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Pion condensate versus chiral density wave at zero temperature - - PowerPoint PPT Presentation

Pion condensate versus chiral density wave at zero temperature Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) June 25, 2018 Strong and ElectroWeak Matter, Barcelona 2018 J. O. Andersen, P.


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Pion condensate versus chiral density wave at zero temperature

Patrick Kneschke (University of Stavanger)

in collaboration with Jens O. Andersen (NTNU Trondheim)

June 25, 2018 Strong and ElectroWeak Matter, Barcelona 2018

  • J. O. Andersen, P. Kneschke :

“Chiral density wave versus pion condensation at finite density and zero temperature”, Phys. Rev. D 97, 076005

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QCD at finite temperature and baryon chemical potential

  • hadronic matter at low energies (T, µB)
  • quark-gluon plasma at high energies
  • exotic phases at large chemical potential

− → inhomogeneous phases predicted around µB = 1 GeV possible

Fukushima et al. Rept.Prog.Phys. 74 (2011) 014001

The task is to find phase boundaries and critical points! Perturbative QCD breaks down at low energies Lattice QCD can be used to find the phase transition at µ = 0, but problematic at non zero chemical potential ⇒ sign problem (complex fermion determinant) Effective theories of QCD, that model chiral symmetry and/or confinement are used to map

  • ut the entire T − µB phase diagram

(Nambu-Jona-Lasinio model, quark meson model, chiral perturbation theory)

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 2

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QCD at finite temperature and isospin chemical potential

The isospin chemical potential µI introduces an imbalance between up- and down quarks. µu = µ + µI , µd = µ − µI At large enough densities bose condensation of charged pions is possible.

TΧ TΡ TBCS

50 100 150 50 100 150 200 ΜI MeV T MeV

  • only chiral condensate for small µI
  • pion condensate above µc

I = mπ 2

  • BEC-BCS crossover at large µI

No sign problem for isospin chemical potential ⇒ Lattice QCD works well and can be used for comparison with model calculations

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 3

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Pion condensation and inhomogeneous phase

Inhomogeneous chiral condensate: Cooper pair of quarks with non-zero net momentum q ⇒ complex order parameter ∆ei

q· x

For simplicity we consider a one-dimensional modulation ∆eiqz At finite temperature the order is destroyed by thermal fluctuations of phonons ⇒ map out the µ − µI phase diagram at zero temperature previous study in 1+1 dimensional NJL model showed pion and inhomogeneous condensate don’t coexist → We extend this to a 3+1 dimensional QM model

  • P. Adhikari, J.O. Andersen, Phys.Rev. D95 (2017), 054020

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 4

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SLIDE 5

Quark Meson Model

Lagrangian of the QM model in Minkowski space is:

  • π± =

1 √ 2 (π1 ± iπ2)

  • L = 1

2

  • (∂µσ)2 + (∂µπ3)2

+ (∂µ + 2iµI δµ,0) π− ∂µ − 2iµI δµ,0 π+ + 1 2 m2(σ2 + π2

3 + 2π+π−) + λ

24 (σ2 + π2

3 + 2π+π−)2 − hσ

+ ψf

  • i /

∂ + γ0(µ + µI τ3) − g(σ + iγ5 τ · π)

  • ψf

Replace the meson fields with constant background fields in mean field approximation. Chiral symmetry is broken by chiral condensate, here in the form of a chiral density wave (CDW): < σ >= φ0 cos(qz) , < π3 >= φ0 sin(qz) Allow for charged pion condensate: < π1 >= π0 , < π2 >= 0 Introducing the new variables ∆ = gφ0 and ρ = gπ0 we get the meson potential: V0 = 1 2 q2 ∆2 g2 + 1 2 m2 g2 ∆2 + 1 2 m2 − 4µ2

I

g2 ρ2 + 1 24 λ g4 (∆2 + ρ2)2 − h g ∆δq,0

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 5

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Quark Meson Model

In the large Nc limit we consider only quark corrections to the potential: V1 = − 1 βV log

  • det β /

D

  • Dirac operator:

/ D = i / ∂ + γ0(µ + µI τ3) − ∆ + 1

2 qτ3γ5γ3 − iργ5τ1

V1 = −Nc

  • f =u,d
  • p

1 2 E ±

f

+ 1 2 E ±

¯ f

+ T log

  • 1 + e−β(E±

f

−µ)

+ T log

  • 1 + e−β(E±

¯ f

+µ)

  • ,

with the quark energies: E ±

u = E(±q, −µI ) ,

E ±

d = E(±q, µI ) ,

E ±

¯ u = E(±q, µI ) ,

E ±

¯ d = E(±q, −µI )

E(q, µI ) =  

  • p2

⊥ +

  • p2

+ ∆2 + q

2 2 + µI 2 + ρ2   1 2

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 6

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SLIDE 7

On-shell Renormalization

  • The divergences of V1 are isolated using dimensional regularization d = 3 − 2ǫ :
  • p
  • p2 − M2 ∼ M4

1 ǫ + log Λ2 M2

  • + 3

2

  • The divergence is absorbed into the bare model parameters: m2 → m2

0 = m2 ren + δm2 etc.

  • We fix the model parameters to physical observables mσ, mπ, mq, fπ:

tree-level: m2 = − 1 2

  • m2

σ − 3m2 π

  • , λ = 3
  • m2

σ − m2 π

  • f 2

π

, h = m2

πfπ , g = mq

  • ne-loop: δm2 = − 1

2

  • δm2

σ − 3δm2 π

  • , δλ = 3
  • δm2

σ − δm2 π

  • f 2

π

− λ δf 2

π

f 2

π

δh = δmπfπ + h δfπ fπ , − δg2 g2 = δf 2

π

f 2

π

= δZπ , δmq = 0

  • OS renormalization constant from OS conditions:

Σσ,π

  • p2 = m2

σ,π

  • − δm2

σ,π = 0

⇒ m2

σ,π,ren = m2 σ,π is pole of the propagator

∂ ˆ Σσ,π ∂p2

  • p2 = m2

σ,π

  • + δZσ,π = 0

⇒ residue at the pole is one

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 7

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Parameter Fixing

  • ne-loop

m2

MS = m2 + 4g2Nc

(4π)2

  • m2 log Λ2

m2

q

− 2m2

q − 1

2

  • m2

σ − 4m2 q

  • F(m2

σ) + 3

2 m2

πF(m2 π)

  • ,

λMS = λ + 12g2Nc (4π)2f 2

π

  • mσ − 4m2

q

  • log Λ2

m2

q

+ F(m2

σ)

  • +m2

σ

  • log Λ2

m2

q

+ F(m2

π) + m2 πF ′(m2 π)

  • −m2

π

  • 2 log Λ2

m2

q

+ 2F(m2

π) + m2 πF ′(m2 π)

  • ,

g2

MS = g2

  • 1 + 4g2Nc

(4π)2

  • log Λ2

m2

q

+ F(m2

π) + m2 πF ′(m2 π)

  • ,

hMS = h

  • 1 + 2g2Nc

(4π)2

  • log Λ2

m2

q

+ F(m2

π) − m2 πF ′(m2 π)

  • V = 1

2 q2 ∆2 g2

MS

+ 1 2 m2

MS

∆2 g2

MS

+ 1 2

  • m2

MS − 4µ2 I

ρ2 g2

MS

+ λMS 24

  • ∆2 + ρ22

g4

MS

− hMS ∆ gMS δ0,q + Vfin

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 8

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Homogeneous Phase Diagram

We set q = 0 and choose mπ = 140 MeV , mσ = 600 MeV , mq = 300 MeV , fπ = 93 MeV

mq ΧSB 2nd order Ρ 1st order Ρ

100 200 300 400 50 100 150 200 Μ MeV ΜI MeV 50 100 150 200 50 100 150 200 250 300 ΜI MeV ,Ρ MeV 100 200 300 400 50 100 150 200 250 300 Μ MeV MeV 50 100 150 200 50 100 150 200 250 300 ΜI MeV ,Ρ MeV

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 9

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Onset of Pion Condensation

We determine the position of the phase transition with a Ginzburg-Landau Analysis: V = α0 + α2ρ2 + α4ρ4; V1 ≈ −2Nc

  • p
  • p2 + ∆2 ± µI + 1

2 ρ2

  • p2 + ∆2 ± µI

− 1 8 ρ4 (

  • p2 + ∆2 ± µI )3
  • Subtract expansion in µI to extract the finite part, divergent part already renormalized:

Vfin,2 = −2Ncρ2

  • p
  • p2 + ∆2

p2 + ∆2 − µI 2 − 1

  • p2 + ∆2 −

µ2

I

(p2 + ∆2)

3 2

  • = − 16Nc

(4π)2 ρ2µ2

I

  • 1 − s arctan

1 s

  • = − 8Ncρ2µ2

I

(4π)2 F(4µ2

I ),

Vfin,4 = 1 4 Ncρ4

  • p

   1

  • p2 + ∆2 ± µI

3 − 2 (p2 + ∆2)

3 2

   = 2Nc (4π)2 ρ4

  • 1

s2 + 1 s3

  • 3∆2

µ2

I

− 2

  • arctan

1 s

  • Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) ()

Pion condensate versus chiral density wave at zero temperature June 25, 2018 10

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Onset of Pion Condensation

Evaluated at the vacuum value ∆ = mq : α2 = 1 2 f 2

π

m2

q

  • m2

π

  • 1 −

4m2

qNc

(4π)2f 2

π

m2

πF ′(m2 π)

  • −4µ2

I

  • 1 −

4m2

qNc

(4π)2f 2

π

  • F(m2

π) + m2 πF ′(m2 π) − F(4µ2 I )

  • ,

α4 = 1 8 m2

σf 2 π

m4

q

  • 1 −

4m2

qNc

(4π)2f 2

π

  • 1 −

4m2

q

m2

σ

  • F(m2

σ) + F(m2 π) + m2 πF ′(m2 π)

  • − 1

8 m2

πf 2 π

m4

q

  • 1 −

4m2

qNc

(4π)2f 2

π

m2

πF ′(m2 π)

  • + 2Nc

(4π)2

  • 1

s2 + 1 s3

  • 3∆2

µ2

I

− 2

  • arctan

1 s

  • For ∆ = mq and µI = mπ

2 we get α2 = 0 and α4 > 0 ⇒ second order phase transition. This also applies for all µ < mq − mπ 2 (vacuum phase)

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 11

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Inhomogeneous Phase Diagram

pion mass dependence

The explicit symmetry breaking term: −hMS ∆ gMS δ0,q ∼ −m2

πfπ

∆ g δ0,q If the pion mass is to large, the homogeneous phase is always preferred. The width of the inhomogeneous phase decreases with increasing pion mass:

260 280 300 320 340 100 200 300 400 μ (MeV) Δ(MeV), q (MeV) 10 20 30 40 300 310 320 330 340 350 mΠMeV ΜMeV

A more general ansatz, like a chiral soliton lattice can save the inhomogeneous phase even at the physical point, but here we stay in the chiral limit.

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 12

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Inhomogeneous Phase Diagram

chiral limit

ΡΡ0 homogeneous inhomogeneous

260 280 300 320 340 50 100 150 ΜMeV ΜIMeV

50 100 150 200 100 200 300 400 ΜI MeV Ρ MeV 280 290 300 310 320 330 340 350 100 200 300 400 Μ MeV ,Ρ,q MeV 280 290 300 310 320 330 340 350 100 200 300 400 Μ MeV Ρ MeV

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 13

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Summary

We find the onset of pion condensation at exactly µI = mπ 2 for µ < mq − mπ 2 CDW only exists for small pion masses (and at zero temperature). No overlap between pion condensate and inhomogeneous condensate is found in the chiral limit. More sophisticated models, like a chiral soliton lattice should be studied. Extension to an inhomogeneous pion condensate possible in the future.

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 14

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Summary

We find the onset of pion condensation at exactly µI = mπ 2 for µ < mq − mπ 2 CDW only exists for small pion masses (and at zero temperature). No overlap between pion condensate and inhomogeneous condensate is found in the chiral limit. More sophisticated models, like a chiral soliton lattice should be studied. Extension to an inhomogeneous pion condensate possible in the future.

Thank you for your attention!

Patrick Kneschke (University of Stavanger) in collaboration with Jens O. Andersen (NTNU Trondheim) () Pion condensate versus chiral density wave at zero temperature June 25, 2018 14