Chiral Magnetic Effect

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    The chiral magnetic effect in stronglycoupledanisotropic plasma

    Ilmar Gahramanov

    DESY Hamburg, Germany

    Talk is based on

    I.G., Tigran Kalaydzhyan, Ingo Kirsch arXiv:1203.4259

    INTERNATIONAL SCHOOL OF SUBNUCLEAR PHYSICSErice, 25 June 2012

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    Motivation

    The chiral magnetic effect represents remarkable implications of anomalies in QFT

    The chiral magnetic effect is a good candidate for the explanationof an experimentally observed charge asymmetry in heavy-ioncollisions at RHIC

    Lattice QCD results suggest the existence of the effect

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    Chiral magnetic effect

    The CME is a hypothetical phenomenon which states that, in thepresence of a magnetic eld B , an electric current is generatedalong B in the background of topologically nontrivial gluon elds.

    j = C5 B [Kharzeev,Fukushima,Warringa,Mclerran]

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    Basics of relativistic hydrodynamics

    Hydrodynamics states is completely determined by conservation lawsassociated with some global symmetries

    T = 0 j = 0

    In equilibrium, for ideal hydrodynamics

    T = ( + P )u u

    P g

    j = u

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    build up of elliptic flow

    P T P L

    plasma phase mixed phase hadronic gas phase

    v

    0 2 4 6 8 10 12 fm0.00

    0.02

    0.04

    0.06

    0.08

    0.10

    0.12

    p

    Why the anisotropic case interesting?Experimental observation: The charge separation is proportionalto the elliptic ow v2 .

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    Anisotropic uidStress-energy tensor T and U (1) currents j :

    T = ( + P T )u u + P T g (P T P L )v v + j = u +

    In the rest frame

    T =

    0 0 00 P T 0 00 0 P T 00 0 0 P L

    In presence of anomalies one need to modify the dissipative part of the current

    j j + + B B

    These transport coefficients can be computed exactly.

    [Erdmenger,Haack,Kaminski,Yarom '08]

    [Son & Surowka '09]

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    In presence of external elds

    Now the energy-momentum tensor and current are not conserved

    T = F a j a j a = C abc E b B c

    2nd law of thermodynamicsPositivity of the entropy production completely xes new transportcoefficients

    = C 2 23 3

    + P T + O(T 2)

    B = C 12

    2

    + P T + O(T 2)

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    Two charge case

    Isotropic case [Sadofyev,Isachenkov 10] For an anisotropic case the conductivities

    = 2 C 5

    + P T 2 +

    253

    B = C 5 1

    + P T

    5 ,B = C 1 1

    2

    + P T

    1 +25

    3 2

    We expand the CME-coefficient B to linear order in p

    B C5 1 + P

    1 p16

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    Holographic principle

    Holographic principleAny theory of quantum gravity in (d + 1) dimensions has a dualdescription in terms of a QFT without gravity in d dimensions

    In its most familiar example, the AdS/CFT correspondence, thequantum theory of gravity is string theory on asymptotically AdSspace , and the theory on the boundary is a conformal eld theory .

    Hydrodynamic approximation

    Duality between the long wavelength asymptotically AdS planarblack hole solution of the EinsteinMaxwell theory with negativecosmological constant and the equations of charged uid dynamics

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    Gravity computation

    We start from a ve-dimensional U (1) n Einstein-Maxwell theory in anasymptotic AdS space

    S =1

    16G 5 d5x g[R 2 F

    aMN F

    aMN

    +S abc

    6 g PKLMN

    AaP F

    bKL F

    cMN

    information about triangle anomalies]

    Solution of the equations of motion: AdS black hole withU (1) V U (1) A

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    Gravity computationAn ansatz for an anisotropic AdS black hole solution

    ds2 =

    f (r )dt2 + 2 drdt + r 2(wT (r )dx2 + wT (r )dy2 + wL (r )dz2)

    Aa = Aa0 (r )dtAn asymptotic solution ( r )

    Aa

    0 (r ) = a +

    3q a2r 2 + O(r

    8

    ) wT (r ) = 1 +w(4)T r 4 + O(r

    8

    )

    f (r )/r 2 = 1 mr 4

    +a

    (q a )2

    r 6+ O(r

    8) wL (r ) = 1 +w(4)Lr 4

    + O(r 8)

    Transverse and longitudinal pressures

    P T =m 4w

    (4)T 4w

    (4)L

    16G 5=

    m(1 + )16G 5

    P L =m 8w

    (4)T

    16G 5=

    m(1 2 )16G 5

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    A roadmap of computation

    Vary 4-velocity and background elds up to rst order

    Solve equations of motion and nd the rst-order corrections Read off U (1) currents from the near-boundary expansion of the

    rst-order corrected background

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    Comparing apples to oranges

    024

    68

    101214161820

    0 2 4 6 8 10 12

    w L

    ( r +

    )

    anisotropy

    hydrodynamics

    holography, numerics

    Comparing

    j a =1

    16G 5 Qa (r + ) + r + A

    a0

    (r + )C

    with the general expansion

    j a = a u u + abB

    u

    Ab

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    The transport coefficients from gravity

    a =4

    16G 5S abc bc

    23

    a

    + P T S bcd bc d

    abB = 416G 5S abc c 12

    a

    + P T S bcd c d

    Vi ringrazio per lattenzione!

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