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Introduction to heavy Introduction to heavy ion physics (NPII_06) ion physics (NPII_06) lect.3 lect.3 Edward Shuryak Edward Shuryak Department of Physics and Astronomy Department of Physics and Astronomy State University of New York State University of New York Stony Brook NY 11794 USA Stony Brook NY 11794 USA
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Page 1: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Introduction to heavy Introduction to heavy ion physics (NPII_06)ion physics (NPII_06)lect.3lect.3

Edward ShuryakEdward ShuryakDepartment of Physics and AstronomyDepartment of Physics and Astronomy

State University of New YorkState University of New York

Stony Brook NY 11794 USAStony Brook NY 11794 USA

Page 2: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Why study the heavy ion physics?

• A ``Bang” like other magnificent explosions like Supernova or Big Bang

• New form of matter formed, the Quark-Gluon Plasma

• It is different from the QCD vacuum phase• New spectroscopy, in spite of deconfinement

and With restored chiral symmetry • Relation to other fields: plasma physics, strongly

coupled atoms, string theory

Page 3: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

The theoretical tools we will need

• Finite T field theory

• Finite T QCD and lattice formulation

• Hydrodynamics

• Transport phenomena (freezeout) and coefficients (viscosity)

• Jet quenching: dE/dx and its origin

Page 4: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Cooling of the Universe (in the inverse order in time)

• T>1 ev ( or 10^4 K) time< 300000 years: atoms cannot exist. After atoms are created, the photons propagate unscattered till today, and we see them as T=2.7K “background radiation”

• T=1-0.05 MeV: time=few mins, size of Universe is about a Solar system. Light nuclei (d,He…Li^7) are created

• T>170 MeV: time 10^(-5) sec, Universe size about 3 km.

Before that there was no “elementary particles” such as protons, neutrons, pions,

and the matter was in a Quark-Gluon Plasma phase

•T>200 GeV quarks,leptons and W,Z get massless: the last phase transition we think we understand. We will not discuss electroweak phase transition in these lectures.

Page 5: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

The Big vs the Little Bang

• Big Bang is an explosion which created our Universe.

• Entropy is conserved because of slow expansion

• Hubble law v=Hr for distant galaxies. H is

isotropic. • “Dark energy”

(cosmological constant) seems to lead to accelrated expansion

• Little Bang is an explosion of a small fireball created

in high energy collision of two nuclei.

• Entropy is also conserved• Also Hubble law, but H is

anisotropic • The ``vacuum pressure”

works against QGP expansion

(And that is why it was so difficult to produce it)

Page 6: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Two main phases ofQuantum Chromodynamics (QCD)

• The vacuum phase: Quarks and gluons cannot

propagate free but are confined into hadrons

(mesons and baryons) with zero total color.

• Color charges are “confined” Attempts to separate them lead to creation of a string between charges and a potential V=Kr

• Another feature of the vacuum: quark pairs are

• condensed, like Cooper pairs in superconductor => <qRqL>

Broken chiral symmetry by a ``quark condensate”

• In QGP phase quarks and gluons are deconfined

and they can propagate as “quasiparticles”. The color charges

are “screened” at large distances (ES,1978) , while also

being antiscreened at small ones (Politzer, Gross and Wilczek 1973)

• New spectroscopy: Recently we learned that

at not too high T=(1-4)Tc

quasiparticles can also be bound in pairs, but in this case

a nonzero color is allowed and such states in fact dominate

High density phases of color superconductivity we will not discuss

Page 7: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

The vacuum vs QGP, continued

• The vacuum is very complicated, dominated by ``topological objects”

Vortices, monopoles and instantons

• Among other changes it shifts its energy down compared to an

“empty” vacuum, known asThe Bag terms:

p=#T4-B =3#T4+B

• The QGP, as any plasma, screens them, and is nearly free from them

• So, when QGP is produced, the vacuum tries to expel it

(recall here pumped out Magdeburg hemispheres

By von Guericke in 1656 we learned at school)

Page 8: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Magdeburg hemispheres 1656

We cannot pump the QCD vacuum out, but we can pump in something else, namely the Quark-Gluon Plasma

Page 9: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Diquarks as a Feshbach resonance

• Point S has the maximal Tc/Mu

• Line of qq marginal stability befurkates

• Line with point D is de-binding of Cooper pairs

Page 10: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Our map: the QCD Phase Diagram

T

The lines marked RHIC and SPS show the paths matter makes while cooling, in Brookhaven (USA) and CERN (Switzerland)

Chemical potential mu

Theory prediction (numerical calculation, lattice QCD, Karsch et al) the pressure as a function of T (normalized to that for free quarks and gluons)

Page 11: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

The zigzags on the phase diagram

• Both bar.charge and entropy are conserved: n_b/s=const(t)

• In resonance gas and QGP different formulae: curves do not meet at the critical line

• Of course they are connected inside the mixed phase –heating while expanding due to latent heat

A decade old plotFrom C.M.Hung and ES,hep-ph/9709264,PRC

Page 12: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Crude zigzags start to appear, but far from being accurate enough…

Effective eos along the line s/n_b=const also have aminimum at e=1 GeV/fm^3

Page 13: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Macro theory expects 3 special points in an energy scan, not 1!

(Macro theory=collision of very large nuclei, so hydro is valid without doubt…)

Focusing effect

See below

longest expansion, K/pi

V2 stops rising,

Elab about

5 GeV*A

Page 14: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

The same thing in log(s)-log(n) coordinates (now the cooling lines are simple, but the

thermodynamics is tricky)

Black=true

Page 15: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

RHIC: a view from space

A dedicated collider for

(i) Heavy ion collisions, AuAu 100+100 GeV/N

(ii) Polarized pp, 250+250 GeV

Page 16: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Relativistic Heavy Ion Collider

Two counter rotating beams in two rings,6 crossing points

Multiple magnets of the ring are all At the liquid HeTemperature – the main Expence during the runs

Page 17: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Two large experiments +2 small

PHENIX

2 e and 2 muon armsSTAR

Large tracking TPC

Page 18: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

One of the first RHIC events at STAR detector,

The average multiplicity at AuAu 200 GeV/N

Is about 5000

Page 19: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Many measurements (up to high pT!)from all 4 detectors

Page 20: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Main findings at RHIC

• Partciles are produced from matter which seems to be well equilibrated (by the time it is back in hadronic phase), N1/N2 =exp(-(M_1-M_2)/T)

• Very robust collective flows, well described by ideal hydro withLattice-based Equation of state (EoS). This indicates very strong

interaction even at early time => sQGP

• Jet quenching: Quarks and gluons with high energy (jets) do not fly away freely but are mostly (up to 90%) absorbed by the matter .

The released energy partly go to hydrodynamical ``conical flow” or sound waves rather than gluons.

Page 21: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Most importantly, we definitely produced ``matter”:

(while many skeptics predicted otherwise) The main condition for that:l << L

(the micro scale) << (the macro scale)(the mean free path) << (system size)

(relaxation time) << (evolution duration)

I

the zeroth order in l/L is ideal hydro with a local stress tensor. Viscosity appears as a first order correction l/L, it has velocity gradients.

(Note that it is inversely proportional to the cross section and thus is the oldest strong coupling expansion)

Page 22: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

If so, Hydrodynamics is simple!Static

•EoS from Lattice QCD•Finite T, field theory•Critical phenomena

Dynamic Phenomena •Expansion, Flow•Space-time evolution of thermodynamic variables

Once we accept localthermalization,life becomes very easy.

Why and when the equilibration takes place is a tough question

one has to answer

Local Energy-momentum

conservation:Conserved number:

Page 23: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Example of Hydro (with Jet Quenching)

Color: parton densityPlot: mini-jets

Au+Au 200AGeV, b=8 fmtransverse plane@midrapidityFragmentation switched off

hydro+jet modelHydro+Jet Hydro+Jet

modelmodel (T.Hirano (T.Hirano & Y.Nara (’02))& Y.Nara (’02))

x

y

Page 24: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

How Hydrodynamics Works at RHIC

Explosion goes in all directionsExplosion goes in all directionsRadial and especiallyRadial and especially

Elliptic flowElliptic flow

The red almond-The red almond-shaped region is shaped region is where the dense where the dense matter is. Yellow matter is. Yellow

region shows region shows “spectators” which “spectators” which

fly by without fly by without interactioninteraction

The so called “jet tomography” of the initial shape of the matter

Page 25: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

“elliptic flow” works as a barometer which measures the pressure of QGP

Origin: spatial anisotropy of the system when created, followed by multiple scattering of particles in the evolving system spatial anisotropy momentum anisotropy

v2: 2nd harmonic Fourier coefficient in azimuthal distribution of particles with respect to the reaction plane

Almond shape overlap region in coordinate space

y2 x2 y2 x2

2cos2 vx

y

p

patan

Page 26: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

More on Elliptic Flow

See recent reviews, P.Huovinen (QM2002) , nucl-th/0305064; P.Kolb and U.Heinz, nucl-th/0305084; E.Shuryak, hep-ph/0312227

Hydro: P.Kolb et al.(’99)(Note: Hydro+RQMD

gives a better description.D.Teaney et al.(’01))

STAR, PRC66(’02)034904

Hydro: P.Huovinen et al.(’01)

PHENIX, PRL91(’03)182301.

Page 27: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Viscosity of QGPQGP at RHIC seem to be the most idealfluid known, viscosity/entropy =.1 or so water would not flow if only a drop with 1000 molecules be made

• viscous corrections1st order correction to dist. fn.:

:Sound attenuation length

Velocity gradiants

Nearly ideal hydro !? D.Teaney(’03)

Page 28: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

What is needed to reproduce themagnitude of v2?

Huge cross sections!!

Page 29: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

How to get 50 times pQCD gg?

quark bound states don’t all melt at Tc

• all q,g have strong rescattering qqbar mesonResonance enhancements (Zahed and

ES,2003)

• Huge cross section due to resonance enhancement causes elliptic flow of trapped Li atoms

Page 30: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

Elliptic flow with ultracold trapped Li6 atoms, a=> infinity regime

The system is extremely dilute, but can be put into a hydro regime, with an elliptic flow, if it is specially tuned into a strong coupling regime via the so called Feshbach resonance

Similar mechanism was proposed (Zahed and myself) for QGP, in which a pair of quasiparticles is in resonance with their bound state at the “zero binding lines”

The coolest thing on Earth, T=10 nK or 10^(-12) eV can actually produce a

Micro-Bang !

Page 31: Introduction to heavy ion physics (NPII_06) lect.3 Edward Shuryak Department of Physics and Astronomy State University of New York Stony Brook NY 11794.

3 more strongly coupled systems

• N=4 Supersymmetric Yang-Mills

• Cold trapped atoms in Feshbach resonance (a=>1)

• Classical plasma with =(Ze)2/RT>>1 is a very good liquid, up to 300, with very small viscosity at » 10 where it has a deep minimum


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