Anisotropic dilepton spectrum induced by chiral anomaly in strong magnetic fields

Post on 24-Feb-2016

51 views 0 download

description

Anisotropic dilepton spectrum induced by chiral anomaly in strong magnetic fields. In collaboration with Kaz . Itakura and Sho Ozak i. Koichi Hattori ( Yonsei Univ.) NFQCD@YITP, 12 th Dec. 2013. Possible signature of the early-time dynamics. Key ingredient 1: Strong fields . - PowerPoint PPT Presentation

Transcript of Anisotropic dilepton spectrum induced by chiral anomaly in strong magnetic fields

Anisotropic dilepton spectrum induced by chiral anomaly in strong magnetic fields

Koichi Hattori (Yonsei Univ.)NFQCD@YITP, 12th Dec. 2013

In collaboration with

Kaz. Itakura and Sho Ozaki

Key ingredient 1: Strong fields

Chromo electromagnetic fields Magnetic fields (QED)

Key ingredients 2: EM probes

Possible signature of the early-time dynamics

Penetrating probes porters carrying information of the early-time dynamics.

Possible effects of strong magnetic fields on 1. neutral pions related to dilepton spectra KH, K.Itakura, S.Ozaki, 20132. direct-photon propagations (vacuum polarization tensor) KH, K. Itakura (I) (II) 2013

Challenging on both theoretical and experimental sides!

Violation of axial current conservation

Absence of radiative correction Adler & Bardeen, 1960Triangle diagram gives the exact result in the all-order perturbation theory

Adler, Bell, Jackiw, 1959

Dominant (98.798 % in the vacuum)

99.996 %

``Dalitz decay ‘’ (1.198 % in the vacuum)

NLO contribution to the total decay rate Only corrections to external legs are possible

LO contribution to the total decay rate

Effects of external magnetic fields

Decay mode possible only in external field

“Bee decay” can be comparable to Dalitz decay and even π0 2γ, depending on B.

Replacement of a photon line by an external field

Decay width of “Bee decay”

WZW effective vertexπ0γ

Dalitz decay

Bee decay

Decay widths

Mean lifetime

femtometer

Branching ratios

Analytical modeling of colliding nuclei, Kharzeev, McLerran, Warringa, NPA (2008)

Pre-equilibrium

QGP

Strong magnetic fields in UrHIC

Event-by-event analysis, Deng, Huang (2012)

Au-Au 200AGeV b=10fm

Lifetime of B-field is shorter than the lifetime of neutral pions.

No chance to observe the new decay mode in the heavy-ion collisions.

Neutral-pion production from prompt γ* in strong B-fieldsPrompt γ* are produced in hard parton scatterings.

Gluon compton scattering in LO annihilation in LO

Without B-fields, mostly converted into dileptons.

+ Prompt photons are produced at the impacts of AA (pp, pA) collisions, so that converted into π0 in B-fields (and π0 decays outside B-fields).

Rapidly decaying B-field

π0γ*

Dilepton-production from γ* are suppressed.

A new neutral-pion production mechanism.

Given amount of γ*

Conversions of prompt γ* to pions in strong B-fieldsπ0 (only in B-fields)

Dileptons

Negative v2 of dileptons

Strong time-dependence of B-fields Energy transfer from B-fieldsLienard-Wiechert potentials Fourier componentTime-dependence

Dilepton yield in the presence of B-field Elliptically anisotropic pion productions

Summary in part 1

We investigated conversions between neutral pions and virtual photons in external magnetic fields.

+ A new decay channel “Bee decay” becomes possible, and becomes even the dominant decay mode in strong B-fields. Can be important in macroscopic systems such as the magnetars (neutron stars).

+ Oriented pion production from prompt virtual photon gives rise to a negative v2 of dileptons (and a positive v2 of neutral pions).

Photon propagations in strong magnetic fields

“Vacuum birefringence” and “real-photon decay”

What is “Birefringence” ?

Doubled image due to a ray-splitting in birefringent substances

Polarization 1Polarization 2

Incident light“Calcite” (方解石 )

Two polarization modes of a propagating photon have different refractive indices.

How about the vacuum with external magnetic fields ?

+ Lorentz & Gauge symmetries n ≠ 1 in general

+ Oriented response of the Dirac sea Vacuum birefringence

Modifications of photon propagations in strong B-fields

Magnetic field

QGP

Refraction of photon in the vacuum with B-fieldswithout medium effects

Real photon decay Dilepton emissions from real photon decay, as well as virtual photon conversions (γ* e+e- )

Could be important in pre-equilibrium stage,

and in QGP additively to medium effects

Photon vacuum polarization tensor:

Modified Maxwell eq. :

Dressed propagators in Furry’s picture

Break-down of naïve perturbation in strong magnetic fields

Naïve perturbation breaks down when B > Bc

Need to take into account all-order diagrams

Critical field strengthBc = me

2 / e

Dressed fermion propagator in Furry’s picture

In heavy ion collisions, B/Bc ~ O(104) >> 1

Resummation w.r.t. external legs by “proper-time method“ Schwinger

Nonlinear to strong external fields

Schwinger, Adler, Shabad, Urrutia, Tsai and Eber, Dittrich and Gies

Exponentiated trig-functions generate strongly oscillating behavior witharbitrarily high frequency.

Integrands having strong oscillations

Photon propagation in a constant external magnetic fieldLorentz and gauge symmetries lead to a tensor structure,

θ: angle btw B-field and photon propagation

B

Summary of relevant scales and preceding calculations

Ultrarelativistic heavy-ion collisions

Strong field limit: the lowest-Landau-level approximation(Tsai and Eber, Shabad, Fukushima )

Numerical computation below the first threshold(Kohri and Yamada) Weak field & soft photon limit

(Adler)

?Untouched so far

General analytic expression

Decomposition into a double infinite sum

Analytic results of integrals without any approximation

Polarization tensor acquires an imaginary part above

Every term results in either of three simple integrals.

Summary of relevant scales revisited- An infinite number of the Landau levels

(Photon momentum) Narrowly spaced Landau levels

Renormalization

+= ・・・+ +

Log divergence

Subtraction term-by-term

Ishikawa, Kimura, Shigaki, Tsuji (2013)

Taken from Ishikawa, et al. (2013)

Finite

Re Im

Complex refractive indices

The Lowest Landau Level (ℓ=n=0)

Dielectric constant at the LLL

Polarization excites only along the magnetic field``Vacuum birefringence’’

Solutions of Maxwell eq. with the vacuum polarization tensor

Self-consistent solutions of the modified Maxwell Eq.

Photon dispersion relation is strongly modified when strongly coupled to excitations (cf: exciton-polariton, etc)

cf: air n = 1.0003, water n = 1.333

𝜔2/4𝑚2

≈ Magnetar << UrHIC in RHIC and LHC

Angle dependence of the refractive indexReal part

No imaginary part

Imaginary part

Summary in 2nd part

We obtained the general analytic form of the resummed 1-loop polarization tensor in magnetic fields as the summation w.r.t. the Landau levels.

+ Confirmed to reproduce the preceding approximate calculations. Ishikawa, Kimura, Shigaki, Tsuji

+ We obtained the complex refractive indices (photon dispersions) by solving the modified Maxwell Eq.

+ Neutral pions and dileptonsClose look at phenomenology including competing effects.

+ Real photonsApplications of photon propagation to phenomenologies in the heavy-ion collisions and the magnetars (neutron stars).

Prospects

Branching of virtual prompt photon

q q2 Im

2 Im q q

Anisotropic on-shell pion production

Fourier component of an external field Anisotropic pion production

Isotropic dilepton production

Effective coupling between π0 and 2γ

(Rest frame)

Neutral pion decay into dilepton

Bext = (0,0,B), Eext = 0

EM current

q q

Neutral pion decay into dilepton (continued)

Decay rates in three modes Mean lifetime

Energy dependence of the decay rates

Field-strength dependence of the branching ratio

Angle dependence of the branching ratio Angle dependence of the lifetime

Primakoff effect

Recent measurement in JLab (2011)(PrimEX collaboration)

Prompt photon from hard parton scatterings

+ Prompt photons are produced at the moment of AA (pp, pA) collisions, so that they have much chance to interact with B-field.

Gluon compton scattering in LO annihilation in LO

Profiles of time-dependence magnetic fields

Time-dependence Fourier component

q0

π0

kq=q0+k

γ

Number of neutral pions increaseNumber of dilepton decrease

Elliptically anisotropic pion productions

Positive v2 of neutral pionsNegative v2 of dileptons

Neutral-pion production from prompt γ* in strong B-fields

Close look at the integrals

What dynamics is encoded in the scalar functions ?

An imaginary part representing a real photon decay

⇔⇔

Invariant mass of a fermion-pair in the Landau levels

Analytic representation of Pmn(q,B)

• Infinite summation w.r.t. n and l = summation over two Landau levels• Numerically confirmed by Ishikawa, et al. arXiv:1304.3655 [hep-ph]• couldn’t find the same results starting from propagators with Landau level decomposition

Dielectric constant at the lowest-Landau-level

Dielectric constant at the LLL

Polarization excites only along the magnetic field

ArcTan : source of an imaginary part above the lowest threshold

Angle dependence of the refractive index

Direction of arrow : direction of photon propagation

Norm of arrow : magnitude of the refraction index

Magnetic field

Shown as a deviation from unit circle

Complex refractive index

Br = (50,100,500,1000,5000,10000, 50000)

Real part of ε on stable branch

Imaginary part of ε on unstable branch

Real part of ε on unstable branch

Relation btw real and imaginary partson unstable branch