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Local P and CP violation in strongly interacting matter D. Kharzeev - PowerPoint PPT Presentation

PHENO 2010 Symposium, Madison, Wisconsin, May 12, 2010 Local P and CP violation in strongly interacting matter D. Kharzeev BNL 1 Outline QCD topology and the strong CP problem Chiral magnetic effect (CME) and topologically induced


  1. PHENO 2010 Symposium, Madison, Wisconsin, May 12, 2010 Local P and CP violation in strongly interacting matter D. Kharzeev BNL 1

  2. Outline QCD topology and the “strong CP problem” Chiral magnetic effect (CME) and topologically induced local P and CP violation in QCDxQED Recent experimental evidence at RHIC P and CP violation in the Early Universe

  3. P and CP invariances are violated by weak interactions C.N.Yang T.D.Lee 1957 CP violation J.W.Cronin, V.L.Fitch 1980 Complex CKM mass matrix Y. Nambu, M. Kobayashi, T. Maskawa 2008

  4. P and CP invariances are violated by weak interactions What about strong interactions? C.N.Yang T.D.Lee 1957 CP violation J.W.Cronin, V.L.Fitch 1980 Complex CKM mass matrix Y. Nambu, M. Kobayashi, T. Maskawa 2008

  5. Very strict experimental limits exist on the amount of global violation of P and CP invariances in strong interactions (mostly from electric dipole moments) But: P and CP conservation in QCD is by no means a trivial issue... Can a local P and CP violation occur in QCD matter?

  6. Annals of Mathematics, 1974

  7. Chern-Simons forms What does it mean for a gauge theory?

  8. Chern-Simons theory What does it mean for a gauge theory? Geometry Physics Riemannian connection Gauge field Curvature tensor Field strength tensor � � � A i F jk + 2 S CS = k d 3 x ǫ ijk 3 A i [ A j , A k ] 8 π M non-Abelian Abelian

  9. Chern-Simons theory � A i F jk + 2 � S CS = k � d 3 x ǫ ijk 3 A i [ A j , A k ] 8 π M Remarkable novel properties: gauge invariant, up to a boundary term topological - does not depend on the metric, knows only about the topology of space-time M when added to Maxwell action, induces a mass for the gauge boson - different from the Higgs mechanism! breaks Parity invariance

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  11. Topological number fluctuations in QCD vacuum 11 D. Leinweber

  12. Sphaleron transitions at finite energy or temperature Energy of gluon field N CS = -2 -1 0 1 2 instanton sphaleron Sphalerons: random walk of topological charge at finite T: 12

  13. Diffusion of Chern-Simons number in QCD: real time lattice simulations P.Arnold and G.Moore, DK, A.Krasnitz and R.Venugopalan, Phys.Rev.D73:025006,2006 Phys.Lett.B545:298-306,2002

  14. Experimental test of Chern-Simons dynamics in hot QCD: Heavy ion collisions LHC NICA, JINR

  15. Is there a way to observe topological charge fluctuations in experiment? Relativistic ions create a strong magnetic field: B

  16. Heavy ion collisions as a source of the strongest magnetic fields available in the Laboratory DK, McLerran, Warringa, Nucl Phys A803(2008)227 46

  17. Heavy ion collisions: the strongest magnetic field ever achieved in the laboratory 47

  18. From QCD back to electrodynamics: Maxwell-Chern-Simons (axion) theory L MCS = − 1 4 F µ ν F µ ν − A µ J µ + c 4 P µ J µ CS . Axial current of quarks J µ CS = ǫ µ νρσ A ν F ρσ , Photons

  19. Magnetic monopole � at finite : the Witten effect θ � E ∇ · � � E = ρ + c � P · � � B, B θ � = 0 q = e θ π 2 P ≡ � � θ = 0 ∇ θ E. Witten; F. Wilczek Induced electric charge:

  20. The Chiral Magnetic Effect I: � Charge separation � B ∇ · � � E = ρ + c � P · � B, ∼ − e θ π · eB θ = 0 2 π P ≡ � � ∇ θ � E θ � = 0 ∼ + e θ π · eB � � � eB · S � e θ � q 2 = L ; 2 π d e = f 2 π π f θ = 0 DK ’04; DK, A. Zhitnitsky ’06; DK arXiv:0911.3715; Annals of Physics (2010)

  21. The chiral magnetic effect II: chiral induction � B θ = 0 J ∼ e ˙ π · e � � θ B 2 π J = − e 2 ˙ θ � = 0 � 2 π 2 ˙ θ � B DK, L. McLerran, H. Warringa ’07; K. Fukushima, DK, H. Warringa ’08; DK, H.Warringa arXiv:0907.5007

  22. Computing the induced current Fukushima, DK, Warringa, ‘08 Chiral chemical potential is formally µ 5 = A 0 equivalent to a background chiral gauge field: 5 In this background, vector e.m. current is not conserved: e 2 ∂ µ J µ = � � � L ˜ R ˜ F µ ν F L,µ ν − F µ ν F R,µ ν 16 π 2 Compute the current through J µ = ∂ log Z [ A µ , A 5 µ ] ∂ A µ ( x ) e The result: Coefficient is fixed J = e 2 � 2 π 2 µ 5 � B by the axial anomaly, no corrections 22

  23. What powers the CME current? Energy of µ R gluon field N CS = -2 -1 0 1 2 µ L − µ R = 2 ˙ θ µ L instanton sphaleron Right Left 49

  24. “Numerical evidence for chiral magnetic effect in lattice gauge theory” , P. Buividovich, M. Chernodub, E. Luschevskaya, M. Polikarpov, ArXiv 0907.0494; PRD’09 Red - positive charge Blue - negative charge

  25. “Chiral magnetic effect in 2+1 flavor QCD+QED” , M. Abramczyk, T. Blum, G. Petropoulos, R. Zhou, ArXiv 0911.1348; Red - positive charge Columbia-Bielefeld-RIKEN-BNL Blue - negative charge 2+1 flavor Domain Wall Fermions, fixed topological sectors, 16^3 x 8 lattice

  26. Charge asymmetry w.r.t. reaction plane as a signature of local strong P violation excess of positive charge + - excess of negative charge Electric dipole moment of QCD matter! DK, Phys.Lett.B633(2006)260 [hep-ph/0406125]

  27. Charge separation = parity violation: � � B B P - reflection P-odd B → � � L → � � � p → − � P : p ; B ; L

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  30. In Brookhaven Collider, Scientists Briefly Break a Law of Nature By DENNIS OVERBYE Published: February 15, 2010 Physicists said Monday that they had whacked a tiny region of space with enough energy to briefly distort the laws of physics, providing the first laboratory demonstration of the kind of process that scientists suspect has shaped cosmic history. Atom smasher shows vacuum of space in a twist Quark Soup 17:27 15 February 2010 by Rachel Courtland Physicists create conditions not seen since the big bang. Feb 16, 2010 Sharon Begley Scientists re-create high temperatures from Big Bang Hottest T emperature Ever Heads Science to Big Bang 30

  31. What are the implications for the Early Universe? 31 T.Hatsuda

  32. What is the origin of cosmic magnetic fields? Primordial magnetic field (E.Fermi, 1949)? Primordial magnetic field generation from P-odd effects at the QCD phase transition? Magnetic field in M51: Polarization of emission Beck 2000

  33. What is the origin of the matter-antimatter asymmetry in the Universe? 1. B violation 2. CP violation 3. Non-equilibrium A.D. Sakharov, dynamics 1967 Generation of Chern-Simons number at the QCD phase transition is analogous to baryon number generation in the electroweak phase transition: sphaleron 33 transitions are responsible for both

  34. Summary The existence of topological solutions is an indispensable property of non-Abelian gauge theories that form the Standard Model Local parity violation in the background magnetic field allows a direct observation of a topological effect in QCD The existence of the Chiral Magnetic Effect (CME) has been confirmed in first-principle lattice QCD calculations There is a recent observation of dynamical fluctuations in charge asymmetry at RHIC - an evidence for the CME 34

  35. Talks online at http://quark.phy.bnl.gov/~kharzeev/cpodd/ 35

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