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Electric quadrupole form factors of singly heavy baryons with spin 3/2

June-Young Kim [email protected] Institut für Theoretische Physik II, Ruhr-Universität Bochum, D-44780 Bochum, Germany Department of Physics, Inha University, Incheon 22212, Republic of Korea    Hyun-Chul Kim [email protected] Department of Physics, Inha University, Incheon 22212, Republic of Korea School of Physics, Korea Institute for Advanced Study (KIAS), Seoul 02455, Republic of Korea
Abstract

We study the electromagnetic form factors of the lowest-lying singly heavy baryons in a pion mean-field approach, which is also known as the SU(3) chiral quark-soliton model. In the limit of the heavy-quark mass, the dynamics inside a singly heavy baryon is governed by the Nc1N_{c}-1 valence quarks, while the heavy quark remains as a mere static color source. In this framework, a singly heavy baryon is described by combining the colored soliton with the singly heavy quark. In the infinitely heavy-quark mass limit, we can compute the electric quadrupole form factors of the baryon sextet with spin 3/2 with the rotational 1/Nc1/N_{c} and linear corrections of the explicit flavor SU(3) symmetry breaking taken into account. We find that the sea-quark contributions or the Dirac-sea level contributions dominate over the valence-quark contributions in lower Q2Q^{2} region. We examined the effects of explicit flavor SU(3) symmetry breaking in detail. The numerical results are also compared with the recent data from the lattice calculation with the unphysical value of the pion mass considered, which was used in the lattice calculation.

Electromagnetic form factors of singly heavy baryons, pion mass dependence, the chiral quark-soliton model
preprint: INHA-NTG-05/2020

I Introduction

Conventional lowest-lying singly heavy baryons consist of a heavy quark and two light valence quarks. In the limit of the infinitely heavy-quark mass (mQm_{Q}\to\infty), the physics of singly heavy baryons becomes simple: The spin of the heavy quark 𝑱Q\bm{J}_{Q} is conserved in this limit and hence it leads also to the conservation of the spin of the light-quark degrees of freedom, i.e. 𝑱L=𝑱𝑱Q\bm{J}_{L}=\bm{J}-\bm{J}_{Q}. This is known as the heavy-quark spin symmetry Isgur:1989vq ; Georgi:1990um . In the mQm_{Q}\to\infty limit, we do not distinguish a charm quark from a bottom quark, which gives up heavy-quark flavor symmetry. On the other hand, chiral symmetry and its spontaneous breakdown still play an important part in describing the singly heavy baryons because of the presence of the light quarks inside a singly heavy baryon Yan:1992gz . Then the singly heavy baryons consisting of two light valence quarks can be represented in terms of irreducible representations of flavor SU(3) symmetry: 𝟑𝟑=𝟑¯𝟔\bm{3}\otimes\bm{3}=\bar{\bm{3}}\oplus\bm{6}, thus we have the two representations for the lowest-lying singly heavy baryons, i.e. the baryon antitriplet and sextet. The baryon antitriplet has the total spin J=1/2J=1/2 that comes from JQ=1/2J_{Q}=1/2 and JL=0J_{L}=0, whereas the baryon sextet can have either J=1/2J=1/2 or J=3/2J=3/2 with JL=1J_{L}=1 and JQ=1/2J_{Q}=1/2.

In a pion mean-field approach, which is also known as the SU(3) chiral quark-soliton model (χ\chiQSM), a singly heavy baryon can be viewed as the Nc1N_{c}-1 valence quarks bound by the pion mean fields that are created from the presence of the Nc1N_{c}-1 valence quarks Diakonov:2010tf ; Yang:2016qdz . In fact, this idea is taken from Witten’s seminal paper on baryons in the large NcN_{c} limit Witten:1979kh . This pion mean-field approach has successfully reproduced the mass spectra of the lowest-lying singly heavy baryons Yang:2016qdz and even explained the nontrivial isospin mass splittings of them Yang:2020klp . Interestingly, the corrections from the heavy quark mass are indeed negligible in the description of the isospin mass splittings of the singly heavy baryons as shown in Ref. Yang:2020klp , although they provide hyperfine interactions to remove the spin degeneracy of the baryon sextet.

Recently, the electromagnetic (EM) form factors of singly heavy baryons have been studied for the first time within lattice QCD Can:2013tna ; Can:2015exa . While there are no experimental data on the EM form factors of the singly heavy baryons to date, the results from the lattice calculation provide a clue to the internal structure of singly heavy baryons. Thus, it is also of great importance to investigate the EM form factors of the singly heavy baryons. In Ref. Kim:2018nqf ; Kim:2019wbg , we have studied the electric monopole and magnetic dipole form factors of the singly heavy baryons in detail, based on the χ\chiQSM. Since we consider the limit of the infinitely heavy-quark mass, there is no physical difference between the heavy baryons with spin 1/2 and those with 3/2 except for the value of the spin. On the other hand, the baryon sextet with spin 3/2 has yet another structure that arises from its higher spin, which is revealed by the electric quadrupole (E2E2) form factor. The E2E2 form factor of a baryon exhibits how the baryon is deformed. It is also known that the pion clouds play a significant role in understanding this deformation Pascalutsa:2006up . This will be also discussed in the present work. We will also examine the effects of flavor SU(3) symmetry breaking on the E2E2 form factors of the baryon sextet with spin 3/2. The numerical results for Ωc0\Omega_{c}^{*0} will be compared with that from the lattice calculation.

The present work is organized as follows: In Section II, we briefly recapitulate the general formalism for the electric quadrupole form factors within the framework of the chiral quark-soliton model. In Section III, we present the numerical results and discuss them in detail. The final Section is devoted to the summary and conclusion.

II Electric quadrupole form factors in the χ\chiQSM

We start with the EM current for a singly heavy baryon, which is defined by

Jμ(x)=ψ¯(x)γμ𝒬^ψ(x)+eQΨ¯γμΨ,\displaystyle J^{\mu}(x)=\bar{\psi}(x)\gamma^{\mu}\hat{\mathcal{Q}}\psi(x)+e_{Q}\bar{\Psi}\gamma^{\mu}\Psi, (1)

where ψ(x)\psi(x) stands for the light-quark field ψ=(u,d,s)\psi=(u,d,s) in SU(3) flavor space and Ψ\Psi denotes the heavy-quark field for the charmed or bottom quark. The charge operator 𝒬\mathcal{Q} is expressed as

𝒬^=(230001300013)=12(λ3+13λ8).\displaystyle\hat{\mathcal{Q}}=\begin{pmatrix}\frac{2}{3}&0&0\\ 0&-\frac{1}{3}&0\\ 0&0&-\frac{1}{3}\end{pmatrix}=\frac{1}{2}\left(\lambda_{3}+\frac{1}{\sqrt{3}}\lambda_{8}\right). (2)

The eQe_{Q} in the second term in Eq. (1) denotes the charge corresponding to a heavy quark, which has the value 2/32/3 for the charm quark and 1/3-1/3 for the bottom quark. The matrix element of JμJ^{\mu} between baryons with spin 3/2 can be parametrized in terms of four different real form factors as follows:

B(p,s)|Jμ(0)|B(p,s)\displaystyle\langle B(p^{\prime},s)|J^{\mu}(0)|B(p,s)\rangle =u¯α(p,s)[γμ{F1B(q2)ηαβ+F3B(q2)qαqβ4MB2}\displaystyle=-\overline{u}^{\alpha}(p^{\prime},s)\left[\gamma^{\mu}\left\{F^{B}_{1}(q^{2})\eta_{\alpha\beta}+F^{B}_{3}(q^{2})\frac{q_{\alpha}q_{\beta}}{4M_{B}^{2}}\right\}\right. (3)
+iσμνqν2MB{F2B(q2)ηαβ+F4B(q2)qαqβ4MB2}]uβ(p,s),\displaystyle\hskip 11.38092pt\left.+\;i\frac{\sigma^{\mu\nu}q_{\nu}}{2M_{B}}\left\{F^{B}_{2}(q^{2})\eta_{\alpha\beta}+F^{B}_{4}(q^{2})\frac{q_{\alpha}q_{\beta}}{4M_{B}^{2}}\right\}\right]{u}^{\beta}(p,s), (4)

where MBM_{B} denotes the mass of a singly heavy baryon in the baryon sextet with spin 3/2. The metric tensor ηαβ\eta_{\alpha\beta} of Minkowski space is defined as ηαβ=diag(1,1,1,1)\eta_{\alpha\beta}=\mathrm{diag}(1,\,-1,\,-1,\,-1). qαq_{\alpha} represents the momentum transfer qα=pαpαq_{\alpha}=p^{\prime}_{\alpha}-p_{\alpha} and its square is written as q2=Q2q^{2}=-Q^{2} with Q2>0Q^{2}>0. uα(p,s)u^{\alpha}(p,\,s) means the Rarita-Schwinger spinor for a singly heavy baryon with spin 3/2, carrying the momentum pp and the spin component ss projected along the direction of the momentum. σμν\sigma^{\mu\nu} designates the antisymmetric tensor σμν=i[γμ,γν]/2\sigma^{\mu\nu}=i[\gamma^{\mu},\,\gamma^{\nu}]/2. Note that when one takes the limit of the infinitely heavy quark mass (mQm_{Q}\to\infty), the heavy-quark current given in the second part of Eq. (1) can be safely neglected for the EM form factors. It gives only a constant contribution to the electric form factors as already shown in Ref. Kim:2018nqf .

It is more convenient to introduce the Sachs-type form factors or the multipole EM form factors, in particular, when the EM structure of a baryon with spin 3/2 is examined. The electric quadrupole form factor reveals how the shape of a baryon with spin 3/2 is deviated from the rotationally symmetric one. The Sachs-type form factors can be expressed in terms of FiBF_{i}^{B} given in Eq. (4)

GE0B(Q2)\displaystyle G_{E0}^{B}(Q^{2}) =(1+23τ)[F1B(Q2)τF2B(Q2)]13τ(1+τ)[F3B(Q2)τF4B(Q2)],\displaystyle=\left(1+\frac{2}{3}\tau\right)[F_{1}^{B}(Q^{2})-\tau F_{2}^{B}(Q^{2})]-\frac{1}{3}\tau(1+\tau)[F_{3}^{B}(Q^{2})-\tau F_{4}^{B}(Q^{2})], (5)
GE2B(Q2)\displaystyle G_{E{2}}^{B}(Q^{2}) =[F1(Q2)τF2(Q2)]12(1+τ)[F3(Q2)τF4(Q2)],\displaystyle=[F_{1}(Q^{2})-\tau F_{2}(Q^{2})]-\frac{1}{2}(1+\tau)[F_{3}(Q^{2})-\tau F_{4}(Q^{2})], (6)
GM1B(Q2)\displaystyle G_{M1}^{B}(Q^{2}) =(1+45τ)[F1B(Q2)+F2B(Q2)]25τ(1+τ)[F3B(Q2)+F4B(Q2)],\displaystyle=\left(1+\frac{4}{5}\tau\right)[F_{1}^{B}(Q^{2})+F_{2}^{B}(Q^{2})]-\frac{2}{5}\tau(1+\tau)[F_{3}^{B}(Q^{2})+F_{4}^{B}(Q^{2})], (7)
GM3B(Q2)\displaystyle G_{M3}^{B}(Q^{2}) =[F1B(Q2)+F2B(Q2)]12(1+τ)[F3B(Q2)+F4B(Q2)],\displaystyle=[F_{1}^{B}(Q^{2})+F_{2}^{B}(Q^{2})]-\frac{1}{2}(1+\tau)[F_{3}^{B}(Q^{2})+F_{4}^{B}(Q^{2})], (8)

where τ=Q2/4MB2\tau=Q^{2}/4M_{B}^{2}. Since GE0BG_{E0}^{B}, GM1BG_{M1}^{B} have been already investigated in Ref. Kim:2018nqf , we will focus on the electric quadrupole form factors of the baryon sextet with spin 3/2, i.e., GE2BG_{E2}^{B} in the present work. At Q2=0Q^{2}=0, GE2(0)G_{E2}(0) yields the electric quadrupole moment

𝒬B\displaystyle\mathcal{Q}_{B} =eMB2GE2B(0)=eMB2[eB12F3B(0)],\displaystyle=\frac{e}{M_{B}^{2}}G_{E2}^{B}(0)=\frac{e}{M_{B}^{2}}\left[e_{B}-\frac{1}{2}F_{3}^{B}(0)\right], (9)

which reveals how much the charge distribution of a baryon is deformed from a spherical shape. If 𝒬B\mathcal{Q}_{B} has a negative value (𝒬B<0\mathcal{Q}_{B}<0), then the baryon takes a cushion shape, whereas if 𝒬B\mathcal{Q}_{B} is positive (𝒬B>0\mathcal{Q}_{B}>0), then it looks like a rugby-ball shape.

We want to mention that the M3M3 form factors vanish in the present work. In fact, any chiral solitonic approaches yield the null results of the M3M3 form factors because of the hedgehog structure Kim:2019gka . However, the experimental data on M3M3 is absent to date and its value should be very tiny even if it is measured. In fact, one could compute the M3M3 form factors if one takes into account the next-to-next-to-leading order in the 1/Nc1/N_{c} expansion. This means that the M3M3 form factors should be strongly suppressed in the large NcN_{c} limit. Thus, we will focus in the present work on the E2E2 form factors of the baryon sextet with spin 3/2.

The SU(3) χ\chiQSM is constructed based on the following low-energy effective partition function in Euclidean space, defined by

𝒵χQSM=𝒟ψ𝒟ψ𝒟Uexp[d4xψD(U)ψ]=𝒟Uexp(Seff),\displaystyle\mathcal{Z}_{\chi\mathrm{QSM}}=\int\mathcal{D}\psi\mathcal{D}\psi^{\dagger}\mathcal{D}U\exp\left[-\int d^{4}x\psi^{\dagger}D(U)\psi\right]=\int\mathcal{D}U\exp(-S_{\mathrm{eff}}), (10)

where ψ\psi and UU denote respectively the quark and pseudo-Nambu-Goldstone boson fields. Having integrated over quark fields, we can express the partition function in terms of the effective chiral action SeffS_{\mathrm{eff}}, which is defined by

Seff(U)=NcTrln(i/+iMUγ5+im^),\displaystyle S_{\mathrm{eff}}(U)\;=\;-N_{c}\mathrm{Tr}\ln(i\hbox to0.0pt{/\hss}{\partial}+iMU^{\gamma_{5}}+i\hat{m})\,, (11)

where Tr\mathrm{Tr} represents the functional trace running over spacetime and all relevant internal spaces. The NcN_{c} denotes the number of colors. MM is the dynamical quark mass that arises from spontaneous symmetry breaking of chiral symmetry. Uγ5U^{\gamma_{5}} represents the chiral field that consists of the pseudo-Nambu-Goldstone (pNG) fields πa\pi^{a}, a=1,8a=1,\cdots 8, which is expressed as

Uγ5=exp(iγ5πaλa)=1+γ52U+1γ52U\displaystyle U^{\gamma_{5}}=\exp(i\gamma_{5}\pi^{a}\lambda^{a})=\frac{1+\gamma_{5}}{2}U+\frac{1-\gamma_{5}}{2}U^{\dagger} (12)

with

U=exp(iπaλa).\displaystyle U=\exp(i\pi^{a}\lambda^{a}). (13)

We assume isospin symmetry, i.e., mu=mdm_{\mathrm{u}}=m_{\mathrm{d}}. The average mass of the up and down quarks is defined by m¯=(mu+md)/2\overline{m}=(m_{\mathrm{u}}+m_{\mathrm{d}})/2. Then, the matrix of the current quark masses is written as m^=diag(m¯,m¯,ms)=m¯+δm\hat{m}=\mathrm{diag}(\overline{m},\,\overline{m},\,m_{\mathrm{s}})=\overline{m}+\delta m. δm\delta m is written as

δm=m¯+ms3𝟏+m¯ms3λ8=m1𝟏+m8λ8,\displaystyle\delta m\;=\;\frac{-\overline{m}+m_{s}}{3}\bm{1}+\frac{\overline{m}-m_{s}}{\sqrt{3}}\lambda^{8}=m_{1}\bm{1}+m_{8}\lambda^{8}\,, (14)

where m1m_{1} and m8m_{8} denote the singlet and octet components of the current quark masses, defined by m1=(m¯+ms)/3m_{1}=(-\overline{m}+m_{\mathrm{s}})/3 and m8=(m¯ms)/3m_{8}=(\overline{m}-m_{\mathrm{s}})/\sqrt{3}, respectively. The single-quark Hamiltonian h(U)h(U) is defined by

h(U)=iγ4γiiγ4MUγ5γ4m¯.\displaystyle h(U)\;=\;i\gamma_{4}\gamma_{i}\partial_{i}-\gamma_{4}MU^{\gamma_{5}}-\gamma_{4}\overline{m}\,. (15)

Since the pion field has flavor indices, one has to combine a minimal symmetric ansatz will be the hedgehog ansatz with which the flavor indices can be coupled to three-dimensional spatial axes. The pion fields are then expressed in terms of a single function P(r)P(r), which is called the profile function, as follows

πa(𝒙)=naP(r)\displaystyle\pi^{a}(\bm{x})=n^{a}P(r) (16)

with na=xa/rn^{a}=x^{a}/r. Then the SU(2) chiral field is written as

USU(2)γ5=exp(iγ5𝒏^𝝉P(r))=1+γ52USU(2)+1γ52USU(2)\displaystyle U_{\mathrm{SU(2)}}^{\gamma_{5}}\;=\;\exp(i\gamma^{5}\hat{\bm{n}}\cdot\bm{\tau}P(r))\;=\;\frac{1+\gamma^{5}}{2}U_{\mathrm{SU(2)}}+\frac{1-\gamma^{5}}{2}U_{\mathrm{SU(2)}}^{\dagger} (17)

with USU(2)=exp(i𝒏^𝝉P(r))U_{\mathrm{SU(2)}}=\exp(i\hat{\bm{n}}\cdot\bm{\tau}P(r)). The SU(3) chiral field can be constructed by Witten’s trivial embedding Witten:1983tx

Uγ5(x)=(USU(2)γ5(x)001),\displaystyle U^{\gamma_{5}}(x)\;=\;\left(\begin{array}[]{lr}U_{\mathrm{SU(2)}}^{\gamma_{5}}(x)&0\\ 0&1\end{array}\right), (20)

which preserves the hedgehog ansatz.

Integration over UU in Eq. (10) quantizes the pNG fields. In the large NcN_{c} limit, the meson mean-field approximation is justified Witten:1979kh ; Witten:1983tx . Thus, we can carry out the integration over UU in Eq. (10) around the saddle point, where δSeff/δP(r)=0\delta S_{\mathrm{eff}}/\delta P(r)=0 is satisfied. This saddle-point approximation yields the equation of motion that can be solved self-consistently. The solution provides the self-consistent profile function Pc(r)P_{c}(r) of the chiral soliton. A detailed method of the self-consistent procedure can be found in Ref. Christov:1995vm .

While the quantum fluctuations of the self-consistent pion fields can be ignored by the large NcN_{c} argument, the fluctuations along the direction of both the rotational and translational zero modes cannot be ignored, since they are not at all small. Note that rotational and translational zero modes are related to rotational and translational symmetries. Thus, the zero modes can be taken into account by the following rotational and translational transformations

U~(𝒙,t)=A(t)U[𝒙𝒁(t)]A,\displaystyle\tilde{U}(\bm{x},t)=A(t)U[\bm{x}-\bm{Z}(t)]A^{\dagger}, (21)

where A(t)A(t) is an SU(3) unitary matrix. So, the functional integral over UU can be approximated by those over zero modes

DU[]DAD𝒁[].\displaystyle\int DU[\cdots]\approx\int DAD\bm{Z}[\cdots]. (22)

The integration over translational zero modes will naturally give the Fourier transform of the EM densities. We refer to Ref. Kim:1995mr for a detailed description of the zero-mode quantization in the present scheme.

Having carried out the zero-mode quantization, we obtain the collective Hamiltonian as

Hcoll=Hsym+Hsb,\displaystyle H_{\mathrm{coll}}=H_{\mathrm{sym}}+H_{\mathrm{sb}}, (23)

where

Hsym\displaystyle H_{\mathrm{sym}} =Mcl+12I1i=13Ji2+12I2p=47Jp2,Hsb=αD88(8)+βY^+γ3i=13D8i(8)J^i.\displaystyle=M_{\mathrm{cl}}+\frac{1}{2I_{1}}\sum_{i=1}^{3}J_{i}^{2}+\frac{1}{2I_{2}}\sum_{p=4}^{7}J_{p}^{2},\;\;\;H_{\mathrm{sb}}=\alpha D_{88}^{(8)}+\beta\hat{Y}+\frac{\gamma}{\sqrt{3}}\sum_{i=1}^{3}D_{8i}^{(8)}\hat{J}_{i}. (24)

I1I_{1} and I2I_{2} denote the moments of inertia for the soliton, of which the explicit expressions can be found in Appendix A. The parameters α\alpha, β\beta, and γ\gamma for heavy baryons arise from the breaking of flavor SU(3) symmetry, which are defined by

α=(Σ¯πN3m0+K2I2Y¯)ms,β=K2I2ms,γ=2(K1I1K2I2)ms.\displaystyle\alpha=\left(-\frac{\overline{\Sigma}_{\pi N}}{3m_{0}}+\frac{K_{2}}{I_{2}}\overline{Y}\right)m_{\mathrm{s}},\;\;\;\beta=-\frac{K_{2}}{I_{2}}m_{\mathrm{s}},\;\;\;\gamma=2\left(\frac{K_{1}}{I_{1}}-\frac{K_{2}}{I_{2}}\right)m_{\mathrm{s}}. (25)

where K1, 2K_{1,\,2} are the anomalous moments of inertia, of which the expressions are found in Appendix A. Note that the number of light valence quarks for a singly heavy baryon is Nc1N_{c}-1. This means that the expression for the valence part of Σ¯πN\overline{\Sigma}_{\pi N} contains also Nc1N_{c}-1 in place of NcN_{c}. It can be related to the πN\pi N sigma term as follows: Σ¯πN=(Nc1)Nc1ΣπN\overline{\Sigma}_{\pi N}=(N_{c}-1)N_{c}^{-1}\Sigma_{\pi N}. The detailed expressions for the moments of inertia and Σ¯πN\overline{\Sigma}_{\pi N} are given in Ref. Kim:2018xlc .

The presence of the symmetry-breaking part in the collective Hamiltonian, HsbH_{\mathrm{sb}}, have the baryon wavefunctions mixed with those in higher SU(3) representations. In the present case, the collective wavefunctions for the baryon antitriplet (J=0J=0) and the sextet (J=1J=1) are obtained respectively as Kim:2018xlc

|B𝟑¯0=|𝟑¯0,B+p15¯B|𝟏𝟓¯0,B,|B𝟔1=|𝟔1,B+q15¯B|𝟏𝟓¯1,B+q24¯B|𝟐𝟒¯1,B,\displaystyle|B_{\overline{\bm{3}}_{0}}\rangle=|\overline{\bm{3}}_{0},B\rangle+p^{B}_{\overline{15}}|\overline{\bm{15}}_{0},B\rangle,\;\;\;|B_{\bm{6}_{1}}\rangle=|{\bm{6}}_{1},B\rangle+q^{B}_{\overline{15}}|{\overline{\bm{15}}}_{1},B\rangle+q^{B}_{\overline{24}}|{{\overline{\bm{24}}}_{1}},B\rangle, (26)

with the mixing coefficients

p15¯B=p15¯[15/1035/20],\displaystyle p_{\overline{15}}^{B}\;\;=\;\;p_{\overline{15}}\left[\begin{array}[]{c}-\sqrt{15}/10\\ -3\sqrt{5}/20\end{array}\right], q15¯B=q15¯[5/530/200],\displaystyle q_{\overline{15}}^{B}\;\;=\;\;q_{\overline{15}}\left[\begin{array}[]{c}\sqrt{5}/5\\ \sqrt{30}/20\\ 0\end{array}\right], q24¯B=q24¯[10/1015/1015/10],\displaystyle q_{\overline{24}}^{B}\;\;=\;\;q_{\overline{24}}\left[\begin{array}[]{c}-\sqrt{10}/10\\ -\sqrt{15}/10\\ -\sqrt{15}/10\end{array}\right], (35)

in the basis [ΛQ,ΞQ]\left[\Lambda_{Q},\;\Xi_{Q}\right] for the antitriplet and [ΣQ,ΞQ,ΩQ]\left[\Sigma_{Q},\;\Xi_{Q}^{\prime},\;\Omega_{Q}\right] for the sextets with both spin 1/2 and 3/2. The parameters p15¯p_{\overline{15}}, q15¯q_{\overline{15}}, and q24¯q_{\overline{24}} are explicitly written as

p15¯=343αI2,\displaystyle p_{\overline{15}}\;\;=\;\;\frac{3}{4\sqrt{3}}\alpha{I}_{2}, q15¯=12(α+23γ)I2,\displaystyle q_{\overline{15}}\;\;=\;\;{\displaystyle-\frac{1}{\sqrt{2}}}\left(\alpha+\frac{2}{3}\gamma\right){I}_{2}, q24¯=4510(α13γ)I2.\displaystyle q_{\overline{24}}\;\;=\;\;\frac{4}{5\sqrt{10}}\left(\alpha-\frac{1}{3}\gamma\right)I_{2}. (36)

The collective wavefunction for the soliton with (Nc1)(N_{c}-1) valence quarks is then obtained in terms of the SU(3) Wigner DD functions

ψ(ν;F),(ν¯;S¯)(R)=dim(ν)(1)QS[DFS(ν)(R)],\displaystyle\psi_{(\nu;\,F),(\overline{\nu};\,\overline{S})}(R)=\sqrt{\mathrm{dim}(\nu)}(-1)^{Q_{S}}[D_{F\,S}^{(\nu)}(R)]^{*}, (37)

where dim(ν)\mathrm{dim}(\nu) represents the dimension of the representation ν\nu and QSQ_{S} a charge corresponding to the soliton state SS, i.e., QS=J3+Y/2Q_{S}=J_{3}+Y^{\prime}/2. FF and SS stand for the flavor and spin quantum numbers corresponding to the soliton for the singly heavy baryon. Finally, the complete wavefunction for a singly heavy baryon can be derived by coupling the soliton wavefunction to the heavy quark spinor

ΨBQ()(R)=J3,JQ3CJ,J3JQJQ3JJ3χJQ3ψ(ν;Y,T,T3)(ν¯;Y,J,J3)(R),\displaystyle\Psi_{B_{Q}}^{(\mathcal{R})}(R)=\sum_{J_{3},\,J_{Q3}}C_{\,J,J_{3}\,J_{Q}\,J_{Q3}}^{J^{\prime}\,J_{3}^{\prime}}\;\mathbf{\chi}_{J_{Q3}}\;\psi_{(\nu;\,Y,\,T,\,T_{3})(\overline{\nu};\,Y^{\prime},\,J,\,J_{3})}(R), (38)

where χJQ3\chi_{J_{Q3}} denote the Pauli spinors for the heavy quark and CJ,J3JQJQ3JJ3C_{\,J,J_{3}\,J_{Q}\,J_{Q3}}^{J^{\prime}\,J_{3}^{\prime}} the Clebsch-Gordan coefficients.

The matrix elements of the EM current (4) can be computed within the χ\chiQSM by representing them in terms of the functional integral in Euclidean space,

B,p|Jμ(0)|B,p\displaystyle\langle B,\,p^{\prime}|J_{\mu}(0)|B,\,p\rangle =1𝒵limTexp(ip4T2ip4T2)d3xd3yexp(i𝒑𝒚+i𝒑𝒙)\displaystyle=\frac{1}{\mathcal{Z}}\lim_{T\to\infty}\exp\left(ip_{4}\frac{T}{2}-ip_{4}^{\prime}\frac{T}{2}\right)\int d^{3}xd^{3}y\exp(-i\bm{p}^{\prime}\cdot\bm{y}+i\bm{p}\cdot\bm{x}) (39)
×𝒟U𝒟ψ𝒟ψJB(𝒚,T/2)ψ(0)γ4γμQ^ψ(0)JB(𝒙,T/2)exp[d4zψiD(U)ψ],\displaystyle\times\int\mathcal{D}U\int\mathcal{D}\psi\int\mathcal{D}\psi^{\dagger}J_{B}(\bm{y},\,T/2)\psi^{\dagger}(0)\gamma_{4}\gamma_{\mu}\hat{Q}\psi(0)J_{B}^{\dagger}(\bm{x},\,-T/2)\exp\left[-\int d^{4}z\psi^{\dagger}iD(U)\psi\right], (40)

where the baryon states |B,p|B,\,p\rangle and B,p|\langle B,\,p^{\prime}| are, respectively, defined by

|B,p\displaystyle|B,\,p\rangle =limx4exp(ip4x4)1𝒵d3xexp(i𝒑𝒙)JB(𝒙,x4)|0,\displaystyle=\lim_{x_{4}\to-\infty}\exp(ip_{4}x_{4})\frac{1}{\sqrt{\mathcal{Z}}}\int d^{3}x\exp(i\bm{p}\cdot\bm{x})J_{B}^{\dagger}(\bm{x},\,x_{4})|0\rangle, (41)
B,p|\displaystyle\langle B,\,p^{\prime}| =limy4exp(ip4y4)1𝒵d3yexp(i𝒑𝒚)0|JB(𝒚,y4).\displaystyle=\lim_{y_{4}\to\infty}\exp(-ip_{4}^{\prime}y_{4})\frac{1}{\sqrt{\mathcal{Z}}}\int d^{3}y\exp(-i\bm{p}^{\prime}\cdot\bm{y})\langle 0|J_{B}^{\dagger}(\bm{y},\,y_{4}). (42)

The heavy baryon current JBJ_{B} can be constructed from the Nc1N_{c}-1 valence quarks

JB(x)=1(Nc1)!ϵi1iNc1ΓJJ3TT3Yα1αNc1ψα1i1(x)ψαNc1iNc1(x),\displaystyle J_{B}(x)=\frac{1}{(N_{c}-1)!}\epsilon_{i_{1}\cdots i_{N_{c}-1}}\Gamma_{JJ_{3}TT_{3}Y}^{\alpha_{1}\cdots\alpha_{N_{c}-1}}\psi_{\alpha_{1}i_{1}}(x)\cdots\psi_{\alpha_{N_{c}-1}i_{N_{c}-1}}(x), (43)

where α1αNc1\alpha_{1}\cdots\alpha_{N_{c}-1} represent spin-flavor indices and i1iNc1i_{1}\cdots i_{N_{c}-1} color indices. The matrices ΓJJ3TT3Yα1αNc1\Gamma_{JJ_{3}TT_{3}Y}^{\alpha_{1}\cdots\alpha_{N_{c}-1}} are taken to consider the quantum numbers JJ3TT3YJJ_{3}TT_{3}Y of the Nc1N_{c}-1 soliton. The creation operator JBJ_{B}^{\dagger} can be constructed in a similar way. The calculation of the baryonic correlation function given in Eq. (40) is a tedious one, so we will present here only the final expressions for the E2E2 form factor, As for the detailed formalism, we refer to Refs. Christov:1995vm ; Kim:1995mr .

The final expressions for the electric quadrupole form factors of the baryon sextet with spin 3/2 can be written as

GE2B6(Q2)\displaystyle G^{B_{6}}_{E{2}}(Q^{2}) =65MB2|𝒒|2d3zj2(|𝒒||𝒛|)𝒢E2B(𝒛),\displaystyle=6\sqrt{{5}}\frac{M^{2}_{B}}{|\bm{q}|^{2}}\int d^{3}z\,j_{2}(|\bm{q}||\bm{z}|){\mathcal{G}}^{B}_{E2}(\bm{z}), (44)

where j2(|𝒒||𝒛|)j_{2}(|\bm{q}||\bm{z}|) stands for the spherical Bessel function with order 2 and the corresponding density of the E2E2 form factors is given as

𝒢E2B(𝒛)=\displaystyle{\mathcal{G}}^{B}_{E2}(\bm{z})= 2(3I1DQ3(8)J3B1I1DQi(8)JiB)1E2(𝒛)\displaystyle-2\left(\frac{3}{I_{1}}\langle D^{(8)}_{Q3}J_{3}\rangle_{B}-\frac{1}{I_{1}}\langle D^{(8)}_{Qi}J_{i}\rangle_{B}\right){\cal{I}}_{1E2}(\bm{z}) (45)
+4m8(K1I11E2(𝒛)𝒦1E2(𝒛))(3D83(8)DQ3(8)BD8i(8)DQi(8)B).\displaystyle+4m_{8}\left(\frac{K_{1}}{I_{1}}\mathcal{I}_{1E2}(\bm{z})-\mathcal{K}_{1E2}(\bm{z})\right)\left(3\langle D^{(8)}_{83}D^{(8)}_{Q3}\rangle_{B}-\langle D^{(8)}_{8i}D^{(8)}_{Qi}\rangle_{B}\right). (46)

The densities of E2E2 form factors 1E2\mathcal{I}_{1E2} and 𝒦1E2\mathcal{K}_{1E2} can be found in Appendix A. In the limit of mQm_{Q}\to\infty, the charge distribution of the heavy quark becomes a point-like static charge given as ρQ(𝒓)=eQδ(3)(𝒓)\rho_{Q}(\bm{r})=e_{Q}\delta^{(3)}(\bm{r}). This leads to 𝒬ij=d3rρQ(𝒓)(3rirjr2δij)=0\mathcal{Q}_{ij}=\int d^{3}r\rho_{Q}(\bm{r})(3r_{i}r_{j}-r^{2}\delta_{ij})=0. This implies that the E2E2 form factors of the singly heavy baryons are solely governed by the light quarks in the mQm_{Q}\to\infty limit.

Having calculated the matrix elements of the collective operators in Eq. (46), we arrive at the final expressions for the E2E2 form factors of the baryon sextet with spin 3/2

𝒢E2B(𝒛)\displaystyle\mathcal{G}^{B}_{E2}(\bm{z}) =𝒢E2B(0)(𝒛)+𝒢E2B(op)(𝒛)+𝒢E2B(wf)(𝒛),\displaystyle=\mathcal{G}^{B(0)}_{E2}(\bm{z})+\mathcal{G}^{B(\text{op})}_{E2}(\bm{z})+\mathcal{G}^{B(\text{wf})}_{E2}(\bm{z}), (47)

where 𝒢E2B(0)\mathcal{G}_{E2}^{B(0)}, 𝒢E2B(op)\mathcal{G}_{E2}^{B(\mathrm{op})}, and 𝒢E2B(wf)\mathcal{G}_{E2}^{B(\mathrm{wf})} denote respectively the symmetric terms, the flavor SU(3) symmetry-breaking ones from the effective chiral action, and those from the mixed collective wavefunctions, expressed explicitly as

𝒢E2B6(0)(𝒛)\displaystyle{\cal{G}}^{B_{6}(0)}_{E2}(\bm{z}) =3101I1QB1E2(𝒛),\displaystyle=\frac{3}{10}\frac{1}{I_{1}}Q_{B}\mathcal{I}_{1E2}(\bm{z}), (48)
𝒢E2B6(op)(𝒛)\displaystyle{\cal{G}}^{B_{6}(\text{op})}_{E2}(\bm{z}) =1405ms(K1I1E2(𝒛)𝒦E2(𝒛))(6QΣc+124QΞc139),\displaystyle=-\frac{1}{405}m_{s}\left(\frac{K_{1}}{I_{1}}\mathcal{I}_{E2}(\bm{z})-\mathcal{K}_{E2}(\bm{z})\right)\left(\begin{array}[]{c c c}6Q_{\Sigma_{c}^{*}}+1\\ -24Q_{\Xi_{c}^{*}}-13\\ 9\end{array}\right), (52)
𝒢E2B6(wf)(𝒛)\displaystyle{\cal{G}}^{B_{6}(\text{wf})}_{E2}(\bm{z}) =2I1[q15¯(295(3QΣc4)1185(15QΞc2)0)+q24¯(1180(3QΣc+5)190(3QΞc+5)340QΩc)]1E2(𝒛),\displaystyle=-\frac{2}{I_{1}}\left[q_{\overline{15}}\left(\begin{array}[]{c c c}{-\frac{2}{9\sqrt{5}}}(3Q_{\Sigma^{*}_{c}}-4)\\ {-\frac{1}{18\sqrt{5}}}(15Q_{\Xi^{*}_{c}}-2)\\ 0\end{array}\right)+q_{\overline{24}}\left(\begin{array}[]{c c c}{-\frac{1}{180}}(3Q_{\Sigma^{*}_{c}}+5)\\ {-\frac{1}{90}}(3Q_{\Xi^{*}_{c}}+5)\\ {\frac{3}{40}}Q_{\Omega^{*}_{c}}\end{array}\right)\right]\mathcal{I}_{1E2}(\bm{z}), (59)

where QBQ_{B} stands for the charge of the light-quark components of the corresponding baryons. We can derive similar sum rules for the electric quadrupole moments of singly heavy baryons with spin 3/2 as follows Kim:2019gka

Bsextet𝒬B=0,\displaystyle\sum_{B\in\mathrm{sextet}}\mathcal{Q}_{B}=0, (60)
𝒬Σc0=𝒬Ξc0=𝒬Ωc0=2𝒬Σc+=2𝒬Ξc+=12𝒬Σc++.\displaystyle\mathcal{Q}_{\Sigma^{*0}_{c}}=\mathcal{Q}_{\Xi^{*0}_{c}}=\mathcal{Q}_{\Omega^{*0}_{c}}=-2\mathcal{Q}_{\Sigma^{*+}_{c}}=-2\mathcal{Q}_{\Xi^{*+}_{c}}=-\frac{1}{2}\mathcal{Q}_{\Sigma^{*++}_{c}}. (61)

Even though the flavor SU(3) symmetry is broken, we still can find the following sum rules

𝒬Σc++𝒬Σc+\displaystyle\mathcal{Q}_{\Sigma^{*++}_{c}}-\mathcal{Q}_{\Sigma^{*+}_{c}} =𝒬Σc+𝒬Σc0,\displaystyle=\mathcal{Q}_{\Sigma^{*+}_{c}}-\mathcal{Q}_{\Sigma^{*0}_{c}}, (62)
𝒬Σc0𝒬Ξc0\displaystyle\mathcal{Q}_{\Sigma^{*0}_{c}}-\mathcal{Q}_{\Xi^{*0}_{c}} =𝒬Ξc0𝒬Ωc0,\displaystyle=\mathcal{Q}_{\Xi^{*0}_{c}}-\mathcal{Q}_{\Omega^{*0}_{c}}, (63)
2(𝒬Σc+𝒬Ξc0)\displaystyle 2(\mathcal{Q}_{\Sigma^{*+}_{c}}-\mathcal{Q}_{\Xi^{*0}_{c}}) =𝒬Σc++𝒬Ωc0.\displaystyle=\mathcal{Q}_{\Sigma^{*++}_{c}}-\mathcal{Q}_{\Omega^{*0}_{c}}. (64)

III Results and discussion

In the χ\chiQSM, there are several parameters to fix. Since the sea-quark or Dirac-sea contributions contain divergent integrals, one has to introduce a regularization to tame the divergences. In the present work, we introduce the proper-time regularizations with the cutoff mass. This can be fixed by using the pion decay constant fπ=93f_{\pi}=93 MeV. The average mass of the up and down current quarks m¯\overline{m} is determined by the physical pion mass mπ=140m_{\pi}=140 MeV (see Appendix B for details). While the mass of the strange current quark msm_{\mathrm{s}} can be also fixed by reproducing the kaon mass, which gives ms=150m_{\mathrm{s}}=150 MeV, we preferably use ms=180m_{\mathrm{s}}=180 MeV, since this value of msm_{\mathrm{s}} yields the best results for the hyperon mass splittings Blotz:1992pw ; Christov:1995vm . The remaining parameter is the dynamical quark mass MM, which is the only free parameter of the model. However, M=420M=420 MeV is known to be the best value in reproducing various observables in the light baryon sector Christov:1995vm . Thus, we will use this value also in the present calculation.

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Figure 1: Valence- and sea-quark contributions to the electric quadrupole form factors of the baryon sextet with spin 3/2. The long-dashed curves draw the valence-quark contributions to the E2E2 form factors, whereas the short-dashed ones depict the sea-quark contributions. The solid ones represent the total results for the E2E2 form factors.

It was shown that in the calculation of the E2E2 form factors of the baryon decuplet the sea-quark contributions turn out to be rather important, we will first examine the valence- and sea-quark contributions separately. In Fig. 1, we draw the numerical results for the E2E2 form factors of the baryon sextet with spin 3/2. As expected, the general behaviors of the valence- and sea-quark contributions to the E2E2 form factors of the heavy singly baryons are rather similar to those of the baryon decuplet. As shown in Fig. 1, the valence-quark contributions decrease off mildly as Q2Q^{2} increases, whereas the sea-quark or Dirac-sea contributions fall off drastically in the smaller Q2Q^{2} region, so that they govern the Q2Q^{2} dependence of the E2E2 form factors. In particular, the magnitudes of the sea-quark contributions are quite larger than in the region of smaller Q2Q^{2}. Thus, they are the main contributions to the electric quadrupole moments of the baryon sextet with spin 3/2. Considering the fact that the electric quadrupole moment exhibits how the corresponding baryon is deformed, the present results provide certain physical implications. Recent investigations on the gravitational form factors of baryons within the χ\chiQSM indicate that the valence quarks are mainly located in the inner part of a baryon, while the sea quarks lie in its outer part Goeke:2007fp ; Kim:2020nug . Thus, the sea-quark contributions, which can be also interpreted as pion clouds, mainly describe how a singly heavy baryon with spin 3/2 is deformed. The present results are in line with what was discussed in Ref. Pascalutsa:2006up , where the significance of the pion clouds in the electric quadrupole moment of the Δ\Delta isobar was discussed .

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Figure 2: The effects of flavor SU(3) symmetry breaking on the electric quadrupole form factors of the baryon sextet with spin 3/2. The dashed curves draw the results for the E2E2 form factors without the msm_{\mathrm{s}} corrections, whereas the solid curves depict the results with the effects of flavor SU(3) symmetry breaking taken into account.

In Fig. 2, we show how much the effects of flavor SU(3) symmetry breaking contribute to the E2E2 form factors of the baryon sextet with spin 3/2. As expressed in Eqs. (52) and (59), there are two different msm_{\mathrm{s}} corrections to the E2E2 form factors. The first one 𝒢E2B6(op)(Q2){\cal{G}}^{B_{6}(\text{op})}_{E2}(Q^{2}) arises from the current-quark mass term in the effective chiral action given in Eq. (11), whereas the second one comes from the wavefunction corrections (26). each correction affects E2E2 form factors in a different way, as shown in Fig. 3. The wavefunction corrections to the E2E2 form factor of Σc++\Sigma_{c}^{*++} are negligibly tiny and the corrections from the current-quark mass term is also small. As a result, the msm_{\mathrm{s}} corrections turn out to be negligible, as shown in the upper left panel of Fig. 2. On the other hand, the wavefunction corrections contribute noticeably to the E2E2 form factors of Σc+\Sigma_{c}^{*+}, while those from the current-quark mass term are of the same order as in the case of Σc++\Sigma_{c}^{*++}. In the case of Σc0\Sigma_{c}^{*0} and Ξc0\Xi_{c}^{*0}, the wavefunction corrections to GE2Σc0,Ξc0G_{E2}^{\Sigma_{c}^{*0},\Xi_{c}^{*0}} are even larger than those from the mass term. This can be understood by examining Eqs. (52) and (59).

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Figure 3: Linear msm_{\mathrm{s}} corrections from the current-quark mass term in the effective chiral action GE2Bc(op)G_{E2}^{B_{c}^{*}(\mathrm{op})} and from the collective wavefunctions GE2Bc(wf)G_{E2}^{B_{c}^{*}(\mathrm{wf})}, which are drawn respectively in the short-dashed and long-dashed curves.
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Figure 4: Electric quadrupole form factors of the baryon sextet with spin 3/2 in comparison with the data from the lattice QCD. The data of the lattice QCD is taken from Ref. Can:2015exa .

In the left panel of Fig. 4, we compare the results for the E2E2 form factors of the Ωc0\Omega_{c}^{*0} baryon with that from the lattice calculation. We employ for this comparison the unphysical pion mass mπ=156m_{\pi}=156 MeV that is used in the lattice calculation. Note that there is only one lattice data with large uncertainty.

We anticipate more accurate lattice data in the near future, so that one can draw a clear conclusion. In the right panel of Fig. 4, we depict the results of GE2Ωc0G_{E2}^{\Omega_{c}^{*0}} as a function of the pion mass mπm_{\pi} with Q2=0.183GeV2Q^{2}=0.183\,\mathrm{GeV}^{2} fixed. As expected, the present results fall off slowly as mπm_{\pi} increases.

Table 1: Electric quadrupole moments of the baryon sextet.
𝒬B\mathcal{Q}_{B} [ee\cdot fm2] Σc++\Sigma^{*++}_{c} Σc+\Sigma^{*+}_{c} Σc0\Sigma^{*0}_{c} Ξc+\Xi^{*+}_{c} Ξc0\Xi^{*0}_{c} Ωc0\Omega^{*0}_{c}
ms=180m_{s}=180 MeV 0.0490-0.0490 0.0058-0.0058 0.03730.0373 0.0234-0.0234 0.03300.0330 0.02860.0286
ms=0m_{s}=0 MeV 0.0518-0.0518 0.0129-0.0129 0.02590.0259 0.0129-0.0129 0.02590.0259 0.02590.0259

For completeness, we present the results for the electric quadrupole moments of the baryon sextet with spin 3/2. Table 1 lists those of the 𝒬B\mathcal{Q}_{B} in the second and third rows, which correspond to the SU(3) symmetric and breaking cases, respectively. As already shown in Fig. 2, those of the charged baryon sextet have negative values of 𝒬B\mathcal{Q}_{B}, which indicates that the positively charged singly heavy baryons with spin 3/2 take oblate shapes. On the other hand, those of the neutral ones get positive values, so they are distorted in prolate forms. It is interesting to see that the 𝒬B\mathcal{Q}_{B} of the doubly positive-charged Σc\Sigma_{c}^{*} is approximately 8 times larger than that of the singly positive-charged one. This can be understood by examining Eqs. (47).

IV Summary and conclusion

In the present work, we have investigated the electric quadrupole form factors of the lowest-lying singly heavy baryons with spin 3/2 in a pion mean-field approach, also knwon as the SU(3) chiral quark-soliton model. In the limit of an infinitely heavy quark, a heavy quark inside a singly heavy baryon can be regarded as a mere static color source. This means that the Nc1N_{c}-1 light valence quarks govern the quark dynamics inside a heavy baryon. The presence of the Nc1N_{c}-1 light valence quarks make the vacuum polarized, which produces the pion mean fields. The Nc1N_{c}-1 valence quarks are bound by the attraction provided by the pion mean fields self-consistently, from which a colored soliton consisting of the Nc1N_{c}-1 valence quarks arises. We call this soliton as a Nc1N_{c}-1 soliton. Then the singly heavy baryon can be constructed by coupling the Nc1N_{c}-1 soliton with a heavy quark. This is called the pion mean-field approach for the singly heavy baryons. Based on this pion mean-field approach, we computed the electric qudrupole form factors of the baryon sextet with spin 3/2, taking into account the rotational 1/Nc1/N_{c} and linear msm_{\mathrm{s}} corrections.

We first examined the valence- and sea-quark contributions separately. As in the case of the baryon decuplet, the contributions from the sea quarks or the Dirac-sea level quarks govern the electric quadrupole form factors, in particular, in the smaller Q2Q^{2} region. Considering the fact that the electric quadrupole moment of a baryon provides information on how the baryon is deformed, we can draw the following physical implications: the deformation of a singly heavy baryon is also mainly governed by the sea-quark contributions or the pion cloud effects. We found a similar feature in the case of the baryon decuplet. The effects of the explicit flavor SU(3) symmetry breaking are also sizable except for the case of the Σc++\Sigma_{c}^{*++} and Ωc0\Omega_{c}^{*0}. Since there are two different linear msm_{\mathrm{s}} corrections, we have scrutinized each effect in detail. To compare the present results with those from the lattice calculation, we have computed the electric quadrupole form factor with the unphysical value mπ=156m_{\pi}=156 MeV adopted, which was used by the lattice work. We also showed how the value of the form factor at a fixed Q2Q^{2} is changed as the mπm_{\pi} increases. As expected from previous works, the value of the form factor falls off as mπm_{\pi} increases. We also presented the results for the electric quadrupole moment. The charged singly-heavy baryons have consistently negative values of the electric quadrupole moments. This indicates that the charged baryons take oblate shapes. On the other hand, the neutral baryons take prolate shapes, having the positive values of the electric quadrupole moments.

Acknowledgements.
The authors are grateful to Gh.-S. Yang for valuable discussions. They want to express the gratitude to M. Oka and K. U. Can for providing us with the lattice data. The present work was supported by Basic Science Research Program through the National Research Foundation of Korea funded by the Ministry of Education, Science and Technology (2018R1A2B2001752 and 2018R1A5A1025563). J.-Y. Kim acknowledges partial support by the DAAD doctoral scholarship.

Appendix A Densities for the E2E2 form factor and moments of inertia

In this Appendix, we provide the explicit expressions for the 1E2\mathcal{I}_{1E2} and 𝒦1E2\mathcal{K}_{1E2} densities of the electric quadrupole form factors in Eq. (46)

1E2(𝒛)\displaystyle\mathcal{I}_{1E2}(\bm{z}) =(Nc1)210nval1EnEvalval|𝝉|nn|𝒛{4πY2τ1}1𝒛|val\displaystyle=-\frac{(N_{c}-1)}{2\sqrt{10}}\sum_{n\neq\mathrm{val}}\frac{1}{E_{n}-E_{\mathrm{val}}}{\langle\mathrm{val}|\bm{\tau}|n\rangle}\cdot{\langle n|\bm{z}\rangle\{\sqrt{4\pi}Y_{2}\otimes\tau_{1}\}_{1}\langle\bm{z}|\mathrm{val}\rangle} (65)
+Nc410n,m3(En,Em)n|𝝉|mm|𝒛{4πY2τ1}1𝒛|n,\displaystyle+\frac{N_{c}}{4\sqrt{10}}\sum_{n,m}{\cal{R}}_{3}(E_{n},E_{m}){\langle n|\bm{\tau}|m\rangle}\cdot{\langle m|\bm{z}\rangle\{\sqrt{4\pi}Y_{2}\otimes\tau_{1}\}_{1}\langle\bm{z}|n\rangle}, (66)
𝒦1E2(𝒛)\displaystyle\mathcal{K}_{1E2}(\bm{z}) =(Nc1)210nval1EnEvalval|γ0𝝉|nn|𝒛{4πY2τ1}1𝒛|val\displaystyle=-\frac{(N_{c}-1)}{2\sqrt{10}}\sum_{n\neq\mathrm{val}}\frac{1}{E_{n}-E_{\mathrm{val}}}{\langle\mathrm{val}|\gamma^{0}\bm{\tau}|n\rangle}\cdot{\langle n|\bm{z}\rangle\{\sqrt{4\pi}Y_{2}\otimes\tau_{1}\}_{1}\langle\bm{z}|\mathrm{val}\rangle} (67)
Nc410n,m5(En,Em)n|γ0𝝉|mm|𝒛{4πY2τ1}1𝒛|n,\displaystyle-\frac{N_{c}}{4\sqrt{10}}\sum_{n,m}{\cal{R}}_{5}(E_{n},E_{m}){\langle n|\gamma^{0}\bm{\tau}|m\rangle}\cdot{\langle m|\bm{z}\rangle\{\sqrt{4\pi}Y_{2}\otimes\tau_{1}\}_{1}\langle\bm{z}|n\rangle}, (68)

where the regularization functions are defined by

3(En,Em)=12π0ϕ(u)duu[euEm2euEn2u(En2Em2)EmeuEm2+EneuEn2En+Em],\displaystyle{\cal{R}}_{3}(E_{n},E_{m})=\frac{1}{2\sqrt{\pi}}\int^{\infty}_{0}\phi(u)\frac{du}{\sqrt{u}}\left[\frac{e^{-uE_{m}^{2}}-e^{-uE_{n}^{2}}}{u(E^{2}_{n}-E^{2}_{m})}-\frac{E_{m}e^{-uE_{m}^{2}}+E_{n}e^{-uE_{n}^{2}}}{E_{n}+E_{m}}\right], (69)
5(En,Em)=sign(En)sign(Em)2(EnEm),\displaystyle{\cal{R}}_{5}(E_{n},E_{m})=\frac{\mathrm{sign}(E_{n})-\mathrm{sign}(E_{m})}{2(E_{n}-E_{m})}, (70)

with the proper-time regulator ϕ(u)\phi(u) Christov:1995vm . Here, |val|\mathrm{val}\rangle and |n|n\rangle denotes the state of the valence and sea quarks with the corresponding eigenenergies EvalE_{\mathrm{val}} and EnE_{n} of the single-quark Hamiltonian h(Uc)h(U_{c}), respectively.

The moments of inertia (I1,I2I_{1},I_{2}) and anomalous moments of inertia (K1,K2K_{1},K_{2}) are expressed respectively as

I1\displaystyle I_{1} =(Nc1)6nval1EnEvalval|𝝉|nn|𝝉|val+Nc12n,mnm|𝝉|nn|𝝉|m3(En,Em),\displaystyle=\frac{(N_{c}-1)}{6}\sum_{n\neq\mathrm{val}}\frac{1}{E_{n}-E_{\mathrm{val}}}\langle\mathrm{val}|\bm{\tau}|n\rangle\cdot\langle n|\bm{\tau}|\mathrm{val}\rangle+\frac{N_{c}}{12}\sum_{n,m\neq n}\langle m|\bm{\tau}|n\rangle\cdot\langle n|\bm{\tau}|m\rangle\mathcal{R}_{3}(E_{n},E_{m}), (71)
I2\displaystyle I_{2} =(Nc1)4n01En0Evalval|n0n0|val+Nc4n0,mm|𝝉|n0n0|m3(En0,Em),\displaystyle=\frac{(N_{c}-1)}{4}\sum_{n^{0}}\frac{1}{E_{n^{0}}-E_{\mathrm{val}}}\langle\mathrm{val}|n^{0}\rangle\langle n^{0}|\mathrm{val}\rangle+\frac{N_{c}}{4}\sum_{n^{0},m}\langle m|\bm{\tau}|n^{0}\rangle\langle n^{0}|m\rangle\mathcal{R}_{3}(E_{n^{0}},E_{m}), (72)
K1\displaystyle K_{1} =(Nc1)6nval1EnEvalval|𝝉|nn|γ0𝝉|val+Nc12n,mnm|𝝉|nn|γ0𝝉|m5(En,Em),\displaystyle=\frac{(N_{c}-1)}{6}\sum_{n\neq\mathrm{val}}\frac{1}{E_{n}-E_{\mathrm{val}}}\langle\mathrm{val}|\bm{\tau}|n\rangle\cdot\langle n|\gamma^{0}\bm{\tau}|\mathrm{val}\rangle+\frac{N_{c}}{12}\sum_{n,m\neq n}\langle m|\bm{\tau}|n\rangle\cdot\langle n|\gamma^{0}\bm{\tau}|m\rangle\mathcal{R}_{5}(E_{n},E_{m}), (73)
K2\displaystyle K_{2} =(Nc1)4n01En0Evalval|n0n0|γ0|val+Nc4n0,mm|𝝉|n0n0|γ0|m5(En0,Em).\displaystyle=\frac{(N_{c}-1)}{4}\sum_{n^{0}}\frac{1}{E_{n^{0}}-E_{\mathrm{val}}}\langle\mathrm{val}|n^{0}\rangle\langle n^{0}|\gamma^{0}|\mathrm{val}\rangle+\frac{N_{c}}{4}\sum_{n^{0},m}\langle m|\bm{\tau}|n^{0}\rangle\langle n^{0}|\gamma^{0}|m\rangle\mathcal{R}_{5}(E_{n^{0}},E_{m}). (74)

Appendix B Fixing the model parameters

The chiral condensate and the pion decay constant can be derive from the effective chiral action given in Eq. (11). The chiral condensate are written as

ψ¯ψ=d4pE(2π)48NcMpE2+M2|reg=MNc2π20ϕ(u)duu2euM2,\displaystyle\langle\overline{\psi}\psi\rangle=-\int\frac{d^{4}p_{E}}{(2\pi)^{4}}\frac{8N_{c}M}{p^{2}_{E}+M^{2}}\bigg{|}_{\mathrm{reg}}=M\frac{N_{c}}{2\pi^{2}}\int^{\infty}_{0}\phi(u)\frac{du}{u^{2}}e^{-uM^{2}}, (75)

and the pion decay constant are given by

fπ2=d4pE(2π)44NcM2(pE2+M2)2|reg=M2Nc4π20ϕ(u)duueuM2,\displaystyle f^{2}_{\pi}=-\int\frac{d^{4}p_{E}}{(2\pi)^{4}}\frac{4N_{c}M^{2}}{(p^{2}_{E}+M^{2})^{2}}\bigg{|}_{\mathrm{reg}}=M^{2}\frac{N_{c}}{4\pi^{2}}\int^{\infty}_{0}\phi(u)\frac{du}{u}e^{-uM^{2}}, (76)

with proper-time regulator ϕ=cθ(uΛ12)+(1c)θ(uΛ22)\phi=c\theta(u-\Lambda^{-2}_{1})+(1-c)\theta(u-\Lambda^{-2}_{2}). The pion mass is determined by the pole position of the pion propagator that is obtained by a low-energy effective chiral theory given by Eq. (11)

mπ2=m¯ψ¯ψfπ2+𝒪(m¯2).\displaystyle m^{2}_{\pi}=\frac{\overline{m}\langle\overline{\psi}\psi\rangle}{f^{2}_{\pi}}+\mathcal{O}(\overline{m}^{2}). (77)

The above-given expressions satisfy the Gell-Mann–Oakes–Renner (GMOR) relation. With Eqs. (75), (76) and  (77), one can determine the cutoff mass. The average value of the up and down current quark masses is obtained as m¯=6.13MeV\overline{m}=6.13~{}\mathrm{MeV}. The strange current quark mass msm_{s} is fixed by the hyperon mass splittings by treating msm_{s} perturbatively up to the second-order corrections  Blotz:1992pw ; Christov:1995vm ; Kim:2018xlc . The preferable value of msm_{s} is found to be ms=180MeVm_{s}=180~{}\mathrm{MeV}.

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