation functions with energy the 2-point function: Tr [1 - U + (x t ) U (y t )] (probability for scattering of a quark-anti-quark dipole on a target) B-JIMWLK in two limits: I) Strong field: exact scaling - f (Q 2 /Q 2s ) for Q < Q s II) Weak field: BFKL

  31. BK: mean field + large N c A closed form equation The simplest equation to include unitarity: T < 1 Exhibits geometric scaling T ( x , r t ) → T [ r t Q s ( x )] for Q 2 s Q s < Q < Λ QCD

  32. Geomtric scaling at HERA

  33. A New Paradigm of QCD Saturation region: dense system of gluons Extended scaling region: dilute system -anomalous dimension Double Log: BFKL meets DGLAP DGLAP: collinearly factorized pQCD

  34. Relation to statistical physics MP α N 2 ∂ y N = ¯ α χ [ − ∂ L ] N − ¯ BK in momentum space can be written as with ∂ t u = ∂ 2 x u + u − u 2 N --> u, y ---> t,L ---> x u = 1 : stable traveling wave solution t t’ > t u = 0 :unstable F-KPP equation in statistical mechanics with applications in biology, ....

  35. Beyond B-JIMWLK (BK) some undesirable features merging vs. splitting 2 --> 1 vs. 1 --> 2 reaction-diffusion in statistical mechanics: sF-KPP Pomeron loops BFKL saturation fluctuation

  36. The new phase diagram The “phase–diagram” revisited

  37. Applications to RHIC and LHC

  38. Colliding sheets of color glass solve the classical eqs. of motion in the forward light cone: subject to initial conditions given by one nucleus solution Classical Fields with occupation # f= Initial energy and multiplicity of produced gluons depends on Q_s Fermion production (Gelis et al.)

  39. Colliding Sheets of Colored Glass adding final state effects: hydro, energy loss

  40. Colliding Sheets of Colored Glass What happens to produced gluons? Is there thermalization of QCD matter? Can it be described by weak coupling ? Bottom up scenario ( Baier, Mueller, Schiff, Son ) Production of “hard” gluons: k ~ Q s Radiation of “soft” gluons: k << Q s Soft gluons thermalize Hard gluons thermalize Thermalization time: Instabilities? Fast thermalization?

  41. Signatures of CGC at RHIC: pA ✤ Multiplicities (dominated by p t < Q s ): energy, rapidity, centrality dependence ✤ Single particle production: hadrons, EM rapidity, p t , centrality dependence Fixed p t : vary rapidity (evolution in x) i) ii) Fixed rapidity: vary p t (transition from dense to dilute) ✤ Two particle production: back to back correlations

  42. CGC: qualitative expectations Classical (multiple elastic scattering): p t >> Q s : enhancement ( Cronin effect ) R pA = 1 + (Q s 2 /p t 2 ) log p t 2 / Λ 2 + … R pA (p t ~ Q s ) ~ log A position and height of enhancement are increasing with centrality Evolution in x: can show analytically the peak disappears as energy/rapidity grows and levels off at R pA ~ A -1/6 < 1 These expectations are confirmed at RHIC

  43. CGC vs. RHIC enhancement suppression BRAHMS

  44. Rapidity and pt dependence What we see is a transition from DGLAP to BFKL to CGC kinematics Centrality, flavor, species dependence

  45. The future is promising!

  46. Exciting time in high energy QCD again ✤ Frenetic pace of theoretical developments ✤ Hints for CGC from HERA ✤ Strong evidence for CGC from RHIC Significant ramifications for strong interaction physics at LHC and eRHIC

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