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Multi-particle production in QCD at high energies Raju Venugopalan Brookhaven National Laboratory
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Outline of Lectures Lecture I: EFT approach to high energy QCD-The Color Glass Condensate; multi-particle production in the CGC Lecture II: Hadronic scattering in the CGC-multiple scattering & quantum evolution effects in limiting fragmentation & quark pair production Lecture III: Plasma instabilities & thermalization in the CGC; computing particle production in Heavy Ion collisions to next-to-leading order (NLO)
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All such diagrams of Order O(1/g) Nucleus-Nucleus Collisions…leading order graphs Inclusive multiplicity even to leading order requires 2 -> n Feynman amplitudes - completely non-perturbative problem! F. Gelis, RV hep-ph/0601209
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Initial conditions from matching eqns. of motion on light cone Yang-Mills Equations for two nuclei Kovner,McLerran,Weigert
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Longitudinal E and B fields created right after the collision - non-zero Chern-Simons charge generated Kharzeev,Krasnitz,RV; Lappi, McLerran
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Hamiltonian in gauge; per unit rapidity, For ``perfect’’ pancake nuclei, boost invariant configurations Solve 2+1- D Hamilton’s equations in real time for space-time evolution of glue in Heavy Ion collisions Lattice Formulation Krasnitz, RV
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Gluon Multiplicity with # dists. are infrared finite PRL 87, 192302 (2001)
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Dispersion relation: Just as for a Debye screening mass
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Classical field / Particle Particle
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Melting CGC to QGP L. McLerran, T. Ludlam, Physics Today Glasma…
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The “bottom up” scenario Baier, Mueller, Schiff, Son Scale for scattering of produced gluons (for t > 1/Q_s) set by Multiple collisions:
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Occupation # Radiation of soft gluons important for Thermalization for: and
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A flaw in the BMSS ointment - Weibel instabilities… Arnold,Lenaghan,Moore,Yaffe; Rebhan, Romatschke, Strickland; Mrowczynski Anisotropic momentum distributions of hard modes cause -exponential growth of soft field modes Changes sign for anisotropic distributions
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Effective potential interpretation: -ve eigenvalue => potential unbounded from below Large magnetic fields can cause O(1) change in hard particle trajectories on short time scales - - possible mechanism for isotropization of hard modes
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THE UNSTABLE GLASMA
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Instabilities from violations of boost invariance ? Boost invariance is never realized: a) Nuclei always have a finite width at finite energies b) Small x quantum fluctuations cause violations of boost invariance that are of order unity over Possible solution: Perform 3+1-D numerical simulations of Yang-Mills equations for Glasma exploding into the vacuum Romatsche + RV
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Construct model of initial conditions with fluctuations: i) ii) Method: Generate random transverse configurations: Generate Gaussian random function in \eta This construction explicitly satisfies Gauss’ Law
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Compute components of the Energy-Momentum Tensor
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Violations of boost invariance (3+1 -D YM dynamics) - leads to a Weibel instability Romatschke, RV PRL 96 (2006) 062302 For an expanding system,
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~ 2 * prediction from HTL kinetic theory
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Instability saturates at late times-possible Non-Abelian saturation of modes ?
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Distribution of unstable modes also similar to kinetic theory Romatschke, Strickland
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Very rapid growth in max. frequency when modes of transverse magnetic field become large - “bending” effect ?
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Accompanied by growth in longitudinal pressure…
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And decrease in transverse pressure… Right trends observed but too little too late…
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How do we systematically compute multi-particle production beyond leading order ? Problem can be formulated as a quantum field theory with strong time dependent external sources
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Power counting in the theory: Order of a generic diagram is given by with n_E = # of external legs, n_L the # of loops and n_J the # of sources. Order of a diagram given by # of loops and external legs
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In standard field theory, For theory with time dependent sources, Generating functional of Green’s functions with sources
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Probability of producing n particles in theory with sources: LSZ Generating Function of moments:
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Action of D[j_+,j_-] generates all the connected Green’s functions of the Schwinger-Keldysh formalism
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Inclusive average multiplicity: [ ]
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I) Leading order: O (1 / g^2) Obtained by solving classical equations - result known! Krasnitz, RV; Krasnitz, Nara, RV; Lappi
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II) Next-to-leading order: O ( g^0 ) + Remarkably, both terms can be computed by solving the small fluctuations equations of motion with retarded boundary conditions! Gelis & RV Similar to Schwinger mechanism in QED
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In QCD, for example, 2 +
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We now have an algorithm (with entirely retarded b.c.) to systematically compute particle production In AA collisions to NLO - particularly relevant at the LHC Pieces of this algorithm exist: Pair production computation of Gelis, Lappi and Kajantie very similar Likewise, the 3+1-D computation of Romatschke and RV Summary and Outlook
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Result will include All LO and NLO small x evolution effects NLO contributions to particle production Very relevant for studies of energy loss, thermalization at the LHC Conceptually issues at a very deep level - diffraction for instance - will challenge our understanding of the separation between “evolution” and “production” - factorization in QCD (Gelis & RV, in progress)
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