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PHYSICAL REVIEW D 102, 014004 (2020)

Spectrum of singly heavy from a chiral effective theory of diquarks

† ‡ Yonghee Kim,1,* Emiko Hiyama,1,2, Makoto Oka ,3,2, and Kei Suzuki 3,§ 1Department of Physics, Kyushu University, Fukuoka 819-0395, Japan 2Nishina Center for Accelerator-Based Science, RIKEN, Wako 351-0198, Japan 3Advanced Science Research Center, Japan Atomic Energy Agency (JAEA), Tokai 319-1195, Japan

(Received 6 March 2020; accepted 5 June 2020; published 6 July 2020)

− − The mass spectra of singly charmed and bottom baryons, Λc=bð1=2 ; 3=2 Þ and Ξc=bð1=2 ; 3=2 Þ, are investigated using a nonrelativistic potential model with a heavy and a light . The masses of the scalar and pseudoscalar diquarks are taken from a chiral effective theory. The effect of UAð1Þ anomaly induces an inverse hierarchy between the masses of strange and nonstrange pseudoscalar diquarks, which leads to a similar inverse mass ordering in ρ-mode excitations of singly heavy baryons.

DOI: 10.1103/PhysRevD.102.014004

I. INTRODUCTION condensates and UAð1Þ anomaly, respectively. Such sym- metry breaking effects should be related to the properties Diquarks, strongly correlated two-quark states, have a of diquarks [29,32,33]. In Ref. [29], a chiral effective long history in physics since the 1960s [1–8] (see theory based on the SUð3ÞR × SUð3ÞL chiral symmetry Refs. [9,10] for reviews). It is an important concept for JP ¼ 0þ J P understanding the various physics in quantum chromody- with the scalar ( , where and are the total namics (QCD), such as the (and also exotic-hadron) angular momentum and parity, respectively) diquarks 3¯ spectra as well as the color superconducting phase. The belonging to the color antitriplet and flavor antitriplet ¯ − properties of various diquarks, such as the mass and size, 3 channel and its pseudoscalar (0 ) counterpart was 1 have been studied by lattice QCD simulations [11–17]. constructed. These are the following new (and interesting) A phenomenon related to diquark degrees of freedom is suggestions: the spectrum of singly heavy baryons (Qqq), where a (i) Chiral partner structures of diquarks—A scalar baryon contains two light (up, down, or strange) diquark and its pseudoscalar partner belong to a (q ¼ u; d; s) and one heavy (charm or bottom) quark chiral multiplet, which is the so-called chiral partner (Q ¼ c; b), so that the two light quarks (qq) might be structure. This structure means that chiral partners are well approximated as a diquark (for model studies about degenerate when the chiral symmetry is completely diquarks in Qqq baryons, e.g., see Refs. [18–29]). In restored. As a result, they also predicted a similar particular, the spectrum of singly heavy baryons is a chiral partner structure for charmed baryons such as Λ ð1=2þÞ Λ ð1=2−Þ Ξ ð1=2þÞ Ξ ð1=2−Þ promising candidate visibly affected by diquark degrees c - c and c - c (for of freedom. For example, the P-wave excited states of similar studies, see Refs. [35,36]). — singly heavy baryons are classified by λ modes (the orbital (ii) Inverse hierarchy of diquark masses The effect U ð1Þ excitations between the diquark and heavy quark) and ρ of the A anomaly leads to an inverse hierarchy modes (the orbital excitations between two light quarks for the masses of the pseudoscalar diquarks: Mðus=ds; 0−Þ

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L ¼ −m2ðd d† þ d d† Þ simply called quark-diquark model). Our approach has the mass 0 R;i R;i L;i L;i following advantages: − ðm2 þ Am2Þðd d† þ d d† (i) It can study the singly heavy-baryon spectrum based 1 2 R;1 L;1 L;1 R;1 † † on the chiral partner structures of diquarks. þ dR;2dL;2 þ dL;2dR;2Þ (ii) It can introduce the inverse hierarchy of the pseu- − ðAm2 þ m2Þðd d† þ d d† Þ; ð Þ doscalar diquark masses originated from the UAð1Þ 1 2 R;3 L;3 L;3 R;3 1 anomaly and examine its effects on the singly heavy baryons. where m0, m1, and m2 are the model parameters. m0 is 2 (iii) It can take into account the contribution from the called the chiral invariant mass. The term with m0 satisfies 2 2 confining (linear and Coulomb) potential. This is an the chiral symmetry, while the terms with m1 and m2 break additional advantage missing in Ref. [29]. the chiral symmetry spontaneously and explicitly. m1 and (iv) It can predict λ-mode excited states of singly heavy m2 are the coefficients of the six-point quark (or diquark- baryons. This is more profitable than the approach in duquark-) interaction motivated by the UAð1Þ Ref. [29], where it will be difficult to calculate anomaly and the eight-point quark (or diquark-duquark- λ-mode excitations only by the effective Lagrangian meson-meson) interaction which conserves the UAð1Þ though the ρ-mode states are naively estimated. symmetry, respectively. A ∼ 5=3 is the parameter of the It should be noted that the diquark-heavy-quark flavor SUð3Þ symmetry breaking due to the quark mass approach can cover all the excitation modes that appear difference, ms >mu ≃ md. in the conventional . The orbital excitations of a three-quark system consist of the λ-mode, in which the B. Mass formulas of diquarks diquark is intact, and the ρ-mode, in which the diquark is internally excited. The latter can be represented by a new By diagonalizing the mass matrix (1) in R=L and flavor type of diquark. In the present approach, we consider only space, we obtain the mass formulas for the diquarks, the scalar and pseudoscalar diquarks, but there are many Mið0 Þ [29], other possible diquarks [29]. Among them the vector and qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi axial-vector diquarks are known to be low-lying and play þ þ 2 2 2 M1ð0 Þ¼M2ð0 Þ¼ m0 − m1 − Am2; ð2Þ major roles in the flavor 6 baryons, such as Σc and Ωc. The chiral effective theory for the vector and axial-vector qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi þ 2 2 2 diquarks and their couplings to the scalar and pseudoscalar M3ð0 Þ¼ m0 − Am1 − m2; ð3Þ diquarks is being considered in the forthcoming paper. qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi This paper is organized as follows. In Sec. II,we M ð0−Þ¼M ð0−Þ¼ m2 þ m2 þ Am2; ð Þ formulate the hybrid approach of the chiral effective theory 1 2 0 1 2 4 and the potential model. In Sec. III, we show the numerical qffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi results. Section IV is devoted to our conclusion and − 2 2 2 M3ð0 Þ¼ m0 þ Am1 þ m2: ð5Þ outlook. From Eqs. (2)–(5), we get II. FORMALISM þ 2 þ 2 − 2 − 2 In this section, we summarize the mass formulas of ½M1;2ð0 Þ − ½M3ð0 Þ ¼½M3ð0 Þ − ½M1;2ð0 Þ diquarks based on the chiral effective theory [29]. After 2 2 ¼ðA − 1Þðm1 − m2Þ: ð6Þ that, we construct a nonrelativistic potential model for singly heavy baryons composed of a heavy quark and a 2 2 From this relation with A>1 and m1 >m2, one finds diquark. the inverse mass hierarchy for the pseudoscalar diquarks: − − M3ð0 Þ >M1;2ð0 Þ, where the nonstrange diquark (i ¼ 3) A. Chiral effective Lagrangian is heavier than the strange diquark (i ¼ 1; 2). In this work, we concentrate on the scalar (0þ) and − ¯ ¯ pseudoscalar (0 ) diquarks with color 3 and flavor 3. In the C. Potential quark-diquark model chiral effective theory of diquarks [29], we consider the In order to calculate the spectrum of singly heavy right-handed and left-handed diquark fields, dR;i and dL;i, baryons, we apply a nonrelativistic two-body potential where i is the flavor index of a diquark. The i ¼ 1 (ds) and model with a single heavy quark and a diquark. i ¼ 2 (su) diquarks include one , while the The nonrelativistic two-body Hamiltonian is written as i ¼ 3 (ud) diquark has no strange quark. SUð3Þ When the chiral symmetry and flavor symmetry p2 p2 are broken, the mass terms for the diquarks are given H ¼ Q þ d þ M þ M þ VðrÞ; ð Þ 2M 2M Q d 7 by [29] Q d

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TABLE I. Potential model parameters used in this work. We apply three types of potentials, Yoshida (Potential Y) [31], Silvestre-Brac (Potential S) [37], and Barnes (Potential B) [38]. α, λ, Cc, Cb, Mc, and Mb are the coefficients of Coulomb and linear terms, constant shifts for charmed and bottom baryons, and masses of constituent charm and bottom quarks, respectively. μ is reduced mass of two-body systems. The values of Cc and Cb are fitted by our model. For Potential B, Mb is not given [38], so that we do not fit Cb.

2 αλðGeV Þ CcðGeVÞ CbðGeVÞ McðGeVÞ MbðGeVÞ Potential Y [31] ð2=3Þ × 90ðMeVÞ=μ 0.165 −0.831 −0.819 1.750 5.112 Potential S [37] 0.5069 0.1653 −0.707 −0.696 1.836 5.227 Potential B [38] ð4=3Þ × 0.5461 0.1425 −0.191 … 1.4794 …

where the indices Q and d denote the heavy quark and constant shifts, Cc for charmed baryons and Cb for bottom diquark, respectively. pQ=d and MQ=d are the momentum baryons. The procedure is as follows: and mass, respectively. r ¼ rd − rQ is the relative coor- (i) Determination of Cc—By inputting the mass of the þ dinate between the two . After subtracting ud scalar diquark, M3ð0 Þ, we determine the con- the kinetic energy of the center of mass motion, the stant shift Cc so as to reproduce the ground-state þ Hamiltonian is reduced to mass of Λc.AsM3ð0 Þ, we apply the value measured from recent lattice QCD simulations with þ p2 2 þ 1 dynamical quarks [17]: M3ð0 Þ¼725 MeV. H ¼ þ M þ M þ VðrÞ; ð Þ Q d 8 As the mass of Λc, we use the experimental value 2μ þ from PDG [42]: MðΛc; 1=2 Þ¼2286.46 MeV. M ð0þÞ M ð0−Þ— MQpd−MdpQ MdMQ (ii) Determination of 1;2 and 3 After where p ¼ M þM and μ ¼ M þM are the relative d Q d Q fixing Cc, we next fix two diquark masses, þ − momentum and reduced mass, respectively. M1;2ð0 Þ and M3ð0 Þ. Here, we apply the following For the potential VðrÞ, in this work, we apply three types two methods: þ of potentials constructed by Yoshida et al. [31], Silvestre- Model I.—The first method is to input M1;2ð0 Þ and − Brac [37], and Barnes et al. [38]. These potentials consist of M3ð0 Þ measured from recent lattice QCD simula- α þ − the Coulomb term with the coefficient and the linear term tions [17]: M1;2ð0 Þ¼906 MeV and M3ð0 Þ¼ with λ, 1265 MeV.2 We call the choice of these parameters Model I, which is similar to Method I in Ref. [29]. α þ VðrÞ¼− þ λr þ C; ð9Þ Model II.—Another method is to determine M1;2ð0 Þ r − and M3ð0 Þ from the potential model and some known baryon masses, which we call Model II. After where C in the last term is a “constant shift” of the þ − fixing Cc, M1;2ð0 Þ and M3ð0 Þ are determined so as potential, which is a model parameter depending on the þ − to reproduce MðΞc; 1=2 Þ and MρðΛc; 1=2 Þ, respec- specific system. Note that, only in Ref. [31], the coefficient α of the tively. As input parameters, we use the experimental values of the ground-state Ξc from PDG [42]: Coulomb term depends on 1=μ. In other word, this is a þ “ ” MðΞc; 1=2 Þ¼2469.42 MeV. For the mass of the mass-dependent Coulomb interaction, which is moti- ρ Λ vated by the behavior of the potential obtained from lattice mode of the negative-parity c, we use the value predicted by a nonrelativistic three-body calculation in QCD simulations [39]. On the other hand, the other − 3 Ref. [31]: MρðΛc; 1=2 Þ¼2890 MeV. potentials [37,38] do not include such an effect. Such a − (iii) Determination of M1;2ð0 Þ—Using the mass rela- difference between the potentials will lead to a quantitative þ tion (6) and our three diquark masses, M3ð0 Þ, difference also in singly heavy-baryon spectra. þ − M M1;2ð0 Þ, and M1;2ð0 Þ, we determine the masses of In this work, the mass c, − us=ds pseudoscalar diquarks, M1;2ð0 Þ. Here, we mass Mb, α, and λ are fixed by the values estimated in the M ð0−Þ previous studies [31,37,38], which are summarized in emphasize that the estimated 1;2 reflects the Table I. The other parameters are determined in Sec. III A. inverse hierarchy for the diquark masses, which has In order to numerically solve the Schrödinger equation, we apply the Gaussian expansion method [40,41]. 2 þ þ We use M3ð0 Þ and M1;2ð0 Þ in the chiral limit in Ref. [17]. − The chiral extrapolation of M3ð0 Þ is not shown in Ref. [17],so M ð0−Þ III. NUMERICAL RESULTS that we use 3 at the lowest quark mass (see Table 8 of Ref. [17]). 3Note that while the known experimental value of negative- A. Parameter determination − parity Λc, MðΛc; 1=2 Þ¼2592.25 MeV [42], is expected to be In this section, we determine the unknown model that of the λ-mode excitation, the resonance corresponding to the parameters such as the diquark masses Mið0 Þ and ρ-mode has not been observed.

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never been considered in previous studies except Next, we focus on the ordering of the pseudoscalar − for Ref. [29]. diquarks. We find the inverse hierarchy M1;2ð0 Þ < − (iv) Determination of Cb—For singly bottom baryons, M3ð0 Þ in all the models, which is consistent with the we also determine the constant shift Cb by inputting prediction in Ref. [29]. We emphasize that the inverse mass þ M3ð0 Þ¼725 MeV and reproducing the mass of hierarchy of diquarks does not suffer from the confining þ the ground state Λb, MðΛb; 1=2 Þ¼5619.60 MeV potential. þ − [42]. For the diquark masses, M1;2ð0 Þ, M3ð0 Þ, and Furthermore, from the diquark masses and Eqs. (2)–(5), − M1;2ð0 Þ, we use the same values as the case of the we can determine the unknown parameters of chiral charmed baryons. effective Lagrangian, m0, m1, and m2, which is also The constant shifts, Cc and Cb, estimated by us are summarized in Table II. By definition, the values in summarized in Table I. The diquark masses predicted Model I are the same as those from Method I in by us are shown in Table II. By definition, the diquark Ref. [29]. Here we compare our estimate from Model II masses in Model I are the same as the values from Method I and a naive estimate from Method II in Ref. [29]. From in Ref. [29]. Here we focus on the comparison of the Models IIY, IIS, and IIB, we conclude that these parameters prediction from Model IIY and that from Method II in are insensitive to the choices of the quark model potential. Ref. [29]. In both the approaches, the input values of We also see that inclusion of the confining potential does þ − MðΞc;1=2 Þ¼2469MeV and MρðΛc;1=2 Þ¼2890MeV not alter the parameters qualitatively. Quantitatively, the þ magnitude of these parameters is larger than that from are the same. Our prediction is M1;2ð0 Þ¼942 MeV, which is larger than 906 MeV estimated in Ref. [29]. Method II in Ref. [29], which is expected to be improved by This difference is caused by the existence of the confining taking into account the confining potential. potential (particularly, linear potential) which is not con- sidered in the estimate in Ref. [29]. This tendency does not B. Spectrum of singly charmed baryons change in the results using the other potentials. Similarly, The values of masses of singly charmed baryons are M ð0−Þ þ þ for 3 , we obtain 1406 MeV, which is significantly summarized in Table II. MðΛc; 1=2 Þ, MðΞc; 1=2 Þ, and − larger than 1329 MeV in Ref. [29]. MρðΛc; 1=2 Þ are the input values. Similarly, to the

þ þ − − TABLE II. List of numerical values of scalar [M3ð0 Þ, M1;2ð0 Þ] and pseudoscalar [M3ð0 Þ, M1;2ð0 Þ] diquark masses, masses of 2 2 2 singly-heavy baryons [MðΛQÞ, MðΞQÞ], coefficients of chiral effective Lagrangian (m0, m1, and m2). We compare the results from our approach using three potential and two parameters, Yoshida (denoted as IYand IIY), Silvestre-Brac (IS and IIS), and Barnes (BI and IIS) with a naive estimate in the chiral EFT [29] (Method I and Method II) and the experimental values from PDG [42]. The asterisk () denotes the input values.

Chiral EFT [29] Potential model (this work) Mass (MeV) Method I Method II IY IS IB IIY IIS IIB Experiment [42] þ M3ð0 Þ 725 725 725 725 725 725 725 725 þ M1;2ð0 Þ 906 906 906 906 906 942 977 983 − M3ð0 Þ 1265 1329 1265 1265 1265 1406 1484 1496 − M1;2ð0 Þ 1142 1212 1142 1142 1142 1271 1331 1341 þ MðΛc; 1=2 Þ 2286 2286 2286 2286 2286 2286 2286 2286 2286.46 þ MðΞc; 1=2 Þ 2467 2469 2438 2415 2412 2469 2469 2469 2469.42 − MρðΛc; 1=2 Þ 2826 2890 2759 2702 2694 2890 2890 2890 … − MρðΞc; 1=2 Þ 2704 2775 2647 2600 2594 2765 2758 2758 (2793.25) − − MλðΛc; 1=2 ; 3=2 Þ ……2613 2703 2734 2613 2703 2734 (2616.16) − − MλðΞc; 1=2 ; 3=2 Þ ……2748 2825 2860 2776 2878 2918 (2810.05) þ MðΛb; 1=2 Þ ……5620 5620 … 5620 5620 … 5619.60 þ MðΞb; 1=2 Þ ……5766 5735 … 5796 5785 … 5794.45 − MρðΛb; 1=2 Þ ……6079 5999 … 6207 6174 … (5912.20) − MρðΞb; 1=2 Þ ……5970 5905 … 6084 6051 …… − − MλðΛb; 1=2 ; 3=2 Þ ……5923 6028 … 5923 6028 … (5917.35) − − MλðΞb; 1=2 ; 3=2 Þ ……6049 6139 … 6076 6188 …… Parameter (MeV2) 2 2 2 2 2 2 2 2 2 m0 ð1031Þ ð1070Þ ð1031Þ ð1031Þ ð1031Þ ð1119Þ ð1168Þ ð1176Þ 2 2 2 2 2 2 2 2 2 m1 ð606Þ ð632Þ ð606Þ ð606Þ ð606Þ ð690Þ ð746Þ ð754Þ 2 2 2 2 2 2 2 2 2 m2 −ð274Þ −ð213Þ −ð274Þ −ð274Þ −ð274Þ −ð258Þ −ð298Þ −ð303Þ

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− − ordering of M1;2ð0 Þ

FIG. 1. The energy spectra of singly charmed and bottom baryons from our numerical results using Model IY.

FIG. 2. The energy spectra of singly charmed and bottom baryons from our numerical results using Model IIY.

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Ξc spectrum is smaller than that in the Λc spectrum: between the orbital angular momentum and the heavy- − − − − jMρðΞc; 1=2 Þ − MλðΞc; 1=2 ; 3=2 Þj < jMρðΛc; 1=2 Þ − quark spin. In the heavy-quark limit (mc → ∞), the two − − − MλðΛc; 1=2 ; 3=2 Þj, where we note that the 1=2 and states are degenerate due to the suppression of the LS 3=2− states for λ modes in our model are degenerate as coupling, so that they are called the heavy-quark spin discussed later. The significant difference between Models doublet. − IY and IIY is caused by MρðΛc; 1=2 Þ which is related to − M3ð0 Þ. From the diquark mass relation (6), a larger C. Spectrum of singly bottom baryons − − M3ð0 Þ leads to a larger M1;2ð0 Þ. Then a heavier For the singly bottom baryons, the input value is only the M ðΛ ; 1=2−Þ M ðΞ ; 1=2−Þ þ ρ c leads to a heavier ρ c .Asa mass of the ground-state Λbð1=2 Þ, and here we give − result, MρðΞc; 1=2 Þ from Model IIY is heavier than predictions for the other states. For the ground state of − þ MρðΞc; 1=2 Þ from Model IY. Ξbð1=2 Þ, our prediction with Models IYand IIY is in good þ Next, we discuss the masses of the λ modes. The λ modes agreement with the known mass MðΞb; 1=2 Þ¼ are the excited states with the orbital angular momentum 5794.45 MeV [42]. This indicates that the quark-diquark þ between the heavy quark and diquark, so that their masses are picture is approximately good for Ξbð1=2 Þ. higher than those of the ground states, which is the “P-wave” The energy spectra for Λb and Ξb from Models IY and states in our two-body potential model. Also, in singly IIY are shown in the right panels of Figs. 1 and 2. Similarly heavy-baryon spectra, the masses of the λ modes are usually to the charmed baryon spectra, we again emphasize the lower than that of the ρ modes, as shown by the three-body difference between the Λb and Ξb spectra. For the calculation [31]. In Models IY and IIY, the excitation ρ modes, we also find the inverse mass hierarchy: − − − − energy from the ground state, MλðΛc; 1=2 ; 1=3 Þ− MρðΞb; 1=2 Þ Mð0þÞ. Then the kinetic energy our results from Models IIY, IIS, and IIB within 50 MeV. of the system with Mð0−Þ is suppressed, and, as a result, Thus, Model IIY can reproduce the known experimental the wave function shrinks compared to its ground state values in any case. In addition, when these experimental with Mð0þÞ. Due to the inverse hierarchy of the diquark values are assigned to the λ modes, the excitation energy of masses, we find also the inverse hierarchy for the rms the λ modes from the ground state is estimated to be about pffiffiffiffiffi pffiffiffiffiffi rˆ2 ðΛ ; 1=2−Þ < rˆ2 ðΞ ; 1=2−Þ 330–340 MeV, which is consistent with the results from distance, ρ c ρ c , which is dif- Models IY and IIY. ferentp fromffiffiffiffiffi the standardp hierarchyffiffiffiffiffi seen in the ground 2 þ 2 þ We comment on the possible splitting in the λ modes. states, rˆ ðΛc; 1=2 Þ > rˆ ðΞc; 1=2 Þ. The splitting between 1=2− and 3=2− states is caused by the The λ modes are the P-wave excitations within a two- spin-orbit (LS) coupling. In order to study this splitting body quark-diquark model, so that their rms distance is within our model, we need to introduce the LS coupling larger than those of the ground and ρ-mode states which is

014004-6 SPECTRUM OF SINGLY HEAVY BARYONS FROM A CHIRAL … PHYS. REV. D 102, 014004 (2020) pffiffiffiffiffi TABLE III. Rms distance rˆ2 between a heavy quark and a is the same as the naive estimate in Ref. [29], but it is diquark. important to note that the effect from the confining potential between a heavy quark and a diquark does Rms distance (fm) IY IS IB IIY IIS IIB pffiffiffiffiffi not change this conclusion. ˆ2 þ 0.587 0.512 0.506 0.587 0.512 0.506 ρ prffiffiffiffiffiðΛc; 1=2 Þ (ii) We found that the mass splitting between the - and 2 þ λ Ξ rˆ ðΞc; 1=2 Þ 0.559 0.476 0.469 0.555 0.466 0.457 -mode excitations in the Q spectrum is smaller pffiffiffiffiffi − 2 − Λ jM ðΞ ; 1=2 Þ − rˆ ρðΛc; 1=2 Þ 0.523 0.431 0.421 0.513 0.412 0.402 than that in the Q spectrum: ρ Q pffiffiffiffiffi − − − rˆ2 ðΞ ; 1=2−Þ 0.534 0.444 0.435 0.523 0.425 0.415 MλðΞQ; 1=2 ; 3=2 Þj < jMρðΛQ; 1=2 Þ − MλðΛQ; pffiffiffiffiffiρ c 1=2−; 3=2−Þj ˆ2 − − 0.832 0.783 0.814 0.832 0.783 0.814 . pffiffiffiffiffir λðΛc; 1=2 ; 3=2 Þ 2 − − The inverse mass hierarchy in singly heavy baryons can rˆ λðΞc; 1=2 ; 3=2 Þ 0.792 0.738 0.767 0.785 0.724 0.752 pffiffiffiffiffi be also investigated by future lattice QCD simulations, as ˆ2 þ 0.548 0.466 … 0.548 0.466 … pffiffiffiffiffir ðΛb; 1=2 Þ studied with quenched simulations [44–50], as well as with ˆ2 þ 0.515 0.424 … 0.510 0.412 … – pffiffiffiffiffir ðΞb; 1=2 Þ dynamical quarks [51 61]. Although studying negative- rˆ2 ðΛ ; 1=2−Þ 0.471 0.368 … 0.459 0.346 … parity baryons from lattice QCD is more difficult than the pffiffiffiffiffiρ b rˆ2 ðΞ ; 1=2−Þ 0.484 0.384 … 0.471 0.362 … positive-parity states, there are a few works for singly pffiffiffiffiffiρ b rˆ2 ðΛ ; 1=2−; 3=2−Þ 0.776 0.724 … 0.776 0.724 … heavy baryons [50,58,60,61]. Our findings give a motiva- pffiffiffiffiffiλ b tion to examine the excited-state spectra from lattice QCD rˆ2 ðΞ ; 1=2−; 3=2−Þ 0.728 0.671 … 0.720 0.654 … λ b simulations. Here, the careful treatment of the chiral and UAð1Þ symmetry on the lattice would be required. “S-wave” states within our model. The rms distances in the Furthermore, the chiral effective Lagrangian for singly bottom baryons are shorter than those of the charmed heavy baryons, as formulated in Sec. III-F of Ref. [29],isa baryons because of the heavier bottom quark mass. useful approach for analytically studying the inverse mass We find that the rms distances from Models IY and IIY hierarchy of heavy baryons. In this Lagrangian, the assign- are larger than those from the other models IS, IB, IIS, and ment of the chiral partners for heavy baryons is the same as IIB. This difference is caused by the coefficient α of the that for the diquarks in this work, so that we can obtain a attractive Coulomb interaction. The Yoshida potential in similar spectrum. Models IY and IIY has the relatively small α, so that its The internal structures of excited states, such as ρ and λ wave function and the rms distance are larger than those modes, can significantly modify their decay properties from other models. [62–70], and to study the decay processes taking into Note that the real wave function of a diquark must have a account the inverse hierarchy will be important. size which is the distance between a light quark and another In this paper, we focused only on the scalar diquark and light quark. In our approach, namely, the quark-diquark its chiral partner. As another important channel, the chiral- þ model, diquarks are treated as a point , so that such a partner structure of the axial-vector (1 ) diquarks with the size effect is neglected. To introduce such an effect would color 3¯ and flavor 6 (the so-called “bad” diquarks [10,34]) 0 be important for improving our model. In particular, it could be related to the spectra of ΣQ, ΣQ, ΞQ, ΞQ, ΩQ, and would be interesting to investigate the form factors of ΩQ baryons. singly heavy baryons with the negative parity by lattice Furthermore, the diquark correlations at high temper- QCD simulations and to compare it with our predictions. ature are expected to modify the production rate of singly heavy baryons in high-energy collision experiments IV. CONCLUSION AND OUTLOOK [71–73]. In extreme environments, such as high temper- In this paper, we investigated the spectrum of singly ature and/or density, chiral symmetry breaking should be heavy baryons using the hybrid approach of the chiral also modified, and it would strongly affect the chiral partner effective theory of diquarks and nonrelativistic quark- structures of diquarks and the related baryon spectra. diquark potential model. Our findings are as follows: ACKNOWLEDGMENTS (i) We found the inverse mass hierarchy in the ρ-mode excitations of singly heavy baryons, We thank Masayasu Harada and Yan-Rui Liu for − − MðΞQ; 1=2 Þ

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