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STAR System size and energy dependence of the near-side of high-pT triggered correlations in STAR Christine Nattrass (Yale University)‏

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Presentation on theme: "STAR System size and energy dependence of the near-side of high-pT triggered correlations in STAR Christine Nattrass (Yale University)‏"— Presentation transcript:

1 STAR System size and energy dependence of the near-side of high-pT triggered correlations in STAR Christine Nattrass (Yale University)‏

2 Christine Nattrass (STAR), Prague, February 5, 2009Outline Introduction The Jet The Ridge Theory Conclusions At the LHC? 3<p t,trigger <4 GeV p t,assoc. >2 GeV Au+Au 0-10% STAR preliminary Ridge Jet 2

3 Christine Nattrass (STAR), Prague, February 5, 2009 Motivation – Jet and Ridge In d+Au peak narrow in ΔΦ, Δη even for small p T trigger Long-range pseudorapidity ( Δη ) correlations observed by STAR in Au+Au at intermediate p T Significant contribution to the near-side yield in central Au+Au at intermediate p T assoc,p T trigger Yield/trigger – number of particles in p T assoc range associated with trigger particle with p T trigger range d+Au √ s NN = 200 GeV nucl-ex/0701074 Au+Au √ s NN = 200 GeV 3

4 Christine Nattrass (STAR), Prague, February 5, 2009 Motivation – Jet and Ridge In d+Au peak narrow in ΔΦ, Δη even for small p T trigger Long-range pseudorapidity ( Δη ) correlations observed by STAR in Au+Au at intermediate p T Significant contribution to the near-side yield in central Au+Au at intermediate p T assoc,p T trigger Yield/trigger – number of particles in p T assoc range associated with trigger particle with p T trigger range d+Au √ s NN = 200 GeV nucl-ex/0701074 Au+Au √ s NN = 200 GeV 3

5 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge previously observed to be independent in Δη in Au+Au To determine relative contributions, find yields for near-side (-1< ΔΦ<1 ), take ΔΦ  projections in 3<p t,trigger <4 GeV p t,assoc. >2 GeV Ridge Jet+ Ridge Ridge Au+Au 0-10% STAR preliminary h+h nucl-ex/0701074 Method: Yield extraction 4

6 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge previously observed to be independent in Δη in Au+Au To determine relative contributions, find yields for near-side (-1< ΔΦ<1 ), take ΔΦ  projections in -0.75< Δη <0.75 Jet + Ridge 3<p t,trigger <4 GeV p t,assoc. >2 GeV Ridge Jet+ Ridge Ridge Au+Au 0-10% STAR preliminary h+h nucl-ex/0701074 Jet+Ridge STAR preliminary Method: Yield extraction 4

7 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge previously observed to be independent in Δη in Au+Au To determine relative contributions, find yields for near-side (-1< ΔΦ<1 ), take ΔΦ  projections in -0.75< Δη <0.75 Jet + Ridge 3<p t,trigger <4 GeV p t,assoc. >2 GeV Ridge Jet+ Ridge Ridge Au+Au 0-10% STAR preliminary h+h nucl-ex/0701074 Jet+Ridge STAR preliminary Method: Yield extraction 4

8 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge previously observed to be independent in Δη in Au+Au To determine relative contributions, find yields for near-side (-1< ΔΦ<1 ), take ΔΦ  projections in -0.75< Δη <0.75 Jet + Ridge 0.75<| Δη |<1.75 Ridge 3<p t,trigger <4 GeV p t,assoc. >2 GeV Ridge Jet+ Ridge Ridge Au+Au 0-10% STAR preliminary h+h nucl-ex/0701074 Jet+RidgeRidge STAR preliminary Method: Yield extraction 4

9 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge previously observed to be independent in Δη in Au+Au To determine relative contributions, find yields for near-side (-1< ΔΦ<1 ), take ΔΦ  projections in -0.75< Δη <0.75 Jet + Ridge 0.75<| Δη |<1.75 Ridge Jet = (Jet+Ridge) – Ridge*.75/1.0 3<p t,trigger <4 GeV p t,assoc. >2 GeV Ridge Jet+ Ridge Ridge Au+Au 0-10% STAR preliminary h+h nucl-ex/0701074 Jet+RidgeRidgeJet STAR preliminary Method: Yield extraction 4

10 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge previously observed to be independent in Δη in Au+Au To determine relative contributions, find yields for near-side (-1< ΔΦ<1 ), take ΔΦ  projections in -0.75< Δη <0.75 Jet + Ridge 0.75<| Δη |<1.75 Ridge Jet = (Jet+Ridge) – Ridge*.75/1.0 Ridge = yield from -1.75< Δη <1.75 – Jet yield 3<p t,trigger <4 GeV p t,assoc. >2 GeV Ridge Jet+ Ridge Ridge Au+Au 0-10% STAR preliminary h+h nucl-ex/0701074 Method: Yield extraction 4

11 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge previously observed to be independent in Δη in Au+Au To determine relative contributions, find yields for near-side (-1< ΔΦ<1 ), take ΔΦ  projections in -0.75< Δη <0.75 Jet + Ridge 0.75<| Δη |<1.75 Ridge Jet = (Jet+Ridge) – Ridge*.75/1.0 Ridge = yield from -1.75< Δη <1.75 – Jet yield Flow contributions to Jet cancel v 2 independent of η for |η|<1 Phys. Rev. C72, 051901(R) (2005), Phys. Rev. Lett. 94, 122303 (2005) ‏ 3<p t,trigger <4 GeV p t,assoc. >2 GeV Ridge Jet+ Ridge Ridge Au+Au 0-10% STAR preliminary h+h nucl-ex/0701074 Method: Yield extraction 4

12 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge previously observed to be independent in Δη in Au+Au To determine relative contributions, find yields for near-side (-1< ΔΦ<1 ), take ΔΦ  projections in -0.75< Δη <0.75 Jet + Ridge 0.75<| Δη |<1.75 Ridge Jet = (Jet+Ridge) – Ridge*.75/1.0 Ridge = yield from -1.75< Δη <1.75 – Jet yield Flow contributions to Jet cancel v 2 independent of η for |η|<1 Phys. Rev. C72, 051901(R) (2005), Phys. Rev. Lett. 94, 122303 (2005) ‏ 3.0 1.5 GeV/c unless otherwise stated 3<p t,trigger <4 GeV p t,assoc. >2 GeV Ridge Jet+ Ridge Ridge Au+Au 0-10% STAR preliminary h+h nucl-ex/0701074 Method: Yield extraction 4

13 Christine Nattrass (STAR), Prague, February 5, 2009 Jet Ridge Putschke WWND08 STAR Preliminary Extent of Ridge in Extent of Ridge in Ridge yield approximately independent of in STAR acceptance  PHOBOS ( arXiv:0804.3038v3 ) showed independence on out to = 4 Jet-like increases with p T trigger, Ridge roughly constant p T assoc > 2 GeV 5

14 Christine Nattrass (STAR), Prague, February 5, 2009 The Jet 3<p t,trigger <4 GeV p t,assoc. >2 GeV Au+Au 0-10% STAR preliminary Ridge Jet 6

15 Christine Nattrass (STAR), Prague, February 5, 2009 1.5 GeV/c<p T assoc <p T trigger p T trigger dependence Yields similar for d+Au, Cu+Cu and Au+Au at same√ s NN Pythia 8.1 describes trends in data up to a scaling factor  Gets energy dependence right → this is a pQCD effect  Stronger deviations at low p T trigger, as expected J. Bielcikova (STAR), arXiv:0806.2261/nucl-ex C. Nattrass (STAR), arXiv:0804.4683/nucl-ex 7

16 Christine Nattrass (STAR), Prague, February 5, 2009 Pythia 8.1 comparisons What can Pythia tell us?  Higher z T (lower jet energy) in 62 GeV for same p T trigger pTHatMin = the parameter in Pythia for the minimum transverse momentum in the hard subprocess 8 3.0 < p T trigger < 6.0 GeV/c 1.5 GeV/c<p T assoc <p T trigger

17 Christine Nattrass (STAR), Prague, February 5, 2009 Pythia 8.1 comparisons What can Pythia tell us?  Higher z T (lower jet energy) in 62 GeV for same p T trigger pTHatMin = the parameter in Pythia for the minimum transverse momentum in the hard subprocess 8 3.0 < p T trigger < 6.0 GeV/c 1.5 GeV/c<p T assoc <p T trigger

18 Christine Nattrass (STAR), Prague, February 5, 2009 p T associated dependence No system dependence Pythia 8.1 slightly harder than data Diverges slightly from Pythia 8.1 at lower p T associated Inverse slope parameter Statistical errors only J. Bielcikova (STAR), arXiv:0806.2261/nucl-ex C. Nattrass (STAR), arXiv:0804.4683/nucl-ex 9 3.0 < p T trigger < 6.0 GeV/c

19 Christine Nattrass (STAR), Prague, February 5, 2009 N part dependence J. Bielcikova (STAR), arXiv:0806.2261/nucl-ex C. Nattrass (STAR), arXiv:0804.4683/nucl-ex No system dependence Some deviations from Pythia 8.1 with increase in N part  Incomplete Ridge subtraction?  Jet modification at low p T ? 10 3.0 < p T trigger < 6.0 GeV/c 1.5 GeV/c<p T assoc <p T trigger

20 Christine Nattrass (STAR), Prague, February 5, 2009 Jet composition Baryon/meson ratios in Jet in Cu+Cu and Au+Au similar to p+p for both strange and non-strange particles M. Lamont (STAR), J.Phys.G32:S105-S114,2006 J. Bielcikova (STAR), v:0707.3100 [nucl-ex] C. Nattrass (STAR), arXiv:0804.4683/nucl-ex 11

21 Christine Nattrass (STAR), Prague, February 5, 2009 The Ridge 3<p t,trigger <4 GeV p t,assoc. >2 GeV Au+Au 0-10% STAR preliminary Jet Ridge 12

22 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge vs N part No system dependence at given N part J. Bielcikova (STAR), arXiv:0806.2261/nucl-ex C. Nattrass (STAR), arXiv:0804.4683/nucl-ex 13 3.0 < p T trigger < 6.0 GeV/c 1.5 GeV/c<p T assoc <p T trigger STAR Preliminary

23 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge vs N part No system dependence at given N part Ridge/Jet Ratio independent of collision energy J. Bielcikova (STAR), arXiv:0806.2261/nucl-ex C. Nattrass (STAR), arXiv:0804.4683/nucl-ex 13 3.0 < p T trigger < 6.0 GeV/c 1.5 GeV/c<p T assoc <p T trigger

24 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge yield persists to high p T trigger STAR preliminary p T associated > 2 GeV Putschke WWND08 14 Ridge yield vs. p T trigger in Au+Au

25 Christine Nattrass (STAR), Prague, February 5, 2009 Spectra of particles associated with Ridge similar to inclusive inclusive STAR Preliminary Putschke WWND08 p T associated > 2 GeV 15 Ridge yield vs. p T associated in Au+Au

26 Christine Nattrass (STAR), Prague, February 5, 2009 Baryon/meson ratios in Ridge similar to bulk for both strange and non-strange particles Suarez, QM08 M. Lamont (STAR), J.Phys.G32:S105-S114,2006 J. Bielcikova (STAR), v:0707.3100 [nucl-ex] C. Nattrass (STAR), arXiv:0804.4683/nucl-ex 16 Ridge composition

27 Christine Nattrass (STAR), Prague, February 5, 2009 Conclusions: RHIC data Pythia describes data well  Scaling factor needed but Pythia 8.1 is not as tuned as earlier versions  Energy dependence in Jet-like yield is pQCD effect  Trends for p T trigger, p T assoc dependence rightJet 17

28 Christine Nattrass (STAR), Prague, February 5, 2009 Conclusions: RHIC data Pythia describes data well  Scaling factor needed but Pythia 8.1 is not as tuned as earlier versions  Energy dependence in Jet-like yield is pQCD effect  Trends for p T trigger, p T assoc dependence right Particle ratios similar to p+p → Jet production mechanism dominated by fragmentationJet 17

29 Christine Nattrass (STAR), Prague, February 5, 2009 Conclusions: RHIC data Pythia describes data well  Scaling factor needed but Pythia 8.1 is not as tuned as earlier versions  Energy dependence in Jet-like yield is pQCD effect  Trends for p T trigger, p T assoc dependence right Particle ratios similar to p+p → Jet production mechanism dominated by fragmentation Jet-like yield agreement between different systems, with scaled Pythia  Simulations can be used to approximate z T distribution for comparisons of data to models?Jet 17

30 Christine Nattrass (STAR), Prague, February 5, 2009 Ridge Conclusions: RHIC data Pythia describes data well  Scaling factor needed but Pythia 8.1 is not as tuned as earlier versions  Energy dependence in Jet-like yield is pQCD effect  Trends for p T trigger, p T assoc dependence right Particle ratios similar to p+p → Jet production mechanism dominated by fragmentation Jet-like yield agreement between different systems, with scaled Pythia  Simulations can be used to approximate z T distribution for comparisons of data to models? Extensive data on Ridge...but what is it?Jet 17

31 Christine Nattrass (STAR), Prague, February 5, 2009 Models: RHIC and LHC 18

32 Christine Nattrass (STAR), Prague, February 5, 2009 19 Naïve assumptions from data... Ridge/Jet roughly independent of collision energy for the same kinematic cuts

33 Christine Nattrass (STAR), Prague, February 5, 2009 19 Naïve assumptions from data... Ridge/Jet roughly independent of collision energy for the same kinematic cuts Spectrum of particles in Ridge falls off rapidly with p T

34 Christine Nattrass (STAR), Prague, February 5, 2009 19 Naïve assumptions from data... Ridge/Jet roughly independent of collision energy for the same kinematic cuts Spectrum of particles in Ridge falls off rapidly with p T Ridge roughly independent of p T trigger

35 Christine Nattrass (STAR), Prague, February 5, 2009 19 Naïve assumptions from data... Ridge/Jet roughly independent of collision energy for the same kinematic cuts Spectrum of particles in Ridge falls off rapidly with p T Ridge roughly independent of p T trigger Dominant errors are systematic due to v 2

36 Christine Nattrass (STAR), Prague, February 5, 2009 19 Naïve assumptions from data... Ridge/Jet roughly independent of collision energy for the same kinematic cuts Spectrum of particles in Ridge falls off rapidly with p T Ridge roughly independent of p T trigger Dominant errors are systematic due to v 2 At the LHC, the Ridge should naïvely be the same size as at RHIC for the same kinematic cuts...

37 Christine Nattrass (STAR), Prague, February 5, 2009 19 Naïve assumptions from data... Ridge/Jet roughly independent of collision energy for the same kinematic cuts Spectrum of particles in Ridge falls off rapidly with p T Ridge roughly independent of p T trigger Dominant errors are systematic due to v 2 At the LHC, the Ridge should naïvely be the same size as at RHIC for the same kinematic cuts... BUT background will be higher, so unless v 2 is much smaller than at RHIC, the background may make measurements unfeasible

38 Christine Nattrass (STAR), Prague, February 5, 2009 arXiv:0711.1991v2arXiv:0711.1991v2Pr uneau et alModels Radial flow+trigger bias S. Voloshin, nucl-th/0312065, Nucl. Phys. A749, 287 C.. Pruneau, S. Gavin, S. Voloshin, arXiv:0711.1991v2 E. Shuryak, Phys.Rev.C76:047901,2007  At RHIC: Works for one set of kinematic cuts in central Au+Au at 200 GeV Need more detailed comparisons (energy dependence)‏ Model needs some refinements (momentum conservation)‏ 20

39 Christine Nattrass (STAR), Prague, February 5, 2009 arXiv:0711.1991v2arXiv:0711.1991v2Pr uneau et alModels Radial flow+trigger bias S. Voloshin, nucl-th/0312065, Nucl. Phys. A749, 287 C.. Pruneau, S. Gavin, S. Voloshin, arXiv:0711.1991v2 E. Shuryak, Phys.Rev.C76:047901,2007  At RHIC: Works for one set of kinematic cuts in central Au+Au at 200 GeV Need more detailed comparisons (energy dependence)‏ Model needs some refinements (momentum conservation)‏  At LHC: Predicts a specific relationship between radial flow and the Ridge Higher radial flow at LHC? → larger Ridge 20

40 Christine Nattrass (STAR), Prague, February 5, 2009 arXiv:0711.1991v2arXiv:0711.1991v2Pr uneau et alModels Radial flow+trigger bias S. Voloshin, nucl-th/0312065, Nucl. Phys. A749, 287 C.. Pruneau, S. Gavin, S. Voloshin, arXiv:0711.1991v2 E. Shuryak, Phys.Rev.C76:047901,2007  At RHIC: Works for one set of kinematic cuts in central Au+Au at 200 GeV Need more detailed comparisons (energy dependence)‏ Model needs some refinements (momentum conservation)‏  At LHC: Predicts a specific relationship between radial flow and the Ridge Higher radial flow at LHC? → larger Ridge Plasma instability QCD magnetic fields, Majumder et al,Phys.Rev.Lett.99:042301,2007 Anisotropic plasma, P. Romatschke, PRC,75014901 (2007)‏  At RHIC: So far unable to make enough Ridge without Radial flow+trigger bias 20 arXiv:0805.2795v2

41 Christine Nattrass (STAR), Prague, February 5, 2009 arXiv:0711.1991v2arXiv:0711.1991v2Pr uneau et alModels Radial flow+trigger bias S. Voloshin, nucl-th/0312065, Nucl. Phys. A749, 287 C.. Pruneau, S. Gavin, S. Voloshin, arXiv:0711.1991v2 E. Shuryak, Phys.Rev.C76:047901,2007  At RHIC: Works for one set of kinematic cuts in central Au+Au at 200 GeV Need more detailed comparisons (energy dependence)‏ Model needs some refinements (momentum conservation)‏  At LHC: Predicts a specific relationship between radial flow and the Ridge Higher radial flow at LHC? → larger Ridge Plasma instability QCD magnetic fields, Majumder et al,Phys.Rev.Lett.99:042301,2007 Anisotropic plasma, P. Romatschke, PRC,75014901 (2007)‏  At RHIC: So far unable to make enough Ridge without Radial flow+trigger bias  At LHC: No quantitative predictions 20 arXiv:0805.2795v2

42 Christine Nattrass (STAR), Prague, February 5, 2009Models Longitudinal flow Longitudinal flow, Armesto et al, PRL 93 (2004)  At RHIC: Problems due to Δη width Armesto et al, PRL 93 (2004) 21

43 Christine Nattrass (STAR), Prague, February 5, 2009Models Longitudinal flow Longitudinal flow, Armesto et al, PRL 93 (2004)  At RHIC: Problems due to Δη width  At LHC: No predictions, but would depend on amount of flow observed Armesto et al, PRL 93 (2004) 21

44 Christine Nattrass (STAR), Prague, February 5, 2009Models Longitudinal flow Longitudinal flow, Armesto et al, PRL 93 (2004)  At RHIC: Problems due to Δη width  At LHC: No predictions, but would depend on amount of flow observed Momentum kick Momentum kick from jet, C.-Y. Wong, Phys.Rev.C76:054908,2007  At RHIC: Fits data well, including energy dependence Armesto et al, PRL 93 (2004) 21

45 Christine Nattrass (STAR), Prague, February 5, 2009Models Longitudinal flow Longitudinal flow, Armesto et al, PRL 93 (2004)  At RHIC: Problems due to Δη width  At LHC: No predictions, but would depend on amount of flow observed Momentum kick Momentum kick from jet, C.-Y. Wong, Phys.Rev.C76:054908,2007  At RHIC: Fits data well, including energy dependence  At LHC: Predictions? Should be straightforward extension Armesto et al, PRL 93 (2004) C.Y. Wong Private communication 21

46 Christine Nattrass (STAR), Prague, February 5, 2009Models Longitudinal flow Longitudinal flow, Armesto et al, PRL 93 (2004)  At RHIC: Problems due to Δη width  At LHC: No predictions, but would depend on amount of flow observed Momentum kick Momentum kick from jet, C.-Y. Wong, Phys.Rev.C76:054908,2007  At RHIC: Fits data well, including energy dependence  At LHC: Predictions? Should be straightforward extension Recombination Medium heating + recombination, Chiu & Hwa, PRC72, 034903  At RHIC: No quantitative comparisons Armesto et al, PRL 93 (2004) C.Y. Wong Private communication 21

47 Christine Nattrass (STAR), Prague, February 5, 2009Models Longitudinal flow Longitudinal flow, Armesto et al, PRL 93 (2004)  At RHIC: Problems due to Δη width  At LHC: No predictions, but would depend on amount of flow observed Momentum kick Momentum kick from jet, C.-Y. Wong, Phys.Rev.C76:054908,2007  At RHIC: Fits data well, including energy dependence  At LHC: Predictions? Should be straightforward extension Recombination Medium heating + recombination, Chiu & Hwa, PRC72, 034903  At RHIC: No quantitative comparisons  At LHC: Should be there if Recombination observed in spectra Armesto et al, PRL 93 (2004) C.Y. Wong Private communication 21

48 Christine Nattrass (STAR), Prague, February 5, 2009 Conclusions: Models Several models available Need more quantitative comparisons Generally expect the Ridge Can it be measured?RHIC LHC 22

49 Christine Nattrass (STAR), Prague, February 5, 2009 STAR Collaboration Argonne National Laboratory - University of Birmingham - Brookhaven National Laboratory - California Institute of Technology - University of California, Davis - University of California - University of California, Los Angeles - Carnegie Mellon University - University of Illinois at Chicago - Creighton University - Nuclear Physics Institute Prague - Laboratory for High Energy (JINR) - Particle Physics Laboratory (JINR) - University of Frankfurt - Institute of Physics, Bhubaneswar - Indian Institute of Technology, Mumbai - Indiana University, Bloomington - Institut de Recherches Subatomiques - University of Jammu - Kent State University - Institute of Modern Physics, Lanzhou - Lawrence Berkeley National Laboratory - Massachusetts Institute of Technology - Max-Planck-Institut fuer Physik - Michigan State University - Moscow Engineering Physics Institute - City College of New York - NIKHEF and Utrecht University - Ohio State University, Columbus - Panjab University - Pennsylvania State University - Institute of High Energy Physics, Protvino, Russia - Purdue University - Pusan National University, Pusan, Republic of Korea - University of Rajasthan, Jaipur - Rice University - Universidade de Sao Paulo - University of Science & Technology of China - Shanghai Institute of Applied Physics - SUBATECH, Nantes, France - Texas A&M University - University of Texas - Tsinghua University - Valparaiso University - Variable Energy Cyclotron Centre, Kolkata, India - Warsaw University of Technology - University of Washington - Wayne State University - Institute of Particle Physics, CCNU (HZNU), Wuhan - Yale University - University of Zagreb 23

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