Renormalisation flow in a Yukawa model with quadratic symmetry - - PowerPoint PPT Presentation

renormalisation flow in a yukawa model with quadratic
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Renormalisation flow in a Yukawa model with quadratic symmetry - - PowerPoint PPT Presentation

Renormalisation flow in a Yukawa model with quadratic symmetry breaking Istv an Kaposv ari, Antal Jakov ac and Andr as Patk os Institute of Physics, E otv os University, Budapest Outline: The model, its symmetries and


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SLIDE 1

Renormalisation flow in a Yukawa model with quadratic symmetry breaking

Istv´ an Kaposv´ ari, Antal Jakov´ ac and Andr´ as Patk´

  • s

Institute of Physics, E¨

  • tv¨
  • s University, Budapest

Outline:

  • The model, its symmetries and spectra

(Reminder of the Cakovec-2016 talk)

  • Spectra in Local Potential Approximation (LPA)

interpretation through RG-flow structure

  • Effect of the wavefunction renormalisation (LPA′):

adiabatic deformation of the LPA-flow

  • Conclusions
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SLIDE 2

The model Complex scalar and single Dirac-fermion with chiral Yukawa-interaction Φ = 1 √ 2(Φ1(x) + iΦ2(x)), ψR/L = 1 2(1 ± γ5)ψ. The symmetric part of the scale dependent action k < Λ: Γ(k)

SY M =

  • d4x
  • Zψ ¯

ψ/ ∂ψ + Zφ∂mΦ∗∂mΦ + Uk(Φ∗Φ) + hk( ¯ ψRψLΦ∗ + ¯ ψLψRΦ)

  • .

Symmetries: ψ → eiαψ, ¯ ψ → e−iα ¯ ψ Φ → Φ, U(1), ψ → eiγ5Θψ, ¯ ψ → ¯ ψeiγ5Θ, Φ → e−2iΘΦ, UA(1). UA(1): fermion mass-term can be generated only via non-zero Φ-condensate.

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SLIDE 3

Quadratic explicit breaking of UA(1) Γ(k)

ESB = Πk

  • p

[Φ(−p)Φ(p) + Φ∗(−p)Φ∗(p)]. Symmetry: U(1) × UA(1) → U(1) × Z(2) Πk : ΦΦ + Φ∗Φ∗k = 0 Superposition of oppositely charged condensates Spontaneous breaking: U (k)

INV = M 2 kΦ∗Φ + λk 6 (Φ∗Φ)2 → U (k) SSB = λk 6

  • Φ∗Φ − v2

k

2

2 Field expectation: Φ0 = Φ∗

0 = uk √ 2 → equations of the condensate:

  • M 2

k − 2|Πk| + λk 6 u2 k

  • uk

√ 2 = 0,

← INV

  • λk

6 (u2 k − v2 k) − 2|Πk|

  • uk

√ 2 = 0,

← SB

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SLIDE 4

Infrared spectrum of the scalar sector (k = 0) Denominator of the bosonic propagators: INV (u0 = 0, ψ = 0) ∆( Γ(2)

B ) = (q2 + M 2 0)2 − 4|Π0|2

→ m2

1 = M 2 0 − 2|Π0|,

m2

2 = M 2 0 + 2|Π0|

SB (u0 = 0, ψ = 0) ∆( Γ(2)

B ) =

  • q2 + λ0

3 v2 0 + 4|Π0|

  • (q2 + 4|Π0|)

→ m2

1 = λ0 3 v2 0 + 4|Π0| = λ0 3 u2 0,

m2

2 = 4|Π0|.

Separation of the symmetric and broken symmetry regions (critical surface): M 2

0 = 2|Π0|

→ m2

1 = 0, m2 2 = 4|Π0|

The masses m2

1 and m2 2 go continuously through the critical surface.

The second mass corresponds in the SB-phase to the pseudo-Goldstone field from the UA(1) breakdown. Fermion mass: mψ = hk=0

u0 √ 2

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SLIDE 5

Strategy for solving RGE Toy model of top-Higgs system with enlarged scalar sector: Is it possible to identify the PGB with the Higgs (mG = m2 = mHiggs)? How large can be made mhb/mG? How does influence ΠΛ the mhb/mG ratio? Strategy: Tune hΛ, M 2

Λ with fixed ΠΛ/M 2 Λ and λΛ

to get h0 = √ 2mtop uSM = 173 246, 8Π0 h2

0u2 SM

= m2

Higgs

m2

top

= 125 173 2 . Read out m2

G

m2

hb

= 3h2 2λ0 m2

Higgs

m2

top

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SLIDE 6

Wetterich RGE’s for the effective action I. symmetric phase ∂tM 2 = −2h2

  • q

ˆ ∂t 1 Z2

ψq2 R

+ 2λ 3

  • q

ˆ ∂t Zφq2

R + M 2

∆(q2

R)

, ∂tλ = 6h4

  • q

ˆ ∂t 1 Z4

ψq4 R

− λ2 3

  • q

ˆ ∂t 5(Zφq2

R + M 2)2 + 16|Π|2

∆2(q2

R)

, ∂th = h3Π

  • q

ˆ ∂t 1 Z2

ψq2 R∆(q2 R),

∂tΠ = −λΠ 3

  • q

ˆ ∂t 1 ∆(q2

R).

Note: Evolution of the Yukawa coupling is very slow with diminishing ΠΛ/M 2

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SLIDE 7

Wetterich RGE’s for the effective action II. broken symmetry phase 3 4∂tm2

G = −2h2 ˆ

∂t

  • q

1 Z2

ψq2 R + m2 ψ

+ λ 6 ˆ ∂t

  • q

4Zφq2

R + m2 hb + m2 G

∆(q2

R)

, ∂tm2

hb = 2h2 ˆ

∂t

  • q

−Z2

ψq2 R + m2 ψ

(Z2

ψq2 R + m2 ψ)2

+λ 6 ˆ ∂t

  • q

1 ∆(q2

R)

  • 4Zφq2

R + 7m2 hb + 3m2 G − m2 hb

∆(q2

R)

  • 4Zφq2

R + m2 hb + m2 G

2 , ∂th = −h3 2 (m2

hb − m2 G)ˆ

∂t

  • q

−Z2

ψq2 R + m2 ψ

(Z2

ψq2 R + m2 ψ)2∆(q2 R)

+ h3m2

hb

4 ˆ ∂t

  • q

1 Z2

ψq2 R + m2 ψ

  • 3

(Zφq2

R + m2 hb)2 −

1 (Zφq2

R + m2 G)2

  • .
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SLIDE 8

Wetterich RGE’s for the effective action III. broken symmetry phase ∂tλ = ∂F

t λ + ∂B t λ,

∆nm = δn+m∆ δΦnδΦ∗m 2 3∂F

t λ = 4h4 ˆ

∂t

  • p

G2

ψ[1 − 4m2 ψGψ + m4 ψG2 ψ],

2 3∂B

t λ = 1

2 ˆ ∂t

  • p
  • ∆22

∆ − 1 ∆2

  • 2∆12∆10 + 2∆21∆01 + 2∆2

11 + ∆20∆02

  • + 2

∆3

  • ∆20∆2

01 + ∆02∆2 10 + 4∆11∆10∆01

  • − 6∆2

10∆2 01

∆4

  • .

GG(q2

R) =

1 ZΦq2

R + m2 G

, Ghb(q2

R) =

1 ZΦq2

R + m2 hb

, Gψ = 1 Z2

ψq2 R + m2 ψ

, ∆ = GGGhb

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SLIDE 9

Phase structure and spectra in LPA, (ηψ = ηφ = 0)

  • 10
  • 8
  • 6
  • 4
  • 2

t 0.0001 0.0002 0.0003 0.0004 0.0005 0.0006

mhb2 Λ2 mG2 Λ2 mψ2 Λ2

|ΠΛ|/M 2

Λ = 0.01,

h ≡ hΛ

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SLIDE 10

Scalar mass ratio vs. ΠΛ/M 2

Λ

▲ ▲ ■ ■ ■ ◆ ◆ ◆ ★ ★ ★ ★

10-15 10-10 10-5

ΠΛ MΛ2

0.4 0.5 0.6 0.7

mG2 mhb2

  • λ=0.5, slope: 0.007184

▲ λ=0.8, slope: 0.0010221 ■ λ=0.94002 ◆ λ=1, slope: -0.0002739 ★ λ=1.4, slope: -0.000963

▲ ▲ ■ ■ ■ ◆ ◆ ★ ★

10-8 10-6 10-4 10-2

ΠΛ MΛ2

0.530 0.535 0.540 0.545 0.550 0.555 0.560

mG2 mhb2

  • λ=0.5

▲ λ=2 ■ λ=5 ◆ λ=8 ★ λ=13

hΛ ≈ 0.7 hΛ ≈ 3 Important observation: Scalar mass ratio apparently approaches a value insensitive to ΠΛ/M 2

Λ

Conjecture: λ(k = 0) for |ΠΛ|/M 2

Λ → 0 is a unique function of hΛ

What is behind this systematics observed from the numerical solution of the RGE’s?

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SLIDE 11

The RG-flow in the symmetric phase RGE’s of dimensionless couplings ∂tΠr + 2Πr = 4λrΠrvd 3 1 + M 2

r

((1 + M 2

r )2 − 4Π2 r)2,

∂tM 2

r + 2M 2 r = 4h2 rvd − 4λrvd

3 (1 + M 2

r )2 + 4Π2 r

((1 + M 2

r )2 − 4Π2 r)2,

∂tλr + (4 − d)λr = −24h4

rvd +

4λ2

rvd(1 + M 2 r )

3((1 + M 2

r )2 − 4Π2 r)3

  • 5(1 + M 2

r )2 + 52Π2 r

  • ,

∂thr + 1 2(4 − d)hr = − 2Πrh3

rvd

(1 + M 2

r )2 − 4Π2 r

  • 2(1 + M 2

r )

(1 + M 2

r )2 − 4Π2 r

+ 1

  • .

Fixed point solution in d = 4: λ∗2

UV

h4

UV

≈ 18 5 , M ∗2

r,UV

h2

UV

≈ 2v4

  • 1 −
  • 2

5

  • ,

Π∗

r,UV = 0,

v4 = (32π2)−1. With hΛ = 173/246 it suggests λ∗

UV ≈ 0.94.

Compare with λΛ belonging to the limiting m2

G/m2 hb ratio!

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SLIDE 12

The RG-flow in the symmetric phase

0.0000 0.0005 0.0010 0.0015 0.0020 0.0025 0.0030 0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 Mr2 λ

Two classes of trajectories: i) running into Landau-singularity, ii) running into instability separated by the renormalized trajectory ending in the fixed point. ∆t needed for the evolution in the broken phase is independent of ΠΛ. The smaller is ΠΛ the longer is the evolution along a flow-line in the symmetric phase.

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SLIDE 13

The RG-flow in the symmetric phase

10 20 30 40 50 60 0.0 0.5 1.0 1.5 log M2

Π 

λ

Fixed λΛ, M 2

Λ/ΠΛ → ∞ selects the renormalized trajectory

Predicts(!) m2

G/m2 hb ≈ 1.5

  • 5/18 × m2

G/m2 ψ (= 0.42 compare to figure!!)

Is this picture robust enough when one improves solutions of the RGE’s?

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SLIDE 14

Effect of wavefunction renormalisation (LPA′) ∂tΠr + (2 − ηφ)Πr = 4λrΠrv4 3 1 + M 2

r

((1 + M 2

r )2 − 4Π2 r)2

  • 1 − ηφ

6

  • ,

∂tM 2

r + (2 − ηφ)M 2 r = 4h2 rv4

  • 1 − ηψ

5

  • − 4λrv4

3 (1 + M 2

r )2 + 4Π2 r

((1 + M 2

r )2 − 4Π2 r)2

  • 1 − ηφ

6

  • ,

∂tλr − 2ηφλr = −24h4

rv4

  • 1 − ηψ

5

  • +

4λ2

rvd(1 + M 2 r )

3((1 + M 2

r )2 − 4Π2 r)3×

×

  • 5(1 + M 2

r )2 + 52Π2 r

1 − ηφ 6

  • ,

∂th2

r−(ηφ+2ηψ)h2 r = −

4Πrh4

rv4

(1 + M 2

r )2 − 4Π2 r

  • 2(1 + M 2

r )

(1 + M 2

r )2 − 4Π2 r

  • 1 − ηφ

6

  • + 1 − ηψ

5

  • .

Algebraic equations of the anomalous dimensions: ηψ = h2

rv4

(1 + M 2

r )2 + 4Π2 r

((1 + M 2

r )2 − 4Π2 r)2

  • 1 − ηφ

5

  • ,

ηφ = h2

rv4(4 − ηψ).

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SLIDE 15

Slow (logarithmic) variation of the Yukawa-coupling h h2

r(t) =

h2

r(t0)

1 − 2h2

r(t0)C(t − t0),

C ≈ v4

  • 4 +

2 1 + M ∗2

rUV

  • <

3 16π2

  • 0.002

0.000 0.002 0.004 0.006 0.008

  • 1

1 2 3 Mr

2

λ 0.000 0.001 0.002 0.003 0.004 0.005 0.0 0.5 1.0 1.5 2.0 Mr

2

λ

hr(t = −∞) = 0.7 Initial data (hrΛ, ΠrΛ) labels the points in the plane. ”Neutral” flow-line separates regions of RG-trajectories ending with instability and RG-trajectories ending with Landau-singularity LPA′-flow → adiabatic overlay of LPA flow patterns belonging to slowly varying hr(t)

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SLIDE 16

Slow (logarithmic) variation of the Yukawa-coupling h The ”neutral” flow-line represents adiabatic shift of the fixed-line of LPA.

  • 0.000

0.001 0.002 0.003 0.004 0.0 0.5 1.0 1.5 2.0 2.5 3.0 Mr

2

λ

No substantial change in the prediction for the scalar mass-ratio

▲ ▲ ■ ■ ■ ■ ■ ◆ ◆ ◆ ★ ★ ★ ★

▼ ▼ ▼ ▼ ▼ ▼

10-15 10-10 10-5

ΠΛ MΛ2

0.4 0.5 0.6 0.7

mG2 mhb2

  • λΛ=0.5

λΛ=0.8

λs=0.94 λs=0.94

λΛ=1

λΛ=1.4

LPA' λs'=0.96

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SLIDE 17

Conclusions Yukawa-models of general global symmetry can be constructed which possess – an LPA fixed line, parametrized by the Yukawa-coupling (invariant in LPA); – the improved (exact?) RG-evolution follows adiabatically the LPA fixed point structure, although no fixed point solution of the exact RGE’s exists. Specific to UL(1) × UR(1) symmetric model: Quadratic explicit symmetry breaking leads to unique prediction of m2

G/m2 hb,

as a function of m2

ψ/m2 G, when M 2 Λ/|ΠΛ| → ∞.