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Rapidity correlations in the CGC

N. Armesto. Rapidity correlations in the CGC. ECT* Workshop on High Energy QCD: from RHIC to LHC Trento, January 9th 2007. N éstor Armesto Departamento de Física de Partículas and Instituto Galego de Física de Altas Enerxías Universidade de Santiago de Compostela with

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Rapidity correlations in the CGC

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  1. N. Armesto Rapidity correlations in the CGC ECT* Workshop on High Energy QCD: from RHIC to LHC Trento, January 9th 2007 Néstor Armesto Departamento de Física de Partículas and Instituto Galego de Física de Altas Enerxías Universidade de Santiago de Compostela with Larry McLerran (BNL) and Carlos Pajares (Santiago de Compostela) Based on Nucl. Phys. A781 (2007) 201 (hep-ph/0607345). 1

  2. N. Armesto Contents 1. Introduction (see Capella and Krzywicki '78). 2. Long-range rapidity correlations (LRC) in the CGC (see also Kovchegov, Levin, McLerran '01). 3. LRC in string models (based on Brogueira and Dias de Deus, hep-ph/0611329). 4. Some numbers at RHIC and the LHC. 5. Summary. 2 Rapidity correlations in the CGC

  3. N. Armesto 1. Introduction (I): • Correlations have always been expected to reflect the features of multiparticle production, including eventual phase transitions. • Simplistic, multipurpose picture of multiparticle production: first formation of sources, then coherent decay of the sources into particles. • Correlations in rapidity characterize, in principle, the process of formation and decay of such clusters: how many of them, which size i. e. how many particles do they produce? 3 Rapidity correlations in the CGC

  4. N. Armesto 1. Introduction (II): • One source characterized by exponentially damped rapidity correlations: * Old multiperipheral models. * e+e- collisions in two-jet events: string models very successful. D2BF=<nBnF> - <nB><nF> D2=D2FF=<nF2> - <nF>2 <nF>(nB)=a+bnB sFB=b=D2BF/D2: correlation strength • In hadronic collisions, D2FF characterizes the short range correlations, related with the number of emitted particles per cluster, while D2BF, long range for a gap > 1.5-2, is related with the number of sources, provided SRC >> LRC as experimentally seen. 4 Rapidity correlations in the CGC

  5. N. Armesto 2. LRC in the CGC (I): • The picture of an AB collision in the CGC (the glasma) corresponds to the creation at short times t~exp(-k/as) of a central region with longitudinal fields (strings, flux tubes) from the passage of the transverse nuclear fields one through each other (Lappi, McLerran '06) . • Neglecting the difference in Qs between projectile and target, in a transverse region of size a~1/Qs the multiplicity becomes KN 5 Rapidity correlations in the CGC

  6. N. Armesto 2. LRC in the CGC (II): • LRC come from production from different sources in the same transverse region a~1/Qs. For gluons: O(g) • In the region where the classical fields are rapidity invariant: O(1/g) • Note that for quarks (baryon production): 6 Rapidity correlations in the CGC

  7. N. Armesto 2. LRC in the CGC (III): • k~1, and the correlated dNcor/dy is order as with respect to the uncorrelated one. • Both diagrams do not interfere, as the average over an odd number of sources in the same nucleus vanish. • Adding the correlated and uncorrelated pieces at Dy/(Dy=0), we get 7 Rapidity correlations in the CGC

  8. N. Armesto 2. LRC in the CGC (IV): • For large enough Dy, so SRC are absent and LRC, which should be little affected by hadronic rescattering, dominate, and assuming that Qs sets the scale for as, Qs growing with energy and Npart: * sFB increases with centrality. * sFB increases with energy. * sFB decreases with Dy. • All said above applies for gluons (mesons); for baryon production, the 1/as factor in coherent production is absent, so the dependence with energy and centrality should be milder. 8 Rapidity correlations in the CGC

  9. N. Armesto 3. LRC in string models (I): • We assume the existence of N sources (strings – longitudinal flux tubes). The multiplicity is: single source (SRC) number of sources (LRC) • For Poissonian sources, • So, for forward and backward rapidity windows, with a large enough gap between them: 9 Rapidity correlations in the CGC

  10. N. Armesto 3. LRC in string models (II): Finally • The (AGK) proportionality of the multiplicity with the number N of strings is corrected by a transverse surface geometric factor computed in 2d percolation: shadowing corrections interpolating between Ncoll and Npart ~ 2A. • h ~ 3 for central AuAu at at RHIC, and BDD assume 10 Rapidity correlations in the CGC

  11. N. Armesto 3. LRC in string models (III): • Comparison (fit) to STAR preliminary, nucl-ex/0606018 for charged: • b increases with centrality (faster in the non-percolation case): • b decreases with energy (provided K ~ hg, g>1/2): percolation 11 Rapidity correlations in the CGC

  12. N. Armesto 4. Some numbers at RHIC and LHC (I): • Just to illustrate the results (no errors considered, no direct work on experimental data with nevertheless are preliminary, no variations of the phenomenological input). • Scaleof as is Qs2 = (Npart/2)1/3 (Ecm/200 AGeV)0.288. • We use the BDD results for b=sFB as input to adjust ours for AuAu collisions at 200 AGeV, considering Dh=1.6 as large enough; We then go to the LHC, 5.5 ATeV, to see the difference in results between string models (BDD) and ours (AMP). 12 Rapidity correlations in the CGC

  13. N. Armesto 4. Some numbers at RHIC and LHC (II): • Qs2 ~ LQCD2 for Npart=2 at 200 GeV. • c ~ 5. • The behavior with centrality may be made similar, the behavior with energy cannot (for K ~ h). 13 Rapidity correlations in the CGC

  14. N. Armesto 5. Summary: • Correlations in rapidity provide information about the dynamics of multiparticle production in hadronic collisions: distribution and nature of the sources (strings, classical fields,...) of particles. • Within the CGC, the qualitative behavior is well defined: The LRC strength b=sFB * Increases with increasing energy. * Increases with increasing centrality. * Decreases with increasing rapidity gap. * Should be smaller for baryons (quarks) than for mesons (gluons). • String models show similar trends except (maybe) the increase with increasing energy. • For quantitative comparisons, the role of hadronic FSI must be considered. 14 Rapidity correlations in the CGC

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