Qualitative and Quantitative Energy Loss?

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Presentation transcript:

Qualitative and Quantitative Energy Loss? W. A. Horowitz University of Cape Town October 11, 2010 With many thanks to Brian Cole, Miklos Gyulassy, Ulrich Heinz, Jiangyong Jia, and Yuri Kovchegov 2/24/2019 HP2010

QGP Energy Loss Learn about E-loss mechanism Most direct probe of DOF AdS/CFT Picture pQCD Picture 2/24/2019 HP2010

pQCD Success at RHIC: (circa 2005) Null Control: RAA(g)~1 Y. Akiba for the PHENIX collaboration, hep-ex/0510008 Consistency: RAA(h)~RAA(p) Null Control: RAA(g)~1 GLV Prediction: Theory~Data for reasonable fixed L~5 fm and dNg/dy~dNp/dy 2/24/2019 HP2010

pQCD Suppression Picture Inadequate Lack of even qualitative understanding p0, h, g RAA well described, BUT e- RAA, v2 are not, even with elastic loss PHENIX, Phys. Rev. Lett. 98, 172301 (2007) Wicks et al., NPA784, 2007 2/24/2019 HP2010

More Reasons for Concern IAA WHDG soon Baryon/Meson Ratio STAR pT pQCD w/ KKP pQCD w/ DSS WAH, in preparation Jamie Nagle, QM09 2/24/2019 HP2010

Death of pQCD at RHIC? Failure at > 9 GeV! Pert. at LHC energies? Important to get to >~ 10 GeV to avoid IS, hadronization effects Rui Wei, for PHENIX, QM09 PHENIX, arXiv:1006.3740 See also J Jia;s plenary on the 11th Pert. at LHC energies? 2/24/2019 HP2010

Before We Make Any Conclusions... While experiments are converging Theoretically, what are the effects of higher orders in as (large) kT/xE (large) MQ/E (large?) opacity (large?) geometry uncertainty in IC (small) coupling to flow (large) better treatment of elastic E-loss E-loss in confined matter 2/24/2019 HP2010

Influence of as Varying as has huge effect Role of running coupling, irreducible uncertainty from non-pert. physics? Also large changes from better elastic treatment S Wicks, PhD Thesis 2/24/2019 HP2010

Uncertainty from Wide Angle Radiation Single inclusive dNg/dx leads to energy loss All current Eloss calculations assume small angle emission (kT << xE) This is a bad assumption for RHIC kinematics WAH and B Cole, PRC81, 2010 2/24/2019 HP2010

Quantification of Collinear Uncertainty Factor ~ 3 uncertainty in extracted medium density! “qhat” values from different formalisms consistent w/i unc. WAH and B Cole, PRC81, 2010 2/24/2019 HP2010

Applicability of Collinear Approximation Unc. wrt some obs. decreases with pT Although not true for all observables 2/24/2019 HP2010

v2: “Collinearly Safe” Fix dNg/dy from RAA, calculate v2 Expect larger v2 for smaller opening angle ( tcoh ~ 1/kT2 ) IAA: coming soon Rad Only Rad + El v2 pT 20-30% p0 20-30% p0 v2 pT WAH, in preparation 2/24/2019 HP2010

Quark Mass Corrections All calculations assume MQ << pT Large corrections expected for observed NPE NB: Mbottom ~ 4.75 GeV 9 GeV e- from ~ 15 GeV b c and b separation will help tremendously Wicks et al., NPA784, 2007 2/24/2019 HP2010

Quantifying Sensitivity to Geometry IC Effects of geom. on, e.g. v2, might be quite large CGC vs. KLN and rotating RP Effect not large enough WAH and J Jia, in preparation Possibly truly outlandish initial geometry? See also Renk et al., arXiv:1010.1635 2/24/2019 HP2010

Coupling of Flow to Eloss Is high-pT v2 huge due to medium push? RAA(f = 0, Npart) vs. RAA(f = p/2, Npart) WS Glauber HN Mixed KLN CGC PHOBOS 2008 Data Npart RAA RAA in RAA out PHENIX Preliminary 7-8 GeV p0 Care taken with dNg/dy(Npart) Horowitz and Jia, in preparation 2/24/2019 HP2010 Smaller influence of fluc.?

Jets in AdS/CFT Model heavy quark jet energy loss by embedding string in AdS space dpT/dt = - m pT m = pl1/2 T2/2Mq J Friess, S Gubser, G Michalogiorgakis, S Pufu, Phys Rev D75 (2007) Similar to Bethe-Heitler dpT/dt ~ -(T3/Mq2) pT Very different from usual pQCD and LPM dpT/dt ~ -LT3 log(pT/Mq) 2/24/2019 HP2010

Compared to Data String drag: qualitative agreement WAH, PhD Thesis 2/24/2019 HP2010

Light Quark and Gluon E-Loss WAH, in preparation Marquet and Renk, PLB685 (2010) SS Gubser, QM08 DLqtherm ~ E1/3 DLqtherm ~ (2E)1/3 Gubser et al., JHEP0810 (2008) Chesler et al., PRD79 (2009) 2/24/2019 HP2010

Baryon to Meson Ratios Distinguishing measurement? STAR STAR AdS/CFT pQCD STAR AdS/CFT pQCD STAR WAH, in preparation 2/24/2019 HP2010

pQCD vs. AdS/CFT at LHC Plethora of Predictions: WAH, M. Gyulassy, PLB666 (2008) Taking the ratio cancels most normalization differences pQCD ratio asymptotically approaches 1, and more slowly so for increased quenching (until quenching saturates) AdS/CFT ratio is flat and many times smaller than pQCD at only moderate pT WAH, M. Gyulassy, PLB666 (2008) 2/24/2019 HP2010

Worldsheet boundary Spacelike if g > gcrit Not So Fast! Speed limit estimate for applicability of AdS drag g < gcrit = (1 + 2Mq/l1/2 T)2 ~ 4Mq2/(l T2) Limited by Mcharm ~ 1.2 GeV Similar to BH LPM gcrit ~ Mq/(lT) No Single T for QGP smallest gcrit for largest T T = T(t0, x=y=0): “(” largest gcrit for smallest T T = Tc: “]” D3 Black Brane D7 Probe Brane Q Worldsheet boundary Spacelike if g > gcrit Trailing String “Brachistochrone” “z” x5 2/24/2019 HP2010

LHC RcAA(pT)/RbAA(pT) Prediction (with speed limits) WAH, M. Gyulassy, PLB666 (2008) T(t0): “(”, corrections likely small for smaller momenta Tc: “]”, corrections likely large for higher momenta Qualitatively, corrections to AdS/CFT result will drive double ratio to unity 2/24/2019 HP2010

Conclusions pQCD fails to simultaneously describe RAA, v2, IAA, ... for p, e Higher order effects are hugely important as, kT/xE, MQ/xE, opacity HO effects can be mitigated in some cases by examining simultaneous observables going to higher energies IC effects seem small and under control Coupling of low-pT flow to E-loss likely very important AdS/CFT qualitatively agrees with p and e RAA Also better agreement with B/M ratio, v2 Lots of interesting theory work needed for rigorous conclusions Higher energies, c and b separation at RHIC and LHC likely key to understanding E-loss mechanism, QGP 2/24/2019 HP2010