Jet Modifications in the RHIC and LHC Era

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Jet Modifications in the RHIC and LHC Era Wayne State, August 20, 2014 In

Jet Modifications in the RHIC and LHC Era Wayne State, August 20, 2014 In Medium Hadronization: Hadrons and Jets Rainer Fries Texas A&M University With Kyongchol Han Che-Ming Ko JET Reco Working Group

Outline n Hadronization and in-medium hadronization n The JET shower recombination module n How

Outline n Hadronization and in-medium hadronization n The JET shower recombination module n How to implement a medium n Some preliminary results with medium n Summary Rainer Fries Jet Mod 2014 2

Hadronization Matters n Example: Hadron chemistry ¨ Does the B/M ratio measure phase space

Hadronization Matters n Example: Hadron chemistry ¨ Does the B/M ratio measure phase space occupation? p+p / p++p- C. Suarez et al, QM 08 p. Ttrig > 4. 0 Ge. V/c 2. 0 < p. TAssoc < p. Ttrig Can effect be measured directly? YES n Example: Elliptic flow in the heavy quark sector. Hadronization in-medium = additional interaction with thermal medium. ¨ More diffusion/thermalization Can effect be measured directly? DIFFICULT ¨ Rainer Fries Jet Mod 2014 [M He, R J Fries, R Rapp, PRC 86 014903 (2012) ] 3

Hadronization Candidates n Lund string fragmentation n Cluster hadronization n Jet recombination Rainer Fries

Hadronization Candidates n Lund string fragmentation n Cluster hadronization n Jet recombination Rainer Fries Jet Mod 2014 4

Why Quark Recombination? n Data indicates a dependence of several important observables on the

Why Quark Recombination? n Data indicates a dependence of several important observables on the number of valence quarks. n Quark coalescence models very successful for hadron production at intermediate PT in HICs. Large baryon/meson ratios ¨ Elliptic flow scaling with quark number QGP signature? ¨ Rainer Fries Jet Mod 2014 5

Hadronization Candidates n No clear strategy how to generalize strings or clusters to in-medium

Hadronization Candidates n No clear strategy how to generalize strings or clusters to in-medium hadronization. n Recombination did not have a working jet shower implementation. Can one get vacuum fragmentation right? n Including medium effects then in principle straight forward; good track record. n JET jet shower recombination module: work in progress (see yesterday’s talk) n This is a project that benefits from feedback from the community. Rainer Fries Jet Mod 2014 6

Summary of JET Recombination n Standard PYTHIA Lund string fragmentation: Lund String n Our

Summary of JET Recombination n Standard PYTHIA Lund string fragmentation: Lund String n Our approach: Force gluon decay String Decay Recombine into hadrons and resonances Remnant strings String Decay Rainer Fries Jet Mod 2014 7

Summary of JET Recombination String Cluster Recombination Gluons Kinks Forced decay Large separation quarks

Summary of JET Recombination String Cluster Recombination Gluons Kinks Forced decay Large separation quarks String breaking Clusters String Breaking Small separation quarks, low mass Indirectly from string breaking Clusters Direct recombination High mass cluster Resonance Small separation Indirectly from quarks, high mass string breaking Rainer Fries Jet Mod 2014 8

Some Results n Longitudinal structure: d. N/dz of stable particles compared to PYTHIA string

Some Results n Longitudinal structure: d. N/dz of stable particles compared to PYTHIA string fragmentation. n How to tune parameters? 100 Ge. V jets Rainer Fries Jet Mod 2014 9

Adding Medium Partons n n Sampling thermal partons from a blastwave models or hydro.

Adding Medium Partons n n Sampling thermal partons from a blastwave models or hydro. Allow recombination of shower partons with thermal partons. Recombine Remnant strings Rainer Fries Jet Mod 2014 10

Space-Time Picture n Space-time picture important. QGP T > Tc Hadronization T ~ Tc

Space-Time Picture n Space-time picture important. QGP T > Tc Hadronization T ~ Tc n Hadronic/vacuum T < Tc Situation not static: T = Tc hypersurface moving. Rainer Fries Jet Mod 2014 11

Space-Time Picture n Space-time picture important. QGP T > Tc Hadronization T ~ Tc

Space-Time Picture n Space-time picture important. QGP T > Tc Hadronization T ~ Tc Hadronic/vacuum T < Tc n Situation not static: T = Tc hypersurface moving. n Jet shower partons born into QGP need to either propagate to the surface or be absorbed by the medium. How this is handled will depend strongly on the shower MC. Hadronization will only be applied to partons at or below Tc. n n Rainer Fries Jet Mod 2014 12

Space-Time Picture n Space-time picture important. QGP T > Tc Hadronization T ~ Tc

Space-Time Picture n Space-time picture important. QGP T > Tc Hadronization T ~ Tc n n n Hadronic/vacuum T < Tc There is a range, say e. g. T = 155 -175 Me. V, during which recombination can happen. This translates to a finite thickness of the critical hypersurface. This should be a physical quantity but it’s not necessarily a known quantity. Rainer Fries Jet Mod 2014 13

Space-Time Picture n Eventually this space-time picture will be determined from the underlying hydro

Space-Time Picture n Eventually this space-time picture will be determined from the underlying hydro event. n Here: a few very preliminary results for shower born 1 fm inside a static QGP phase. Thickness of the critical hypersurface is another fermi. Rainer Fries Jet Mod 2014 14

Results in a Semi-Realistic Setup n n n Modification of low-z spectra for 100

Results in a Semi-Realistic Setup n n n Modification of low-z spectra for 100 Ge. V jets by presence of a medium at hadronization. Showers: PYTHIA vacuum showers. Point of origin 1 fm inside the QGP Rainer Fries Jet Mod 2014 15

Results in a Semi-Realistic Setup n n n Modification of PT-spectra (all z) for

Results in a Semi-Realistic Setup n n n Modification of PT-spectra (all z) for 100 Ge. V jets by presence of a medium at hadronization. Showers: PYTHIA vacuum showers. Point of origin 1 fm inside the QGP Rainer Fries Jet Mod 2014 16

Varying the Point of Origin (Preliminary) n Modification of z-spectra for 100 Ge. V

Varying the Point of Origin (Preliminary) n Modification of z-spectra for 100 Ge. V jets by presence of a medium at hadronization. 3 fm 1 fm n Trade some sh-sh to sh-th but almost no change in overall spectrum. Rainer Fries Jet Mod 2014 17

How will Hadronization Matter? n We need to get the physics of in-medium hadronization

How will Hadronization Matter? n We need to get the physics of in-medium hadronization at least approximately right in simulations. No effect? Fine, but we needed to check. ¨ Large effects? Fine!! We need to look into the physics more closely. Explore parameter space. ¨ n Generally: in-medium hadronization is just another layer of interaction with the medium Energy and momentum exchange with the medium. ¨ In principle interaction continues in the hadronic phase! ¨ n Hadrons: hadronization will only affect small and intermediate momentum hadrons. Chemistry effects: should be measurable; expect increased baryon/meson ratio ¨ Momentum diffusion/broadening: size of the effect needs to be studied in simulations, maybe hard to distinguish from other sources of diffusion/broadening. ¨ Rainer Fries Jet Mod 2014 18

How will Hadronization Matter? n Inclusive jets: hadronization effects suppressed by design. No access

How will Hadronization Matter? n Inclusive jets: hadronization effects suppressed by design. No access to chemistry ¨ Diffusion/broadening can contribute to in-cone/out-of-cone effects. ¨ n Jet-hadron correlations/fragmentation functions: most promising to see hadronization effects. ¨ Both hadrochemistry and momentum redistribution. n None of this has been investigated on the MC level. n JET MCs should be able to do that within a year. Rainer Fries Jet Mod 2014 19