[-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other...

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Baryon form factors in perturbative chiral quark model Xuyang Liu 1,2 , K. Khosonthongkee 2 , A. Limphirat 2 , Y. Yan 2 1. School of Mathematics and Physics, Bohai University 2. School of Physics, Suranaree University of Technology Xuyang Liu APFB 2017 August 25-30, 2017 1 / 20

Transcript of [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other...

Page 1: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Baryon form factors in perturbative chiral

quark model

Xuyang Liu1,2, K. Khosonthongkee2, A. Limphirat2, Y. Yan2

1. School of Mathematics and Physics, Bohai University2. School of Physics, Suranaree University of Technology

Xuyang Liu APFB 2017 August 25-30, 2017 1 / 20

Page 2: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

OUTLINE

Perturbative chiral quark model

EM and axial form factors

Sea-quark contributions

Neutron charge form factor

Summary & Outlook

Xuyang Liu APFB 2017 August 25-30, 2017 2 / 20

Page 3: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Perturbative chiral quark model

Perturbative chiral quark model (PCQM)

Linv(x) = ψ̄(x)[i∂/− γ0V (r)]ψ(x)︸ ︷︷ ︸Lq

+F 2

4Tr[∂µU∂

µU†]

︸ ︷︷ ︸LΦ

−ψ̄(x)S(r)

[U + U†

2+ γ5U − U†

2

]ψ(x)︸ ︷︷ ︸

Lint

Model potential

V (r) : vector potential, S(r) : scalar potential.

Model parameter

F = 88 MeV.

In SU(3) flavor symmetry

q− field : ψ(x) =

u(x)d(x)s(x)

, χ− field : U = exp

[iΦ̂

F

]' 1 + i

Φ̂

F+ o

(Φ̂

F

),

meson field : Φ̂ =

8∑i=1

Φiλi =

π0 + 1√3η

√2π+

√2K+

√2π− −π0 + 1√

3η√

2K0

√2K−

√2K̄0 − 2√

.

Xuyang Liu APFB 2017 August 25-30, 2017 3 / 20

Page 4: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Perturbative chiral quark model PCQM

Chiral symmetry

Linv(x) is invariant under the transformation

ψL → ULψL

ψR → URψR

U → URUU†L

where

ψL/R =1

2(1∓ γ5)ψ

UL = exp(− i

8∑a=1

ΘLa

λa2

)UR = exp

(− i

8∑a=1

ΘRa

λa2

)Xuyang Liu APFB 2017 August 25-30, 2017 4 / 20

Page 5: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Perturbative chiral quark model Previous works

Previous WorksPRC64 065203(2001); PRD63 054026(2001); PLB520 204(2001); PRC65 025202(2002); PRC66 055204(2002);PRC68 015205(2003); EPJA20 317(2004); JPG30 793(2004); JPG35 025005(2008).

V (r) and S(r) assumed being the harmonicoscillator interaction, and hence the valance quarkwave functions are in the Gaussian form.

Previous works includesElectromagnetic properties of baryonsLow-energy meson-baryon scatteringStrange nucleon form factorsElectromagnetic excitation of nucleon resonancesAxial form factor of the nucleon· · · · · ·

Xuyang Liu APFB 2017 August 25-30, 2017 5 / 20

Page 6: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Perturbative chiral quark model Feymann diagrams

Feymann Diagrams

Diagrams contributing to EM form factor

Diagrams contributing to axial form factor

Xuyang Liu APFB 2017 August 25-30, 2017 6 / 20

Page 7: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

EM and axial form factors Quark Wavefunction

Quark WavefunctionX. Y. Liu et al, J. Phys. G: Nucl. Part. Phys. 41 (2014) 055008.

Quark WF will be determined by fitting theoretical results of pcharge form factor to the experimental data.

The radial parts g(r) and f(r) are expanded in Sturmian basis

g(r) =∑n

AnSn0(r)

r,

f(r) =∑n

BnSn0(r),

where Sturmian functions

Snl =

[n!

(n+ 2l + 1)!

]1/2

(2br)l+1e−brL2l+1n (2br),

An, Bn, and b are free expansion parameters.Xuyang Liu APFB 2017 August 25-30, 2017 7 / 20

Page 8: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

EM and axial form factors EM form factors

Electromagnetic form factorsX. Y. Liu et al, J. Phys. G: Nucl. Part. Phys. 41 (2014) 055008.

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Xuyang Liu APFB 2017 August 25-30, 2017 8 / 20

Page 9: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

EM and axial form factors Axial form factors

Axial form factorsX. Y. Liu et al, Phys. Rev. D 91 (2015) 034022.

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Xuyang Liu APFB 2017 August 25-30, 2017 9 / 20

Page 10: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Sea-quark contributions Magnetic moments

π, K and η mesons contribute to the µB

Meson loopsπ K η

µp 0.281 0.002 −0.006

µn −0.339 0.018 0.004

µΣ+ 0.032 0.055 −0.008

µΣ0 −0.039 −0.062 −0.004

µΣ− −0.109 0.068 0

µΛ 0 −0.052 0.004

µΞ0 −0.008 −0.055 0.012

µΞ− −0.027 −0.058 0.010

Meson cloud contributing to EM form factors is about 10%.

π-meson dominates nucleon magnetic moments.

K-meson contributions to hyperons are in the same oder.

η-meson contributions are negligible.

Xuyang Liu APFB 2017 August 25-30, 2017 10 / 20

Page 11: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Sea-quark contributions Axial charge

π, K and η mesons contribute to the gBA

Meson loopsπ K η

gNA 0.375 0.045 −0.002gΣA 0.118 0.104 −0.002gΞA −0.030 −0.077 −0.001

Meson cloud contributing to axial form factor is about 30%

π-meson dominates nucleon axial charges.

K-meson contributions to hyperons axial charges are in thesame order as the π ones.

η-meson contributions are negligible.

Xuyang Liu APFB 2017 August 25-30, 2017 11 / 20

Page 12: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Sea-quark contributions EM and axial form factors

EM and axial form factorsX. Y. Liu et al, SciRep. 7, 8139 (2017)

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0.0 0.2 0.4 0.6 0.8 1.00.0

0.5

1.0

1.5

2.0

2.5

Q2(GeV2)

GMp(Q2)

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0.0 0.2 0.4 0.6 0.8 1.00.0

0.2

0.4

0.6

0.8

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Q2(GeV2)

GΑΝ(Q2)

Leading order (solid) and loop (dashed) contributions to the protonmagnetic (left panel) form factor and neutron axial (right panel)form factor.

Xuyang Liu APFB 2017 August 25-30, 2017 12 / 20

Page 13: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Sea-quark contributions EM and axial form factors

Meson cloud distributions

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r [fm]rρAN(r)

Comparisons between the LO and meson cloud distributions forproton magnetic (left panel) and axial (right panel) form factors inr-space.

Xuyang Liu APFB 2017 August 25-30, 2017 13 / 20

Page 14: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Sea-quark contributions Other results

Other results of meson cloud distributions

Shown as the dashed lines are the densities of nucleon chargecontributed by the pion cloud, taken from EPJA 17, 607 (2003).Left panel: r2ρ(r) for the electric form factor of the proton. Rightpanel: r2ρ(r) for the electric form factor of the neutron.

Xuyang Liu APFB 2017 August 25-30, 2017 14 / 20

Page 15: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Sea-quark contributions Other results

Other results of meson cloud distributions

The densities of charge and magnetization from the pion cloudtaken from PLB 586, 291 (2004). Left panel: 4πr2ρ(r) for theisovector Pauli (upper band) and Dirac (lower band) form factors.Right panel: 4πr2ρ(r) for the isovector magnetic (upper band) andelectric (lower band) Sachs form factors.

Xuyang Liu APFB 2017 August 25-30, 2017 15 / 20

Page 16: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Neutron charge form factor Wave functions of the valence quarks

Ground state wave functions of valence quarksX. Y. Liu et al, J. Phys. G: Nucl. Part. Phys. 41 (2014) 055008.

gHrLfHrL

0 2 4 6 8 10 12 140

0.02

0.04

0.06

0.08

0.1

0.12

0.14

r @GeV-1D

gHrL

and

fHrL

Normalized radial wave function of the valence quarks for the uppercomponent g(r) and the lower component f(r), which aredetermined by fitting the theoretical results of the proton chargeform factor to the experimental data.

Xuyang Liu APFB 2017 August 25-30, 2017 16 / 20

Page 17: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Neutron charge form factor Extracted PCQM potentials

Extracted PCQM potentialsX. Y. Liu et al, submitted to PRC

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0.0

0.5

1.0

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r [GeV-1 ]

Σ(r)[GeV

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r [GeV-1 ]Δ(r)[GeV

]

Δ(�)=�(�)-�(�)

The extracted PCQM potentials based on the predetermined groundstate quark wavefunction. Left panel: Σ(r) potential, right panel:∆(r) potential.

Xuyang Liu APFB 2017 August 25-30, 2017 17 / 20

Page 18: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Neutron charge form factor Diagrams contributing to neutron charge form factor

Diagrams contributing to neutron charge form factor

(a) (b)

(c) (d)

Diagrams contributing to the charge form factor of neutron: mesoncloud (a), vertex correction (b), self-energy I (c) and II (d).

Xuyang Liu APFB 2017 August 25-30, 2017 18 / 20

Page 19: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Neutron charge form factor Neutron charge form factor in PCQM

Neutron charge form factor

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Xuyang Liu APFB 2017 August 25-30, 2017 19 / 20

Page 20: [-0.2] Baryon form factors in perturbative chiral quark ... · Sea-quark contributions Other results Other results of meson cloud distributions Shown as the dashed lines are the densities

Neutron charge form factor Summary

Summary

Valence quark wave functions determined by fitting the PCQM result ofproton charge form factor dictate a Conrnell-like quark-quark potential.

Sea-quark contribution to EM form factors is about 10%.

Sea-quark contribution to axial form factors is about 30%.

Axial meson cloud is smaller than the EM one.

Axial meson cloud is smaller than the axial quark core.

Contributions of quark excited states in quark propagators areconsiderable to the charge form factor of neutron.

OutlookThe PCQM result of the neutron charge form factor is still much smallerthan the experimental values. The center-of-mass correction is beingconsidered.

Xuyang Liu APFB 2017 August 25-30, 2017 20 / 20