strong cp violation in hot qcd: from heavy ion collisions to cosmology d. kharzeev bnl winter...

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Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633 (2006) 260 + work in progress

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Page 1: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Strong CP violation in hot QCD: from heavy ion collisions to cosmology

D. Kharzeev

BNL

Winter Workshop on Nuclear Dynamics, La Jolla, 2006

Phys.Lett.B633 (2006) 260,+ work in progress

Page 2: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

QCD and the UA(1) problem

.i

Invariant under chiral transformations in the limit of massless quarks

UL(Nf)xUR(Nf) chiral symmetry parity doubling in the hadron spectrum (not seen!)

If broken spontaneously, Nf2 = 9 Goldstone bosons.

Only 8 exist; the ninth, ’ is heavier than the proton!

Left Right

=> Something is wrong with the flavor-singlet UA(1)…

Page 3: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Axial anomaly

Consider the flavor singlet currentIt is not conserved even in the m -> 0 limit due to quantum effects:

Divergence can be written down asa surface term, and so is seemingly irrelevant:

Page 4: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Instantons and the UA(1) problem

But: sometimes, surface terms are important

Instantons: classical Euclidean solutions of QCD which map color SU(2) onto the sphere S3;in Minkowski space, describe quantum tunneling between degenerate vacua with different topological Chern-Simons numbers

QuickTime™ and aTIFF (Uncompressed) decompressorare needed to see this picture.

As a result, chiral chargeis no longer conserved

Page 5: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

QCD vacuum as a Bloch crystal

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

“quasi-momentum” “coordinate”

“ - vacuum”

Page 6: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

The lost symmetries of QCD

The prescription

with the “Bloch” weight

is equivalent to adding to the Lagrangian a new piece

which is odd under P, T, CP symmetries !

Page 7: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

The strong CP problem

Unless =0, P, T and CP invariances are lost!

Experiment:(e.d.m. of the neutron)

Why is so small? Axions? - PVLAS -recent evidence?

Will assume =0 for the rest of the talk

Page 8: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

The strong CP problemand the structure of QCD vacuum

Vafa-Witten theorem: P and CP cannot be broken spontaneously in QCD

But: 1. it does not constrain metastable states 2. it does not apply at finite temperature, finite baryon density, finite isospin density

Page 9: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

CP-odd domains in heavy ion collisions:how to look for them?

v.e.v. of the field is equivalent to non-zero

DK,Pisarski,Tytgat‘98

Page 10: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Diffusion of Chern-Simons number in QCD:

real time lattice simulations

DK, A.Krasnitz and R.Venugopalan,Phys.Lett.B545:298-306,2002

P.Arnold and G.Moore,Phys.Rev.D73:025006,2006

What are the experimental signatures?

Page 11: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

What are the observable signatures of strong CP violation?

rotate all CP violating phase into the quark piece of the Lagrangian:

is a complex mass parameter

In a CP-odd domain,

This leads to the asymmetry between “left” and “right” quarks

What is “left” and what is “right”? Quarks are massive, so the definition of chirality depends on the frame…

Page 12: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Azimuthal anisotropy:collective flow of strongly interacting matter

Hydro limit

STAR

PHOBOS

Hydro limit

STAR

PHOBOS

Description in terms of relativistic hydrodynamics

Page 13: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

A.Nakamura and S.Sakai, hep-lat/0406009

Quark-gluon plasma: more fluid than water?

KSS bound:strongly coupled SUSY QCD = classical supergravity

Superfluidhelium

Page 14: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Azimuthal anisotropy = angular momentum

What happens if a superfluid is rotated?

Page 15: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Magnetic vortices in rotating super-fluids

J. R. Abo-Shaeer, C. Raman, J. M. Vogels, and W. Ketterle, Observation of Vortex Lattices in Bose-Einstein Condensates, Science 292, 476 (2001).

E.J. Yarmchuk, M.J.V. Gordon, and R.E. Packard,

Observation of Stationary VortexArrays in Rotating Superfluid Helium, Phys. Rev. Lett. 43, 214 (1979).

Page 16: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Magnetic vortices

“Higgs” field Energy density

Page 17: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Magnetic vortices in QCD superfluid and CP violation

E

Pz

Left quarksRight anti-quarks

Fluctuation of chromo-electric field in the presence of chromo-magnetic vortex produces left quarks and right anti-quarks (level crossing at the 0th Landau level)

Page 18: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Magnetic vortices in QCD superfluid and CP violation

Left quarks: in the electric field, energy increases:

Decreases by the same amount for right anti-quarks.

Density of states = longitudinal x transverse:

Rate of chirality generation:

Analogous to cosmic strings, except not 1D

Page 19: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Magnetic vortices in QCD superfluid and CP violation

The Fermi momentum has to be smaller than the mass of the quark in the fluid:

otherwise, energetically unfavorable - quarkcan escape into the fluid

(no CP violation for massless quarks!)

What is M in a strongly coupled fluid?

Page 20: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Magnetic vortices in QCD superfluid and CP violation

Analogs:

Magnetic monopole - induced baryon decay Cosmic strings Chirality generation in superfluid 3He

…………

Page 21: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Charge asymmetry w.r.t. reaction plane as a signature of strong CP violation

+

-

excess of positivecharge

excess of negativecharge

Electric dipole moment of QCD matter!

Page 22: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

QuickTime™ and aTIFF (LZW) decompressor

are needed to see this picture.

Charge asymmetry w. r.t. reaction plane violates T, P, and (by CPT theorem) CP:

Page 23: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Analogy to P violation in weak interactions

Page 24: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Charge asymmetry w.r.t. reaction plane: how to detect it?

+

-

m

kS.Voloshin, hep-ph/0406311

Expect

Page 25: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Do we see strong CP violation?

I. Selyuzhenkov et al., STAR Coll., nucl-ex/0510069; October 25, 2005

Need to analyze the systematics and to understand if the effect is real

QuickTime™ and aTIFF (Uncompressed) decompressor

are needed to see this picture.

Page 26: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Other signatures?I. Separation of baryon number with respect to reaction plane?

Protons and anti-protons

II. Other observables composed of pion momenta?

Chern-Simons number of chiral fields

III. Lambda helicity correlations? J. Sandweiss

Page 27: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

What are the implications for the Early Universe?

Page 28: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

What is the origin of cosmic magnetic fields?

Magnetic field in M51:Polarization of emission

Beck 2000

Magnetic fields are abundantin the Universe at large scales:

3 G field in Milky Way;

1-40 G fields in clusters of galaxies

Page 29: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

What is the origin of magnetic fields in the Universe?

Primordial magnetic field (E.Fermi, 1949)?

Dynamo in proto-galaxy? Stars? Galaxy?

Domain walls and vortices associated with the vacua carry magnetic field;(“magnetic helicity”,…)Primordial magnetic field generation at the QCD phase transition?

Page 30: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Baryons in the Universe

Baryons in the Universe are rare:

1 baryon per ~ 2 billions photons in the Cosmic Microwave Background Radiation

~ 400 photons/cm3

~ 1 proton/m3

(Almost) no visible antimatter - why the asymmetry?

Page 31: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

What is the origin of the matter-antimatter asymmetry

in the Universe?

QuickTime™ and aTIFF (Uncompressed) decompressor

are needed to see this picture.

1. B violation2. CP violation3. Non-equilibrium dynamics

A.D. Sakharov,JETP Lett. 5 (1967) 24

Page 32: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Baryon asymmetry in the Universe and strong CP violation

1. Generation of Chern-Simons number at the QCD phase transition is analogous to baryon number generation in the electroweak phase transition

2. Strong CP violation separation of matter and antimatter in the Universe at the QCD phase transition ?

e.g. V.Kuzmin, V.Rubakov and M.Shaposhnikov, Phys.Lett.B155(1985)36

Page 33: Strong CP violation in hot QCD: from heavy ion collisions to cosmology D. Kharzeev BNL Winter Workshop on Nuclear Dynamics, La Jolla, 2006 Phys.Lett.B633

Summary

1. P and CP violation in hot QCD is not forbidden

2. “All what is not forbidden is allowed” and may exist; a specific dynamical mechanism - magnetic vortices

3. Rejecting or confirming the signal of P and CP violation at RHIC is an urgent problem of fundamental importance