A strongly coupled view of the quark gluon plasma
Jorge Casalderrey-Solana
A strongly coupled view of the quark gluon plasma Jorge - - PowerPoint PPT Presentation
A strongly coupled view of the quark gluon plasma Jorge Casalderrey-Solana QCD Matters A new phase: Quark Gluon Plasma Filled the universe s after Big Bang Colour is liberated A gas of quark and gluons phase transition
Jorge Casalderrey-Solana
Birmingham Particle Physics Group
07th June 2017
A new phase: Quark Gluon Plasma Hadron Gas
Tc “phase transition” Tc ≈ 2×1012 K ≈ 170 MeV What are the properties of the plasma close to the transition?
2
Birmingham Particle Physics Group
07th June 2017
3
Wuppertal-Budapest Col. arXiv: 1007.2580
Rapid cross over transition:
Birmingham Particle Physics Group
07th June 2017
4
At T>104 GeV:
≪
T 1 gT 1
≪
g2T 1
inter-particle spacing Interaction range mean free path Resummations can extend the validity of perturbative methods to much lower temperatures!
Birmingham Particle Physics Group
07th June 2017
αs=0.3⟹g=2
5
T~gT~g2T
At T~0.2 GeV Is it a gas of quark and gluons? Is it a system without long lived excitations? Is it a system without quasiparticles?
Birmingham Particle Physics Group
07th June 2017
6
➤ About 20.000 particles ➤ Up to 400 participating nucleons ➤ ET ∼1 GeV per particles ➤ Very large initial energy density
ετ ~ 16 GeV/(fm2c)
Birmingham Particle Physics Group
07th June 2017
7
Very strong collective effects
๏ Emission of 20.000 particles correlated
with the impact parameter
The quark gluon plasma is a very good fluid
๏ Hydrodynamic explosion ๏ Correlation measured in
terms of Fourier coefficients
) c (GeV/
tp
1 2 3 4 5
{4-particle cumulant method}
2v
0.05 0.1 0.15 0.2 0.25
10-20% 20-30% 30-40% 10-20% (STAR) 20-30% (STAR) 30-40% (STAR)ALICE
Birmingham Particle Physics Group
07th June 2017
8
๏ It is the smallest value ever measured in any substance.
The Quark Gluon Plasma is the most perfect fluid!
๏ It was predicted in 2001 (Policastro, Son, Starients)
= =0.08
4π 1 s
η
... but for a large class of non-abelian gauge theories at infinite coupling via holography
๏ It is incompatible with quasiparticles
Boltzmann equation ⇒
Birmingham Particle Physics Group
07th June 2017
9
๏ This all may be a remarkable coincidence
Different theories, different matter content, different symmetries...
๏ But there is certain degree of universality
Some properties are the same in all theories with holographic duals Different theories, different matter content, different symmetries... Despite:
๏ All those strongly coupled theories
have plasmas with no quasi particles
Birmingham Particle Physics Group
07th June 2017
10
Holographic Direction
1/Q
Tμν Tμν QFT Gravity Horizon
Dictionary
Tμν↔ gμν
heavy quark↔ string
M
T↔ black hole λ=g2Nc→∞
Gauge/String Duality, Hot QCD and Heavy Ion Collisions
Casalderrey-Solana, Liu, Mateos, Rajagopal and Wiedemann Gauge/String Duality, Hot QCD and Heavy Ion Collisions Jorge Casalderrey-Solana, Hong Liu, David Mateos, Krishna Rajagopal and Urs Achim Wiedemann Heavy ion collision experiments recreating the quark–gluon plasma that fjlled the microseconds-old universe have established that it is a nearly perfect liquid that fmows with such minimal dissipation that it cannot be seen as made of particles. String theory provides a powerful toolbox for studying matter with such properties. This book provides a comprehensive introduction to gauge/string duality and its applications to the study of the thermal and transport properties of quark–gluon plasma, the dynamics of how it forms, the hydrodynamics of how it fmows, and its response to probes including jets and quarkonium mesons. Calculations are discussed in the context of data from RHIC and LHC and results from fjnite temperature lattice QCD. The book is an ideal reference for students and researchers in string theory, quantum fjeld theory, quantum many-body physics, heavy ion physics, and lattice QCD. Jorge Casalderrey-Solana is a Ramón y Cajal Researcher at the Universitat deflavor↔ brane
Birmingham Particle Physics Group
07th June 2017
11
ε∕ρ4
ρz
ρt
๏ Simulation of full collision dynamics
➤ Collisions of lump of energies
shock wave collisions
JCS, M. Heller, D. Mateos W. van der Schee 13,14 Chesler and Yaffe 11
๏ Fast onset of hydrodynamics thydro = 0.63 / Thydro
dual model
➤ Hydrodynamics without isotropy ➤ Hydrodynamics without equation of state
Attems, JCS, et. al. 16 Chesler & Yaffe, Wu & Romatschke, Heller, Janik & Witaszczyk, Heller, Mateos, van der Schee, Trancanelli
Birmingham Particle Physics Group
07th June 2017
12
e e
๏ Can we probe the system?
Birmingham Particle Physics Group
07th June 2017
13
➤ strong non-abelian bremsstrahlung ➤ Jets: sprays of particles within a fixed resolution R
๏ Energetic Quarks are produced in pairs ๏ Hard process
Birmingham Particle Physics Group
07th June 2017
14
Birmingham Particle Physics Group
07th June 2017
15
Birmingham Particle Physics Group
07th June 2017
16
ET1 ET2<ET1
12 fm
JCS, Milhano, Wiedemann 10
Birmingham Particle Physics Group
07th June 2017
p k,c q1,a1 q2,a2 q3,a3 q4,a4 q5,a5 t t0 t1 t2 t3 t4 t5
BDMPS-Z 96 (GLV, ASW, AMY, HT ...)
Range of interaction 1 mD ⌧ 1 λm. f. p mean free path
(Review: JCS & C. Salgado arXiv:0712.3443 ) 17
๏ Medium Induced gluon bremsstrahlung
dE dx = 1 2 ˆ qL
ˆ q = (mean transferred momentum)2 length ⇠ m2
D
λm. f. p
๏ Non-abelian energy loss:
Birmingham Particle Physics Group
07th June 2017
18
๏ How do jets loose energy in a system
with no quasiparticles?
๏ Holography provides a tool to address
this problem
Birmingham Particle Physics Group
07th June 2017
19
๏ Heavy Quark ⇔ classical string attached to boundary ๏ Energy loss ⇔ flux of momentum along the string
dp dt = ηDp ηD = π p λT 3 2MT
JCS & Teaney (2006)
Herzong, Karch, Kovtun,Kozcaz, Yaffe (2006)
๏ Compatible with lattice extractions!
D ⇥ 1 2πT
αsymN ⇥1/2
Langevin
0.5 1 1.5 2 2.5 3 3.5 4 1.4 1.6 1.8 2 2.2 2.4 2.6 2.8 3 2TD T/Tc 0.5 1 1.5 2 2.5 3 3.5 4 1.4 1.6 1.8 2 2.2 2.4 2.6 2.8 3 2TD T/Tc
Birmingham Particle Physics Group
07th June 2017
20
1 Ein dE dx = 4 π x2 x2
stop
1 q x2
stop x2
xstop = 1 2 κsc E1/3
in
T 4/3 ,
๏ Light Quark ⇔ free end point ๏ Energy loss rate
Chesler & Rajagopal 14, 15 Gubser et al 08, Chesler et al. 08, Ficnar and Gubser 13
Birmingham Particle Physics Group
07th June 2017
➤ Hard evolutions (perturbative) ➤ Exchanges at medium scale ➤ Soft jet fragments
strong coupling
➤ Leave jet evolution unmodified (Q>>T) ➤ Each in-medium parton losses energy ➤ Hard production (perturbative)
JCS, Gulhan, Milhano, Pablos and Rajagopal 2014, 2015, 2016
21
➤ We assume that all differences between theories can be packed
into one single (fit) parameter
Birmingham Particle Physics Group
07th June 2017
22
γ
Birmingham Particle Physics Group
07th June 2017
23
0.05 0.1 0.15 0.2 0.25 0.3 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 Event Fraction AJ 0 − 10% Centrality Vacuum+Smearing Data Strong Coupling 0.2 0.4 0.6 0.8 1 1.2 100 120 140 160 180 200 220 240 260 280 300 Jet RAA PT (GeV) 0-10% Centrality Strong Coupling Data 0.5 1 1.5 2 30 40 50 60 70 80 90 100 IAA Jet PT 0 − 30% Centrality P jet T > 30 GeV ∆φ > 7π/8 60 < P γ T < 80 GeV Strong Coupling Data 0.2 0.4 0.6 0.8 1 1.2 1.4 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2 1 Nγ dNJγ dxJγ xJγ 0 − 10% Centrality P jet T > 30 GeV ∆φ > 7π/8 Strong Coupling Smeared pp Data 0.2 0.4 0.6 0.8 1 40 50 60 70 80 90 100 110 RJγ P γ T 0 − 30% Centrality P jet T > 30 GeV ∆φ > 7π/8 Strong Coupling Smeared pp Data5 observables 1 fit parameter pT and centrality
Birmingham Particle Physics Group
07th June 2017
24
Core features of the model have been validated by e.g. photon-jet observables predictions
Birmingham Particle Physics Group
07th June 2017
25
Chesler &Yaffe 06
➤ Medium response to Eloss must be collective ➤ Strong coupling computations provide an explicit example
JCS, Shuryak & Teaney 06
➤ Collectivity starts at short distance 1/T from the jet ➤ There is a strong momentum flux along the jet direction ➤ Essential to understand soft particle distribution around jets.
Birmingham Particle Physics Group
07th June 2017
26 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∆
CMS
Leading Jet Associated Jet
➤ No additional parameters
Birmingham Particle Physics Group
07th June 2017
27
from D. Caffarri’s talk on Tue
ET1 ET2<ET1
12 fm
➤ Puzzling result ➤ Removing soft fragments ⇒ Jet mass narrowing
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=0.4Charged jet mass
Birmingham Particle Physics Group
07th June 2017
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 Back No Back CMS Data
R
r
➤ All current models fail in some observable
JCS, Gulhan, Milhano, Pablos and Rajagopal 16
28
Birmingham Particle Physics Group
07th June 2017
29
๏ Perturbative analysis of non-abelian classical currents
r⊥
๏ Colour exchanges decorrelate the currents
1 ˆ qL
τcoh = θc θq¯
q
2/3 L θ2
c =
1 ˆ qL3
๏ Coherence is lost at a time ๏ Fragments at small angles cannot be resolved
JCS, Iancu arXiv:1105.1760 Mehtar-Tani, Tywoniuk, Salgado arXiv:1009.2965, 1102.4317 arXiv:1112.5031, 1205.5739
Birmingham Particle Physics Group
07th June 2017
Interferences
30
๏ Double emission rate off in-medium quark
Hard Vertex Hard Gluon Soft Gluon
τf = 2ω k2⊥ ➤ Confirms the classical calculation on interferences ➤ Supplements time structure of the process
JCS, Pablos and Tywoniuk 16
Birmingham Particle Physics Group
07th June 2017
0.2 0.4
0.2 0.4 5 10 15 20 25
0.2 0.4
0.2 0.4 5 10 15 20 25
r⊥ Λmed r⊥ Λmed
Rmed Rmed
JCS, Mehtar-Tani, Tywoniuk, Salgado arXiv:1210.7765
Rmed 2 ✓Z d⌅ ⌅2ˆ q(⌅) ◆−1/2
ξ ≡ path length
➤ Effective emitters control energy loss fluctuations
31
๏ Jet substructure is resolved by the medium
Birmingham Particle Physics Group
07th June 2017
xêzH yêzH z zH
10 20
5
0.0
JCS, Ficnar 1512.00371
32
5 10 15 20
2 4 6
x ê zH y ê zH
5 10 15 20
2 4 6
x ê zH y ê zH
resolved jets un-resolved jets
Birmingham Particle Physics Group
07th June 2017
33
0.2 0.4 0.6 0.8 1 1.2 1 10 100 1000 Lres = 2/πT w/ nPDF LO EPS09
Hadron PT (GeV) Strong Coupling 0-10% Strong Coupling 10-30% Strong Coupling 10-30% CMS 0-10 % CMS 10-30 % CMS 30-50 %
√s = 5.02 ATeV
imp ag
JCS, Gulhan, Hylcher, Milhano, Pablos, Rajagopal in preparation
๏ Resolution effects are important for single particle suppression
0.2 0.4 0.6 0.8 1 1.2 1 10 100 1000 No Res w/ nPDF LO EPS09
Hadron PT (GeV) Strong Coupling 0-10% Strong Coupling 10-30% Strong Coupling 10-30% CMS 0-10 % CMS 10-30 % CMS 30-50 %
te ce
√s = 5.02 ATeV
0.2 0.4 0.6 0.8 1 10 Nuc PDF 0 − 5% AuAu √s = 200 AGeV π0 RAA Hadron PT (GeV) Lres = 2/πT No Res PHENIX Data under scrutiny
Preliminary
๏ But also to reconcile the √s dependence of quenching
➤ A common problem in all models of jet quenching
Birmingham Particle Physics Group
07th June 2017
34
๏ Heavy ion collisions provide access to the QGP
➤ Deconfined matter ➤ A very good fluid ➤ A system with no quasiparticles
๏ Hard probes provide access to the microscopic dynamics
➤ Promising description based on strong coupling techniques ➤ Dynamical implementation: allows us to understand successes and limitations ➤ Ultimate goal: can we understand the nature of plasma degrees of freedom from these measurements?
Birmingham Particle Physics Group
07th June 2017
35
Birmingham Particle Physics Group
07th June 2017
36
0.5 1 1.5 2 30 40 50 60 70 80 90 100 IAA Jet PT 0 − 30% Centrality P jet T > 30 GeV ∆φ > 7π/8 60 < P γ T < 80 GeV Strong Coupling Radiative Collisonal Data 0.2 0.4 0.6 0.8 1 1.2 1.4 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2 1 Nγ dNJγ dxJγ xJγ 0 − 10% Centrality pjet T > 30 GeV ∆φ > 7π/8 Strong Coupling Radiative Collisonal Smeared pp Data 0.2 0.4 0.6 0.8 1 40 50 60 70 80 90 100 110 RJγ P γ T 0 − 30% Centrality P jet T > 30 GeV ∆φ > 7π/8 Strong Coupling Radiative Collisonal Smeared pp Data 0.05 0.1 0.15 0.2 0.25 0.3 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 Event Fraction AJ 0 − 10% Centrality Vacuum+Smearing Data Strong Coupling Radiative Collisonal 0.2 0.4 0.6 0.8 1 1.2 100 120 140 160 180 200 220 240 260 280 300 Jet RAA PT (GeV) 0-10% Centrality Strong Coupling Radiative Data Collisional −0.5 0.5 1 1.5 2 2.5 3 0.5 1 1.5 2 2.5 3 0 − 30% P Z0 T > 60 GeV, P jet T > 30 GeV |ηjet| < 1.6, |ηZ0| < 2.5 1 NZ0 dNJZ0 d∆φJZ ∆φ Strong Coupling Radiative Collisional Smeared pp PbPb CMS 0.2 0.4 0.6 0.8 1 1.2 1.4 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2 0 − 30% Centrality P jet T > 30 GeV ∆φ > 7π/8 1 NZ0 dNJZ0 dxJZ0 xJZ0 Strong Coupling Radiative Collisonal Smeared pp PbPb CMSBirmingham Particle Physics Group
07th June 2017
Lund string model: gluons associated to kinks in the string
37
๏ Hard gluon emission by an energetic q-q pair
Birmingham Particle Physics Group
07th June 2017
38
θres = 24/3 π Γ(3/4)2 Γ(5/4)2 ✓ E p λT ◆2/3
๏ Resolution angle infinite medium
Finite length medium
๏ At weak coupling: ๏ Infinite medium, maximal length= stopping distance
jet, ∆x [42], the as θpQCD
res
/ E3/4 erstand whether th
๏ Fluctuations in jet energy loss may help distinguish between the
different microscopic realisations
Birmingham Particle Physics Group
07th June 2017
39
Birmingham Particle Physics Group
07th June 2017
40
Birmingham Particle Physics Group
07th June 2017
41
➤ Comment on crude
hadronic treatment
Birmingham Particle Physics Group
07th June 2017
42
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∆
CMS