axial charge generation at strong coupling

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Axial charge generation at strong coupling Shu Lin RBRC I. Iatrakis, SL, Y. Yin 1405.XXXX

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Axial charge generation at strong coupling. Shu Lin RBRC. I. Iatrakis , SL, Y. Yin 1405.XXXX. Outline. Axial charge in electroweak theory and QCD Review of axial charge generation at weak coupling and strong coupling A close look at anomaly equation - PowerPoint PPT Presentation

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Page 1: Axial charge generation at strong coupling

Axial charge generation at strong coupling

Shu LinRBRC

I. Iatrakis, SL, Y. Yin 1405.XXXX

Page 2: Axial charge generation at strong coupling

Outline

• Axial charge in electroweak theory and QCD• Review of axial charge generation at weak coupling

and strong coupling• A close look at anomaly equation• Holographic realization of axial anomaly• Correlators of axial charge and topological charge

density at strong coupling• Dynamics of axial charge fluctuation• Conclusion

Page 3: Axial charge generation at strong coupling

Axial anomalies in natureAxial anomaly in Electroweak theory leads to baryogenesis

Axial anomaly in QCD leads to axial charge generation

]~')~(2[32

''222

FFgFFtrgN

j fB

)~(16 2

2

5

GGtr

Ngj fs

0~ ,0~ 2 GtrGGtrG

)~(16

)( 42

205

35 GGxtrd

NgxxjdtdQ fs

For QCD, axial charge is generated through

It averages to zero, but has nonvanishing fluctuations.

ΔQ5: important input to anomaly induced effects in HIC, such as chiral magnetic effect and chiral vortical effect.

Page 4: Axial charge generation at strong coupling

Sources of axial charge generation at weak coupling

Consider weakly coupled SU(N) gauge theory plasma, coupled to Nf flavors of quenched massless quarks

)~(16 2

2

5

GGtr

Ngj f

Nonperturbative contributions exponentially suppressed

instanton

sphaleronE

2#ge

However, at finite temperature, there are fluctuations of arbitrary size, turning the exponential suppression into a power law suppression.

Arnold, McLerran PRD 1987

Page 5: Axial charge generation at strong coupling

Perturbative generation of axial charge?

(e.g. parallel chromo-E and chromo-B field)?

)~(16 2

2

5

GGtr

Ngj f

Only topologically nontrivial field configurations contribute. Perturbative contribution should be excluded.

N. Christ, PRD 1980

Page 6: Axial charge generation at strong coupling

Bodeker’s effective theoryEffective theory at scale g2T and below

σ: conductivityζ: noise due to interaction with field above scale g2T

Bodeker, PLB 1998

Different scales in weakly coupled SU(N) gauge theoryT: temperature scalegT: electric screening scale, weakly coupledg2T: magnetic screening scale, strongly coupled

Page 7: Axial charge generation at strong coupling

Sphaleron rate from real time lattice simulation

24102

2

2

24

255

~#vol*time

1~)0(~16

)(~16

4))0()((

csph

sph

NTgGtrGgxGtrGgxd

VtQtQ

time ~ 1/(g4T), volume ~ 1/(g2T)^3

Arnold, Son, YaffeMoore, Tassler, JHEP 2011

Page 8: Axial charge generation at strong coupling

Sphaleron rate at strong coupling

43

24

256TNg c

sph

Son, Starinets, JHEP 2002

Sphaleron rate from non-perturbative contribution in both weak coupling and strong coupling.

Is nontrivial topology necessary?

time ~ 1/(gT), volume ~ 1/(gT)^3 ??

Page 9: Axial charge generation at strong coupling

A close look at anomaly equation)~(

16 2

2

5

FFtr

Nej f

Subtleties• Operator implicitly time ordered in the equation• Proof of the non-renormalization is done for matrix element at special

kinematics

Robustness• Equation not modified at finite temperature, chemical potential etc• Not renormalization by radiative correction

Adler, Bardeen, PR 1969Adler, 2004 review

Page 10: Axial charge generation at strong coupling

Anomaly for fully retarded correlator

For simplicity, consider response of axial charge to external electromagnetic field

fully retarded correlatorIn QED

vanishes identically when

nonvanishing when

Ordering of operators matters!

Page 11: Axial charge generation at strong coupling

ImplicationsWhat can’t generate axial charge• turning on E and B fields simultaneously

What can generate axial charge• turning on E field in a background B field (level crossing for

fermions in LLL)• exiciting nonperturbative field configuration, where operator

ordering doesn’t matter.

Nontrivial topology not a necessary condition for axial charge generation

Page 12: Axial charge generation at strong coupling

More questions

sphVtQtQ 4))0()(( 255

1. Does renormalization of gluons modify the anomaly equation for dynamical gluons?

2. The accumulation of net axial charge Q5 creates an chiral imbalance μ5, which disfavors further generation of Q5. When does the saturation of Q5 happen?

3. How does the accumulation of Q5 effect the dynamics of gluons?

4. What is more complete time evolution of fluctuations beyond linear growth?

Try to seek answer in a holographic model

Direct access to correlators of axial charge and topological charge density

Page 13: Axial charge generation at strong coupling

The Sakai-Sugimoto model (D4/D8)Nc D4 branes wrapped on S1 circle + Nf D8/anti D8 branes being a point on S1.

4+1D gluons 3+1D left/right handed quarks

Intrinsic mass scale 𝑀𝐾𝐾=1𝑅4

T T

Confined, chiral symmetry broken Deconfined, chiral symmetry restored

Sakai, Sugimoto, Prog.Theor.Phys, 2005

Aharony, Sonnenschein, Yankielowicz, Annal. Phys. 2006

Page 14: Axial charge generation at strong coupling

The deconfined backgroundS1 circle

Describe plasma of strongly coupled 4+1D gluons, and 3+1D quarks as defect.Dynamics determined by:

Set Nf=1

Aharony, Sonnenschein, Yankielowicz, Annal. Phys. 2006

Page 15: Axial charge generation at strong coupling

Holographic realization of axial anomaly

SDBI and SRR gauge invariantSWZ gauge invariant upto a boundary term

𝑆𝑊𝑍 (𝐹 ,𝐶7 )=𝑆𝑊𝑍 (𝐴 ,𝐶1 )

axial anomaly

AL/AR source JL/JR, θ sources topological charge density:

𝐽𝐿=𝛿𝑆𝛿 𝐴𝐿

; 𝐽 𝑅=𝛿𝑆𝛿 𝐴𝑅

; 116𝜋 2 𝑡𝑟𝐺

~𝐺=𝛿𝑆𝛿𝜃

as in YM action 𝑆=−𝑑4 𝑥 14𝑔2 𝑡𝑟𝐺𝐺+𝑑4 𝑥 𝜃

16𝜋2 𝑡𝑟𝐺~𝐺

Under flavor gauge transformation: )~(

16 2

2

5 GGtrgj

No renormalization yet!

Page 16: Axial charge generation at strong coupling

Nc counting of bulk fields and boundary correlators

𝐴𝑡 (𝜔 ) 1 ;𝐶7(𝜔) 𝑁𝑐

Consider fluctuations of and C7 at k=0 and arbitrary ω

To leading order in Nc

Page 17: Axial charge generation at strong coupling

Naive expectation from anomaly equation

can be verified by LO calculation

can’t be verified by LO calculation

Page 18: Axial charge generation at strong coupling

Holographic renormalization

U: holographic coordinate;U = corresponds to UVThe divergence in on-shell should be removed by counter terms, which are polynomial in

at order Nc

source

source

vev

vev

Page 19: Axial charge generation at strong coupling

Understanding anomaly equation

verified, disappointing result, maybe not surprising.

At strong coupling, all gluonic fluctuations are non-perturbative, operator ordering doesn’t matter.

Renormalization doesn’t change anomaly equation

?

Page 20: Axial charge generation at strong coupling

Extrapolation

not verified, but will be used to calculate

Page 21: Axial charge generation at strong coupling

Time evolution of

spectral density of 05j ⟨∆𝑄5(𝑡)2 ⟩=𝛿 ⟨∆𝑄5(𝑡)2 ⟩+ 4 𝜆3𝑇6

36 𝜋𝑀𝐾𝐾2 𝑉𝑡

long time limitSphaleron rate

correctionpole at the origin

Page 22: Axial charge generation at strong coupling

Speculated finite Nc pole structure2 𝐼𝑚𝐺𝑅 (𝜔 )=𝐺𝑅 (𝜔 )−𝐺𝐴 (𝜔 )

ωGR/GA has poles in the lower/upper half plane of ω

~ 1/Nc

It can be shown the pole contribution gives the Sphaleron rate.

Page 23: Axial charge generation at strong coupling

Effects invisible at large Nc1. Dissipation of axial charge:

2. Backreaction of axial charge to dynamics of gluon plasma, suppressed by Nf/Nc , need to consider backreaction of D8/anti D8 branes

Dissipation time scale ~ Nc/Nf →

Page 24: Axial charge generation at strong coupling

Conclusion

• We investigated the issue of operator ordering for anomaly equation in perturbative regime. Operator ordering does matters!

• We suggested nontrivial topology is not a necessary condition for axial charge generation.

• We verified the naive anomaly equation holds at leading order in Nc and strong coupling.

• We presented the full time evolution of axial charge fluctuation, and identified sphaleron rate only as long time behavior.

Page 25: Axial charge generation at strong coupling

Thank you!

Page 26: Axial charge generation at strong coupling

Sphaleron rate in Sakai-Sugimoto model

Γ h𝑠𝑝 =2𝜆3𝑇 6

36𝜋 𝑀𝐾𝐾2

Reminiscent of a 6D theory, from which SS model descents from

Craps, Hoyos, Surowka, Taels, JHEP 2012