Holography and the problem of parton energy loss in a quark-gluon - - PowerPoint PPT Presentation

holography and the problem of parton energy loss in a
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Holography and the problem of parton energy loss in a quark-gluon - - PowerPoint PPT Presentation

Holography and the problem of parton energy loss in a quark-gluon plasma Daniel Pablos SEWM 18 Barcelona 25th May 2018 Absence of quasiparticles? Most satisfactory description of QGP involves an almost ideal liquid phase pp pPb PbPb


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SLIDE 1

Holography and the problem

  • f parton energy loss in a

quark-gluon plasma

Daniel Pablos

SEWM ‘18 Barcelona 25th May 2018

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SLIDE 2

Absence of quasiparticles?

studies of QGP formation in small systems suggest common hydrodynamic origin for flow effects!

pp pPb PbPb

Most satisfactory description of QGP involves an almost ideal liquid phase

Weller & Romatschke - PLB ‘17

2

Daniel Pablos McGill / JETSCAPE

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SLIDE 3

Absence of quasiparticles?

Small value of shear viscosity over entropy density ratio

η s ∼ 0.08

η s = 1 4π

τqp ∼ 5η s 1 T ∼ 1 T

challenges quasiparticle description Predicted by Policastro, Son and Starinets (2001) for a large class of non-abelian gauge theories at strong coupling which have a gravity dual

pp pPb PbPb

Bernhard et al. - PRC ‘16 York & Moore - PRD ‘08

3

Daniel Pablos McGill / JETSCAPE

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SLIDE 4

Absence of quasiparticles?

pp pPb PbPb

Chesler - PRL ‘15, JHEP ‘16

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Daniel Pablos McGill / JETSCAPE

Hydrodynamics at work with large gradients at very early times Natural situation at strong coupling

R ∼ 1 T

Even for system sizes of order hydrodynamic expansion is well behaved Appealing picture of hydrodynamization for all system sizes within strong coupling

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SLIDE 5

Absence of quasiparticles?

would like to have description of jet/QGP interaction in harmony with sQGP hypothesis traditional pQCD computations need to assume separation of scales

λD ⌧ λm.f.p.

g ⌧ 1

for ex: neglect correlations among scatterers

q ∼ √ ET

But the typical virtuality exchanged between the jet and the medium

E T

β1 loop(q)

g ∼ 2

q

There is motivation to explore an alternative, non-perturbative, description of jet quenching that does not assume the presence of quasiparticles

5

Daniel Pablos McGill / JETSCAPE

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SLIDE 6

Holography: a non-perturbative tool

quarks are dual to open strings attached to probe flavour branes having a plasma in the gauge theory represents a black hole in the bulk

J Friess, et al., PRD75 (2007)

and QCD have very different vacuums but share similarities bulk metric perturbations encode boundary stress energy variations

N = 4 SYM

T 6= 0

T > Tc

N = 4

and QCD

! ?

6

Daniel Pablos McGill / JETSCAPE

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SLIDE 7

Proxies for jets as falling strings

presence of string perturbs metric satisfies linearised Einstein’s equations near boundary expression

  • f energy-momentum tensor

string sourced hydro (long wavelength) non-hydro (jet modes)

dressed quarks are open strings attached to a D7 flavour brane charged under U(1) gauge field sourcing baryon current at boundary depth of string endpoint determines localisation of excitation at boundary

7

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Chesler et al. - PRD ‘09 Chesler & Rajagopal, JHEP ‘16 horizon boundary

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SLIDE 8

Null falling string approximation

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Daniel Pablos McGill / JETSCAPE

Nambu-Goto action

null geodesics endpoint angle string profile

σ∗

Chesler & Rajagopal - PRD ‘15, JHEP ‘16

Schwarzschild-AdS Solve E.O.M. by finding null geodesic profile: xgeo(t), ugeo(t) Find energy carried by each geodesic: (peaks at the endpoint)

Πτ

0(σ)

Construct the string energy-momentum tensor:

1. 2. 3.

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SLIDE 9

Null falling strings

with rate:

as the jet loses energy … it also gets wider Fractional energy loss

  • nly depends on

initial jet opening angle

most energy at endpoint: Bragg-like peak

9

Daniel Pablos McGill / JETSCAPE

Chesler & Rajagopal - PRD ‘15, JHEP ‘16

Unambiguous determination of boundary jet properties: Pieces of string falling below horizon energy-momentum into hydro modes xtherm = 1 2κ E1/3

in

T 4/3

Also, quite interestingly:

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SLIDE 10

Hybrid strong/weak coupling approach

High energy jet starts with a high virtuality, much greater than medium scale Parton shower well approximated by vacuum-like splittings (late stages?) Use non-perturbative holographic prescription for partonic energy loss Energy flowing into hydro modes: Estimate the hadronic spectra coming from medium response (assume small perturbation, instantaneous hydrodynamization) Lost jet energy converted into soft particles at large angles (corr. bkgd.)

Pablos et al. - JHEP ‘14, ‘16, ‘17

O(1)

Plasma-jet interaction dominated by temperature scale

free parameter

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SLIDE 11

Jet induced medium excitations

string acts as a perturbation in the large Nc limit agreement between hydrodynamics & wake of a quark in gauge/gravity duality energy-momentum conservation in the jet+plasma interplay wake hadron distribution estimate

small perturbation on top of hydro

  • nly valid for soft hadrons

no extra free parameter (within hybrid model)

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Chesler & Yaffe - PRD ‘08

}

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SLIDE 12

Phenomenology at LHC

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Constraining the free parameter

ATLAS-CONF-2017-009 JHEP 1704 (2017) 039

Use hadron and jet suppression data for central collisions at LHC to fit the free parameter

Hadron suppression Jet suppression

# inelastic collisions per heavy ion collision estimated through the Glauber model Perform a global fit and extract the best value of κSC

13

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SLIDE 14

Fit results

0.3 0.4 0.5 0.6 0.7 0.8 CMS Had 5.02 ATLAS Had 5.02 CMS Had 2.76 ATLAS Had 2.76 RHIC Had 0.20 CMS Jets R=0.2 2.76 CMS Jets R=0.3 2.76 CMS Jets R=0.4 2.76 ATLAS Jets R=0.4 5.02 ATLAS Jets R=0.4 2.76 κ 2 σ 1 σ Global Fit Hadrons 0-5% Jets 0-10%

*

* with LHC data only

In preparation

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Consistent, but some tension between hadrons & jets preferred value

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SLIDE 15

Fit results

0.3 0.4 0.5 0.6 0.7 0.8 CMS Had 5.02 ATLAS Had 5.02 CMS Had 2.76 ATLAS Had 2.76 RHIC Had 0.20 CMS Jets R=0.2 2.76 CMS Jets R=0.3 2.76 CMS Jets R=0.4 2.76 ATLAS Jets R=0.4 5.02 ATLAS Jets R=0.4 2.76 κ 2 σ 1 σ Global Fit Hadrons 0-5% Jets 0-10%

*

* with LHC data only

In preparation

15

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Consistent, but some tension between hadrons & jets preferred value

Finite resolution effects (a.k.a. coherence in pQCD) affect hadron & jet relative suppression (see back-up)

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SLIDE 16

Hadron and Jet suppression

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0.2 0.4 0.6 0.8 1 1.2 1.4 10 100 1000 RAA Hadron or Jet pT [GeV] Hadrons Jets R = 0.4

Which is the observable that relates hadrons and jets?

In preparation

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SLIDE 17

Connection between hadrons and jets

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0.2 0.4 0.6 0.8 1 1.2 1.4 10 100 1000 RAA Hadron or Jet pT [GeV] Hadrons Jets R = 0.4

In preparation

jet fragmentation functions (FFs)

High z enhancement

ATLAS-CONF-2017-005

Count the average number of hadrons, per jet, with energy fraction z ATLAS

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SLIDE 18

Connection between hadrons and jets

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0.6 0.8 1 1.2 1.4 1.6 1.8 0.5 1 1.5 2 2.5 3 3.5 4 Jet FFs ratio ln(1/z) Actual jet FFs

PbPb jet FFs

0.2 0.4 0.6 0.8 1 1.2 1.4 10 100 1000 RAA Hadron or Jet pT [GeV] Hadrons Jets R = 0.4 Jets ⊗ FF actual

High z enhancement

In preparation

Count the average number of hadrons, per jet, with energy fraction z HYBRID MODEL

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SLIDE 19

Connection between hadrons and jets

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Vacuum jet FFs

0.2 0.4 0.6 0.8 1 1.2 1.4 10 100 1000 RAA Hadron or Jet pT [GeV] Hadrons Jets R = 0.4 Jets ⊗ FF actual Jets ⊗ FF vacuum

0.6 0.8 1 1.2 1.4 1.6 1.8 0.5 1 1.5 2 2.5 3 3.5 4 Jet FFs ratio ln(1/z) Actual jet FFs Vacuum jet FFs

Flat FFs ratio PbPb jet FFs Jet substructure is important for jet quenching phenomenology

In preparation

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SLIDE 20

Jet narrowing

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Daniel Pablos McGill / JETSCAPE

Wider, more active jets lose more energy than narrower, hard fragmenting ones Steeply falling jet spectrum bias inclusive jet sample to narrower ones, explains high z enhancement High pT hadrons belong to such subsample

  • f narrow jets, which get less quenched,

and so

Rjet

AA

Rhad

AA >

R

R

∆Enarrow < ∆Ewide

Effect seen in the literature, for different models,

  • n different observables - see for instance:

Milhano & Zapp - EPJ ‘16 Brewer et al. - JHEP ‘18 Pablos et al. - JHEP ‘17

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0.2 0.4 0.6 0.8 1 1.2 10 100 RAA Jet pT [GeV] R=0.1 R=0.2 R=0.3 R=0.4 R=0.5 R=0.6 R=0.7 R=0.8

Wider jets lose more energy decreases with increasing jet radius

Rjet

AA

WITHOUT MEDIUM RESPONSE

Pablos et al. - JHEP ‘16

RAA vs R

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SLIDE 22

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RAA vs R

Opening the jet radius allows the recovery of some of the lost energy WITH MEDIUM RESPONSE

0.2 0.4 0.6 0.8 1 1.2 10 100 RAA Jet pT [GeV] R=0.1 R=0.2 R=0.3 R=0.4 R=0.5 R=0.6 R=0.7 R=0.8

Hint of ordering reversal around R ∼ 0.7 Characteristic behaviour of strong coupling: efficient energy transfer into hydro modes Upcoming precise data from CMS Stay tuned!

Pablos et al. - JHEP ‘16

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23

0.05 0.1 0.15 0.2 0.25 5 10 15 20 25 0 − 10% R = 0.4 60 < PT, ch jet < 80 GeV Event Fraction Mch jet (GeV) Back No Back pp reference (PYTHIA) ALICE Data R=0.4 0.05 0.1 0.15 0.2 0.25 5 10 15 20 25 0 − 10% R = 0.4 80 < PT, ch jet < 100 GeV Event Fraction Mch jet (GeV) Back No Back pp reference (PYTHIA) ALICE Data R=0.4 0.05 0.1 0.15 0.2 0.25 5 10 15 20 25 0 − 10% R = 0.4 100 < PT, ch jet < 120 GeV Event Fraction Mch jet (GeV) Back No Back pp reference (PYTHIA) ALICE Data R=0.4

quenching back-reaction

cancellation between two effects

Charged jet mass

M = q E2 − p2

T − p2 z

jet narrowing reduces jet mass soft particles at edges rapidly increase mass

In preparation

Daniel Pablos McGill / JETSCAPE

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SLIDE 24

24

New generation observables

Grooming techniques:

Measured anti-kT jet Soft Drop condition: Analytically well understood observable: strongly relates to QCD splitting function Provides momentum balance between the two groomed subjets

pT 1 pT 2

R12 R0

Remove large angle & soft:

zcut = 0.1

β = 0

Taken from M. Verweij’s slides @ MIT HI workshop ‘16 Larkoski et al. - JHEP ‘14, PRD ‘15

Daniel Pablos McGill / JETSCAPE

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SLIDE 25

25

Recursive Splittings

Count the number of times that the same jet satisfies the Soft Drop condition

0.1 0.2 0.3 0.4 0.5 0.6 1 2 3 4 5 6 7 R = 0.4 80 < P ch

T,jet < 120 GeV

1/Njets dN/dnSD nSD PYTHIA Hybrid Model

No enhancement in the # splittings passing Soft Drop in medium Suppression of wide structures tends to slightly reduce nSD

In preparation

  • H. Andrew’s talk

(ALICE) in QM ‘18

Daniel Pablos McGill / JETSCAPE

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SLIDE 26

26

Momentum balance distribution

Wide structure suppression modifies probability

  • f finding subjet at large angles w.r.t. pp

Data not unfolded:

  • bkgd. embedding effect does not

necessarily cancel in the ratio!

0.5 1 1.5 2 0.1 0.2 0.3 0.4 0.5 0 − 5% R = 0.4, 80 < P ch

T,jet < 120 GeV

1/Njets dN/dzg (PbPb/pp) zg all ∆R ∆R < 0.1 ∆R > 0.2

∆R ≡ R12

angular cuts Shape of the distribution not modified because our model assumes vacuum-like shower

In preparation

Daniel Pablos McGill / JETSCAPE

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SLIDE 27

27

Lund map

1 2 3 4 5 ln(1/∆R) −10 −8 −6 −4 −2 ln(z ∆R) −0.1 −0.08 −0.06 −0.04 −0.02 0.02 0.04 0.06 0.08 0.1

In preparation

Suppression Enhancement

Fill a 2D density map by using both momentum balance (zg) and angular separation (ΔR) PbPb − pp A suppression of large angle splittings and enhancement of collinear splittings is observed - consistent with observation in zg measurement

In qualitative agreement with the Hybrid Model

  • H. Andrew’s talk (ALICE) in QM ‘18

Daniel Pablos McGill / JETSCAPE

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SLIDE 28

28

Conclusions

energy loss at strong coupling is a necessary tool to assess the nature of QGP dynamics degree of hydrodynamization of lost energy can be tested with current observables much progress has been made in developing models that can be compared to data further effort is needed on bringing holographic models to a next level of sophistication

  • rthogonal to pQCD radiative based energy loss paradigm

by taking the core ingredients from pQCD that apply in HIC due to scale separation need a systematic confrontation with data within a common framework

  • full medium response,
  • medium modified hadronization,
  • possibility of (rare?) hard momentum transfers inducing extra splittings

v1.0 has been now released!

https://github.com/JETSCAPE

Modular simulator of all aspects of heavy ion collisions Energy loss modules: MATTER, LBT, MARTINI, AdS/CFT Will soon feature concurrent Jet+Hydro evolution!

Daniel Pablos McGill / JETSCAPE

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SLIDE 29

29

Outlook

Can we constrain QGP transport coefficients by confronting to data the effect of medium response to the presence of the jet? (or, inversely, can we constrain e-loss models based on their consistency with extracted transport coefficients from minimum bias soft physics?) Hydro can describe flow in small systems, but there is absence of jet quenching… Strong coupling e-loss has a strong path length dependence, which means very small quenching in pPb, but… how do we explain high pT v2? Strong coupling prescription determines the rate of energy transfer from hard (and hardish) modes into hydro modes If jet hydrodynamization is related to hydrodynamic behaviour appearance itself… can we use holography insights to develop a model of mini-jet quenching for the bulk?

Daniel Pablos McGill / JETSCAPE

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SLIDE 30

Backup Slides

Daniel Pablos McGill / JETSCAPE

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SLIDE 31

Jet suppression: Photon-Jet events

Core features of the model have been validated by e.g. photon-jet observables predictions No strong evidence so far of hard point-like scatterers Talk by R. Bi on Wed

31

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SLIDE 32

J

A

0.1 0.2 0.3 0.4

[GeV] 〉

|| T

p 〈

  • 40
  • 20

20 40

PbPb - pp R = 0.3, 0-10%

J

A

0.1 0.2 0.3 0.4

  • 40
  • 20

20 40

|| T

p 〈 0.5-1.0 1.0-2.0 2.0-4.0 4.0-8.0 8.0-300.0

PbPb - pp R = 0.3, 10-30%

Where does lost energy go to?

Daniel Pablos McGill / JETSCAPE

40 30 20 10 10 0.1 0.3 0.5 0.7 0.9 1.1 1.3 1.5 1.7 1.9 Quenching Only h/ pk

T i

∆ 40 30 20 10 10 0.1 0.3 0.5 0.7 0.9 1.1 1.3 1.5 1.7 1.9 PbPb R=0.3, 0-30% Quenching + Medium Response h/ pk

T i

∆ 8.0-300.0 4.0-8.0 2.0-4.0 1.0-2.0 0.5-1.0 h/ pk

T i∆

‘missing-pt’ observables

40 20 20 40 0.1 0.2 0.3 0.4 PbPb-pp R=0.3, 0-10% 0.1 0.2 0.3 0.4 PbPb-pp R=0.3, 10-30% h/ pk

T i [GeV]

AJ AJ 8.0-300.0 4.0-8.0 2.0-4.0 1.0-2.0 0.5-1.0 h/ pk

T iΣ

CMS

CMS

leading jet subleading jet

energy is recovered at large angles in the form of soft particles data suggests that implementation of back-reaction might mistreat semi-hard particles

32

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SLIDE 33

J

A

0.1 0.2 0.3 0.4

[GeV] 〉

|| T

p 〈

  • 40
  • 20

20 40

PbPb - pp R = 0.3, 0-10%

J

A

0.1 0.2 0.3 0.4

  • 40
  • 20

20 40

|| T

p 〈 0.5-1.0 1.0-2.0 2.0-4.0 4.0-8.0 8.0-300.0

PbPb - pp R = 0.3, 10-30%

Where does lost energy go to?

Daniel Pablos McGill / JETSCAPE

40 30 20 10 10 0.1 0.3 0.5 0.7 0.9 1.1 1.3 1.5 1.7 1.9 PbPb R=0.3, 0-30% Quenching + Medium Response h/ pk

T i

∆ 8.0-300.0 4.0-8.0 2.0-4.0 1.0-2.0 0.5-1.0 h/ pk

T i∆

‘missing-pt’ observables

40 20 20 40 0.1 0.2 0.3 0.4 PbPb-pp R=0.3, 0-10% 0.1 0.2 0.3 0.4 PbPb-pp R=0.3, 10-30% h/ pk

T i [GeV]

AJ AJ 8.0-300.0 4.0-8.0 2.0-4.0 1.0-2.0 0.5-1.0 h/ pk

T iΣ

CMS

CMS

leading jet subleading jet

energy is recovered at large angles in the form of soft particles data suggests that implementation of back-reaction might mistreat semi-hard particles

CMS

33

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SLIDE 34

An estimate of finite resolution effects

Weak coupling: interplay between antenna angle, formation time and emission wavelength medium interactions can destroy antenna color correlations radiation from the global charge only if system not resolved by QGP Strong coupling: quark-gluon system emulated by string with kink stopping distance modulated by angular separation between endpoint & kink In Hybrid Model: unresolved dipoles lose energy as a single effective excitation two partons are resolved if their separation is greater than resolution length

Casalderrey & Ficnar - arXiv:1512.00371 Hulcher et al. - JHEP ‘18 Mehtar-Tani et al. - PLB ‘12

needs further study!

Casalderrey & Iancu - JHEP ‘11 Casalderrey et al. - PLB ‘13

Lres ∼ λD

Daniel Pablos McGill / JETSCAPE

34

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SLIDE 35

Fit results

Daniel Pablos McGill / JETSCAPE

0.3 0.4 0.5 0.6 0.7 0.8 CMS Had 5.02 ATLAS Had 5.02 CMS Had 2.76 ATLAS Had 2.76 RHIC Had 0.20 CMS Jets R=0.2 2.76 CMS Jets R=0.3 2.76 CMS Jets R=0.4 2.76 ATLAS Jets R=0.4 5.02 ATLAS Jets R=0.4 2.76 κ 2 σ 1 σ Global Fit

With increasing , hadrons & jets preferred value is more similar…

Lres = 2/πT

Lres

*

Hadrons 0-5% Jets 0-10%

* with LHC data only

In preparation

35

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SLIDE 36

Fit results

36

Daniel Pablos McGill / JETSCAPE

κ ∈ {0.420, 0.445} (global fit)

Lres = 2/πT

0.2 0.4 0.6 0.8 1 1.2 10 100 RAA Hadron or Jet PT (GeV) √s = 2.76 ATeV

√s = 5.02 ATeV

slide-37
SLIDE 37

Extracted jet FFs

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Daniel Pablos McGill / JETSCAPE

0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2 0.01 0.1 1 125 < pjet

T

< 160 GeV |y| < 2.1, R = 0.4 PbPb/pp z ATLAS Prelim. Data Lres = 0 Lres = 2/πT

√s = 5.02 ATeV κ ∈ {0.395, 0.420} κ ∈ {0.420, 0.445}

(global fits)

slide-38
SLIDE 38

ALICE Preliminary results on zg

38

Daniel Pablos McGill / JETSCAPE

all ΔR

Not unfolded data: need to smear theory results

slide-39
SLIDE 39

Understanding groomed observables

39

Daniel Pablos McGill / JETSCAPE

0.1 0.2 0.3 0.4 0.5 zg 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 Rg 5 10 15 20 25 30 35 40

Correlation between momentum balance & subjet angular separation Absolute Normalisation pp (PYTHIA)

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SLIDE 40

Understanding groomed observables

40

Daniel Pablos McGill / JETSCAPE

Correlation between momentum balance & subjet angular separation Separately normalised for each zg

0.1 0.2 0.3 0.4 0.5 zg 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 Rg 20 40 60 80 100 120

High zg does NOT mean large angle splitting

pp (PYTHIA)

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SLIDE 41

Understanding groomed observables

41

Daniel Pablos McGill / JETSCAPE

2 4 6 8 10 12 14 16 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 R = 0.4 80 < P ch

T,jet < 120 GeV

1/NRg dN/dRg Rg nSD=1 nSD=2 nSD=3 nSD=4 nSD=5 nSD=6

Strong correlation between subjet angular separation and number of Soft Drop splitting Suppression of wide structures Reduction of nSD pp (PYTHIA)

slide-42
SLIDE 42

Understanding groomed observables

42

Daniel Pablos McGill / JETSCAPE

Rough independence of momentum balance w.r.t. nSD Suppression of wide structures Not necessarily modifies zg

1 2 3 4 5 6 7 8 0.1 0.2 0.3 0.4 0.5 R = 0.4 80 < P ch

T,jet < 120 GeV

1/Nzg dN/dzg zg nSD=1 nSD=2 nSD=3 nSD=4 nSD=5 nSD=6

pp (PYTHIA)

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SLIDE 43

Finite resolution effects @ strong coupling

Daniel Pablos McGill / JETSCAPE smallest angular separation between two jets that the medium can resolve? assign a transverse structure to the string such that a quark-gluon system is emulated holographic description of 3-jet events study the stopping distances as a function of

  • pening angle and energy

different scaling than pQCD in a dense plasma

θpQCD

res

∝ E−3/4

Casalderrey & Ficnar - arXiv:1512.00371

43

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SLIDE 44

Holographic quenching with pure strings

competing effects: each individual jet widens, while wider jets lose more energy the string is treated as a model for the jet as a whole consider ensemble of jets by choosing initial distributions of energy & angle from pQCD

effect also observed in pQCD

measures jet angle in pQCD for the same jet suppression different final angle dist.

TSYM = b TQCD

44

Daniel Pablos McGill / JETSCAPE

Rajagopal et al. - PRL ‘16 Milhano & Zapp - EPJ ‘16

slide-45
SLIDE 45

Holographic quenching with pure strings

use pp jet shapes to determine angle distribution nuclear jet shape modification captures core dynamics - lacks contribution from medium response

a ∈ {1.8, 2.5}

as the string nullifies, different initial choices tend to converge

45

Daniel Pablos McGill / JETSCAPE

determine string energy density by considering different initial profiles evolved within full string dynamics

Brewer et al. - JHEP ‘18

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SLIDE 46

Heavy quark trailing string

Daniel Pablos McGill / JETSCAPE the heavy quark transfers energy to the plasma via frictional drag external force required to keep quark’s velocity constant need to consider the fluctuations within the thermal bath for a sensible phenomenology

zh zq

bdy

(coloured noise) (validity regime)

l i m i t

  • f

v a l i d i t y ?

∝ M

Herzog et al., Gubser, Casalderrey&Teaney ‘06 Casalderrey-Solana & Teaney ‘06, Gubser ‘07 Horowitz ‘15

46

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SLIDE 47

Transverse momentum broadening

Daniel Pablos McGill / JETSCAPE compute distance square travelled by the endpoint as it falls in holographic direction

  • fluct. for heavy quarks moving

faster than speed limit wobbly limp noodle interpolation between heavy quark and light quark results

(2 − 4)π √ λT 3

2π √ λT 3 v

a(t)

speed at which endpoint falls ˆ qLRW ' 7.5 p λT 3

ˆ qGubser = 2π √ λT 3 v √γ

light quark heavy quark

v = 0

(late times)

  • ballistic early times, diffusive late times
  • behaviour at late times solely dependent on near horizon dynamics

Moerman & Horowitz ‘16

47

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SLIDE 48

Proxies for HE jets

Daniel Pablos McGill / JETSCAPE light quark endpoint can fall unimpeded towards the black brane external boosted U(1) fields semiclassical string description Arnold & Vaman ‘11 Chesler et al. ‘09

κsc ∝ λ0

robust result at strong coupling zq → 0

48

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SLIDE 49

F.E.M. shooting strings

Daniel Pablos McGill / JETSCAPE from Gubser's ‘14 talk in ECT*

finite endpoint momentum strings: energy loss = energy flux from endpoint to bulk of string including higher derivative corrections (Gauss-Bonnet), but need to rescale LHC temperature string endpoint starts close to the horizon, then stops at boundary and falls back again

Ficnar et al. ‘14

49

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SLIDE 50

Intra-jet broadening

Daniel Pablos McGill / JETSCAPE

0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 0.05 0.1 0.15 0.2 0.25 0.3 0-10% Centrality 100 < P jet

T

< 300 GeV 0.3 < |η| < 2, r < 0.3 P parton

T

> 1 GeV PbPb/pp r K=100 K=40 K=20 K=0 CMS Data 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 0.2 0.4 0.6 0.8 1 0-10% Centrality 5 < P hadron

T

< 10 GeV PbPb/pp r K=100 K=40 K=20 K=0

Inclusive jets - all tracks Subleading jets - semi-hard tracks strong quenching suppresses the effect of broadening early wide fragments quenched late narrow fragments survive selection bias towards narrower jets, merely a jet axis deflection kinematical limits chosen such that:

  • no effect from background (soft tracks)
  • intra-jet activity above average (hard tracks)

deviations from such Gaussian broadening hard momentum transfers from QGP quasiparticles

50