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Photon production induced by magnetic fields in HICs: photon yield and elliptic flow. Luis A. Hernandez September 11, 2017 Instituto de Ciencias Nucleares, UNAM. 1 / 23 Outline 1 Motivation 2 Production of s . 3 Results 4


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Photon production induced by magnetic fields in HICs: photon yield and elliptic flow.

Luis A. Hernandez September 11, 2017 Instituto de Ciencias Nucleares, UNAM.

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Outline

1 Motivation 2 Production of γ′s. 3 Results 4 Conclusion

2 / 23

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Motivation

Thermal photon puzzle.

J-F Paquet et al.,Phys. Rev. C 93, (2016) 044906

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SLIDE 4

Motivation

Thermal photon puzzle.

J-F Paquet et al.,Phys. Rev. C 93, (2016) 044906 3 / 23

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SLIDE 5

Motivation

Thermal photon puzzle.

J-F Paquet et al.,Phys. Rev. C 93, (2016) 044906

Data status of direct photons. Data/model comparisons. Excess at low pt. New processes to explain the excess.

3 / 23

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SLIDE 6

Motivation

Data vs Models 2014

  • O. Linnyk, E. L. Bratkovskaya and W. Cassing, Prog. Part. Nucl. Phys. 87

(2016) 50-115.

Transport model: O. Linnyk, E. L. Bratkovskaya and W. Cassing, Phys. Rev. C89, 034908 (2014). Fireball model: H. van Hees, C. Gale and R. Rapp, Phys. Rev. C84, 054906 (2011). Hydro model: C. Shen, U. W. Heinz, J.-F. Paquet and C. Gale, Phys. Rev. C89, 044910 (2014). 4 / 23

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Motivation

Update Data vs Models 2016

PHENIX compared to models.

  • C. Shen, arXiv:1601.02563.

5 / 23

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SLIDE 8

Motivation

Conditions for a new mechanism to pro- duce γ’s

By Chun Shen

We compute the production of prompt photons from the perturbative fusion of low momentum gluons coming from the shattered glasma.

6 / 23

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Motivation

Magnetic fields in HICs.

  • R. Snellings, J. Phys. 13, (2011) 055008
  • D. E. Kharzeev, L. D. McLerran and H. J. Warringa, Nucl. Phys. A

803, 227 (2008)

  • V. Voronyuk et al.,Phys. Rev. C 83, 054911

(2011)

  • V. Skokov, A. Y. Illarionov and V. Toneev,
  • Int. J. Mod. Phys. A 24, 5925 (2009)

7 / 23

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Motivation

Nonequilibrate gluons.

Over-occupied initial state called the glasma. Saturation effects → times of order τs ∼ 1/Λs Λs ≡ saturation scale. ∆τs ≃ 1 − 1.5fm

By Larry McLerran, ISMD2008 8 / 23

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Production of γ′s.

Photons from magnetic fields.

Trace anomaly converts energy-momentum of gluon bulk into photons.

  • G. Basar, D. Kharzeev and V. V.

Skokov, Phys. Rev. Lett. 109, 202303 (2012). Photon emission by quarks synchrotron radiation.

  • K. Tuchin, Phys. Rev. C91,

0124902 (2015).

9 / 23

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SLIDE 12

Production of γ′s.

Gluon fusion induced by eB

The quark propagator is written in its coordinate space representation as

S(x,x′)=Φ(x,x′)

  • d4p

(2π)4 e−ip·(x−x′)S(p) ,

where

Φ(x,x′)=exp{i|qf | x

x′ dξµ[Aµ+ 1 2 Fµν(ξ−x′)ν]},

the Schwinger phase factor.

10 / 23

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Production of γ′s.

Strong magnetic fields.

The translational invariant part of the propagator is written in terms of Landau levels, since the strength of the magnetic fields is dominant, therefore we consider the Lowest Landau Level (LLL) or at most the first Landau Level (1LL) SLLL(p) = −2ie

p2 ⊥ |qf B| p

p2

  • O+

,

S1LL(p) = e

p2 ⊥ |qf B|

p2

− 2|qf B|

  • pO+
  • 1 − 2p2

|qf B|

  • − pO−

+ 4p⊥

  • .

with O±

= [1 ± (sign(qf B))iγ1γ2] /2

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Production of γ′s.

Notation

B = B ˆ z. Vector potential Aµ = B

2 (0, −y, x, 0) (symmetric gauge).

⊥ ≡ (0, p1, p2, 0),

≡ (p0, 0, 0, p3),

p2

⊥ ≡ p2 1 + p2 2 and

p2

≡ p2 0 − p2 3,

therefore p2 = p2

− p2 ⊥.

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Production of γ′s.

The amplitude for the process.

  • M

= −

  • d4xd4yd4z
  • d4r

(2π)4 d4s (2π)4 d4t (2π)4 × e−it·(y−x)e−is·(x−z)e−ir·(z−y)e−ip·ze−ik·yeiq·x ×

  • Tr
  • iqf γαiS(s)igγµtciS(r)igγνtdiS(t)
  • +

Tr

  • iqf γαiS(t)igγνtdiS(r)igγµtciS(s)

× Φ(x, y)Φ(y, z)Φ(z, x)ǫµ(λp)ǫν(λk)ǫα(λq) Three steps. Compute:

1

Product of Schwinger phase factors/integrals over the space-time points.

2

Tensor structures.

3

Integrals over the momenta.

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Production of γ′s.

Computing process

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Production of γ′s.

Computing process

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Production of γ′s.

Computing process

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Production of γ′s.

Computing process

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Production of γ′s.

Computing process

to be continued...

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Production of γ′s.

Photon production probability.

1 4

  • pol

| M|2 = (2π)4δ(4) (q − k − p) Vτs 1 4

  • pol

|M|2,

Average over the initial gluons. Vτs is the space-time volume

Explicitly 1 4

  • pol

|M|2 = q2

f αemα2 s

(2π)ω2

q

  • ω2

p + 3ω2 k

  • q2

⊥ exp

q2

qf Bω2

q

  • ω2

p + ω2 k − ωpωk

  • .

We have already used that the produced photon needs to move in the original gluon’s direction. pµ = ωp(1, ˆ p) = (ωp/ωq) qµ, kµ = ωk(1, ˆ k) = (ωk/ωq) qµ.

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Production of γ′s.

Invariant photon momentum distribution.

ωq dNmag d3q = χV∆τs 2(2π)3

  • d3p

(2π)32ωp

  • d3k

(2π)32ωk n(ωp)n(ωk) × (2π)4δ(4) (q − k − p) 1 4

  • pol,f

|M|2.

Three flavours. n(ω), distribution of gluons. χ, overlap region (semicentral collision).

High occupation gluon number n(ω) = η eω/Λs − 1.

η high gluon occupation factor. Λs the saturation scale

We introduced a flow velocity factor, that is, ωp,k → (p, k) · u. With uµ = γ(1, β) and γ = 1/

  • 1 − β2

16 / 23

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Production of γ′s.

Elliptic flow coefficient

The azimuthal distribution with respect to the reaction plane can be given in terms of a Fourier decomposition as dNmag dφ = Nmag 2π

  • 1 +

  • i=1

2vn(ωq) cos(nφ)

  • ,

with total number of photons, Nmag is Nmag =

  • d3q

(2π)3 dNmag d3q Elliptic flow coefficient v2(ωq) =

dNmag dωq (ωq) v

mag

2

(ωq) + dNdirect

dωq (ωq) v direct 2

(ωq)

dNmag dωq (ωq) + dNdirect dωq (ωq)

,

17 / 23

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Results

γ’s invariant momentum distribution

Figure: Difference between PHENIX photon invariant momentum distribution [1] and direct (points) or direct minus prompt (zigzag) photons from [2] αs = 0.3, Λs = 2 GeV, η = 3, ∆τs = 1.5 fm, R = 7 fm, β = 0.25 and χ = 0.8

[1] A. Adare et al. [PHENIX Collaboration], Phys. Rev. C 91, 064904 (2015). [2] J.-F. Paquet, C. Shen, G. S. Denicol, M. Luzum, B. Schenke, S. Jeon, C. Gale, Phys. Rev. C 93, 044906 (2016). 18 / 23

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Results

γ’s invariant momentum distribution (β = 0)

Figure: Difference between PHENIX photon invariant momentum distribution [1] and direct (points) or direct minus prompt (zigzag) photons from [2]

[1] A. Adare et al. [PHENIX Collaboration], Phys. Rev. C 91, 064904 (2015). [2] J.-F. Paquet, C. Shen, G. S. Denicol, M. Luzum, B. Schenke, S. Jeon, C. Gale, Phys. Rev. C 93, 044906 (2016). 19 / 23

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Results

Coefficient v2

Figure: Harmonic coefficient v2, using the direct photon result of [1] together with

  • ur calculation, also compared to PHENIX data [2]

[1] J.-F. Paquet, C. Shen, G. S. Denicol, M. Luzum, B. Schenke, S. Jeon, C. Gale, Phys. Rev. C 93, 044906 (2016). [2] A. Adare et al. [PHENIX Collaboration], Phys. Rev. C 94, 064901 (2016). 20 / 23

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Results

Coefficient v2 (β = 0)

Figure: Harmonic coefficient v2, using the direct photon result of [1] together with

  • ur calculation, also compared to PHENIX [2]

[1] J.-F. Paquet, C. Shen, G. S. Denicol, M. Luzum, B. Schenke, S. Jeon, C. Gale, Phys. Rev. C 93, 044906 (2016). [2] A. Adare et al. [PHENIX Collaboration], Phys. Rev. C 94, 064901 (2016). 21 / 23

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Conclusion

Summary

In a semi-central HICs, a magnetic field of a large intensity is produced. When eB is the most intense are also the scales associated to the production

  • f a large number of small momentum gluons.

eB provides the mechanism to allow that gluons fuse and convert into photons in excess over other well studied mechanisms. eB also provides an initial asymmetry for the development of an azimuthal anisotropy quantified in terms of a substantial v2 (particularly at low photon momenta).

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Thank you!!! Enjoy your stay in Tlaxcala!!!

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