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Interpretation of the η1(1855)\eta_{1}(1855) as a KK¯1(1400)+K\bar{K}_{1}(1400)+ c.c. molecule

Xiang-Kun Dong CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences,
Zhong Guan Cun East Street 55, Beijing 100190, China
School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
   Yong-Hui Lin Helmholtz-Institut für Strahlen- und Kernphysik and Bethe Center for Theoretical Physics,
Universität Bonn, D-53115 Bonn, Germany
   Bing-Song Zou zoubs@itp.ac.cn CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences,
Zhong Guan Cun East Street 55, Beijing 100190, China
School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China School of Physics, Central South University, Changsha 410083, China
Abstract

An exotic state with JPC=1+J^{PC}=1^{-+}, denoted by η1(1855)\eta_{1}(1855), was observed by BESIII collaboration recently in J/ψγηηJ/\psi\to\gamma\eta\eta^{\prime}. The fact that its mass is just below the threshold of KK¯1(1400)K\bar{K}_{1}(1400) stimulates us to investigate whether this exotic state can be interpreted as a KK¯1(1400)+K\bar{K}_{1}(1400)+ c.c molecule or not. Using the one boson exchange model, we show that it is possible for KK¯1(1400)K\bar{K}_{1}(1400) with JPC=1+J^{PC}=1^{-+} to bind together by taking the momentum cutoff Λ2\Lambda\gtrsim 2 GeV and yield the same binding energy as the experimental value when Λ2.5\Lambda\approx 2.5 GeV. In this molecular picture, the predicted branch ratio Br(η1(1855)ηη)15%\mathrm{Br}(\eta_{1}(1855)\to\eta\eta^{\prime})\approx 15\% is consistent with the experimental results, which again supports the molecular explanation of η1(1855)\eta_{1}(1855). Relevant systems, namely KK¯1(1400)K\bar{K}_{1}(1400) with JPC=1J^{PC}=1^{--} and KK¯1(1270)K\bar{K}_{1}(1270) with JPC=1±J^{PC}=1^{-\pm}, are also investigated, some of which can be searched for in the future experiments.

pacs:
12.40.Vv,13.25.Jx,14.40.Cs
Keyword: hadronic molecule, exotic hadrons, one boson exchange

I Introduction

Many efforts have been put into searching for non-conventional hadrons other than quark-antiquark mesons or 3-quark baryons since the quark model was proposed by Gell-Mann Gell-Mann (1964) and Zweig Zweig (1964). Quantum Chromodynamics (QCD), the most fundamental theory describing the strong interaction, does not forbid the existence of multi-quark states, hybrid states or glueballs, collectively called exotic hadrons. Actually, there were several candidates for exotic hadrons before the beginning of this century but none of them are identified unambiguously Klempt and Zaitsev (2007). For example, even now there is not a widely accepted explanation for the nature of Λ(1405)\Lambda(1405), which was ever discovered almost 60 years ago Dalitz and Tuan (1959, 1960); Alston et al. (1961), see the discussions in the most recent reviews Hyodo and Niiyama (2021); Mai (2021).

Since the discovery of the charmonium-like state X(3872) Choi et al. (2003), the last twenty years has witnessed the booming experimental evidence of exotic states, see Refs. Chen et al. (2016); Hosaka et al. (2016); Richard (2016); Lebed et al. (2017); Esposito et al. (2017); Guo et al. (2018); Ali et al. (2017); Olsen et al. (2018); Altmannshofer et al. (2019); Kalashnikova and Nefediev (2019); Cerri et al. (2019); Liu et al. (2019); Brambilla et al. (2020); Guo et al. (2020); Yang et al. (2020); Ortega and Entem (2021); Dong et al. (2021a, b) for recent reviews. To identify exotic states or their candidates, the following guidelines may be helpful: a) In the charmonium and bottomonium sectors, quark models give quite precise descriptions of the conventional mesons (see, e.g., Refs. Godfrey and Isgur (1985); Capstick and Isgur (1985)). If the observed resonances do not fit such properties, they can be considered as candidates of exotic states, such as X(3872) and Y(4260) Aubert et al. (2005); b) In some cases, the decay channels imply the resonances consist of multiquarks and therefore, these states are exotic definitely, such as Zc(s)Z_{c(s)} states Ablikim et al. (2013); Liu et al. (2013); Ablikim et al. (2021), Pc(s)P_{c(s)} states Aaij et al. (2015, 2019, 2021a) and most recently observed doubly charmed TccT_{cc} state Aaij et al. (2021b, c); c) Some combinations of JPCJ^{PC} for conventional mesons are forbidden, such as 0,(even)+0^{--},(\rm{even})^{+-} and (odd)+(\rm{odd})^{-+}. Therefore, a state with such forbidden quantum numbers must be exotic. Up to now there are two well-established states with exotic JPCJ^{PC} in light quark sector, π1(1400),π1(1600)\pi_{1}(1400),\pi_{1}(1600) Zyla et al. (2020) and one possible state π1(2015)\pi_{1}(2015) Kuhn et al. (2004); Lu et al. (2005)111See Ref. Meyer and Swanson (2015) for a recent review on the experimental status of these π1\pi_{1}’s., all of which have JPC=1+J^{PC}=1^{-+}, while no experimental signals appear in the heavy quark sector.

Recently, BESIII Collaboration Ablikim et al. (2022a, b) reported a resonance, denoted as η1(1855)\eta_{1}(1855), with m=1855±91+6m=1855\pm 9^{+6}_{-1} MeV and Γ=188±188+3\Gamma=188\pm 18^{+3}_{-8} MeV, in the invariant mass distribution of ηη\eta\eta^{\prime} in J/ψγηηJ/\psi\to\gamma\eta\eta^{\prime} with a significance of 19 σ\sigma. Its quantum numbers JPC=1+J^{PC}=1^{-+} ensure it to be an exotic state, which immediately stimulates the explanation of η1(1875)\eta_{1}(1875) being an isoscalar hybrid candidate Chen et al. (2022); Qiu and Zhao (2022). Notice that this state locates at just around 40 MeV below the KK¯1(1400)K\bar{K}_{1}(1400) threshold and therefore, it is natural to interpret it as a molecule of KK¯1(1400)+K\bar{K}_{1}(1400)+ c.c.(KK¯1K\bar{K}_{1} for short in the following), which can decay into ηη\eta\eta^{\prime} via KK^{*} exchange on the hadronic level.

In this paper, we investigate whether KK¯1K\bar{K}_{1} can form a bound state via the interaction driven by one boson exchange as shown in Fig. 1. Pseudoscalar exchange between KK¯1K\bar{K}_{1} is forbidden by parity conservation. Hence it is expected that the σ\sigma and vector meson (ρ,ω,ϕ\rho,\omega,\phi) exchanges dominate the interaction. In the Review of Particle Physics (RPP) Zyla et al. (2020) there are two K1K_{1}’s, K1(1270)K_{1}(1270) with mass 1270 MeV and K1(1400)K_{1}(1400) with mass 1403 MeV. These two mass eigenstates have quite different decay behaviors and are considered as the mixing of two flavor eigenstates from the P13{}^{3}P_{1} and P11{}^{1}P_{1} octets Burakovsky and Goldman (1997); Suzuki (1993); Cheng (2003); Yang (2011); Hatanaka and Yang (2008); Tayduganov et al. (2012); Divotgey et al. (2013); Zhang et al. (2018). It was also explored in Refs. Roca et al. (2005); Geng et al. (2007); Wang et al. (2019) that the K1(1270)K_{1}(1270) may have a two-pole structure in vector-pseudoscalar scattering. In this paper we adopt the former treatment to investigate their interactions.

With the above considerations we find that a) the meson exchange potential with reasonable cutoff is strong enough for KK¯1(1400)K\bar{K}_{1}(1400) to form a bound state; b) The branch ratio of the predicted molecule decaying into ηη\eta\eta^{\prime} is consistent with the experimental data of BESIII Ablikim et al. (2022a, b), Br(J/ψγη1(1855)γηη)=(2.70±0.410.35+0.16)×106(J/\psi\rightarrow\gamma\eta_{1}(1855)\rightarrow\gamma\eta\eta^{\prime})=\left(2.70\pm 0.41_{-0.35}^{+0.16}\right)\times 10^{-6}; c) Its CC-parity partner are predicted to have a similar binding energy and the πρ\pi\rho, ηω\eta\omega and KK¯K\bar{K} channels are good places to search for it. The properties predicted in this paper serve as guidance for further experimental explorations of these states and future experiments can in turn test our molecular state assignment for the observed η1(1855)\eta_{1}(1855).

II Possible bound states of KK¯1(1400)K\bar{K}_{1}(1400)

Due to the U(3)VU(3)_{V} flavor symmetry breaking effect derived from the mass difference between u/du/d and ss quarks, the axialvector K1AK_{1A} (P13{}^{3}P_{1} state) and pseudovector K1BK_{1B} (P11{}^{1}P_{1} state) can mix with each other and generate the two physical resonances K1(1270)K_{1}(1270) and K1(1400)K_{1}(1400). Following Ref. Divotgey et al. (2013) the mixing is parameterized as

(|K1(1270)|K1(1400))=(cosθisinθisinθcosθ)(|K1A|K1B)\displaystyle\left(\begin{array}[]{cc}{\left|K_{1}(1270)\right\rangle}\\ {\left|K_{1}(1400)\right\rangle}\end{array}\right)=\left(\begin{array}[]{cc}{\cos\theta}&{-i\sin\theta}\\ {-i\sin\theta}&{\cos\theta}\end{array}\right)\left(\begin{array}[]{c}{\left|K_{1A}\right\rangle}\\ {\left|K_{1B}\right\rangle}\end{array}\right) (7)

where the mixing angle θ\theta is determined to be (56.4±4.3)(56.4\pm 4.3)^{\circ}. The flavor wave functions of |KK¯1|K\bar{K}_{1}\rangle with positive and negative C-parity read

C=±:12(|KK¯1±𝒞|KK1)\displaystyle C=\pm:\frac{1}{\sqrt{2}}\left(|K\bar{K}_{1}\rangle\pm\mathcal{C}|KK_{1}\rangle\right) (8)

with the following conventions, 𝒞|K=|K¯\mathcal{C}|K\rangle=|\bar{K}\rangle, 𝒞|K1A=|K¯1A\mathcal{C}|K_{1A}\rangle=|\bar{K}_{1A}\rangle and 𝒞|K1B=|K¯1B\mathcal{C}|K_{1B}\rangle=-|\bar{K}_{1B}\rangle. Here 𝒞\mathcal{C} is the charge conjugation operator.

ρ,ω,ϕ,σ\rho,\omega,\phi,\sigmaK(K¯)K(\bar{K})K¯1(K1)\bar{K}_{1}(K_{1})K1(K¯1)K_{1}(\bar{K}_{1})K¯(K)\bar{K}(K)qqp1p_{1}p2p^{\prime}_{2}p2p_{2}p1p^{\prime}_{1}ρ,ω,ϕ,σ\rho,\omega,\phi,\sigmaK(K¯)K(\bar{K})K¯1(K1)\bar{K}_{1}(K_{1})K(K¯)K(\bar{K})K¯1(K1)\bar{K}_{1}(K_{1})qqp1p_{1}p1p^{\prime}_{1}p2p_{2}p2p^{\prime}_{2}
Figure 1: Feynman diagrams for direct (top) and cross (bottom) meson exchange between KK¯1K\bar{K}_{1}.

Working with the chiral perturbation theory, the pseudoscalar-pseudoscalar-vector coupling is described by Meissner (1988)

PPV\displaystyle\mathcal{L}_{\rm{PPV}} =i2GVTr([μP,P]Vμ)\displaystyle=i\sqrt{2}\,G_{\rm V}\,{\rm{Tr}}\left([\partial_{\mu}P,P]V^{\mu}\right) (9)

and analogously, we assume the following couplings

AAV\displaystyle\mathcal{L}_{{AAV}} =i2GVTr([μAν,Aν]Vμ)\displaystyle=i\sqrt{2}\,G_{\rm V}^{\prime}\,{\rm{Tr}}\left([\partial_{\mu}A^{\nu},A_{\nu}]V^{\mu}\right) (10)
BBV\displaystyle\mathcal{L}_{{BBV}} =i2GVTr([μBν,Bν]Vμ)\displaystyle=i\sqrt{2}\,G_{\rm V}^{\prime}\,{\rm{Tr}}\left([\partial_{\mu}B^{\nu},B_{\nu}]V^{\mu}\right) (11)
APV\displaystyle\mathcal{L}_{APV} =iaTr(Aμ[Vμ,P]),\displaystyle=ia\ {\rm Tr}(A_{\mu}[V^{\mu},P]), (12)
BPV\displaystyle\mathcal{L}_{BPV} =bTr(Bμ{Vμ,P})\displaystyle=b\ {\rm Tr}(B_{\mu}\{V^{\mu},P\}) (13)

with

P=(π02+η6π+K+ππ02+η6K0KK¯023η),\displaystyle P=\left(\begin{array}[]{ccc}\frac{\pi^{0}}{\sqrt{2}}+\frac{\eta}{\sqrt{6}}&\pi^{+}&K^{+}\\ \pi^{-}&-\frac{\pi^{0}}{\sqrt{2}}+\frac{\eta}{\sqrt{6}}&K^{0}\\ K^{-}&\bar{K}^{0}&-\sqrt{\frac{2}{3}}\eta\end{array}\right), (17)
V=(ω2+ρ02ρ+K+ρω2ρ02K0KK¯0ϕ),\displaystyle V=\left(\begin{array}[]{ccc}\frac{\omega}{\sqrt{2}}+\frac{\rho^{0}}{\sqrt{2}}&\rho^{+}&K^{*+}\\ \rho^{-}&\frac{\omega}{\sqrt{2}}-\frac{\rho^{0}}{\sqrt{2}}&K^{*0}\\ K^{*-}&\bar{K}^{*0}&\phi\end{array}\right), (21)

and

A(B)=(K1A(B)+K1A(B)0K1A(B)K¯1A(B)0).\displaystyle A(B)=\left(\begin{array}[]{ccc}{*}&{*}&{K_{1A(B)}^{+}}\\ {*}&{*}&{K_{1A(B)}^{0}}\\ {K_{1A(B)}^{-}}&{\bar{K}_{1A(B)}^{0}}&*\end{array}\right). (25)

Here all irrelevant axialvector and pseudovector states are labeled as “*” in the multiplet matrix Eq. (25). The coupling constant GV3.0G_{\rm V}\approx 3.0 was estimated from the decay width of ρππ\rho\to\pi\pi Zhang et al. (2006) and we assumed the magnitude of GVG^{\prime}_{V} is comparable with GVG_{\rm V}, i.e., |GV|GV|G^{\prime}_{\rm V}|\approx G_{\rm V}. Moreover, taking the mixing angle obtained in Ref. Divotgey et al. (2013) and fitting to the experimental widths of K1(1270)K_{1}(1270)/K1(1400)K_{1}(1400) decaying to KρK\rho, one can determine the coupling constants as a1.92±0.09a\approx 1.92\pm 0.09 GeV and b2.47±0.08b\approx-2.47\pm 0.08 GeV Dong and Zou (2021).

In our previous work Dong et al. (2020), we have discussed the DD¯1+D\bar{D}_{1}+ c.c. bound state via one boson exchange to understand the nature of Y(4260). KK1KK_{1} system behaves similarly with DD1DD_{1} system in the one boson exchange picture, just replacing the cc quarks in DD1DD_{1} with ss quarks, except that KK1KK_{1} can couple to ϕ\phi while DD1DD_{1} can not. Therefore one can expect that they have the same Lagrangian except the slightly different values of coupling constants. Note that the DDVDDV coupling constant is 0.9 of the KKVKKV coupling Casalbuoni et al. (1997); Isola et al. (2003). These observations make us confident that the Language in Eqs. (10, 11) can give a good description of the K1K1VK_{1}K_{1}V vertices and also indicate the following couplings,

KKσ\displaystyle\mathcal{L}_{KK\sigma} =2gσmKK¯Kσ,\displaystyle=-2g_{\sigma}m_{K}\bar{K}K\sigma, (26)
K1K1σ\displaystyle\mathcal{L}_{K_{1}K_{1}\sigma} =2gσ′′mK1K1μ¯K1μσ,\displaystyle=-2g^{\prime\prime}_{\sigma}m_{K_{1}}\bar{K^{\mu}_{1}}K_{1\mu}\sigma, (27)
K1Kσ\displaystyle\mathcal{L}_{K_{1}K\sigma} =263hσfπmKmK1(K¯1μK+K¯K1μ)μσ\displaystyle=-\frac{2\sqrt{6}}{3}\frac{h_{\sigma}^{\prime}}{f_{\pi}}\sqrt{m_{K}m_{K_{1}}}\left(\bar{K}_{1}^{\mu}K+\bar{K}K_{1}^{\mu}\right)\partial_{\mu}\sigma (28)

with fπ=132MeVf_{\pi}=132\ \rm{MeV} the pion decay constant. As a rough approximation, we take gσ=gσ′′=0.76g_{\sigma}=g^{\prime\prime}_{\sigma}=-0.76, hσ=0.35h^{\prime}_{\sigma}=0.35 Bardeen et al. (2003). We have ignored the mixing nature of K1(1270)K_{1}(1270) and K1(1400)K_{1}(1400) in Eqs.(27, 28), which does not matter here.

The potential of KK¯1K\bar{K}_{1} in the non-relativistic limit reads

V~(𝒒)=4mKmK1\tilde{V}(\bm{q})=-\frac{\mathcal{M}}{4m_{K}m_{K_{1}}} (29)

with \mathcal{M} the invariant scattering amplitude of KK¯1KK¯1K\bar{K}_{1}\to K\bar{K}_{1}. The potentials in momentum space for the direct and cross scatterings, see the top and bottom diagram in Fig. 1, are written as

V~V,d(𝐪)\displaystyle\tilde{V}_{\rm V,d}({\bf q}) =fIgV,dgV,d1|𝐪|2+mV2,\displaystyle=f_{\mathrm{I}}g_{\rm{V,d}}g^{\prime}_{\rm{V,d}}\frac{1}{|{\bf q}|^{2}+m_{\rm V}^{2}}, (30)
V~V,c(𝐪)\displaystyle\tilde{V}_{\rm{V,c}}({\bf q}) =fIgV,c24mKmK1(1+ϵ1𝒒ϵ2𝒒/mV2)|𝒒|2+m~V2,\displaystyle=\frac{f_{\mathrm{I}}g^{2}_{\rm{V,c}}}{4m_{\rm{K}}m_{{\rm{K}_{1}}}}\frac{\left(1+{\bm{\epsilon}}_{1}\cdot\bm{q\epsilon}_{2}^{*}\cdot\bm{q}/m_{\rm{V}}^{2}\right)}{|{\bm{q}}|^{2}+\tilde{m}_{\rm V}^{2}}, (31)
V~σ,d(𝐪)\displaystyle\tilde{V}_{\sigma,\rm{d}}({\bf q}) =gσgσ′′1|𝐪|2+mσ2,\displaystyle=-g_{\sigma}g^{\prime\prime}_{\sigma}\frac{1}{|{\bf q}|^{2}+m_{\sigma}^{2}}, (32)
V~σ,c(𝐪)\displaystyle\tilde{V}_{\sigma,\rm{c}}({\bf q}) =2hσ23fπ2ϵ1𝒒ϵ2𝒒|𝒒|2+m~σ2\displaystyle=\frac{-2h^{{}^{\prime}2}_{\sigma}}{3f_{\pi}^{2}}\frac{{\bm{\epsilon}}_{1}\cdot\bm{q\epsilon}_{2}^{*}\cdot\bm{q}}{|{\bm{q}}|^{2}+\tilde{m}_{\sigma}^{2}} (33)

with m~V/σ2=mV/σ2(mK1mK)2\tilde{m}_{\rm{V}/\sigma}^{2}=m_{\rm V/\sigma}^{2}-(m_{\rm{K}_{1}}-m_{\rm{K}})^{2}. The coupling constants are

gρ,d\displaystyle g_{\rho,\rm d} =gω,d=12gϕ,d=GV\displaystyle=g_{\omega,\rm d}=-\frac{1}{\sqrt{2}}g_{\phi,\rm d}=G_{\rm V} (34)
gρ,d\displaystyle g^{\prime}_{\rho,\rm d} =gω,d=12gϕ,d=GV\displaystyle=g^{\prime}_{\omega,\rm d}=-\frac{1}{\sqrt{2}}g^{\prime}_{\phi,\rm d}=G^{\prime}_{\rm V} (35)
gρ,c2\displaystyle g^{2}_{\rho,\rm c} =gω,c2=12gϕ,c2=12(asinθ±bcosθ)2\displaystyle=g^{2}_{\omega,\rm c}=\frac{1}{2}g^{2}_{\phi,\rm c}=\frac{1}{2}(a\sin\theta\pm b\cos\theta)^{2} (36)

with “++” for K1(1400)K_{1}(1400) and “-” for K1(1270)K_{1}(1270) and the isospin factors, fIf_{\mathrm{I}}, are

f0={3ρ1ω1ϕf1={1ρ1ω1ϕ.\displaystyle f_{0}=\left\{\begin{array}[]{cc}{3}&{\rho}\\ {1}&{\omega}\\ {1}&{\phi}\end{array}\right.\ \ \ \ f_{1}=\left\{\begin{array}[]{cc}{-1}&{\rho}\\ {1}&{\omega}\\ {1}&{\phi}\end{array}\right.. (43)

A form factor should be introduced at each vertex to account for the finite size of the involved mesons. Here we take the commonly used monopole form factor,

F(q,m,Λ)=Λ2m2Λ2q2,F(q,m,\Lambda)=\frac{\Lambda^{2}-m^{2}}{\Lambda^{2}-q^{2}}, (44)

which in position space can be looked upon as a spherical source of the exchanged mesons Tornqvist (1994). The potentials in position space can be obtained by Fourier transformation of Eqs.(30, 31), together with the form factor Eq. (44),

VV,d(𝐫)\displaystyle V_{\rm{V,d}}\left(\mathbf{r}\right) =fIgV,dgV,d(mVY(mVr)ΛY(Λr)\displaystyle=f_{\mathrm{I}}g_{\rm{V,d}}g^{\prime}_{\rm{V,d}}{\Big{(}}m_{\rm{V}}Y(m_{\rm{V}}r)-\Lambda Y(\Lambda r)
12(Λ2mV2)rY(Λr)),\displaystyle\ \ \ \ -\frac{1}{2}(\Lambda^{2}-m_{\rm{V}}^{2})rY(\Lambda r)\Big{)}, (45)
VV,c(𝐫)\displaystyle V_{\rm{V,c}}\left(\mathbf{r}\right) =fIgV,c24mKmK1{[m~VY(m~Vr)Λ~Y(Λ~r)\displaystyle=\frac{f_{\mathrm{I}}g^{2}_{\rm{V,c}}}{4m_{\rm{K}}m_{{\rm{K}_{1}}}}\Big{\{}\Big{[}\tilde{m}_{\rm{V}}Y(\tilde{m}_{\rm{V}}r)-\tilde{\Lambda}Y(\tilde{\Lambda}r)
12(Λ~2m~V2)rY(Λ~r)]\displaystyle\ \ \ \ -\frac{1}{2}(\tilde{\Lambda}^{2}-\tilde{m}^{2}_{\rm{V}})rY(\tilde{\Lambda}r)\Big{]}
13mV2[m~V2(m~VY(m~Vr)Λ~Y(Λ~r))\displaystyle\ \ \ \ -\frac{1}{3m_{\rm{V}}^{2}}\Big{[}\tilde{m}^{2}_{\rm{V}}\left(\tilde{m}_{\rm{V}}Y(\tilde{m}_{\rm{V}}r)-\tilde{\Lambda}Y(\tilde{\Lambda}r)\right)
12λ2(Λ~2m~V2)rY(Λ~r)]}\displaystyle\ \ \ \ -\frac{1}{2}\lambda^{2}(\tilde{\Lambda}^{2}-\tilde{m}^{2}_{\rm{V}})rY(\tilde{\Lambda}r)\Big{]}\Big{\}} (46)
Vσ,d(𝐫)\displaystyle V_{\rm{\sigma,d}}\left(\mathbf{r}\right) =gσgσ′′(mσY(mσr)ΛY(Λr)\displaystyle=-g_{\sigma}g^{\prime\prime}_{\sigma}\Big{(}m_{\sigma}Y(m_{\sigma}r)-\Lambda Y(\Lambda r)
12(Λ2mσ2)rY(Λr)),\displaystyle\ \ \ \ -\frac{1}{2}(\Lambda^{2}-m_{\sigma}^{2})rY(\Lambda r)\Big{)}, (47)
Vσ,c(𝐫)\displaystyle V_{\sigma,\rm{c}}\left(\mathbf{r}\right) =2hσ29fπ2{[m~σ2(m~σY(m~σr)Λ~Y(Λ~r))\displaystyle=\frac{2h^{{}^{\prime}2}_{\sigma}}{9f_{\pi}^{2}}\Big{\{}\Big{[}\tilde{m}^{2}_{\sigma}\left(\tilde{m}_{\sigma}Y(\tilde{m}_{\sigma}r)-\tilde{\Lambda}Y(\tilde{\Lambda}r)\right)
12λ2(Λ~2m~σ2)rY(Λ~r)]}\displaystyle\ \ \ \ -\frac{1}{2}\lambda^{2}(\tilde{\Lambda}^{2}-\tilde{m}^{2}_{\sigma})rY(\tilde{\Lambda}r)\Big{]}\Big{\}} (48)

where Y(x)=ex/4πxY(x)=e^{-x}/4\pi x and Λ~2=Λ2(mK1mK)2.\tilde{\Lambda}^{2}=\Lambda^{2}-(m_{\rm K_{1}}-m_{\rm K})^{2}. Note that the Fourier transformation of Eqs.(31,33) contains a δ\delta function, which is omitted in some works, see the discussion in Ref. Burns and Swanson (2019). The δ\delta potential is from short distance physics, which we are blind to, and may contain contributions from the exchange of heavier mesons not considered here. In Ref. Yalikun et al. (2021), the δ\delta contribution is varied in the range of 010\sim 1 to take into account the uncertainty of the unknown short distance interaction in the formation of PcP_{c} states. Here we consider the marginal cases where the δ\delta function is kept and omitted, corresponding to λ=Λ~\lambda=\tilde{\Lambda} and λ=m~V\lambda=\tilde{m}_{\rm V} in Eqs. (46, 48), respectively. We take the real part of potentials when they are complex. The total potential for positive or negative C-parity KK¯1K\bar{K}_{1} system reads

VI,C=±=(VV,dI+Vσ,d)±(VV,cI+Vσ,c)\displaystyle V^{{I},C=\pm}=\left(V_{\rm V,d}^{I}+V_{\sigma,\rm d}\right)\pm\left(V_{\rm V,c}^{I}+V_{\sigma,\rm c}\right) (49)

with I=0,1I=0,1. We take the following masses from RPP Zyla et al. (2020) to perform numerical calculations, mK=0.495GeVm_{{K}}=0.495\ \rm{GeV}, mK1(1400)=1.403GeVm_{{K_{1}}(1400)}=1.403\ \rm{GeV}, mK1(1270)=1.272GeVm_{{K_{1}}(1270)}=1.272\ \rm{GeV}, mρ=0.775GeVm_{\rho}=0.775\ \rm{GeV}, mω=0.783GeVm_{\omega}=0.783\ \rm{GeV}, mϕ=1.019GeVm_{\phi}=1.019\ \rm{GeV} and mσ=0.600GeVm_{\sigma}=0.600\ \rm{GeV}.

Refer to caption
Figure 2: The binding energies of the isoscalar KK¯1(1400)K\bar{K}_{1}(1400) bound states.

The Schrödinger equations for both KK¯1(1400)K\bar{K}_{1}(1400) and KK¯1(1270)K\bar{K}_{1}(1270) systems are solved numerically. For the isovector cases, no bound states are found since contributions from ρ\rho and ω\omega exchanges cancel with each other. Now we focus on the isoscalar cases. The binding energies for KK¯1(1400)K\bar{K}_{1}(1400) with different cutoffs are shown in Fig. 2. We can see that the 1+1^{-+} system can form a bound state when Λ1.9\Lambda\gtrsim 1.9 GeV. We need Λ2.5\Lambda\approx 2.5 GeV to produce a binding energy of 40 MeV, the experimental value of the newly observed exotic state by BESIII. With the same cutoff, the binding energy of the 11^{--} KK¯1(1400)K\bar{K}_{1}(1400) state is predicted to be 103010\sim 30 MeV where the uncertainty comes from whether the δ\delta potential is included or not. Due to the large coupling of K1(1270)KVK_{1}(1270)KV, the potential between KK¯1(1270)K\bar{K}_{1}(1270) is repulsive for C=+C=+ and therefore, no bound states are expected. On the other hand, the potential is too attractive for C=C=- to form a molecule with a reasonable binding energy if we use a cutoff about 2.52.5 GeV. Even when Λ1.5\Lambda\sim 1.5 GeV the binding energy is larger than 100 MeV, which is not acceptable for a shallow bound state, for which our previous treatments hold valid.

III Decay properties of KK¯1K\bar{K}_{1} molecules

Refer to caption
Figure 3: Two-body and three-body decays of molecules composed of KK¯1K\bar{K}_{1}.

With reasonable cutoff we have obtained the possible bound states of KK¯1(1400)K\bar{K}_{1}(1400) with JPC=1±J^{PC}=1^{-\pm}, denoted as XX temporarily. It is now desirable to estimate the decay patterns of the predicted molecular states, especially the ηη\eta\eta^{\prime} channel, to compare with BESIII observation and provide guidance to further experimental investigations. It is natural that such molecules decay through their components, as illustrated in Fig. 3. Since K1K_{1}’s have a quite large decay width, we assume that the three-body decays of the molecules are dominated by the process shown in the right diagram in Fig. 3, where P,V=π,KP,V=\pi,K^{*} or K,ρ/ωK,\rho/\omega. Two-body strong decay channels considered here are listed in Table 1.

The coupling between a hadronic molecule and its components can be constructed as

XKK1=yXμKK1μ+h.c.\displaystyle\mathcal{L}_{XKK_{1}}=yX^{\mu}K^{\dagger}K^{\dagger}_{1\mu}+h.c. (50)

where yy is the coupling constant and XX denotes the field of the molecule. For a loosely bound state, one can estimate the coupling constant in a model-independent way by means of Weinberg compositeness criterion Weinberg (1965); Baru et al. (2004); Guo et al. (2018), which is developed to estimate the amount of compact and molecular components in a given state, where the molecular components consist of two stable (or narrow 222“narrow” is relative to the binding energy of that molecular state, that is, the widths of the molecular components should be much smaller than its binding energy.) compact states. However, K1(1400)K_{1}(1400) has a width of 174 MeV, much larger than the obtained binding energy in our case. Strictly speaking, one should consider the dynamics between the sub-ingredients of K1(1400)K_{1}(1400) and kaon, such as KK¯πK\bar{K}^{*}\pi three-body system, like what were done for X(3872)X(3872) Baru et al. (2011) and Tcc+T_{cc}^{+} Du et al. (2022). On the other hand, the decay width of K1(1400)K_{1}(1400) is much smaller than the masses of exchanged ρ\rho and ω\omega, and hence it should not jeopardize the molecular interpretation of η1(1855)\eta_{1}(1855) as argued in Ref. Guo and Meissner (2011).

To obtain a better estimate of the coupling yy, we consider in the following the pole position of the XX on the complex s\sqrt{s} plane by assuming that the XX is a purely molecular state of KK¯1(1400)K\bar{K}_{1}(1400). The dominant decay channel of K1(1400)K_{1}(1400) is KπK^{*}\pi with a branching ratio of 94% and for simplicity, we take it to be 100% by ignoring all other channels. The pole position of KK¯(1400)K\bar{K}(1400) system with coupled channel effects ignored is determined by

1VG=01-VG=0 (51)

where VV, assumed to be constant, is the interaction strength of KK¯(1400)K\bar{K}(1400) and GG is the scalar two particle loop propagator,

G(s)=d4l(2π)41l2mK2+iϵ1(Pl)2mK12+imK1ΓK1.\displaystyle G(s)=\int\frac{{\rm d}^{4}l}{(2\pi)^{4}}\frac{1}{l^{2}-m_{K}^{2}+i\epsilon}\frac{1}{(P-l)^{2}-m_{K_{1}}^{2}+im_{K_{1}}\Gamma_{K_{1}}}. (52)

with PP the total momentum. Note that we have ignored the spin structures of the intermediate K1K_{1}, the corrections from which, as argued in Refs Roca et al. (2005); Molina et al. (2008), are at the order of lon2/mK12l_{\rm on}^{2}/m_{K_{1}}^{2} with lonl_{\rm on} the on-shell 3-momentum of KK¯1K\bar{K}_{1}. A hard cutoff, Λ\Lambda, of the 3-momentum 𝒍\bm{l} will be introduced to regularize the UV divergence. The running width of K1K_{1} reads

ΓK1(s)=gK12|𝒒|16πmK12(3+𝒒2mK2)\displaystyle\Gamma_{K_{1}}(s)=g_{K_{1}}^{2}\frac{|{\bm{q}}|}{16\pi m_{K_{1}}^{2}}\left(3+\frac{{\bm{q}}^{2}}{m_{K^{*}}^{2}}\right) (53)

with gK1=3.65g_{K_{1}}=3.65 GeV the coupling constant of K1KπK_{1}K^{*}\pi and 𝒒\bm{q}, depending on ss, the 3-momentum of KK^{*} in the center of mass frame of K1K_{1}.

The pole trajectory when varying VV is shown in Fig. 4. As expected, the partial width of η1(1855)K(K¯1(1400)K¯π)\eta_{1}(1855)\to K(\bar{K}_{1}(1400)\to\bar{K}^{*}\pi) gets smaller when the binding energy becomes larger and the pole will touch the KK¯1(1400)K\bar{K}_{1}(1400) cut, around 1900i871900-i87 MeV, if the binding energy goes to zero. For the measured η1\eta_{1} mass, the three body decay width of XX is around 105105 MeV, which weakly depends on the hard cutoff Λ\Lambda in the phenomenological reasonable range of 0.610.6\sim 1 GeV. By matching the three body decay width of XX to the obtained pole position, we have an estimate of the coupling constant,

y=13.6GeV.y=13.6\ \rm GeV. (54)
Refer to caption
Figure 4: Pole trajectory of the KK¯1K\bar{K}_{1} molecule in the SS-wave KK¯1K\bar{K}_{1} single channel model. Red line shows the pole trajectory with Λ=0.8\Lambda=0.8 GeV and red shadow is the uncertainties caused by varying the hard momentum cut from 0.6 GeV to 1.0 GeV. Open blue circle denotes the branch point corresponding to the KK¯1K\bar{K}_{1} threshold and the blue line indicates the corresponding branch cut. The vertical black dot-dashed line is the KK¯πK\bar{K}^{*}\pi three-body threshold. The orange band shows the observed η1\eta_{1} mass.

We refer to our previous work for other relevant couplings Dong and Zou (2021). In particular, a non-zero DD-wave component is introduced in the vertex K1KπK_{1}K^{*}\pi and K1KηK_{1}K^{*}\eta as similar with D1DπD_{1}D^{*}\pi interaction used in Ref. Dong and Zou (2021). The ratio of DD-wave component over the SS-wave from RPP Zyla et al. (2020) is 0.04±0.010.04\pm 0.01. When performing the loop integral in the triangle diagram of the two-body decays, a Gaussian regulator f1f_{1} (at the vertex of XKK¯1XK\bar{K}_{1}) and a multipole form factor f2f_{2} (at one of the vertices where the exchanged particle AA is involved), formulated as follows, are included to regularize the ultraviolet divergence.

f1(𝒑2/Λ02)=exp(𝒑2/Λ02),\displaystyle f_{1}(\bm{p}^{2}/\Lambda_{0}^{2})={\rm{exp}}(-\bm{p}^{2}/\Lambda_{0}^{2}), (55)
f2(q2)=Λ14(m2q2)2+Λ14,\displaystyle f_{2}(q^{2})=\frac{\Lambda_{1}^{4}}{(m^{2}-q^{2})^{2}+\Lambda_{1}^{4}}, (56)

where 𝒑\bm{p} are the three dimensional space part of momentum of KK or K¯1\bar{K}_{1}, mm and qq is the mass and momentum of the exchanged particle.

Table 1: Partial widths of the isoscalar KK¯1(1400)K\bar{K}_{1}(1400) molecular states with quantum numbers 11^{--} and 1+1^{-+} with Λ0=1.3\Lambda_{0}=1.3 GeV and Λ1=2.5\Lambda_{1}=2.5 GeV. All the decay widths are in unit of MeV\mathrm{MeV}. Here, we assume 5%5\% DD-wave contribution in the K1KπK_{1}K^{*}\pi and K1KηK_{1}K^{*}\eta vertex.
  Mode Widths (MeV\mathrm{MeV})
3 
1EB=20MeV1^{--}~{}E_{B}=20~{}\mathrm{MeV} 1+EB=40MeV1^{-+}~{}E_{B}=40~{}\mathrm{MeV}
  KK¯K^{*}\bar{K}^{*} 38.1 26.3
KK¯K\bar{K} 0.5 0
KK¯K\bar{K}^{*} 1.0 0.9
a1πa_{1}\pi 0 9.2
f1ηf_{1}\eta 0 0.2
ηη\eta\eta^{\prime} 0 26.9
σω\sigma\omega 0.2 0
ρρ\rho\rho 0 0.04
πρ\pi\rho 6.4 0
ηω\eta\omega 0.4 0
ωω\omega\omega 0 0.01
ωϕ\omega\phi 0 0.4
KK¯πK\bar{K}^{*}\pi 130.0 105.0
  2-body 46.5 64.0
Total 176.5 169.0
 
Refer to caption
Refer to caption
Figure 5: Parameter sensitivity of the KK¯K^{*}\bar{K}^{*} (top) and ηη\eta\eta^{\prime} (bottom) two-body partial widths. All curvatures indicate the dependence of KK¯K^{*}\bar{K}^{*} and ηη\eta\eta^{\prime} widths on the parameter Λ0\Lambda_{0} with the Λ1\Lambda_{1} and the ratio of DD-wave component fixed. Solid/Dashed/DotDashed lines show the results with 5%5\%/4%4\%/3%3\% DD-wave component and red/orange/blue lines show those with Λ1=1.5\Lambda_{1}=1.5/2.02.0/2.52.5 GeV.

The decay patterns of 11^{--} and 1+1^{-+} KK¯1(1400)K\bar{K}_{1}(1400) molecules for Λ0=1.3\Lambda_{0}=1.3 GeV and Λ1=2.5\Lambda_{1}=2.5 GeV are shown in Table 1. Our results show that the three-body KK¯πK\bar{K}^{*}\pi is the largest decay channel for both 11^{--} and 1+1^{-+} KK¯1K\bar{K}_{1} molecules. And their dominant two-body decay channel is also the same, i.e., KK¯K^{*}\bar{K}^{*}. Moreover, the 1+1^{-+} exotic state also couples strongly to the ηη\eta\eta^{\prime} channel. It is quite similar with the properties of DD¯1D\bar{D}_{1} molecules where the DD¯D^{*}\bar{D}^{*} and ηηc\eta\eta_{c} channels contribute dominantly to the two-body decay widths Dong et al. (2020). In general, one can find that the molecular scenario always seems to support the strong couplings with the open-flavor channels. In addition, we find that the 1+1^{-+} molecule has also a strong coupling with a1πa_{1}\pi channel, which is also reflected in a recent lattice simulation Woss et al. (2021). In that work, the exotic 1+1^{-+} hybird meson with negative GG-parity decays dominantly into b1πb_{1}\pi channel which translates to a1πa_{1}\pi channel for the positive GG-parity 1+1^{-+} state. The parameter sensitivity of partial widths of two dominant two-body decay channels for the 1+1^{-+} KK¯1(1400)K\bar{K}_{1}(1400) molecule, namely KK¯K^{*}\bar{K}^{*} and ηη\eta\eta^{\prime}, is presented in Fig. 5.

IV Summary

We have used the one boson exchange potential between the KK¯1K\bar{K}_{1}, for both JPC=1J^{PC}=1^{--} and JPC=1+J^{PC}=1^{-+} systems, to investigate if it is possible for them to form bound states. It turns out that with a momentum cutoff Λ2.5\Lambda\approx 2.5 GeV, the attractive force between KK¯1(1400)K\bar{K}_{1}(1400) with JPC=1+J^{PC}=1^{-+} is strong enough to form a bound state with a binding energy of around 40 MeV, which can be related to the newly observed η1(1855)\eta_{1}(1855). The C-parity partner of this molecule is predicted to exist with a binding energy around 10 \sim 30 MeV. While for the K1(1270)K_{1}(1270), the strong coupling between K1(1270)KVK_{1}(1270)KV results in a repulsive force for C=+C=+ and a much deeply attractive force for C=C=-, neither of which is expected to form a molecular state.

The decay properties of the two possible molecules of KK¯1(1400)K\bar{K}_{1}(1400) are investigated. For both the 11^{--} and 1+1^{-+} states, the three body channel KK¯πK\bar{K}^{*}\pi dominates due to the large decay width of K1(1400)KπK_{1}(1400)\to K^{*}\pi. The KK¯K^{*}\bar{K}^{*} and ηη\eta\eta^{\prime} channels have the largest contributions among the two body decays. The presented decay pattern of 1+1^{-+} KK¯1(1400)K\bar{K}_{1}(1400) molecule is compatible with BESIII’s measurements.

In summary, it is shown that the newly observed exotic state η1(1855)\eta_{1}(1855) can be explained as a KK¯1(1400)K\bar{K}_{1}(1400) molecule. This interpretation can be checked by searching for η1(1855)\eta_{1}(1855) in ωϕ\omega\phi channel and its CC-partner in πρ\pi\rho, ηω\eta\omega and KK¯K\bar{K} channels, in addition to KK¯K^{*}\bar{K}^{*} channel.

We thank Feng-Kun Guo, Xiao-Yu Li, Jia-Jun Wu and Mao-Jun Yan for useful discussions. This work is supported by the NSFC and the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) through the funds provided to the Sino German Collaborative Research Center TRR110 Symmetries and the Emergence of Structure in QCD (NSFC Grant No.12070131001, DFG Project-ID 196253076-TRR 110), by the NSFC Grants No. 11835015 and No. 12047503, and by the Chinese Academy of Sciences (CAS) under Grant No.XDB34030000.

References