Jet quenching: future experiments and ‘End Game’ · 7.01.2018  · Jet quenching: future...

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Jet quenching: future experiments and ‘End Game’ Marco van Leeuwen, Nikhef, CERN JETSCAPE Workshop, 5-7 January 2018 LBNL, Berkeley

Transcript of Jet quenching: future experiments and ‘End Game’ · 7.01.2018  · Jet quenching: future...

  • Jet quenching: future experiments 
and ‘End Game’ 

    Marco van Leeuwen, Nikhef, CERN

    JETSCAPE Workshop, 5-7 January 2018LBNL, Berkeley

  • Jet quenching: future experiments 
and ‘End Game’ 

    Marco van Leeuwen, Nikhef, CERN

    JETSCAPE Workshop, 5-7 January 2018LBNL, Berkeley

    Disclaimer:We are (I am) not in a position yet to design the End Game yet, 
but will try to do the next best thing….

  • The physics of parton energy loss — what do want/can we aim to learn?

    2

    Plus a host of technical questions, e.g. role of event-by-event/geometry fluctuations

    Two broad categories: nature of energy loss mechanism and nature of the medium

    Nature of the energy loss mechanism

    Nature of the medium

  • The physics of parton energy loss — what do want/can we aim to learn?

    • Flavour dependence of energy loss• Path length dependence of energy loss• Interference: do jets lose energy as a single parton?

    • Also formation time effects• Transverse broadening: relate transverse and longitudinal dynamics

    • Testing our understanding of the medium/dominant process

    2

    Plus a host of technical questions, e.g. role of event-by-event/geometry fluctuations

    Two broad categories: nature of energy loss mechanism and nature of the medium

    Nature of the energy loss mechanism

    Nature of the medium

  • The physics of parton energy loss — what do want/can we aim to learn?

    • Flavour dependence of energy loss• Path length dependence of energy loss• Interference: do jets lose energy as a single parton?

    • Also formation time effects• Transverse broadening: relate transverse and longitudinal dynamics

    • Testing our understanding of the medium/dominant process

    2

    Plus a host of technical questions, e.g. role of event-by-event/geometry fluctuations

    • Density of the medium/value of qhat (vs temperature)• Distribution of radiated energy; approach to thermalisation?• Nature of the scattering centers?

    • Large angle deflection

    Two broad categories: nature of energy loss mechanism and nature of the medium

    Nature of the energy loss mechanism

    Nature of the medium

  • The physics of parton energy loss — what do want/can we aim to learn?

    • Flavour dependence of energy loss• Path length dependence of energy loss• Interference: do jets lose energy as a single parton?

    • Also formation time effects• Transverse broadening: relate transverse and longitudinal dynamics

    • Testing our understanding of the medium/dominant process

    2

    Plus a host of technical questions, e.g. role of event-by-event/geometry fluctuations

    • Density of the medium/value of qhat (vs temperature)• Distribution of radiated energy; approach to thermalisation?• Nature of the scattering centers?

    • Large angle deflection

    Two broad categories: nature of energy loss mechanism and nature of the medium

    Nature of the energy loss mechanism

    Nature of the medium

    Goal of the field: answer as many of these questions as we can, as well as we canTechnical questions have lower priority, but some may need answers to get to the interesting ones!

    Corollary: connections — Need coherent modeling of multiple observables

  • Part I: basic observables‘the bread and butter’

  • Simple observables; program and plan

    • Observables/measurements:• Single particle RAA, vn • Di-hadron, recoil suppression IAA• Heavy flavor RAA, vn

    4

    Progress to be made by:- Coherent modeling of multiple observables- Improving precision, pT reach, comparing RHIC+LHC

    • Density of the medium: value, time evolution of qhat• Path length dependence of energy loss• Heavy flavour energy loss; 


    dead cone effect, importance of elastic scattering vs radiation• Scale dependence of energy loss, medium properties?

    Address an important subset of the questions raised in the intro

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    CUJET2.0(αmax,fE,fM)

    CMS 0-5%ALICE 0-5%

    (0.20,1,0)(0.21,1,0)(0.22,1,0)(0.23,1,0)(0.24,1,0)(0.25,1,0)(0.26,1,0)(0.27,1,0)(0.28,1,0)(0.29,1,0)(0.30,1,0)(0.31,1,0)(0.32,1,0)

    Example of a systematic exploration: RHIC and LHC

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    Burke et al, JET Collaboration, arXiv:1312.5003

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    PHENIX 2012 (0-5%)

    RHIC

    RHIC

    LHC

    LHCSystematic comparison of energy loss models with dataMedium modelled by Hydrodynamics (2+1D, 3+1D)

    pT dependence matches reasonably well

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    Example of a systematic exploration: RHIC and LHC

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    Burke et al, JET Collaboration, arXiv:1312.5003

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    LHC

    LHCSystematic comparison of energy loss models with dataMedium modelled by Hydrodynamics (2+1D, 3+1D)

    pT dependence matches reasonably well

    RHIC:

    LHC:

    (Ti = 370 MeV)

    (Ti = 470 MeV)

  • What do we learn from ‘knowing’ qhat?

    6

    RHIC:

    LHC:

    (Ti = 370 MeV)

    (Ti = 470 MeV)

    i.e.

  • What do we learn from ‘knowing’ qhat?

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    RHIC:

    LHC:

    (Ti = 370 MeV)

    (Ti = 470 MeV)

    i.e.

    Arnold and Xiao, arXiv:0810.1026

    HTL expectation:

    relation qhat - T depends on number of degrees of freedom, 𝛼S

  • What do we learn from ‘knowing’ qhat?

    6

    RHIC:

    LHC:

    (Ti = 370 MeV)

    (Ti = 470 MeV)

    i.e.

    Arnold and Xiao, arXiv:0810.1026

    HTL expectation:

    relation qhat - T depends on number of degrees of freedom, 𝛼S

    Conclusion for now: values are in the right ballpark — we semi-quantitatively understand parton energy loss

  • What do we learn from ‘knowing’ qhat?

    6

    RHIC:

    LHC:

    (Ti = 370 MeV)

    (Ti = 470 MeV)

    i.e.

    Arnold and Xiao, arXiv:0810.1026

    HTL expectation:

    relation qhat - T depends on number of degrees of freedom, 𝛼S

    Conclusion for now: values are in the right ballpark — we semi-quantitatively understand parton energy loss

    Future direction: can we make this quantitative? 
E.g. determine number of degrees of freedom with a meaningful uncertainty? 
Or constrain T-dependence of qhat?

  • What do we learn II: transport coefficient and viscosity

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    H. Song et al, PRC

    83, 054912

    0 20 40 60 80centrality

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    RHIC: η/s=0.16LHC: η/s=0.16LHC: η/s=0.20LHC: η/s=0.24

    STAR

    ALICEv

    2{4}

    MC-KLNReaction Plane

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    Au+Au at 0.2 TeV

    Pb+Pb at 2.76 TeVqN/T3 (DIS)effˆ

    T (GeV)

    0

    q/T

    ≈≈

    ??

    ????

    NL

    O S

    YM

    Hints of increase of η/s and decrease of q/T3 
could have a common origin?

    Elliptic flow

    (Scaled) viscosity slightly larger at LHC Scaled transport coefficient
 slightly smaller at LHC

    Parton gas expectation: qhat and eta are inversely relatedMajumder, Muller and Wang, PRL99, 192301

    NB: effects not significant (yet); can we narrow down the uncertainties?

    Transport coefficient from RAA

  • More systematics: compare soft scattering formalism

    8

    Armesto et al, arXiv:1606.04837

    q̂ = 2K ✏3/4

    pQCD expectation:K = 1 (by definition)

    ↵S =1

    3

    Similar fit to the data, as the JET paper, but using multiple-soft equations

    Large difference (factor ~2)between scale factor at RHIC and LHC

    Energy loss: BDMPS-ASW multiple soft scatteringMedium: Hydrodynamics; Hirano, Luzum&Romatschke

    Conclusion seems different from JET collaboration workShould follow up to find out what drives this

    Points to modeling uncertainties? Can we reduce those?

  • 5 6 7 8 9 10pT [GeV]

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    20 - 30 %, ASW

    (a)

    High-pT v2, RAA in and out of plane

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    Xu et al, CU

    JET, arXiv:1402.2956

    T. Renk, arXiv:1010.1635

    Sensitive to medium evolution models
(freeze-out temp)

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    CMS Pb+Pb 2.76ATeV h± 20-30%CUJET2.0 π (0.23,1,0) ∆φ=0° & (0.26,1,0) ∆φ=90°

    CUJET2.0 π (0.20,1,0) b=7.5fm @LHC(0.21,1,0)(0.22,1,0)(0.23,1,0)(0.24,1,0)(0.25,1,0)(0.26,1,0)(0.27,1,0)(0.28,1,0)(0.29,1,0)(0.30,1,0)(0.31,1,0)(0.32,1,0)(0.33,1,0)(0.34,1,0)(0.35,1,0)

    Current state: Hydro+E-loss models do not produce enough v2

    Potential with more precise data, and some effort:Use high-pT data to co-validate/constrain medium evolution (models)

    CUJETYaJEM

    RHICLHC

    Qin and Majumder, arXiv:0910.3016

    Various points under discussion:- Effect of fluctuations

    - HT gets higher v2?Noronha-Hostler et al, arXiv:1602.03788

  • Another handle on path length dependence: di-hadrons

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    8 < pT,trig < 15 GeV

    Near side trigger, 
biases to small E-loss

    Away-side large L

    STA

    R P

    RL 95, 152301

    Away-side (recoil) suppression IAA 
samples longer path-lengths than inclusive RAA

    Can be modelled with the same tools as inclusive particle production

  • IAA modeling

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    Armesto et al,  J.Phys. G

    37, 025104

    RAA and IAA fit with similar density

    Confirms ~L2 dependence Calculations with elastic loss give too little suppressionH

    Zhang et al, PRL 98, 212301 

    →π

    ± ±

    ±

    ε0

    →π

    ± ±

    ±

    χ2

    Medium model: Glauber profileEnergy loss: Higher Twist

    Medium model: (ideal) HydroEnergy loss: BDMPS-ASW multiple soft

    T. Renk, PRC, arXiv:1106.1740

  • IAA modeling

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    Armesto et al,  J.Phys. G

    37, 025104

    RAA and IAA fit with similar density

    Confirms ~L2 dependence Calculations with elastic loss give too little suppressionH

    Zhang et al, PRL 98, 212301 

    →π

    ± ±

    ±

    ε0

    →π

    ± ±

    ±

    χ2

    Medium model: Glauber profileEnergy loss: Higher Twist

    Medium model: (ideal) HydroEnergy loss: BDMPS-ASW multiple soft

    T. Renk, PRC, arXiv:1106.1740

    So far, model calculations only exist for RHIC:
- Would like to see LHC calculations to put modeling to the test- Experimentally: extend pT range

  • IAA at the LHC

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    Transition enhancement → suppression @ pT ~ 2 GeV

    CMS-PA

    S-HIN-12-010

    19.2 - 24.0 GeVpTtrig (GeV):

    14.0 - 28.8 GeV 28.8-35.2 GeV 35.2-48.0 GeV

    peripheral 50-60%

    central 0-10%

    )c (GeV/T

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    c < 16 GeV/trigT

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    bkg)n

    -hadron (v0π

    AMPT model

    JEWEL model

    NLO pQCD model

    ALICE, PLB 763, 238
PRL 108, 092301

    Data already exist — 
it’s really ‘just’ a matter 
of running the models/calculations !

  • Heavy flavour RAA; mass dependence

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    |

  • Relating heavy and light flavor modeling: Ds and

    14

    qhat(T=400 MeV) = 3 GeV2/fm

    However, perturbative estimate Ds = 30/2 𝜋 T —> qhat ~ 0.6 GeV2/fm

    E.g.: Why is the perturbative estimate of Ds so large?LO: Svetitsky, PRD 37, 2484

    2⇡ TDs = 8⇡CFCA

    T 3

    q̂(approximate relation; 
Ds and qhat are different regimes)

    Trying out some numbers:

    Cao, Qin, Bass, PRC 88, 044907

    Ds = 6/2 𝜋 T

    Should connect heavy and light flavor phenomenology

  • Relating heavy and light flavor modeling: Ds and

    14

    qhat(T=400 MeV) = 3 GeV2/fm

    However, perturbative estimate Ds = 30/2 𝜋 T —> qhat ~ 0.6 GeV2/fm

    E.g.: Why is the perturbative estimate of Ds so large?LO: Svetitsky, PRD 37, 2484

    2⇡ TDs = 8⇡CFCA

    T 3

    q̂(approximate relation; 
Ds and qhat are different regimes)

    Trying out some numbers:

    Cao, Qin, Bass, PRC 88, 044907

    Ds = 6/2 𝜋 T

    Should connect heavy and light flavor phenomenology

  • Jets: multi-parton states

  • High-pT jets vs hadrons

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    AAR

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    = 5.02 TeV, this analysisNNsATLAS,

    = 2.76 TeV, arXiv: 1411.2357NNsATLAS,

    PreliminaryATLAS = 0.4 jetsR tkanti-

    0 - 10 %| < 2.1y|

    -12015 Pb+Pb data, 0.49 nb-1 data, 25 pbpp2015

    Jets: RAA < 1 out to high pT

    Single particles: consistent with expected constant (log E) dependence

    CMS, JHEP 04, 039

    ATLAS-CONF-2017-009

    Charged particle RAA Jet RAA

    pT-dependence driven by energy dependence of E-loss Different for single particles and jets! ?

    Jets suggest increase of ΔE vs E

    Tentative interpretation: in jets, multiple partons lose energy; more partons in high-E jets —> more E-loss

  • High-pT jets vs hadrons

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    = 5.02 TeV, this analysisNNsATLAS,

    = 2.76 TeV, arXiv: 1411.2357NNsATLAS,

    PreliminaryATLAS = 0.4 jetsR tkanti-

    0 - 10 %| < 2.1y|

    -12015 Pb+Pb data, 0.49 nb-1 data, 25 pbpp2015

    Jets: RAA < 1 out to high pT

    Single particles: consistent with expected constant (log E) dependence

    CMS, JHEP 04, 039

    ATLAS-CONF-2017-009

    Charged particle RAA Jet RAA

    pT-dependence driven by energy dependence of E-loss Different for single particles and jets! ?

    Jets suggest increase of ΔE vs E

    Tentative interpretation: in jets, multiple partons lose energy; more partons in high-E jets —> more E-loss

    First glimpse of jets as scale-dependent probes !Opens up a field of study: pT-dependence of jet modifications

  • First look at the models

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    Zapp, Krauss, Wiedemann, 
 arXiv:1212.1599

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    ALICE data, 0-5% centrality

    JEWEL+PYTHIA

    Eyalavalli and Zapp, JHEP 1707, 141

    w/ Recoils, 4MomSubw/ Recoils, GridSub1w/ Recoils, GridSub2w/o Recoilsanti-k⊥ R=0.4 jetsp

    jet⊥ > 100 GeV

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    JEWEL seems to capture the trends quite wellSome quantitative questions to be worked out; 
e.g. increase of hadron RAA too slow at 5 TeV? Hybrid model: similar conclusion at first sight:

    increase of jet RAA less steep than hadron RAAAlso consistent with energy shift + small corrections?

    Take home message: need large pT range to draw strong conclusionssmall range: flat vs increase hard to disentangle; limited precision of models and data

    D Pablos, this meeting

  • Where does the lost energy go ?

    18

    Results clearly show that lost energy 
goes to large angle and soft particles

    Should try to go beyond this qualitative statement

    • Is the transport to large-angle consistent with 
expectations from pQCD?

    • Does it require ‘thermalisation’?• Can we learn more about coherence effects?

    Several studies exist: JEWEL, Hybrid model, CCNUgive partial answers…

    ∆0.5 1 1.5

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    InclusiveJA

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    R = 0.3tanti-k

    ∆〉

    ||

    Tp〈PbPb

    ∆0,〉||

    Tp〈PbPb

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    ||

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    2η|,|

    1η|

    PbPb 0-30%

    ∆0.5 1 1.5

    -5

    0

    5 (PbPb 0-30%) - pp

    CMS, JHEP 01 (2016) 006Requires careful modeling of soft physics — not easy

    and exploration of model uncertainties

  • Fragmentation functions/hadron distributions

    19

    CMS-PAS-FTR-17-002Mehtar-Tani and Tywoniuk, Phys. Lett. B744(2015) 284

    jetξ

    0.5 1 1.5 2 2.5 3 3.5 4 4.5

    jet

    ξdtrk

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    5PbPb Cent. 0-10 %Current Unc.Projected Unc.

    pp (smeared)Current Unc.Projected Unc.

    > 1 GeV/ctrkT

    p

    jet R = 0.3Tanti-k

    > 30 GeV/cjetT

    p

    | < 1.6jetη|

    > 60 GeV/cγT

    p

    | < 1.44γη|

    8π7 >

    γjφ∆

    = 5.02 TeVNNs-1, pp 650 pb-1PbPb 10 nb

    CMSProjection

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    /

    dℓ

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    Ratio

    CohCoh + Decoh

    VacuumCMS Prelim.: medium, 0-10%

    CMS Prelim.: vacuum

    CohCoh + Decoh

    CMS Preliminary, 0-10%

    High-z: hadron vs jet RAA; scale dependence of energy lossLow-z: mechanism of thermalisation in the medium vs soft fragmentation

    Effects tend to be small: Experimentally: need good precision and study pT dependenceModels: need to consider systematic uncertainties on models/missing physics

  • Jet acoplanarity

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    Gaussian width: sensitive to momentum broadening

    Potential for direct sensitivity
to scattering centers in the medium

    0 5 10 15 20 250.00

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    1 �d� dq

    ?

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    HJ [9, 30]+[12, 18]

    HJ [9, 30]+[18, 48]

    HH [5, 10]+[3, 5]

    HH [5, 10]+[5, 10]

    HH [12, 20]+[3, 5]

    LHC

    HJ [9, 30]+[18, 48]

    HJ [20, 50]+[60, 90]

    HH [5, 10]+[5, 10]

    Chen, Qin, et al, arXiv:1607.01932

    2.4 2.6 2.8 3.00.0

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    passoT,J = [18, 48] GeV

    ��

    1 �d� d��

    STAR 60-80%

    STAR 0-10%

    hp2?i = 0 GeV2

    hp2?i = 13 GeV2

    K Rajagopal, this workshop

    Relation momentum broadening - energy loss
depends on nature of medium

    hq2?i = q̂L q̂ = KT 3

    Tails:‘Rutherford scattering’

    K = 2-5 in QCDlarger in strong coupling

  • Competing effects for acoplanarity: Sudakov broadening and E loss

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    1 �d� dq

    ?

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    HJ [9, 30]+[12, 18]

    HJ [9, 30]+[18, 48]

    HH [5, 10]+[3, 5]

    HH [5, 10]+[5, 10]

    HH [12, 20]+[3, 5]

    LHC

    HJ [9, 30]+[18, 48]

    HJ [20, 50]+[60, 90]

    HH [5, 10]+[5, 10]

    Chen, Qin, et al, arXiv:1607.01932Hybrid model, Solana et al, arXiv:1609.05842

    0

    0.5

    1

    1.5

    2

    2.5

    3

    0 0.5 1 1.5 2 2.5 3

    0� 10%

    PLt > 35 GeV, PSt > 10 GeV, |⌘| < 2

    EventFraction

    ��

    K=0

    K=20

    K=40

    K=100

    Vacuum

    Energy loss causes narrowing (shift from high to low pT)

    0

    1

    2

    3

    4

    5

    6

    7

    8

    0 0.5 1 1.5 2 2.5 3

    0� 10%

    PLt > 35 GeV, PSt > 10 GeV, |⌘| < 0.5

    EventFraction

    ��

    K=0

    K=5

    K=20

    K=50

    Vacuum

    RHIC

    LHC

    Natural width of h-jet, jet-jet distributions

    hq2?i = (2� 5 GeV)2

  • Putting things together: dialing the biasesLeveraging the differences in geometric and energy loss bias in observables

    Conceptually powerful, but needs simultaneous modeling of 
geometry, energy loss, and experimental selection

  • 23

    T. Renk, arXiv:1212.0646RHIC

    LHC

    h-h jet-h jet-jet (AJ)

    Surface bias differs between probes: largest for hadrons
and energy/collider: stronger at RHIC

    Main ingredients: surface bias vs fluctuations

  • Using biases: examples/ideas

    • Disentangle geometric effects and fluctuations• Inclusive vs recoil• gamma-jet (or EW boson-jet) vs di-jets

    • Select quark/heavy quark jets• Dial the biases to tease out the small acoplanarity signals?• Select jets that experience a large energy loss to increase ‘signal’

    • ‘Natural’ fluctuations from geometry and the intrinsic process are very large; ‘average’ not always useful• Explicitly study energy loss dependence on e.g. opening angle? 


    Needs development/study: ideally have two classes of variables:• Variable(s) that preserve properties of the ‘vacuum jet’, i.e. not (much) affected by energy loss• Variable(s) that are explicitly sensitve to energy loss

    24

  • Using biases: examples/ideas

    • Disentangle geometric effects and fluctuations• Inclusive vs recoil• gamma-jet (or EW boson-jet) vs di-jets

    • Select quark/heavy quark jets• Dial the biases to tease out the small acoplanarity signals?• Select jets that experience a large energy loss to increase ‘signal’

    • ‘Natural’ fluctuations from geometry and the intrinsic process are very large; ‘average’ not always useful• Explicitly study energy loss dependence on e.g. opening angle? 


    Needs development/study: ideally have two classes of variables:• Variable(s) that preserve properties of the ‘vacuum jet’, i.e. not (much) affected by energy loss• Variable(s) that are explicitly sensitve to energy loss

    24

    This is where jet shape variables have great potential!Many options under study; unfortunately no time to review…

  • Example: AJ at RHIC

    25

    JA0.2− 0 0.2 0.4 0.6 0.8

    Fraction

    0

    0.05

    0.1

    0.15

    0.2

    0.25

    >2 GeV/c:CutT

    With p>20 GeV/c

    T,lead p

    >10 GeV/cT,sublead

    p

    Au+Au, 0-20%, R=0.4TAnti-k

    >2 GeV/c:CutT

    p Au+Au MB⊕p+p HT

    Au+Au HT

    >0.2 GeV/c, Matched:CutT

    p Au+Au MB⊕p+p HT

    Au+Au HT

    STAR, arXiv:1609.03878

    Observation: di-jet imbalance small at RHICwhen selecting ‘hard-core jets’

    Is this driven by the hard core selection?—> Hard core selects jet (pairs) that lose little energyCan be tested at LHC

    What about other biases/effects:- Steeper spectrum at RHIC- Smaller overall energy loss at RHIC vs LHC?- Quark vs gluon jets?

    Promising avenue, needs follow-up to extract the physics

  • Example II: compare 𝛾-jet and jet-jet

    26

    z

    2−10 1−10 1

    ratio

    of D

    (z)

    0.6

    0.8

    1

    1.2

    1.4

    1.6

    PreliminaryATLASpp0-30% Pb+Pb /

    -tagged jets 5.02 TeVγ

    inclusive jets 2.76 TeV(0-10%)

    ATLAS-CONF-2017-074

    Comparing 𝛾-jet and jet-jet changes:- Energy loss bias


    reco jet energy is ‘after energy loss’ - Flavour content


    quark vs gluon jets

    Leads to difference in frag function modification

    Leverage this with models + increasing data precisionto extract the physics

  • Example III: h-jet at RHIC and LHC

    27

    LHC: recoil jet suppressionΔIAA ~ 0.5 with R=0.2

    STAR, PRC96, 024905

    )c(GeV/chT,jet

    p0 10 20 30 40 50 60 70 80 90 100

    PY

    TH

    IAre

    coil

    ∆/P

    bP

    bre

    coil

    ∆=

    AA

    I∆

    0

    0.2

    0.4

    0.6

    0.8

    1

    1.2

    1.4

    1.6

    1.8

    ALICE data

    Shape uncertainty

    Correlated uncertainty

    = 2.76 TeVNNs0-10% Pb-Pb

    Ha

    dro

    n T

    rig

    ge

    r T

    hre

    sho

    ld

    = 0.2R charged jets, TkAnti- < 0.6ϕ∆ − π

    TT{8,9}− TT{20,50}

    ALICE

    RHIC: recoil jet suppressionΔIAA ~ 0.3 with R=0.2

    Suppression numerically quite different at RHIC and LHC. What drives this? Kinematic selection, different surface bias, …

    ALICE, JHEP 09 (2015) 170

  • Future experiments: HL-LHC

    28

    https://indico.cern.ch/event/647676/timetable/J.Jow

    ett, HL-H

    C w

    orkshop

    1 nb-1 PbPb ~ 43 NN-equiv pb-1

    HL-LHC: expect factor ~3 increase of lumi; 2.8 nb-1/year

    Current target lumi : 10 nb-1 in run 3 + 4 (2021-2029)(ALICE request)

    Increase in statistics compared to run 1, 2:- 5x for triggers in ATLAS+CMS- 10x for triggers in ALICE- 100x for MB-like in ALICE

    0.7 nb-1

    LHC HI lumi over the years

    https://indico.cern.ch/event/647676/timetable/http://www.apple.com

  • Future experiments: HL-LHC

    28

    https://indico.cern.ch/event/647676/timetable/J.Jow

    ett, HL-H

    C w

    orkshop

    1 nb-1 PbPb ~ 43 NN-equiv pb-1

    HL-LHC: expect factor ~3 increase of lumi; 2.8 nb-1/year

    Current target lumi : 10 nb-1 in run 3 + 4 (2021-2029)(ALICE request)

    Increase in statistics compared to run 1, 2:- 5x for triggers in ATLAS+CMS- 10x for triggers in ALICE- 100x for MB-like in ALICE

    0.7 nb-1

    LHC HI lumi over the years

    The HI program for run 3, 4 and beyond is 
being discussed in a series of workshops→ European Strategy for Particle Physics

    https://indico.cern.ch/event/647676/timetable/http://www.apple.com

  • Future experiments: sPHENIX at RHIC

    29

    Slide from: G Roland, 
CERN HI jet workshop 2017

    Planned start: 
2022 ~ LHC run 3

  • Instead of a summary…

    30

    sPHEN

    IX, G. Roland

    Main directions

    • Increased precision and pT reach 
Non-trivial improvement of physics potential!

    • More differential studies
Leveraging the biases

    • Better overlap between RHIC and LHC

    Theory/modeling:• Need coherent/simultaneous description 
of multiple observables to constrain the physics

    • Need competing/alternative models/mechanisms to compare and contrast
Also within a single group/code!

    Experiment:

  • Thanks for your attention!

  • More distant future: FCC and HE-LHC

    32

    √s = 27 TeV pp, √sNN = 10.6 TeV Pb-PbEarliest possible realisation 2040

    FCCFuture Circular Collider very large project; requires new tunnel ~ 100 km

    √s = 100 TeV for pp, √sNN = 39.4 TeV for Pb-Pb

    More info: see HL-LHC workshops and FCC weeks, e.g.: http://fcw2018.web.cern.ch

    HE-LHCHigh-Energy LHC

    http://fcw2018.web.cern.ch

  • Simple observables; how to model them?

    • A lot of experience exists with simple modeling:• Production, energy loss, and fragmentation• Plus full hydro background or a good approximation in most cases

    • Main advantage: keeps the model tractable (clear what is put in)• Disadvantage: no natural extension to jet observable

    • Simple modeling may be good enough for single particle observables• Except, maybe via jet functions, but long and tedious road

    • Also not always obvious how to implement path-length dependence in a non-uniform medium

    33

    Note: should not forget model uncertainties/freedoms- Important part of the story; may point to new questions/directions!- Several aspects have been explored; many connections still missing

  • Summary of transport coefficient study

    34

    0

    1

    2

    3

    4

    5

    6

    7

    0 0.1 0.2 0.3 0.4 0.5

    McGill-AMY

    HT-M

    HT-BW GLV-CUJET

    MARTINI

    Au+Au at RHIC

    Pb+Pb at LHCqN/T

    3 (DIS)eff

    ˆ

    T (GeV)

    q/T

    RHIC:

    LHC:

    Burke et al, JET Collaboration, arXiv:1312.5003

    (Ti = 370 MeV)

    (Ti = 470 MeV)

    values from different models consistent

  • Summary of transport coefficient study

    34

    0

    1

    2

    3

    4

    5

    6

    7

    0 0.1 0.2 0.3 0.4 0.5

    McGill-AMY

    HT-M

    HT-BW GLV-CUJET

    MARTINI

    Au+Au at RHIC

    Pb+Pb at LHCqN/T

    3 (DIS)eff

    ˆ

    T (GeV)

    q/T

    RHIC:

    LHC:

    Burke et al, JET Collaboration, arXiv:1312.5003

    (Ti = 370 MeV)

    (Ti = 470 MeV)

    Arnold and Xiao, arXiv:0810.1026

    HTL expectation:Sizeable uncertainties from 𝛼S, treatment of logs etc expected

    values from different models consistent

  • Summary of transport coefficient study

    34

    0

    1

    2

    3

    4

    5

    6

    7

    0 0.1 0.2 0.3 0.4 0.5

    McGill-AMY

    HT-M

    HT-BW GLV-CUJET

    MARTINI

    Au+Au at RHIC

    Pb+Pb at LHCqN/T

    3 (DIS)eff

    ˆ

    T (GeV)

    q/T

    RHIC:

    LHC:

    Burke et al, JET Collaboration, arXiv:1312.5003

    (Ti = 370 MeV)

    (Ti = 470 MeV)

    Arnold and Xiao, arXiv:0810.1026

    HTL expectation:Sizeable uncertainties from 𝛼S, treatment of logs etc expected

    Values found are in the right ballpark compared (p)QCD estimateMagnitude of parton energy loss is understood

    values from different models consistent

  • Transport coefficient and viscosity

    35

    Transport coefficient:momentum transfer per unit path length

    basically measures the density

  • Transport coefficient and viscosity

    35

    Transport coefficient:momentum transfer per unit path length

    basically measures the density

    Viscosity: General relation:

  • Transport coefficient and viscosity

    35

    Transport coefficient:momentum transfer per unit path length

    basically measures the density

    Viscosity: General relation:

    Expect for a QCD medium

    Majumder, Muller and Wang, PRL99, 192301

  • MC tools: JEWEL

    36

    Ti = 530 MeV @ 𝜏0 = 0.5 fm/c

    Zapp, Krauss, Wiedemann, arXiv:1212.1599

    0

    0.2

    0.4

    0.6

    0.8

    1

    1.2

    1.4

    1.6

    1.8

    2

    10 100 1000

    RA

    A

    pt [GeV]

    charged hadrons

    CMS data, 0-5% centrality

    ALICE data, 0-5% centrality

    JEWEL+PYTHIA

    0

    0.2

    0.4

    0.6

    0.8

    1

    4 6 8 10 12 14 16 18 20 22 24 26

    RA

    A

    pt [GeV]

    π0

    PHENIX data, 0-10% centrality

    JEWEL+PYTHIA

    RHIC LHC

    Elastic+radiative energy loss; follows BDMPS-Z in appropriate limits
Medium: Bjorken-expanding Glauber overlap

    Ti = 350 MeV @ 𝜏0 = 0.8 fm/c

    Good agreement with JET collaboration values

    Publicly available

  • T vs t in EPOS/MC@HQ

    37

    EPOS2, b=0PbPb

    s =2.76 TeV

    1.0 10.05.02.0 20.03.01.5 15.07.0

    1.00

    0.50

    0.20

    0.30

    0.15

    0.70

    tHfmêcL

    THGeVL

    JET collabTinit = 470 MeV

    P Gossiaux, private comm

    Medium parameters in MC@HQ agree well with light flavour fits

    Q: how does the relation compare?

    Werner, et al, arXiv:1203.5704

    x [fm]-8 -6 -4 -2 0 2 4 6 8

    y [fm

    ]

    -8

    -6

    -4

    -2

    0

    2

    4

    6

    8

    0

    50

    100

    150

    200 = 0.35 fm/c) τ= 0.0 , sη] (

    3energy density [GeV/fm

    �E(T )

  • Model(ing) uncertainties for high-pT v2

    • Initial time/treatment• Freeze-out temperature/treatment• Length sampling in a non-uniform medium• Event-by-event fluctuations

    38

    When reporting a model/calculation; make sure to specify these things

  • Noronha-Hostler et al: fluctuations

    39

    Observation: high-pT v2 is 
measured wrt to low pT v2

    Noronha-Hostler et al, arXiv:1602.03788

    Fluctuations bias v2

    Basically, measure ⌦v22↵

    NB: no energy loss fluctuations; not so clear how geometry was implemented (L)

  • v2 in CUJET

    40

    aS runs, with cut-off at low Q

    Cut-off is the main model parameter

    0

    0.04

    0.08

    0.12

    0.16

    10 20 30 40 50

    v 2(p

    T)

    pT (GeV/c)

    ALICE Pb+Pb 2.76ATeV h± 20-30%ATLAS Pb+Pb 2.76ATeV h± 20-30%

    CMS Pb+Pb 2.76ATeV h± 20-30%CUJET2.0 π (0.23,1,0) ∆φ=0° & (0.26,1,0) ∆φ=90°

    CUJET2.0 π (0.20,1,0) b=7.5fm @LHC(0.21,1,0)(0.22,1,0)(0.23,1,0)(0.24,1,0)(0.25,1,0)(0.26,1,0)(0.27,1,0)(0.28,1,0)(0.29,1,0)(0.30,1,0)(0.31,1,0)(0.32,1,0)(0.33,1,0)(0.34,1,0)(0.35,1,0)

    CUJETXu et al, C

    UJET, arXiv:1402.2956

    Black dashed line: depends onAdds v2 ‘by hand’

    GLV-based E-loss

    Standard settings underpredict v2

    However, see also: CUJET3.0Xu et al, arXiv:1509.00552

    ↵max

    ��

  • v2 in Higher Twist

    41

    Qin and Majumder, arXiv:0910.3016

  • Relating qhat to medium density, or T

    42

    [GeV]partonE0 5 10 15 20 25 30 35 40 45 50

    /fm]

    2 [G

    eVq

    1

    10

    210

    Quark-Gluon Gas2µ> = 2 = 2

  • Comparison to LBT

    43

    Cao, et al, arXiv:1703.000822

    Factor ~1.5 between LBT fits and JET values; probably within uncertainties

    Heavy+light energy loss

  • Di-hadrons and single hadrons at LHC

    44

    Need simultaneous comparison to 
several measurements 
to constrain geometry and E-loss

    Here: RAA and IAA

    Three models: ASW: radiative energy loss YaJEM: medium-induced virtuality YaJEM-D: YaJEM with L-dependent 
 virtuality cut-off (induces L2)

  • Di-hadron modeling

    45

    T. Renk, PRC, arXiv:1106.1740

    L2 (ASW) fits data L3 (AdS) slightly below

    Modified shower 
generates increase at low zT

    L (YaJEM): too little suppression L2 (YaJEM-D) slightly above

    Model ‘calibrated’ on single hadron RAA

    Clear sensitivity to L dependence

  • Di-hadron with high-pT trigger

    46

    pttrig > 20 GeV at LHC: strong signals even at low pTassoc 1-3 GeVCMS-PAS-HIN-12-010

    19.2 - 24.0 GeVpTtrig (GeV): 14.0 - 28.8 GeV 28.8-35.2 GeV 35.2-48.0 GeV

    CMS-PAS-H

    IN-12-010

  • CMS di-hadrons: near side

    47

    19.2 - 24.0 GeVpTtrig (GeV):

    14.0 - 28.8 GeV 28.8-35.2 GeV 35.2-48.0 GeV

    Transition enhancement → suppression @ pT ~ 3 GeV

    also compatible with IAA=1 at pT > 3 GeV?

    peripheral 50-60%

    central 0-10%

    CMS-PA

    S-HIN-12-010

  • Some open and partially-answered questions

    48

    Energy loss mechanismphysics of hard partons in a plasma

    Nature of the mediumdensity, character of constituents

    Flavor dependence of energy loss

    Role of interference effects
Do all partons in a jet lose energy?

    Angular broadeninglarge-angle scattering

    Thermalisation of the lost energy

    Path length dependence of energy loss—> tomography of the medium

    Scale dependence 
of energy loss?