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Towards the establishment of the light JP(C)=1(+)J^{P(C)}=1^{-(+)} hybrid nonet

Lin Qiu1,2111E-mail address: qiulin@ihep.ac.cn, and Qiang Zhao1,2,3222E-mail address: zhaoq@ihep.ac.cn 1 Institute of High Energy Physics and Theoretical Physics Center for Science Facilities,
Chinese Academy of Sciences, Beijing 100049, China
2 School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China 3 China Center of Advanced Science and Technology, Chinese Academy of Sciences, Beijing 100080, China
Abstract

The observation of the light hybrid candidate η1(1855)\eta_{1}(1855) by the BESIII Collaboration brings great opportunities for advancing our knowledges about exotic hadrons in the light flavor sector. We show that this observation provides a crucial clue for establishing the JP(C)=1(+)J^{P(C)}=1^{-(+)} hybrid nonet. Based on the flux tube model picture, the production and decay mechanisms for the JP(C)=1(+)J^{P(C)}=1^{-(+)} hybrid nonet in the J/ψJ/\psi radiative decays into two pseudoscalar mesons are investigated. In the I=0I=0 sector, we find that the SU(3) flavor octet and singlet mixing is non-negligible and apparently deviates from the flavor ideal mixing. Since only signals for one isoscalar η1(1855)\eta_{1}(1855) are observed in the ηη\eta\eta^{\prime} channel, we investigate two schemes of the nonet structure in which η1(1855)\eta_{1}(1855) can be either the higher or lower mass state that strongly couples to ηη\eta\eta^{\prime}. Possible channels for detecting the multiplets are suggested. In particular, a combined analysis of the hybrid production in J/ψVHJ/\psi\to VH, where VV and HH stand for the light vector mesons and 1(+)1^{-(+)} hybrid states, may provide further evidence for this nonet structure and finally establish these mysterious exotic species in experiment.

I Introduction

In the conventional quark model mesons are made of quark-anti-quark (qq¯q\bar{q}) and baryons are made of three quarks (qqqqqq). Such a simple picture have made great successes in the description of hadron spectra based on the constituent quark degrees of freedom. Meanwhile, QCD as the fundamental theory for strong interactions predicts the existence of hadrons with more sophisticated structures, namely, exotic hadrons. These states, of which the structures are beyond the conventional quark model, have been a crucial probe for the non-perturbative phenomena of QCD. Among all the exotic candidates, hadrons with such quantum numbers that cannot be accommodated by the conventional quark model, would serve as a “smoking gun” for the existence of exotic hadrons. In particular, “hybrid”, which contains the explicit excitations of the constituent-like gluonic degrees of freedom, can access the exotic quantum numbers of JPC=1+J^{PC}=1^{-+} as the lowest eigenstates. Its study has always attracted a lot of attention from both experiment and theory.

In Refs. besiii-hybrid ; besiii-hybrid-pwa the BESIII Collaboration reports the first observation of the 1+1^{-+} isoscalar hybrid candidate η1(1855)\eta_{1}(1855) in the partial wave analysis of J/ψγη1(1855)γηηJ/\psi\to\gamma\eta_{1}(1855)\to\gamma\eta\eta^{\prime}. Its mass and width are (1855±91+6)(1855\pm 9^{+6}_{-1}) MeV and (188±188+3)(188\pm 18^{+3}_{-8}) MeV, respectively. This progress may provide a great opportunity for a better understanding of these mysterious species of the QCD-predicted exotic states.

Historically, evidences for the 1+1^{-+} hybrid were found by various experiments SLACHybridFacilityPhoton:1991oug ; VES:1993scg ; Lee:1994bh ; Aoyagi:1993kn ; E852:1997gvf ; E852:1999xev , and two light hybrid candidates, π1(1400)\pi_{1}(1400) and π(1600)\pi(1600), were reported. However, due to the limited statistics, their existences were far from broadly accepted. A comprehensive review of the early experimental results can be found in Refs. Klempt:2007cp ; Meyer:2015eta . Strong indication of the 1+1^{-+} hybrid π1(1600)\pi_{1}(1600) is from the COMPASS Collaboration based on their partial wave analysis (PWA) result for πppπ+ππ\pi^{-}p\to p\pi^{+}\pi^{-}\pi^{-} COMPASS:2009xrl ; E852:2001ikk ; COMPASS:2014vkj ; COMPASS:2018uzl . In a recent detailed analysis COMPASS:2018uzl by COMPASS, it shows that the π1(1600)\pi_{1}(1600) signal cannot be accounted for by the Deck effect Deck:1964hm . A reanalysis of the COMPASS data with the coupled-channel approach also supports that the π1(1600)\pi_{1}(1600) signal should be originated from a pole structure in the scattering amplitude JPAC:2018zyd . These results have provided strong evidences for π1(1600)\pi_{1}(1600) as a well-established 1+1^{-+} hybrid candidate. In contrast, the signals for π1(1400)\pi_{1}(1400) turn out to be vague. According to the analysis of Ref. JPAC:2018zyd , there is no need for the π1(1400)\pi_{1}(1400) to be present in the ρπ\rho\pi channel.

Phenomenological studies of the 1+1^{-+} hybrid state can be found in the literature. By treating the gluonic excitation as an explicit constituent degree of freedom, phenomenological models were constructed to understand the exotic hadron spectrum or describe the mechanisms for their productions and decays Horn:1977rq ; Barnes:1982zs . Among all these efforts, the flux tube model has made a great success in accommodating the broadly adopted quark pair creation (QPC) model for the strong decays of conventional hadrons and the gluonic excitations of QCD exotics Isgur:1984bm ; Barnes:1995hc ; Page:1998gz ; Close:2003af . Calculations in the framework of QCD sum rules also provide interesting results on the properties of the light hybrid π1\pi_{1} state Zhu:1999wg ; Huang:2010dc . In Refs. Chen:2010ic the decay properties are studied for π1\pi_{1} and its non-strange isoscalar partner. In Ref. Zhang:2019ykd , it is investigated that an isoscalar with IG(JPC)=0+(1+)I^{G}(J^{PC})=0^{+}(1^{-+}) may be formed as a bound state of ηK¯K\eta\bar{K}K^{*}. However, the mass is much lower than η1(1855)\eta_{1}(1855).

There is no doubt that lattice QCD (LQCD) simulations should play a crucial role in guiding the search for the hybrid states. In Ref. Dudek:2013yja the first systematic LQCD study of the excited isoscalar meson spectra was presented. It is interesting to see the emergence of the mixing patterns between the SU(3) flavor singlet and octet such as the η\eta and η\eta^{\prime} mixing. In the 1+1^{-+} hybrid sector, some hints for the mixings between the non-strange and strange configurations are found. Meanwhile, its prediction of the isoscalar 1+1^{-+} hybrid spectrum indicates relatively higher masses than the light axial vector mesons. It implies an unusual behavior of the excitations of the gluonic degrees of freedom in comparison with the orbital excitations within conventional qq¯q\bar{q} systems.

In light of the discovery of η1(1855)\eta_{1}(1855) by BESIII besiii-hybrid ; besiii-hybrid-pwa and the LQCD simulations Dudek:2011bn ; Dudek:2013yja , we propose a nonet scheme for the 1(+)1^{-(+)} hybrid states. In this scheme π1(1600)\pi_{1}(1600) is the I=1I=1 state with the lowest mass, and η1(1855)\eta_{1}(1855) is identified as one of the I=0I=0 multiplets. The strange I=1/2I=1/2 partner is assigned to K(1680)K^{*}(1680) which is the only strange vector meson found in the vicinity of 1.61.91.6\sim 1.9 GeV mass region. Although the strange hybrid does not have a fixed charge conjugate parity, hence it cannot be easily distinguished from the conventional qq¯q\bar{q} vector meson, there is no strong reason that such an exotic object should not exist. Considering the flavor-blind property of QCD, the strange hybrid of qs¯g~q\bar{s}\tilde{g} should at least share similar dynamics as the I=1I=1 partner π1(1600)\pi_{1}(1600). In Ref. Dudek:2013yja the mass splitting between the flavor singlet and octet is found to be significant. This is attributed to the important effects from the quark annihilations in the I=0I=0 sector.

As follows, we first analyse the mixing between η1(1855)\eta_{1}(1855) and its isoscalar partner, and the mass relations among the 1(+)1^{-(+)} hybrid nonet. Two schemes, in which η1(1855)\eta_{1}(1855) is assigned to be either the higher or lower mass state in the I=0I=0 sector, are explored based on the flux tube model picture. Phenomenological consequences will be discussed in their productions and decays in several typical processes. A brief summary will be given in the end.

II Productions and decays of the 1(+)1^{-(+)} hybrid states

II.1 Emergence of the 1(+)1^{-(+)} hybrid nonet

On the SU(3) flavor basis the light hybrid mesons are described by a pair of qq¯q\bar{q} associated by gluonic quasiparticle excitations. Taking the flux tube model picture, the qq¯q\bar{q} inside hybrid mesons are separated static color sources and they are connected by the gluonic flux tube to form an overall color singlet. The transverse oscillations of the flux tube that manifests the explicit effective gluonic degrees of freedom, will give rise to energy spectrum of the hybrid mesons. As studied in the literature, the lowest energy flux tube motion has JgPC=1+J_{g}^{PC}=1^{+-}. Namely, the lightest hybrid multiplet can be formed by the relative SS-wave coupling between a gluonic lump of JgPC=1+J_{g}^{PC}=1^{+-} and a SS-wave qq¯q\bar{q} pair. With the total gluon spin JgPC=1+J_{g}^{PC}=1^{+-}, the lowest hybrid multiplets can be obtained: (0, 1, 2)+, 1(0,\ 1,\ 2)^{-+},\ 1^{--} Bali:2003jq ; Dudek:2011bn . Alternatively, in the constituent gluon picture the lowest energy flux tube excitation can be described by the motion of quasigluon in a PP wave with respect to the SS-wave qq¯q\bar{q}.

The gluonic excitations additive to the SS-wave constituent qq¯q\bar{q} configuration suggests that for each SS-wave qq¯q\bar{q} pair, there should exist an SU(3) flavor nonet as the eigenstates of the corresponding Hamiltonian. For the same coupling mode involving the gluonic lump, these states can be related to each other by the Gell-Mann-Okubo mass relation similar to that for the ground states in the qq¯q\bar{q} scenario. This conjecture may have a caveat when the strange multiplets are included. Since the charged and strange states do not have the fixed CC parity, it may raise the question whether a nonet scheme makes sense or not. Note that signals for charged π1(1600)\pi_{1}(1600) have been seen in the decay channels of ρ0π\rho^{0}\pi^{-} COMPASS:2009xrl and ηπ\eta^{\prime}\pi^{-}  E852:2001ikk ; COMPASS:2014vkj . Similar dynamics should appear in the strange sector and a nonet structure among the 1(+)1^{-(+)} multiplets should be a good guidance for a better understanding of the underlying dynamics.

Taking the 1+1^{-+} hybrid as an example, it should contain flavor multiplets as follows:

π1+,π1,π10\displaystyle\pi_{1}^{+},\ \pi_{1}^{-},\ \pi_{1}^{0} :\displaystyle: ud¯g~,du¯g~,12(uu¯dd¯)g~,\displaystyle u\bar{d}\tilde{g},\ d\bar{u}\tilde{g},\ \frac{1}{\sqrt{2}}(u\bar{u}-d\bar{d})\tilde{g}\ , (1)
η1(8)\displaystyle\eta_{1}^{(8)} :\displaystyle: 16(uu¯+dd¯2ss¯)g~,\displaystyle\frac{1}{\sqrt{6}}(u\bar{u}+d\bar{d}-2s\bar{s})\tilde{g}\ , (2)
η1(1)\displaystyle\eta_{1}^{(1)} :\displaystyle: 13(uu¯+dd¯+ss¯)g~,\displaystyle\frac{1}{\sqrt{3}}(u\bar{u}+d\bar{d}+s\bar{s})\tilde{g}\ , (3)
K+,K0,K,K¯0\displaystyle K^{*+},\ K^{*0},\ K^{*-},\ \bar{K}^{*0} :\displaystyle: us¯g~,ds¯g~,su¯g~,sd¯g~,\displaystyle u\bar{s}\tilde{g},\ d\bar{s}\tilde{g},\ s\bar{u}\tilde{g},\ s\bar{d}\tilde{g}\ , (4)

where g~\tilde{g} represents the gluonic lump with JgPC=1+J_{g}^{PC}=1^{+-}. For the flavor octet η1(8)\eta_{1}^{(8)} and singlet η1(1)\eta_{1}^{(1)} with isospin I=0I=0, they may mix with each other to form the corresponding physical states similar to the familiar η\eta-η\eta^{\prime} mixing.

Considering the mixing between the hybrid flavor singlet and octet, the physical states can be expressed as

(η1Lη1H)\displaystyle\left(\begin{array}[]{c}\eta_{1L}\\ \eta_{1H}\end{array}\right) =\displaystyle= (cosθsinθsinθcosθ)(η1(8)η1(1))=(cosαsinαsinαcosα)(nn¯g~ss¯g~),\displaystyle\left(\begin{array}[]{cc}\cos\theta&-\sin\theta\\ \sin\theta&\cos\theta\end{array}\right)\left(\begin{array}[]{c}\eta_{1}^{(8)}\\ \eta_{1}^{(1)}\end{array}\right)=\left(\begin{array}[]{cc}\cos\alpha&-\sin\alpha\\ \sin\alpha&\cos\alpha\end{array}\right)\left(\begin{array}[]{c}n\bar{n}\tilde{g}\\ s\bar{s}\tilde{g}\end{array}\right)\ , (15)

where θ\theta is the mixing angle between the flavor octet and singlet, and α\alpha is the mixing angle defined on the flavor basis nn¯g~n\bar{n}\tilde{g} (with nn¯(uu¯+dd¯)/2n\bar{n}\equiv(u\bar{u}+d\bar{d})/\sqrt{2}) and ss¯g~s\bar{s}\tilde{g}.

The Gell-Mann-Okubo relation can provide a constraint on the mixing angle θ\theta via the following equation:

tanθ\displaystyle\tan\theta =\displaystyle= 4mKmπ13mη1L22(mπ1mK),\displaystyle\frac{4m_{K^{*}}-m_{\pi_{1}}-3m_{\eta_{1L}}}{2\sqrt{2}(m_{\pi_{1}}-m_{K^{*}})}\ , (16)

where η1L\eta_{1L} is the lower mass state in Eq. (15) and the sign of θ\theta can be determined here. We note that the same relation is also satisfied for the quadratic masses. The Gell-Mann-Okubo relation also leads to the following mass relation,

(mη1H+mη1L)(4mKmπ1)3mη1Hmη1L\displaystyle(m_{\eta_{1H}}+m_{\eta_{1L}})(4m_{K^{*}}-m_{\pi_{1}})-3m_{\eta_{1H}}m_{\eta_{1L}} =\displaystyle= 8mK28mKmπ1+3mπ12,\displaystyle 8m_{K^{*}}^{2}-8m_{K^{*}}m_{\pi_{1}}+3m_{\pi_{1}}^{2}\ , (17)

which is symmetric for η1L\eta_{1L} and η1H\eta_{1H} although it is the lower mass state η1L\eta_{1L} defined in Eq. (15) to appear in Eq. (16). With the masses of π1(1600)\pi_{1}(1600) and η1(1855)\eta_{1}(1855) as the input for Eqs. (16) and (17), we are still unable to determine these three quantities, i.e. θ\theta, mη1H/mη1Lm_{\eta_{1H}}/m_{\eta_{1L}} and mKm_{K^{*}}. Also, it is unclear whether η1(1855)\eta_{1}(1855) is the lower or higher mass state in Eq. (15). However, we will show later that the ηη\eta\eta^{\prime} channel is informative to impose constraint on the determination of the 1(+)1^{-(+)} nonet.

II.2 1(+)1^{-(+)} nonet decays into pseudoscalar meson pairs

The flavor-blindness of the strong interactions also allows us to relate the SU(3) decay channels together Close:2000yk ; Close:2005vf ; Zhao:2007ze ; Zhao:2006cx . Considering the two-body decay of η1L\eta_{1L} and η1H\eta_{1H} into pseudoscalar meson pair PPPP^{\prime} 333Due to Bose symmetry, the 1+1^{-+} hybrid cannot decay into two identical mesons. Namely, the decays into π0π0\pi^{0}\pi^{0}, ηη\eta\eta, and ηη\eta^{\prime}\eta^{\prime} are forbidden. Also, the GG-parity conservation will forbid the decays of π1\pi_{1} and η1\eta_{1} into ππ\pi\pi and KK¯K\bar{K}. , two independent transition mechanisms can be identified and they are illustrated by Fig. 1 (a) and (b). The transition of Fig. 1 (a) represents the flux tube string breaking with the quark pair creation. It is similar to the decay of a conventional qq¯q\bar{q} state into two mesons by the quark pair creation (QPC) mechanism. In the flux tube scenario it corresponds to the flux excitation mode along the displacement between the quark and anti-quark, for which the potential is denoted as V^L\hat{V}_{L}. The transition of Fig. 1 (b) corresponds to the flux excitation mode transverse to the displacement between the quark and anti-quark. The quark pair created from this mode will recoil the initial color-octet qq¯q\bar{q} via the transverse flux motion. For a conventional qq¯q\bar{q} decay via the P03{}^{3}P_{0} QPC mechanism, the kinematic regime as Fig. 1 (b) will be relatively suppressed with respect to Fig. 1 (a). Since in such a case, in order to balance the color, an additional relatively-hard gluon will be exchanged between the recoiled qq¯q\bar{q} and the created qq¯q\bar{q}. In contrast, such a transition in the hybrid decay can naturally occur via the transverse mode of the flux tube oscillations Kokoski:1985is . Namely, the created qq¯q\bar{q} can easily get the color balanced by soft gluon exchanges which can be absorbed into the effective potential without suppression. Such a transition through the transverse mode of the flux tube motions can be parametrized by the effective potential V^T\hat{V}_{T}.

Refer to caption
Refer to caption
Figure 1: Illustration of the 1(+)1^{-(+)} isoscalar hybrid decays into two mesons.

The transition amplitude for a 1+1^{-+} hybrid of qq¯g~q\bar{q}\tilde{g} decaying into two pseudoscalar mesons can then be expressed as

a\displaystyle{\cal M}_{a} =\displaystyle= (q1q¯4)M1(q3q¯2)M2|V^L|q1q¯2g~g1|𝐤|,\displaystyle\langle(q_{1}\bar{q}_{4})_{M_{1}}(q_{3}\bar{q}_{2})_{M_{2}}|\hat{V}_{L}|q_{1}\bar{q}_{2}\tilde{g}\rangle\equiv g_{1}|{\bf k}|\ , (18)

and

b\displaystyle{\cal M}_{b} =\displaystyle= (q1q¯2)M1(q3q¯4)M2|V^T|q1q¯2g~g2|𝐤|,\displaystyle\langle(q_{1}\bar{q}_{2})_{M_{1}}(q_{3}\bar{q}_{4})_{M_{2}}|\hat{V}_{T}|q_{1}\bar{q}_{2}\tilde{g}\rangle\equiv g_{2}|{\bf k}|\ , (19)

for these two decay modes, respectively. In the above two equations, 𝐤{\bf k} is the three-vector momentum of the final-state meson in the c.m. frame of the hybrid, and the quarks (anti-quarks) are the non-strange quarks (anti-quarks). Note that the QPC only contributes to a flavor singlet g~(uu¯+dd¯+ss¯)/3\tilde{g}\to(u\bar{u}+d\bar{d}+s\bar{s})/\sqrt{3}. We mention that when the ss¯s\bar{s} pair is created, an SU(3) flavor symmetry breaking parameter will be included. Also, in the above two amplitudes the interchanges of the final-state hadron indices are implied.

This parametrization leads to a connection among the couplings of an initial hybrid state to different SU(3) channels, and they are collected in Table 1. Interesting features with the hybrid nonet decays can be learned as follows:

  • It is rather clear that if the final states do not contain isoscalar mesons, the transitions will be via the string breaking potential V^L\hat{V}_{L} along the displacement between the quark and anti-quark. Namely, the transitions are similar to the conventional P03{}^{3}P_{0} process. For KK^{*} decays into KπK\pi, it will be difficult to distinguish it from the conventional qq¯q\bar{q} vector mesons.

  • For the π1\pi_{1} and KK^{*} decays into η\eta or η\eta^{\prime} plus a I0I\neq 0 state, such as π10ηπ0\pi_{1}^{0}\to\eta\pi^{0} and ηπ0\eta^{\prime}\pi^{0}, the couplings involve interferences between processes of Fig. 1 (a) and (b). Since the mixing angle between η\eta and η\eta^{\prime} is αP42\alpha_{P}\simeq 42^{\circ}, the couplings for the channels between η\eta and η\eta^{\prime} would be very different.

  • η1L\eta_{1L} and η1H\eta_{1H} decays into ππ\pi\pi and KK¯K\bar{K} are forbidden by the Bose symmetry and GG-parity conservation. They can only access ηη\eta\eta^{\prime} via the octet and singlet mixing. The coupling strengths have non-trivial dependence of the mixing angle α\alpha. One can see that the decay pattern for these channels in a combined analysis should be sensitive to the value of α\alpha.

Table 1: The coupling constants for the 1(+)1^{-(+)} hybrid nonet decays into pseudoscalar meson pairs. The couplings for the negative charge states are implied. The SU(3) flavor symmetry breaking parameter RR is also included.
Processes Couplings
π10ηπ0\pi_{1}^{0}\to\eta\pi^{0} 12(g1+g2)cosαPRg2sinαP\frac{1}{\sqrt{2}}(g_{1}+g_{2})\cos\alpha_{P}-Rg_{2}\sin\alpha_{P}
π10ηπ0\pi_{1}^{0}\to\eta^{\prime}\pi^{0} 12(g1+g2)sinαP+Rg2cosαP\frac{1}{\sqrt{2}}(g_{1}+g_{2})\sin\alpha_{P}+Rg_{2}\cos\alpha_{P}
π1+ηπ+\pi_{1}^{+}\to\eta\pi^{+} 2(g1+g2)cosαPRg2sinαP\sqrt{2}(g_{1}+g_{2})\cos\alpha_{P}-Rg_{2}\sin\alpha_{P}
π1+ηπ+\pi_{1}^{+}\to\eta^{\prime}\pi^{+} 2(g1+g2)sinαP+Rg2cosαP\sqrt{2}(g_{1}+g_{2})\sin\alpha_{P}+Rg_{2}\cos\alpha_{P}
η1Lηη\eta_{1L}\to\eta\eta^{\prime} 12(g1+g2)sin2αP(cosα+Rsinα)+g2cos2αP(Rcosαsinα)\frac{1}{2}(g_{1}+g_{2})\sin 2\alpha_{P}(\cos\alpha+R\sin\alpha)+g_{2}\cos 2\alpha_{P}(R\cos\alpha-\sin\alpha)
η1Hηη\eta_{1H}\to\eta\eta^{\prime} 12(g1+g2)sin2αP(sinαRcosα)+g2cos2αP(Rsinα+cosα)\frac{1}{2}(g_{1}+g_{2})\sin 2\alpha_{P}(\sin\alpha-R\cos\alpha)+g_{2}\cos 2\alpha_{P}(R\sin\alpha+\cos\alpha)
K+K+π0K^{*+}\to K^{+}\pi^{0} 12g1\frac{1}{\sqrt{2}}g_{1}
K+K0π+K^{*+}\to K^{0}\pi^{+} g1g_{1}
K+K+ηK^{*+}\to K^{+}\eta g1(12cosαPRsinαP)+g2(2cosαPRsinαP)g_{1}(\frac{1}{\sqrt{2}}\cos\alpha_{P}-R\sin\alpha_{P})+g_{2}(\sqrt{2}\cos\alpha_{P}-R\sin\alpha_{P})
K+K+ηK^{*+}\to K^{+}\eta^{\prime} g1(12sinαP+RcosαP)+g2(2sinαP+RcosαP)g_{1}(\frac{1}{\sqrt{2}}\sin\alpha_{P}+R\cos\alpha_{P})+g_{2}(\sqrt{2}\sin\alpha_{P}+R\cos\alpha_{P})

II.3 J/ψγη1γηηJ/\psi\to\gamma\eta_{1}\to\gamma\eta\eta^{\prime}

Refer to caption
Figure 2: Illustration of the 1+1^{-+} isoscalar hybrid production in J/ψγη1J/\psi\to\gamma\eta_{1}.

A typical process for the production of a JPC=1+J^{PC}=1^{-+} hybrid in the J/ψJ/\psi radiative decays is illustrated by Fig. 2. It shows that the annihilations of the charm and anti-charm quark can create a pair of light SS-wave qq¯q\bar{q} associated by a constituent gluon in a relative PP-wave to the qq¯q\bar{q}. At the hadronic level, the Lagrangian for a general vector-vector-vector field interaction at the leading-order can be described by

VVV=igVVV(V1,νμV2νV3,μ+V1,μV2νμV3,ν+V2,μV3νμV1,ν),\mathcal{L}_{VVV}=ig_{VVV}(V_{1,\nu}\overleftrightarrow{\partial^{\mu}}V_{2}^{\nu}V_{3,\mu}+V_{1,\mu}V_{2}^{\nu}\overleftrightarrow{\partial^{\mu}}V_{3,\nu}+V_{2,\mu}V_{3}^{\nu}\overleftrightarrow{\partial^{\mu}}V_{1,\nu})\ , (20)

where V1V_{1}, V2V_{2}, V3V_{3} denotes the vector fields. For the radiative decay of J/ψγη1J/\psi\to\gamma\eta_{1}, since the photon is transversely polarized, the above Lagrangian will reduce to the following form:

J/ψγη1=igJ/ψη1γFμνVJ/ψμVη1ν,{\cal L}_{J/\psi\to\gamma\eta_{1}}=ig_{J/\psi\eta_{1}\gamma}F_{\mu\nu}V_{J/\psi}^{\mu}V_{\eta_{1}}^{\nu}\ , (21)

where FμνμAννAμF_{\mu\nu}\equiv\partial_{\mu}A_{\nu}-\partial_{\nu}A_{\mu}, and the vector fields VJ/ψV_{J/\psi}, AA, and Vη1V_{\eta_{1}} stand for the initial J/ψJ/\psi, final-state photon, and hybrid η1\eta_{1} fields, respectively; gJ/ψη1γg_{J/\psi\eta_{1}\gamma} is the coupling constant. Note that the leading transition of J/ψγη1J/\psi\to\gamma\eta_{1} is via a PP wave. In the center of mass (c.m.) frame of J/ψJ/\psi the squared transition amplitudes for the two I=0I=0 states can be expressed like below:

|i(J/ψγη1L)|2\displaystyle|i{\cal M}(J/\psi\to\gamma\eta_{1L})|^{2} \displaystyle\propto gJ/ψη1Lγ2|𝐪L|2(1+mJ/ψ2/mη1L2),\displaystyle g_{J/\psi\eta_{1L}\gamma}^{2}|{\bf q}_{L}|^{2}(1+m_{J/\psi}^{2}/m_{\eta_{1L}}^{2})\ , (22)
|i(J/ψγη1H)|2\displaystyle|i{\cal M}(J/\psi\to\gamma\eta_{1H})|^{2} \displaystyle\propto gJ/ψη1Hγ2|𝐪H|2(1+mJ/ψ2/mη1H2),\displaystyle g_{J/\psi\eta_{1H}\gamma}^{2}|{\bf q}_{H}|^{2}(1+m_{J/\psi}^{2}/m_{\eta_{1H}}^{2})\ , (23)

where 𝐪L{\bf q}_{L} and 𝐪H{\bf q}_{H} are the three-vector momenta of η1L\eta_{1L} and η1H\eta_{1H} in the J/ψJ/\psi rest frame, respectively. The subscripts, “LL” and “HH”, stand for the low and high mass states, respectively. The two coupling constants, gJ/ψη1Lγg_{J/\psi\eta_{1L}\gamma} and gJ/ψη1Hγg_{J/\psi\eta_{1H}\gamma}, which account for the production mechanism for these two isoscalars, can be parametrized out:

gJ/ψη1Lγ\displaystyle g_{J/\psi\eta_{1L}\gamma} =\displaystyle= g0(2cosαRsinα),\displaystyle g_{0}(\sqrt{2}\cos\alpha-R\sin\alpha)\ , (25)
gJ/ψη1Hγ\displaystyle g_{J/\psi\eta_{1H}\gamma} =\displaystyle= g0(2sinα+Rcosα),\displaystyle g_{0}(\sqrt{2}\sin\alpha+R\cos\alpha)\ , (26)

where Rfπ/fK0.93R\simeq f_{\pi}/f_{K}\simeq 0.93 indicates the SU(3) flavor symmetry breaking effects in the production of the ss¯s\bar{s} pair in comparison with the non-strange qq¯q\bar{q} pairs, and g0g_{0} describes the coupling strength for the production of a light hybrid configuration qq¯g~q\bar{q}\tilde{g} of JPC=1+J^{PC}=1^{-+} in the J/ψJ/\psi radiative decays. It can be expressed as

g0(qq¯g~)1+|H^em|J/ψ,g_{0}\equiv\langle(q\bar{q}\tilde{g})_{1^{-+}}|\hat{H}_{em}|J/\psi\rangle\ , (27)

where H^em\hat{H}_{em} contains the dynamics for the transition of Fig. 2.

The coupling relation in Eq. (25) leads to the relative production rate for η1L\eta_{1L} and η1H\eta_{1H} as follows:

rL/H\displaystyle r_{L/H} \displaystyle\equiv BR(J/ψγη1L)BR(J/ψγη1H)=(|𝐪L||𝐪H|)3(2cosαRsinα)2(2sinα+Rcosα)2mη1H2(mJ/ψ2+mη1L2)mη1L2(mJ/ψ2+mη1H2),\displaystyle\frac{BR(J/\psi\to\gamma\eta_{1L})}{BR(J/\psi\to\gamma\eta_{1H})}=\left(\frac{|{\bf q}_{L}|}{|{\bf q}_{H}|}\right)^{3}\frac{(\sqrt{2}\cos\alpha-R\sin\alpha)^{2}}{(\sqrt{2}\sin\alpha+R\cos\alpha)^{2}}\frac{m_{\eta_{1H}}^{2}(m_{J/\psi}^{2}+m_{\eta_{1L}}^{2})}{m_{\eta_{1L}}^{2}(m_{J/\psi}^{2}+m_{\eta_{1H}}^{2})}\ , (28)

which seems to be sensitive to the mixing angle α\alpha. Note that, in Ref. besiii-hybrid ; besiii-hybrid-pwa the η1(1855)\eta_{1}(1855) signal is actually observed in its decays into ηη\eta\eta^{\prime}. Moreover, the PWA results suggest that only one I=0I=0 hybrid state has been clearly seen in the 1+1^{-+} partial wave amplitude. As shown in Subsection II.2, the decays of η1L\eta_{1L} and η1H\eta_{1H} into ηη\eta\eta^{\prime} are strongly correlated with the mixing angle α\alpha and mechanisms for the flux tube breaking. It means that the following branching ratio fractions can serve as constraints on the mixing angle:

Scheme-I :\displaystyle: Rη1L/η1(1855)BR(J/ψγη1Lγηη)BR(J/ψγη1(1855)γηη)<10%,\displaystyle R_{\eta_{1L}/\eta_{1}(1855)}\equiv\frac{BR(J/\psi\to\gamma\eta_{1L}\to\gamma\eta\eta^{\prime})}{BR(J/\psi\to\gamma\eta_{1}(1855)\to\gamma\eta\eta^{\prime})}<10\%\ , (29)

and

Scheme-II :\displaystyle: Rη1H/η1(1855)BR(J/ψγη1Hγηη)BR(J/ψγη1(1855)γηη)<10%,\displaystyle R_{\eta_{1H}/\eta_{1}(1855)}\equiv\frac{BR(J/\psi\to\gamma\eta_{1H}\to\gamma\eta\eta^{\prime})}{BR(J/\psi\to\gamma\eta_{1}(1855)\to\gamma\eta\eta^{\prime})}<10\%\ , (30)

where we have assigned η1(1855)\eta_{1}(1855) as either the higher mass state (Scheme-I) or the lower mass state (Scheme-II). The relative rate 10%10\% is the production upper limit for the partner of η1(1855)\eta_{1}(1855) from the experimental measurement besiii-hybrid ; besiii-hybrid-pwa .

With the production and decay couplings extracted earlier, the general form for the joint branching ratio fraction can be expressed as

Rη1L/η1H\displaystyle R_{\eta_{1L}/\eta_{1H}} =\displaystyle= (|𝐪L||𝐪H|)3(2cosαRsinα)2(2sinα+Rcosα)2mη1H2(mJ/ψ2+mη1L2)mη1L2(mJ/ψ2+mη1H2)(|𝐤L||𝐤H|)3(ΓHmη1HΓLmη1L)2\displaystyle\left(\frac{|{\bf q}_{L}|}{|{\bf q}_{H}|}\right)^{3}\frac{(\sqrt{2}\cos\alpha-R\sin\alpha)^{2}}{(\sqrt{2}\sin\alpha+R\cos\alpha)^{2}}\frac{m_{\eta_{1H}}^{2}(m_{J/\psi}^{2}+m_{\eta_{1L}}^{2})}{m_{\eta_{1L}}^{2}(m_{J/\psi}^{2}+m_{\eta_{1H}}^{2})}\left(\frac{|{\bf k}_{L}|}{|{\bf k}_{H}|}\right)^{3}\left(\frac{\Gamma_{H}m_{\eta_{1H}}}{\Gamma_{L}m_{\eta_{1L}}}\right)^{2} (31)
×\displaystyle\times [(1+δ)tan2αP(cosα+Rsinα)+2δ(Rcosαsinα)]2[(1+δ)tan2αP(sinαRcosα)+2δ(Rsinα+cosα)]2,\displaystyle\frac{[(1+\delta)\tan 2\alpha_{P}(\cos\alpha+R\sin\alpha)+2\delta(R\cos\alpha-\sin\alpha)]^{2}}{[(1+\delta)\tan 2\alpha_{P}(\sin\alpha-R\cos\alpha)+2\delta(R\sin\alpha+\cos\alpha)]^{2}}\ ,

where ΓL\Gamma_{L} and ΓH\Gamma_{H} are the total widths of the lower and higher mass states, respectively; 𝐪L,H{\bf q}_{L,H} and 𝐤L,H{\bf k}_{L,H} are the three-vector momenta of the photon and pseudoscalar meson in the rest frames of J/ψJ/\psi and ηL,H\eta_{L,H}, respectively; δg2/g1\delta\equiv g_{2}/g_{1} indicates the relative strength between the two decay mechanisms for the flux tube breaking. As discussed earlier, |δ|1|\delta|\simeq 1 is for the hybrid decays, while |δ|<<1|\delta|<<1 for conventional qq¯q\bar{q} decays. In Eq. (31) if we approximate ΓH/ΓL1{\Gamma_{H}}/{\Gamma_{L}}\simeq 1, ratio Rη1L/η1HR_{\eta_{1L}/\eta_{1H}} will strongly depend on α\alpha and δ\delta.

II.4 Results and analyses

Before we go to the detailed studies of the two schemes, we briefly summarize the present experimental information on the strange vector mesons. As listed by the Particle Data Group (PDG) ParticleDataGroup:2020ssz , two excited KK^{*} states are observed in experiment, i.e. K(1410)K^{*}(1410) and K(1680)K^{*}(1680). While K(1410)K^{*}(1410) can be well accommodated by the first radial excitations of the vector meson nonet, the property of K(1680)K^{*}(1680) is far from well explored. Note that the second radial excitations of the isoscalar pseudoscalar mesons can be occupied by η(1760)\eta(1760) and η(1860)\eta(1860) in the Regge trajectory Yu:2011ta , the mass of K(1680)K^{*}(1680) as the second radial excitation in the conventional qq¯q\bar{q} vector nonet seems to be too small. We also note that the strange pseudoscalar partner in the second radial excitation nonet has not yet been established in experiment though K(1630)K(1630) could be a candidate ParticleDataGroup:2020ssz . In the following analysis we first treat K(1680)K^{*}(1680) as the strange partner of the 1(+)1^{-(+)} nonet and examine whether it fits the constraint. If not, we then investigate the mass correlation of KK^{*} with the mixing angle and other multiplets as required by the Gell-Mann-Okubo relation.

II.4.1 Scheme-I

With the η1(1855)\eta_{1}(1855) assigned as the higher mass state, and π1(1600)\pi_{1}(1600) and K(1680)K^{*}(1680) assigned as the I=1I=1 and strange partner, respectively, we extract mη1L=1712.5±8.7m_{\eta_{1L}}=1712.5\pm 8.7 MeV from Eq. (17), and the mixing angle α=30±13\alpha=30^{\circ}\pm 13^{\circ}. The uncertainties are given by the mass uncertainties from π1(1600)\pi_{1}(1600) and K(1680)K^{*}(1680) via the Gell-Mann-Okubo relation. We note that the PDG values ParticleDataGroup:2020ssz are adopted for the masses of these two states, i.e. mπ1=1661±13m_{\pi_{1}}=1661\pm 13 MeV and mK=1718±18m_{K^{*}}=1718\pm 18 MeV. From Eq. (16), we can extract the correlation between the mixing angle and the KK^{*} mass, and the results are presented in Fig. 3.

Refer to caption
Figure 3: The correlation of the mixing angle α\alpha with the KK^{*} mass. The uncertainties are due to the mass uncertainties for those input states. The shadowed area indicates the mass range of KK^{*} from PDG ParticleDataGroup:2020ssz .

Although the uncertainties of the mixing angle α\alpha seem to be rather large, it indicates significant mixings between the flavor octet and singlet, and apparently deviates from the ideal mixing. This seems to be a necessary consequence if there is only one I=0I=0 hybrid state observed in the ηη\eta\eta^{\prime} channel in J/ψγηηJ/\psi\to\gamma\eta\eta^{\prime}. Nevertheless, it favors the hybrid scenario to have important contributions from the transverse mode of the flux tube motions. To illustrate this, we first look at Eq. (28) where by taking the limit of ideal mixing, i.e. α=0\alpha=0^{\circ}, the production ratio rL/H2r_{L/H}\simeq 2 can be obtained. Note that the ratio rL/Hr_{L/H} is insensitive to the phase space factor and the SU(3) flavor symmetry breaking parameter RR.

In the case that η1(1855)\eta_{1}(1855) is the higher mass state, it is the ratio Rη1L/η1HR_{\eta_{1L}/\eta_{1H}} defined in Eq. (31) can be compared with the experimental observables with Rη1L/η1(1855)<10%R_{\eta_{1L}/\eta_{1}(1855)}<10\%. In the ideal mixing limit, one has

Rη1L/η1(1855)\displaystyle R_{\eta_{1L}/\eta_{1}(1855)} \displaystyle\simeq (|𝐪L||𝐪H|)3(|𝐤L||𝐤H|)3mη1H2(mJ/ψ2+mη1L2)mη1L2(mJ/ψ2+mη1H2)(ΓHmHΓLmL)22R2[(1+δ)tan2αP+2RδR(1+δ)tan2αP2δ]2.\displaystyle\left(\frac{|{\bf q}_{L}|}{|{\bf q}_{H}|}\right)^{3}\left(\frac{|{\bf k}_{L}|}{|{\bf k}_{H}|}\right)^{3}\frac{m_{\eta_{1H}}^{2}(m_{J/\psi}^{2}+m_{\eta_{1L}}^{2})}{m_{\eta_{1L}}^{2}(m_{J/\psi}^{2}+m_{\eta_{1H}}^{2})}\left(\frac{\Gamma_{H}m_{H}}{\Gamma_{L}m_{L}}\right)^{2}\frac{2}{R^{2}}\left[\frac{(1+\delta)\tan 2\alpha_{P}+2R\delta}{R(1+\delta)\tan 2\alpha_{P}-2\delta}\right]^{2}\ . (32)

Note that the product (|𝐪L||𝐪H|)3(|𝐤L||𝐤H|)3mη1H2(mJ/ψ2+mη1L2)mη1L2(mJ/ψ2+mη1H2)(ΓHmHΓLmL)2\left(\frac{|{\bf q}_{L}|}{|{\bf q}_{H}|}\right)^{3}\left(\frac{|{\bf k}_{L}|}{|{\bf k}_{H}|}\right)^{3}\frac{m_{\eta_{1H}}^{2}(m_{J/\psi}^{2}+m_{\eta_{1L}}^{2})}{m_{\eta_{1L}}^{2}(m_{J/\psi}^{2}+m_{\eta_{1H}}^{2})}\left(\frac{\Gamma_{H}m_{H}}{\Gamma_{L}m_{L}}\right)^{2} actually enhances the ratio, and tan2αP10\tan 2\alpha_{P}\simeq 10 will further push up the ratio. It thus relies on the value of δ\delta to decide the value of Rη1L/η1HR_{\eta_{1L}/\eta_{1H}}. As discussed earlier, for conventional qq¯q\bar{q} meson decays, one would expect δ0\delta\to 0. It actually leads to Rη1L/η1H>1R_{\eta_{1L}/\eta_{1H}}>1 which is in contradiction with the experimental observation. For the hybrid decays, the transverse mode of the flux tube motions plays an important role in the decays. It means |δ|1|\delta|\simeq 1, or even to be the dominant transition mechanism with |δ|>1|\delta|>1. Eventually, to have Rη1L/η1(1855)<10%R_{\eta_{1L}/\eta_{1}(1855)}<10\% as suggested by the experimental data, one finds δ\delta should take a negative value and the absolute value is at 𝒪(1){\cal O}(1).

In Fig. 4, with the mixing angle α\alpha within its uncertainty range, i.e. α=30±13\alpha=30^{\circ}\pm 13^{\circ}, we plot the ratios rL/Hr_{L/H} and Rη1L/η1(1855)R_{\eta_{1L}/\eta_{1}(1855)}. For demonstration, we adopt δ=0.8,1.0,1.2\delta=-0.8,\ -1.0,\ -1.2 to calculate Rη1L/η1(1855)R_{\eta_{1L}/\eta_{1}(1855)}. It shows that rL/Hr_{L/H} is not sufficiently suppressed while the decays via the transverse mode play a dominant role to suppress the low-mass state. Although we cannot give a precise value for δ\delta based on the present experimental results, we find that the relative sign between g1g_{1} and g2g_{2} and their relative strength can consistently reflect the hybrid features.

Refer to caption
Figure 4: The dependence of the ratios rL/Hr_{L/H} and Rη1L/η1(1855)R_{\eta_{1L}/\eta_{1}(1855)} on the mixing angle α\alpha within the preferred range of α(17, 43)\alpha\in(17^{\circ},\ 43^{\circ}). In Scheme-I η(1855)\eta(1855) is the high-mass state. On the left panel the solid line is for rL/Hr_{L/H}, while on the right panel the dashed, dot-dashed, and dotted lines correspond to the ratio Rη1L/η1(1855)R_{\eta_{1L}/\eta_{1}(1855)} with δ=0.8,1.0,1.2\delta=-0.8,\ -1.0,\ -1.2, respectively.

In Fig. 5, we illustrate the 1(+)1^{-(+)} nonet in Scheme-I. The shadowed ranges are the mass uncertainties and the central dashed lines denote the preferred mass.

Refer to caption
Figure 5: The 1(+)1^{-(+)} hybrid nonet with mass uncertainties determined in Scheme-I. Namely, η1(1855)\eta_{1}(1855) is assigned as the higher mass state with I=0I=0.

II.4.2 Scheme-II

With the η1(1855)\eta_{1}(1855) assigned as the lower mass state, and keep π1(1600)\pi_{1}(1600) as the I=1I=1 partner, the determination of the lower I=0I=0 state will be correlated with the mass of the strange partner differently. It means that K(1680)K^{*}(1680) is no longer suitable for being the strange partner of the nonet. This can be seen easily via Eq. (17) which is symmetric to η1L\eta_{1L} and η1H\eta_{1H}. If the same KK^{*} mass is taken, the solution for the other η1\eta_{1} mass will be a lower one as in Scheme-I, and η1(1855)\eta_{1}(1855) will keep to be the higher mass state.

Searching for the higher mass partner of η1(1855)\eta_{1}(1855) thus needs a higher KK^{*} mass as input. As discussed earlier, so far we still lack experimental information about the vector strange spectrum. Fortunately, if we impose again the BESIII observation as a constraint, we should have the inverse form of Eq. (31) to satisfy Eq. (30). In such a case, we find that the mixing angle is still located around α(25,45)\alpha\in(25^{\circ},45^{\circ}) corresponding to mK1.831.90m_{K^{*}}\simeq 1.83\sim 1.90 GeV. Meanwhile, it shows that δ\delta is still at 𝒪(1){\cal O}(1), but favors a positive sign. In fact, the sign and magnitude of δ\delta turn out to be very sensitive to the experimental constraint which can be seen analytically via Eq. (31).

Similar to Fig. 3, we plot in Fig. 6 the correlation between the mixing angle α\alpha and the KK^{*} mass. The preferred KK^{*} mass is mK1.831.90m_{K^{*}}\simeq 1.83\sim 1.90 GeV corresponding to the range of α=2545\alpha=25^{\circ}\sim 45^{\circ}.

Refer to caption
Figure 6: The correlation of the mixing angle α\alpha with the KK^{*} mass in Scheme-II. The uncertainties are due to the mass uncertainties for those input states.

In Fig. 7, we present the results for rH/Lr_{H/L} and Rη1H/η1(1855)R_{\eta_{1H}/\eta_{1}(1855)} in terms of the mixing angle α\alpha within its uncertainty range, i.e. α=2545\alpha=25^{\circ}\sim 45^{\circ}. It is interesting to see that in Scheme-II the production of η(1855)\eta(1855) in J/ψγη1L,1HJ/\psi\to\gamma\eta_{1L,1H} as the low-mass state is actually comparable with the higher one. It is the decay transition of η1Lηη\eta_{1L}\to\eta\eta^{\prime} that strongly enhances the signal of η1(1855)\eta_{1}(1855) in the ηη\eta\eta^{\prime} channel while the higher mass state is suppressed due to its weak coupling to the ηη\eta\eta^{\prime} channel. Again, we see the dominance of the transverse mode in the hybrid decays. For demonstration, we adopt δ=0.8, 1.0, 1.2\delta=0.8,\ 1.0,\ 1.2 to calculate Rη1H/η1(1855)R_{\eta_{1H}/\eta_{1}(1855)} which are presented on the right panel of Fig. 7.

Refer to caption
Figure 7: The dependence of the ratios rH/Lr_{H/L} and Rη1H/η1(1855)R_{\eta_{1H}/\eta_{1}(1855)} on the mixing angle α\alpha within the preferred range of α(25, 45)\alpha\in(25^{\circ},\ 45^{\circ}). In Scheme-II, η1(1855)\eta_{1}(1855) is the low-mass state. On the left panel the solid line is for rH/Lr_{H/L}, while on the right panel the dashed, dot-dashed, and dotted lines correspond to the ratio Rη1H/η1(1855)R_{\eta_{1H}/\eta_{1}(1855)} with δ=0.8, 1.0, 1.2\delta=0.8,\ 1.0,\ 1.2, respectively.

In Fig. 8, we illustrate the 1(+)1^{-(+)} nonet in Scheme-II. The shadowed ranges are the mass uncertainties and the central dashed lines denote the preferred mass.

Refer to caption
Figure 8: The 1(+)1^{-(+)} hybrid nonet with mass uncertainties determined in Scheme-II. Namely, η1(1855)\eta_{1}(1855) is assigned as the lower mass state with I=0I=0.

Comparing these two nonet schemes, it shows that the transverse mode plays an important role for understanding the decay pattern observed in experiment. The relative sign between the transverse mode and the longitudinal mode should decide which scheme is the physical one. Based on the present experimental information, it is however impossible to conclude. We would look forward to further observables to provide a constraint on the sign from experiment. Meanwhile, we note that the LQCD calculations of these two decay modes may also be useful for determining their relative sign.

II.5 Predictions for J/ψVHJ/\psi\to VH

In order to further investigate the characters arising from the nonet structure of the 1(+)1^{-(+)} hybrid states, we analyse the hadronic decays of J/ψVHJ/\psi\to VH and look for signals for the I=0I=0 partner of η1(1855)\eta_{1}(1855). Here, VV stands for the vector mesons ρ\rho, ω\omega, and ϕ\phi, while HH stands for the light hybrid multiplets. This process is illustrated by Fig. 9 and the leading-order Lagrangian has been given in Eq. (20). The coupling for J/ψ[qq¯]1[qq¯g~]1+J/\psi\rightarrow[q\bar{q}]_{1^{--}}[q\bar{q}\tilde{g}]_{1^{-+}} can be parametrized as,

gP[qq¯]1[qq¯g~]1+|V^P|J/ψ,\displaystyle g_{P}\equiv\langle[q\bar{q}]_{1^{--}}[q\bar{q}\tilde{g}]_{1^{-+}}|\hat{V}_{P}|J/\psi\rangle\ , (33)

where V^P\hat{V}_{P} represents the potential for the hadronic decays of J/ψVHJ/\psi\to VH. And the detailed coupling constants for different decay channels list as following:

gJ/ψρ+π1\displaystyle g_{J/\psi\rho^{+}\pi_{1}^{-}} =\displaystyle= gP,\displaystyle g_{P},
gJ/ψωη1L\displaystyle g_{J/\psi\omega\eta_{1L}} =\displaystyle= gPcosα,\displaystyle g_{P}\cos\alpha\ ,
gJ/ψωη1H\displaystyle g_{J/\psi\omega\eta_{1H}} =\displaystyle= gPsinα,\displaystyle g_{P}\sin\alpha\ ,
gJ/ψϕη1L\displaystyle g_{J/\psi\phi\eta_{1L}} =\displaystyle= gPR2sinα,\displaystyle-g_{P}R^{2}\sin\alpha\ ,
gJ/ψϕη1H\displaystyle g_{J/\psi\phi\eta_{1H}} =\displaystyle= gPR2cosα,\displaystyle g_{P}R^{2}\cos\alpha\ ,
gJ/ψK+KH\displaystyle g_{J/\psi K^{*+}K_{H}^{*-}} =\displaystyle= gPR,\displaystyle g_{P}R\ , (34)

where RR is the SU(3) flavor symmetry breaking factor defined earlier. In this Section to distinguish the hybrid KK^{*} from K(892)K^{*}(892), we denote it as KHK^{*}_{H}. Apart from the partial wave factor (|𝐪|3\propto|{\bf q}|^{3}) which should be included for each channel and a mass function which has the same form for each channel, the branching ratio fractions among all the VHVH decay channels will be driven by the following relative strengths:

ρ+π1:ωη1L:ωη1H:ϕη1L:ϕη1H:K+KH\displaystyle\rho^{+}\pi_{1}^{-}:\omega\eta_{1L}:\omega\eta_{1H}:\phi\eta_{1L}:\phi\eta_{1H}:K^{*+}K_{H}^{*-} (35)
=\displaystyle= 1:cos2α:sin2α:R4sin2α:R4cos2α:R2.\displaystyle 1:\cos^{2}\alpha:\sin^{2}\alpha:R^{4}\sin^{2}\alpha:R^{4}\cos^{2}\alpha:R^{2}\ .

Note that for the total of ρπ\rho\pi, a factor of 3 should be multiplied to the ρ+π1\rho^{+}\pi_{1}^{-} channel, while the total of KK¯H+c.c.K^{*}\bar{K}_{H}+c.c., a factor of 4 should be multiplies to the K+KHK^{*+}K_{H}^{*-} channel.

If we take into account the effects from the partial wave factor and the SU(3) flavor symmetry breaking factor RR, we find that the ρπ1\rho\pi_{1} channel has the largest branching ratio, while the production strengths for most of the other channels are actually comparable with α30\alpha\sim 30^{\circ}. In particular, it suggests that the production of η1L\eta_{1L} and η1H\eta_{1H} are accessible in the same channel such as J/ψωηηJ/\psi\to\omega\eta\eta^{\prime}. This is different from the case of J/ψγηηJ/\psi\to\gamma\eta\eta^{\prime}.

Refer to caption
Figure 9: Illustration of the production process for the 1(+)1^{-(+)} hybrid states in J/ψVHJ/\psi\to VH where VV stands for the light vector mesons ρ\rho, ω\omega, ϕ\phi and K(892)K^{*}(892).

It should also be interesting to study the J/ψKK¯H+c.c.J/\psi\to K^{*}\bar{K}_{H}^{*}+c.c. channel. Since KHK_{H}^{*} has JP=1J^{P}=1^{-} which are the same as the radial excitation states of the vector K(892)K^{*}(892), it is difficult to identify the hybrid-like state. But as discussed earlier, the isolated K(1680)K^{*}(1680), either as a radial excitation state of K(892)K^{*}(892) or a hybrid state, will bring crucial understandings of the KK^{*} spectrum. In the hybrid scenario KHK_{H}^{*} will favor to decay into K1πKππK_{1}\pi\to K^{*}\pi\pi. It means that J/ψKK¯πππJ/\psi\to K\bar{K}\pi\pi\pi will be ideal for the search of KHK_{H}^{*}.

In Fig. 10, we plot the branching ratio fractions in Scheme-I for each channels in respect with J/ψρ+π1J/\psi\to\rho^{+}\pi_{1}^{-} for which we set it as unity, and the other channels are normalized to the ρ+π1\rho^{+}\pi_{1}^{-} channel with R=0.93R=0.93 adopted. The favored range of the mixing angle is about α(17,43)\alpha\in(17^{\circ},43^{\circ}). But a relatively broad range is plotted in Fig. 10 as an illustration. The dependence of the mixing angle produces certain patterns which makes the combined study of the VHVH channel useful for further confirmation of the 1(+)1^{-(+)} nonet.

For the results of Scheme-II, the ωη1H\omega\eta_{1H} and ϕη1H\phi\eta_{1H} thresholds are higher than the J/ψJ/\psi mass. A combined study can be done in other higher heavy quarkonium decays such as ΥVH\Upsilon\to VH.

Refer to caption
Figure 10: Predicted branching ratio fractions for BR(J/ψVH)/BR(J/ψρ+π1)BR(J/\psi\to VH)/BR(J/\psi\to\rho^{+}\pi_{1}^{-}) in terms of α\alpha in Scheme-I.

III Summary

Inspired by the observation of the isoscalar 1+1^{-+} hybrid candidate η1(1855)\eta_{1}(1855) in J/ψγη1(1855)γηηJ/\psi\to\gamma\eta_{1}(1855)\to\gamma\eta\eta^{\prime}, we investigate its SU(3) flavor partners using a parametrization method based on the flux tube model picture. We show that, although the present experimental information is still limited, it is possible to depict the 1(+)1^{-(+)} nonet of which the production and decays are consistent with the expectations of the flux tube model. We find that the observation of a single η1(1855)\eta_{1}(1855) in the ηη\eta\eta^{\prime} channel is informative and can impose quite strong constraint on the hybrid scenario. In particular, it suggests that the flavor octet and singlet mixing would be apparently deviated from the SU(3) ideal mixing which indicates the importance of the quark annihilation effects. In the flux tube model, it suggests that the transverse mode of the flux tube motions is important.

We examine two schemes for the 1(+)1^{-(+)} hybrid nonet by assigning the observed η1(1855)\eta_{1}(1855) to be either the high or low mass state with I=0I=0. In both cases, we find that the requirement that one I=0I=0 state should be highly suppressed in J/ψγηηJ/\psi\to\gamma\eta\eta^{\prime} will also impose a strong constraint on the hybrid KK^{*} mass. For the case that η1(1855)\eta_{1}(1855) is the higher mass state, K(1680)K^{*}(1680) seems to be able to fill the nonet chart reasonably well. For η1(1855)\eta_{1}(1855) being the lower mass state, a new state K(1860)K^{*}(1860) is predicted. We find that one of the main differences between these two solutions lies on the relative sign between the transverse and longitudinal mode of the gluonic motions in the decay of the I=0I=0 hybrid states. It means that additional constraint from other processes are needed. As a strongly correlated process, we suggest a combined study of J/ψVHJ/\psi\to VH to clarify the difference between these two schemes. Notice that the ρπ1\rho\pi_{1} production rate is expected to be significant and specific pattern actually arises from the hybrid scenario. Thus, further evidences for η1(1855)\eta_{1}(1855) and its partner in J/ψVHJ/\psi\to VH at BESIII would be crucial for finally establishing the 1(+)1^{-(+)} nonet.

Acknowledgements.
The authors thank Xiao-Hai Liu and Alessandro Pilloni for useful comments and discussions. This work is supported, in part, by the National Natural Science Foundation of China (Grant Nos. 11425525 and 11521505), DFG and NSFC funds to the Sino-German CRC 110 “Symmetries and the Emergence of Structure in QCD” (NSFC Grant No. 12070131001, DFG Project-ID 196253076), Strategic Priority Research Program of Chinese Academy of Sciences (Grant No. XDB34030302), and National Key Basic Research Program of China under Contract No. 2020YFA0406300.

References

  • [1] M. Ablikim et al., BESIII Collaboration, arXiv:220200621[hep-ex].
  • [2] M. Ablikim et al., BESIII Collaboration, arXiv:220200623[hep-ex].
  • [3] G. T. Condo et al. [SLAC Hybrid Facility Photon], Phys. Rev. D 43, 2787-2791 (1991) doi:10.1103/PhysRevD.43.2787
  • [4] G. M. Beladidze et al. [VES], Phys. Lett. B 313, 276-282 (1993) doi:10.1016/0370-2693(93)91224-B
  • [5] J. H. Lee, S. U. Chung, H. G. Kirk, D. P. Weygand, H. J. Willutzki, R. Crittenden, A. Dzierba, P. Smith, D. Zieminska and D. Son, et al. Phys. Lett. B 323, 227-232 (1994) doi:10.1016/0370-2693(94)90296-8
  • [6] H. Aoyagi, S. Fukui, T. Hasegawa, N. Hayashi, N. Horikawa, J. Iizuka, S. Inaba, S. Ishimoto, Y. Ishizaki and T. Iwata, et al. Phys. Lett. B 314, 246-254 (1993) doi:10.1016/0370-2693(93)90456-R
  • [7] D. R. Thompson et al. [E852], Phys. Rev. Lett. 79, 1630-1633 (1997) doi:10.1103/PhysRevLett.79.1630 [arXiv:hep-ex/9705011 [hep-ex]].
  • [8] S. U. Chung et al. [E852], Phys. Rev. D 60, 092001 (1999) doi:10.1103/PhysRevD.60.092001 [arXiv:hep-ex/9902003 [hep-ex]].
  • [9] E. Klempt and A. Zaitsev, Phys. Rept. 454, 1-202 (2007) doi:10.1016/j.physrep.2007.07.006 [arXiv:0708.4016 [hep-ph]].
  • [10] C. A. Meyer and E. S. Swanson, Prog. Part. Nucl. Phys. 82, 21-58 (2015) doi:10.1016/j.ppnp.2015.03.001 [arXiv:1502.07276 [hep-ph]].
  • [11] M. Alekseev et al. [COMPASS], Phys. Rev. Lett. 104, 241803 (2010) doi:10.1103/PhysRevLett.104.241803 [arXiv:0910.5842 [hep-ex]].
  • [12] E. I. Ivanov et al. [E852], Phys. Rev. Lett. 86, 3977-3980 (2001) doi:10.1103/PhysRevLett.86.3977 [arXiv:hep-ex/0101058 [hep-ex]].
  • [13] C. Adolph et al. [COMPASS], Phys. Lett. B 740, 303-311 (2015) [erratum: Phys. Lett. B 811, 135913 (2020)] doi:10.1016/j.physletb.2014.11.058 [arXiv:1408.4286 [hep-ex]].
  • [14] M. Aghasyan et al. [COMPASS], Phys. Rev. D 98, no.9, 092003 (2018) doi:10.1103/PhysRevD.98.092003 [arXiv:1802.05913 [hep-ex]].
  • [15] G. D. Alexeev et al. [COMPASS], Phys. Rev. D 105, no.1, 012005 (2022) doi:10.1103/PhysRevD.105.012005 [arXiv:2108.01744 [hep-ex]].
  • [16] R. T. Deck, Phys. Rev. Lett. 13, 169-173 (1964) doi:10.1103/PhysRevLett.13.169
  • [17] A. Rodas et al. [JPAC], Phys. Rev. Lett. 122, no.4, 042002 (2019) doi:10.1103/PhysRevLett.122.042002 [arXiv:1810.04171 [hep-ph]].
  • [18] D. Horn and J. Mandula, Phys. Rev. D 17, 898 (1978) doi:10.1103/PhysRevD.17.898
  • [19] T. Barnes and F. E. Close, Phys. Lett. B 116, 365-368 (1982) doi:10.1016/0370-2693(82)90301-X
  • [20] N. Isgur and J. E. Paton, Phys. Rev. D 31, 2910 (1985) doi:10.1103/PhysRevD.31.2910
  • [21] T. Barnes, F. E. Close and E. S. Swanson, Phys. Rev. D 52, 5242-5256 (1995) doi:10.1103/PhysRevD.52.5242 [arXiv:hep-ph/9501405 [hep-ph]].
  • [22] P. R. Page, E. S. Swanson and A. P. Szczepaniak, Phys. Rev. D 59, 034016 (1999) doi:10.1103/PhysRevD.59.034016 [arXiv:hep-ph/9808346 [hep-ph]].
  • [23] F. E. Close and J. J. Dudek, Phys. Rev. D 70, 094015 (2004) doi:10.1103/PhysRevD.70.094015 [arXiv:hep-ph/0308099 [hep-ph]].
  • [24] S. L. Zhu, Phys. Rev. D 60, 097502 (1999) doi:10.1103/PhysRevD.60.097502 [arXiv:hep-ph/9903537 [hep-ph]].
  • [25] P. Z. Huang, H. X. Chen and S. L. Zhu, Phys. Rev. D 83, 014021 (2011) doi:10.1103/PhysRevD.83.014021 [arXiv:1010.2293 [hep-ph]].
  • [26] H. X. Chen, Z. X. Cai, P. Z. Huang and S. L. Zhu, Phys. Rev. D 83, 014006 (2011) doi:10.1103/PhysRevD.83.014006 [arXiv:1010.3974 [hep-ph]].
  • [27] X. Zhang and J. J. Xie, Chin. Phys. C 44, no.5, 054104 (2020) doi:10.1088/1674-1137/44/5/054104 [arXiv:1906.07340 [nucl-th]].
  • [28] J. J. Dudek et al. [Hadron Spectrum], Phys. Rev. D 88, no.9, 094505 (2013) doi:10.1103/PhysRevD.88.094505 [arXiv:1309.2608 [hep-lat]].
  • [29] J. J. Dudek, Phys. Rev. D 84, 074023 (2011) doi:10.1103/PhysRevD.84.074023 [arXiv:1106.5515 [hep-ph]].
  • [30] G. S. Bali and A. Pineda, Phys. Rev. D 69, 094001 (2004) doi:10.1103/PhysRevD.69.094001 [arXiv:hep-ph/0310130 [hep-ph]].
  • [31] F. E. Close and A. Kirk, Phys. Lett. B 483, 345-352 (2000) doi:10.1016/S0370-2693(00)00623-7 [arXiv:hep-ph/0004241 [hep-ph]].
  • [32] F. E. Close and Q. Zhao, Phys. Rev. D 71, 094022 (2005) doi:10.1103/PhysRevD.71.094022 [arXiv:hep-ph/0504043 [hep-ph]].
  • [33] Q. Zhao, Phys. Lett. B 659, 221-227 (2008) doi:10.1016/j.physletb.2007.10.062 [arXiv:0705.0101 [hep-ph]].
  • [34] Q. Zhao, Phys. Lett. B 636, 197-200 (2006) doi:10.1016/j.physletb.2006.03.043 [arXiv:hep-ph/0602216 [hep-ph]].
  • [35] R. Kokoski and N. Isgur, Phys. Rev. D 35, 907 (1987) doi:10.1103/PhysRevD.35.907
  • [36] P. A. Zyla et al. [Particle Data Group], PTEP 2020, no.8, 083C01 (2020) doi:10.1093/ptep/ptaa104
  • [37] J. S. Yu, Z. F. Sun, X. Liu and Q. Zhao, Phys. Rev. D 83, 114007 (2011) doi:10.1103/PhysRevD.83.114007 [arXiv:1104.3064 [hep-ph]].