frithjof karsch bielefeld university & brookhaven national ...qcd in a nutshell,...

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1 F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017 Lattice QCD at non-zero temperature and density Frithjof Karsch Bielefeld University & Brookhaven National Laboratory QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations the phase diagram on strongly interacting matter, chiral symmetry restoration, the equation of state finite density QCD, cumulants of conserved charge fluctuations, thermal masses & transport properties

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Page 1: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

1F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Lattice QCD at non-zero temperature anddensity

Frithjof Karsch

Bielefeld University & Brookhaven National Laboratory

QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations

the phase diagram on strongly interacting matter, chiral symmetry restoration, the equation of state

finite density QCD, cumulants of conserved charge fluctuations, thermal masses & transport properties

Page 2: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

2F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Literature

● M. Creutz, Quarks, Gluons and Lattices

● H. Rothe, Lattice Gauge Theories

● T. DeGrand, C. DeTar, Lattice Methods for Quantumchromodynamics

● C. Gattringer and C.B. Lang, Quantum Chromodynamics on the Lattice

● I. Montvay, G. Muenster, Quantum Fields on a Lattice

● J. Zinn-Justin, Quantum Field Theory and Critical Phenomena

● H.T. Ding, FK, S. Mukherjee, Thermodynamics of strong-interaction Matter from Lattice QCD, Int. J. Mod. Phys. E24 (2015) 153007

Page 3: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

3F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Motivation

Why lattice (gauge) theory?

Many phenomena in physics are of 'non-perturbative' nature

● Spontaneous symmetry breaking: - Phase transitions (spontaneous magnetization, Ising model) - Higgs mechanism - chiral symmetry breaking

● The origin of mass, hadron spectra - MeV, but MeV

● Long distance properties of Quantum Field Theories - confinement, screening

Page 4: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

4F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

The theory of strong-interaction Quantum Chromo Dynamics (QCD)

F. Wilczek, QCD made simple,Phys. Today 53N8 (2000) 22

Page 5: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

5F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

The theory of strong-interaction Quantum Chromo Dynamics (QCD)

– non-abelian gauge theory, constructed in analogy to QED

– matter fields (quarks [fermions]) and force carrier (gluons [bosons])

– a new quantum number – color

– quarks live in the fundamental representation of the SU(3) color group:

– each quark species/flavor carries one of three possible colors

– gluons live in the adjoint representation; there are 8 different gluons

– unlike the photon in QED the gluons not only interact with quarks but also among themselves (three- and four-gluon vertices) quark-gluon

vertex3-gluon and 4-gluon vertices vertex

Page 6: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

6F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

The theory of strong-interaction Quantum Chromo Dynamics (QCD)

quark-gluon vertex 3-gluon and 4-gluon vertices vertex

F. Wilczek, QCD made simple,Phys. Today 53N8 (2000) 22

jets in jets in high energyhigh energy e+e- collisions e+e- collisions

– asymptotic freedomasymptotic freedom --

weakly interacting quarks& gluons atweakly interacting quarks& gluons at high-T high-T

Page 7: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

7F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

The theory of strong-interaction Quantum Chromo Dynamics (QCD)

F. Wilczek, QCD made simple,Phys. Today 53N8 (2000) 22

Y. Aoki et al, Nature 443 (2006) 675

Hadron spectrum in the vacuumHadron spectrum in the vacuum Hadrons in a thermal heat bathHadrons in a thermal heat bath

– confinementconfinement --

melting of heavy quark bound states

T. Matsui and H. Satz, Phys. Lett. B178 (1986) 416

H.-T. Ding et al., Phys. Rev. D86 (2012) 014509

Page 8: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

8F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Phases of strong-interaction matter

physics of the early universe

hot

experimentally accessible inHeavy Ion Collisions at SPC, RHIC, LHC, FAIR, NICA

may exist in the interior ofcompact stars,

dense

Page 9: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

9F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Phases of strong-interaction matter

physics of the early universe

hot

experimentally accessible inHeavy Ion Collisions at SPC, RHIC, LHC, FAIR,NICA

may exist in the interior ofcompact stars,

dense

thermodynamics of a hadron resonance gas

Page 10: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

10F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Phases of strong-interaction matter

physics of the early universe

hot

experimentally accessible inHeavy Ion Collisions at SPC, RHIC, LHC, FAIR,NICA

may exist in the interior ofcompact stars,

dense

thermodynamics of a hadron resonance gas

thermodynamics of quarks and gluons: high-T – QCD perturbation theory

Page 11: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

11F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Phases of strong-interaction matter

physics of the early universe

hot

experimentally accessible inHeavy Ion Collisions at SPC, RHIC, LHC, FAIR,NICA

may exist in the interior ofcompact stars,

dense

thermodynamics of a hadron resonance gas

thermodynamics of quarks and gluons: high-T – QCD perturbation theory

strongly interacting, highlynon-perturbative region close tophase boundaries need for lattice QCD calculations

Page 12: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

12F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Quantum Chromo Dynamics (QCD)

– QCD is expected to explain ALL aspects of strong interaction physics

– a rich spectrum of hadrons (including the values of their masses)

– the peculiar role of the lightest hadrons → pions – the mass splitting among parity partners – the mass-splitting of pion and delta (a_0)

spontaneous breaking of chiral symmetries

– the absence of its basic constituents (quarks and gluons) from the experimentally observed particle spectrum

confinement

– the simple properties of deep inelastic scattering

asymptotic freedom

– – the existence (?) of phase transitionsthe existence (?) of phase transitions

deconfinementdeconfinement & & chiral symmetry resorationchiral symmetry resoration

Page 13: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

13F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

– start with the Euclidean version of the QCD Lagrangian:

field strength tensor:

gluons: real 4-vector

quarks: 4-spinor, Grassmann variables

Lattice regularized Quantum Chromo Dynamics (QCD)

(suppress E again)

Page 14: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

14F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Gauge field theories

gauge transformation:

complex matrix:

is gauge invariant

is gauge invariant

is gauge invariant

Page 15: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

15F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

introduce gauge fields that interpolate between sites and parallel transporter:

gauge transformation:

Phys. Rev. D 10 (1974) 2445

I) introduce gauge degrees of freedom (vector fields) on links

ii) replace gauge fields by elements of the relevant symmetry group

QCD:

The idea of K. Wilson: lattice gauge theory regularize QCD by introducing a discrete space-time lattice;

– violates various symmetries, but...

– minimal requirement: preserve ''local'' gauge invariance

latticespacing

Page 16: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

16F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

lattice discretization:

introduce gauge degrees of freedom on links,

matrix

the plaquette variable

Page 17: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

17F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

lattice discretization:

introduce gauge degrees of freedom on links

matrix

the plaquette variable

- matrices do not commute- cyclic permutation under trace

Page 18: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

18F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

{use Baker-Hausdorff repeatedly

use Baker-Hausdorff formula

not the inverse temperature!!

Page 19: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

19F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

{use Baker-Hausdorff repeatedly

use Baker-Hausdorff formula

not the inverse temperature!!

lattice spacing ''a'' disappeared''lattice spacing ''a'' disappeared''

Page 20: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

20F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Continuum limit

long distance behavior of 2-point function:

correlation length (statistical physics)

mass of a scalar particle in lattice units;

continuum limit: implies for any fixed (physical) mass

divergent correlation length (2nd order) phase transitionin statistical physics terminologybehavior of defines the

lattice spacing

a

Page 21: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

21F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Continuum limit

long distance behavior of 2-point function:

continuum limit: implies for any fixed (physical) mass

divergent correlation length (2nd order) phase transitionin statistical physics terminologybehavior of defines the

lattice spacing

a

correlation length (statistical physics)

mass of a scalar particle in lattice units;

for instance:

Page 22: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

22F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

The continuum limit of lattice regularized QCDThe continuum limit of lattice regularized QCD

- at present we consider only SU(Nc) gauge theories

- the only free parameter is the gauge coupling or

Continuum limit:

The gauge coupling needs to approach a critical point

at which the 'correlation lengths', defined through 2-point functions,diverge, e.g.

divergent correlation length

Page 23: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

23F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

- at present we consider only SU(Nc) gauge theories

- the only free parameter is the gauge coupling or

The gauge coupling needs to approach a critical point

at which the 'correlation lengths', defined through 2-point functions,diverge, e.g.

<= often used notation, but not quite correct

Continuum limit: divergent correlation length

The continuum limit of lattice regularized QCDThe continuum limit of lattice regularized QCD

Page 24: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

24F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Continuum limit: physical observables, do not depend on the lattice spacing (cut-off)

- observables calculated in a regularized QFT depend on the cut-off, e.g. they depend on the lattice spacing

- observables calculated on the lattice are dimensionless, i.e. they are calculated in appropriate units of the lattice spacing

(1) now reads:

(1)

with -function

Page 25: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

25F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Continuum limit: physical observables, do not depend on the lattice spacing (cut-off)

- observables calculated in a regularized QFT depend on the cut-off, e.g. they depend on the lattice spacing

- observables calculated on the lattice are dimensionless, i.e. in general they are calculated in appropriate units of the lattice spacing

(1) now reads:

(1)

with -function

renormalization group equation

Page 26: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

26F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

The -function:

Page 27: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

27F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

The -function:

The -function

- controls the variation of the lattice spacing as function of the gauge coupling

- provides a solution to the renormalization group equation

Page 28: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

28F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

The -function:

continuum limit:

-function needs to have a zero (fixpoint)

Page 29: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

29F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

a special case:

Asymptotic Freedom Asymptotic Freedom

fixpoints:

QCD beta-functionQCD beta-function

Page 30: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

30F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Asymptotic Freedom and theAsymptotic Freedom and theHeavy Quark PotentialHeavy Quark Potential

M. Creutz, M. Creutz, Phys. Rev. D21 (1980) 2308Phys. Rev. D21 (1980) 2308

SU(2) SU(2) string tensionstring tension

asymptoticasymptoticfreedom &freedom &confinementconfinement

heavy quark potential:

Mike Creutz

Monte Carlo simulationMonte Carlo simulation 19791979

Page 31: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

31F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Monte Carlo SimulationsMonte Carlo Simulations

Observables = Expectation values

integrate out fermions:

distribute gauge field configurations according to

the probability distribution

calculate expectation values:

Monte Carlo algorithms(detailed balance) generates Markov chain

Page 32: Frithjof Karsch Bielefeld University & Brookhaven National ...QCD in a nutshell, non-perturbative physics, lattice-regularized QCD, Monte Carlo simulations ... physics of the early

32F. Karsch, NNPSS 2017 F. Karsch, NNPSS 2017

Different regularization schemesDifferent regularization schemes for fermions (and gauge sector)

Improved actionsImproved actions

try to eliminate discretization errors in the continuum limit

– pure gauge sector: Symanzik improvement, e.g. at 6-link terms to action– fermion sector: higher order discretization schemes, e.g. add three link terms: naïve staggered → Naik action → Highly improved staggered quarks (HISQ) Wilson fermions have errors, add ''clover-term'' to arrive at

– staggered fermions → doublers– Wilson fermions → explict chiral symmetry breaking

– Domain Wall Fermions → 5-dimensional formulation, ''almost'' exact chiral symmetry, ''residual mass''

– Overlap fermions → chiral fermion formulation (obeys Ginsparg-Wilson relation)

chiral fermions are computationally demanding

overlap 100 x staggered