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Radiative decays of the spin-22 partner of X(3872)X(3872)

Pan-Pan Shi [email protected] CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics,
Chinese Academy of Sciences, Beijing 100190, China
School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
   Jorgivan M. Dias [email protected] CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics,
Chinese Academy of Sciences, Beijing 100190, China
   Feng-Kun Guo [email protected] CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics,
Chinese Academy of Sciences, Beijing 100190, China
School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China Peng Huanwu Collaborative Center for Research and Education, Beihang University, Beijing 100191, China
Abstract

It has been generally expected that the X(3872)X(3872) has a spin-2 partner, X2X_{2}, with quantum numbers JPC=2++J^{PC}=2^{++}. In the hadronic molecular model, its mass was predicted to be below the DD¯D^{*}\bar{D}^{*} threshold, and the new structure reported in the γψ(2S)\gamma\psi(2S) invariant mass distribution by the Belle Collaboration with mass M=(4014.3±4.0±1.5)M=(4014.3\pm 4.0\pm 1.5) MeV and decay width Γ=(4±11±6)\Gamma=(4\pm 11\pm 6) MeV, with a global significance of 2.8 σ\sigma, is a nice candidate for it. We consider the radiative decay widths for the X2γψX_{2}\to\gamma\psi with ψ=J/ψ,ψ(2S)\psi=J/\psi,\psi(2S) treating the X2X_{2} as a DD¯D^{*}\bar{D}^{*} shallow bound state, and estimate the events of X2X_{2} in two-photon collisions that can be collected in the γJ/ψγ+\gamma J/\psi\to\gamma\ell^{+}\ell^{-} (=e,μ\ell=e,\mu) final states at Belle. Based on the upper limit for the ratio of decay widths of X(3872)γψ(2S)X(3872)\to\gamma\psi(2S) and X(3872)γJ/ψX(3872)\to\gamma J/\psi measured by BESIII, we predict the similar ratio Γ(X2γψ(2S))/Γ(X2γJ/ψ)\Gamma(X_{2}\to\gamma\psi(2S))/\Gamma(X_{2}\to\gamma J/\psi) to be smaller than 1.01.0. We suggest searching for the X2X_{2} signal in the γJ/ψ\gamma J/\psi invariant mass distribution via two-photon fusions. The results will lead to insights into both the X(3872)X(3872) and the new structure observed by Belle.

I Introduction

The hadron spectroscopy of mesons and baryons with heavy quarks (charm and bottom) has been an important laboratory in the quest for understanding quantum chromodynamics (QCD) at the confinement scale due to the large bulk of experimental information accumulated over the last two decades. Many new hadronic states observed in the heavy sector seem to not fit into the predictions from the potential quark models such as the well-known Godfrey-Isgur quark model [1]. This fact has triggered a debate about the nature of those hadrons, and assumptions of different multiquark configurations beyond the conventional quark-antiquark/three quarks were put forward in order to explain their properties, such as mass, decay width, and the JPCJ^{PC} quantum numbers, i.e., the total angular momentum JJ, parity PP, and charge conjugation CC (see the reviews [2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13]).

Among these models, the molecular picture seems to be a natural one since the majority of the new hadrons are near some hadron-hadron threshold. In the charm sector, for instance, the X(3872)X(3872) state is just at the DD¯D\bar{D}^{*} (D¯D)(\bar{D}D^{*}) threshold, and its properties are suitably described considering the X(3872)X(3872) as a DD¯D\bar{D}^{*} molecular state (for a review focusing on the hadonic molecular model of the X(3872)X(3872), see Ref. [14]). In fact, the X(3872)X(3872) was the first among those new hadrons observed experimentally by the Belle Collaboration in 2003 [15], with JPC=1++J^{PC}=1^{++} quantum numbers determined by the LHCb Collaboration a decade later [16]. It is, to date, the most well-studied state, and it is not a surprise that its experimental and theoretical information is used as inputs for predictions of new hadronic states in the heavy quark sector. In Ref. [17], the authors assumed the X(3872)X(3872) as a DD¯D\bar{D}^{*} molecule and concluded that a DD¯D^{*}\bar{D}^{*} state should exist as a consequence of the heavy-quark spin symmetry for the system under consideration. Specifically, using a contact-range (pionless) effective field theory, they claimed that the new state, from now on called X2X_{2}, is the spin-22 partner of the X(3872)X(3872), with a similar value for the binding energy and mass of about 40124012 MeV. Such a state was first predicted in Ref. [18] long ago with a mass M=4015M=4015 MeV and later in Refs. [19, 17, 20, 21, 22, 23, 24, 25, 26, 27, 28, 29, 30, 31, 32, 33, 34] using various phenomenological models.

Recently, the Belle collaboration reported a hint of an isoscalar structure with mass M=(4014.3±4.0±1.5)M=(4014.3\pm 4.0\pm 1.5) MeV and width ΓX2=(4±11±6)\Gamma_{X_{2}}=(4\pm 11\pm 6) MeV, seen in the γψ(2S)\gamma\psi(2S) invariant mass distribution via a two-photon process [35]. The global significance is 2.8σ2.8\sigma. This new structure is located near the DD¯D^{*}\bar{D}^{*} threshold which leads us to conclude that it is a promising candidate for the DD¯D^{*}\bar{D}^{*} shallow bound state.111In Refs. [36, 37], this structure was assumed to be a DD¯D^{*}\bar{D}^{*} molecule with JPC=0++J^{PC}=0^{++}. In addition, the mass value predicted in Refs. [17, 23] is in good agreement with the experimental one reported by Belle [35], and the measured width well matches the predicted one, of the order of a few MeV, in Ref. [27] despite that there is a sizeable uncertainty in the theoretical predictions [27, 28]. Thus, this narrow structure could be a hint for the X2X_{2} state, supporting the theoretical predictions in Refs. [17, 18, 23].

Alternatively, by looking at the spectra of tetraquarks, there also exists spin partners of 1++1^{++} states that reproduce the 2++2^{++} quantum numbers of X2X_{2} as well as its mass [38, 39, 40, 41]. Although the authors of these works were not particularly aiming at the X2X_{2} state, it is still possible to assign the results to such a structure. On the other hand, a 2++2^{++} tensor state with a similar mass could also be described as a conventional 2P2P charmonium state [1, 42]; in this case, the χc2(3930)\chi_{c2}(3930) [43] would be an exotic meson.

One way to disentangle those different multiquark configurations from the molecular point of view is to check the mass splitting between the 2++2^{++} and 1++1^{++} states. In Refs. [17, 23], the corresponding mass splitting is approximately equal to that between the vector and pseudoscalar charmed mesons, that is

mX2mXmDmD140MeV,m_{X_{2}}-m_{X}\sim m_{D^{*}}-m_{D}\sim 140~{}\textrm{MeV}\,, (1)

with mD(mD)m_{D}(m_{D^{*}}) the pseudoscalar (vector) charmed meson mass. On the other hand, within the tetraquark approach, for instance, in Ref. [38] the 2++1++2^{++}-1^{++} is about 8080 MeV, which is smaller than the difference given in Eq. (1). A similar conclusion is found for the difference between the first radially excited charmonia 2++2^{++} and 1++1^{++} by looking at the results for both the Godfrey-Isgur quark model [1] and the one using a screened potential [42], which are about 3030 MeV and 4040 MeV, respectively.

Even though only the Belle experiment has reported a signal relevant to the spin-22 partner of the X(3872)X(3872), such a structure can also be searched for in other ongoing and future experiments, e.g., BESIII and its upgrade, LHCb, and PANDA. Belle II also has plans to search for the X2X_{2} state soon. In line with the current and upcoming experiments that will provide more information about such a structure, it is crucial to extend the theoretical studies surveying the X2X_{2} system. In other words, we should further explore the 2++2^{++} tensor state to help discriminate the various multiquark models used to describe the X2X_{2} structure.

The decays of a 2++2^{++} tensor structure have been studied in Refs. [44, 45]. In particular, considering that state as the first radial excitation of the PP-wave χc2\chi_{c2} (23P22^{3}P_{2}) charmonium, the quark model adopted in Ref. [44, 45] provides width estimates for the X2X_{2} decay to charmed mesons around tens of MeV. Moreover, the hadronic decays of the DD¯D^{*}\bar{D}^{*} SS-wave hadronic molecule, into DD¯D\bar{D} and DD¯D\bar{D}^{*} meson pairs were estimated to be of the order of a few MeV in Ref. [27] and can be as large as 50 MeV in Ref. [28].

Furthermore, the X2γDD¯X_{2}\to\gamma D\bar{D}^{*} decay width was also calculated in Ref. [27] to be of the keV order. In contrast to the hadronic decays that, according to Ref. [27], has a strong dependence on the ultraviolet (UV) form factors and therefore are sensitive to the short-distance details, radiative decays into γDD¯\gamma D\bar{D}^{*} are more sensitive to the long-distance structure of the resonance. Thus, as argued in Ref. [27], one can extract valuable information about the X2X_{2} wave function, as well as about DD¯D\bar{D}^{*} interactions, by surveying such decays. It is not difficult to understand this feature. In the (DD¯)γDD(D^{*}\bar{D}^{*})\to\gamma DD^{*} process, the final state receives leading contribution from the one-body transition DDγD^{*}\to D\gamma, which has no direct relation to the two-body interaction accounting for the short-distance part of the X2X_{2} state. Therefore, the long-range structure of X2X_{2} that determines its coupling to DD¯D^{*}\bar{D}^{*} has an essential role in its radiative decay into γDD¯\gamma D\bar{D}^{*}.

Additional interesting decay modes of the X2X_{2} which have not been explored before include the radiative decays into γψ(2S)\gamma\psi(2S) and γJ/ψ\gamma J/\psi channels. Such a study may help to discriminate the X2X_{2} nature from the cc¯c\bar{c} meson χc2(2P)\chi_{c2}(2P) possibility. As discussed in, e.g., Ref. [46], the radiative decay matrix element is proportional to the overlap between the wave functions corresponding to the initial and final states. Specifically, for transitions between two charmonia, that overlap is influenced by the position of the nodes of the wave function. Hence, the one-node wave function for the ψ(2S)\psi(2S) state has an overlap with the χc2(2P)\chi_{c2}(2P) larger than that for the J/ψJ/\psi one, which is nodeless, such that the following ratio

RX2Br(X2γψ(2S))Br(X2γJ/ψ),\displaystyle R_{X_{2}}\equiv\frac{\text{Br}\left(X_{2}\to\gamma\psi(2S)\right)}{\text{Br}\left(X_{2}\to\gamma J/\psi\right)}, (2)

should be much larger than the one if the initial particle is the χc2(2P)\chi_{c2}(2P) charmonium. Table 1 shows some results for RX2R_{X_{2}} obtained in different quark models [44, 45]. Therefore, to confront these results, we evaluate the X2X_{2} radiative decays into γψ(2S)\gamma\psi(2S) and γJ/ψ\gamma J/\psi, assuming that the X2X_{2} resonance is a DD¯D^{*}\bar{D}^{*} molecular partner of the X(3872)X(3872) state, predicted in Refs. [17, 23] according to heavy quark spin symmetry (HQSS).

Table 1: Some results for the radiative decays of the 23P22^{3}P_{2} charmonium calculated with quark model. Γψ\Gamma_{\psi} denotes the decay width for 23P2γψ2^{3}P_{2}\to\gamma\psi with ψ=J/ψ,ψ(2S)\psi=J/\psi,\psi(2S).
ΓJ/ψ\Gamma_{J/\psi} [keV] Γψ(2S)\Gamma_{\psi(2S)} [keV] RX2R_{X_{2}}
Ref. [44] 53 207 3.9
Ref. [45] 81 304 3.8

In order to calculate those radiative decay widths, we employ the couplings of the ψ\psi mesons to charmed mesons respecting HQSS and the magnetic and electric couplings of charmed mesons and a photon. The nonrelativistic effective field theory is applied to depict the coupling of the X2X_{2} to DD¯D^{*}\bar{D}^{*}, which is related to the binding energy of X2X_{2}. After calculating the radiative decay widths for X2ψγX_{2}\to\psi\gamma with ψ=J/ψ,ψ(2S)\psi=J/\psi,\psi(2S), the upper limit of the ratio RX2R_{X_{2}} is predicted with the use of the experimental result reported by the BESIII collaboration RX(3872)<0.59R_{X(3872)}<0.59 at 90%90\% confidence level [47], and the results for the radiative decays of X(3872)X(3872) in the hadronic molecular picture [46]. Taking into account the signal yield of X2X_{2} in the γψ(2S)\gamma\psi(2S) invariant mass distribution measured by Belle [35], and the predicted upper bound of RX2R_{X_{2}}, we also estimate the lower limit of the signal yield of X2X_{2} in the γJ/ψ\gamma J/\psi mode via the two-photon process at Belle, with J/ψJ/\psi reconstructed in lepton-antilepton pairs.

The structure of the paper is as follows. In Section II, we discuss the interaction Lagrangians and the main parameters used as well as the relevant Feynman diagrams contributing to the decay process X2γψX_{2}\to\gamma\psi. The radiative decay ratio RX2R_{X_{2}} and the signal yield of X2X_{2} in the γJ/ψ\gamma J/\psi mode are predicted in Section III. A summary is given in Section IV. Finally, in Appendix A, we provide an update for the results corresponding to the radiative decay widths for X(3872)γψX(3872)\to\gamma\psi discussed in Ref. [46].

II Formalism

II.1 The Lagrangian and vertices

As discussed in Refs. [48, 49, 50] hadron loops play an important role in certain hadron transitions. For pure hadronic molecules, those loops are the leading order contribution to the corresponding transition amplitudes due to the large coupling of the molecule to its constituents. In our case, the X2X_{2} radiative decays under consideration proceeds through the loops depicted in Fig. 1.

Refer to caption
(a)
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(b)
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(c)
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(d)
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(e)
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(f)
Figure 1: Feynman diagrams for X2γψX_{2}\rightarrow\gamma\psi (ψ=J/ψ,ψ(2S)\psi=J/\psi,\psi(2S)).

In order to evaluate each diagram displayed in Fig. 1, we need first to define the interaction Lagrangian that describes all the vertices involved in such loops. We start by the X2DD¯X_{2}\,D^{*}\bar{D}^{*} interaction vertex that is described by the following Lagrangian

X2=χnr0X2D0μμνD¯ν+χnrcX2D+μμνDν+h.c.,\displaystyle{\cal L}_{X_{2}}=\chi^{0}_{\text{nr}}X_{2}{}_{\mu\nu}^{{\dagger}}D^{*0\mu}{\bar{D}}^{*\nu}+\chi^{c}_{\text{nr}}X_{2}{}_{\mu\nu}^{{\dagger}}D^{*+\mu}D^{*-\nu}+\text{h.c.}, (3)

where χnr0\chi_{\text{nr}}^{0} and χnrc\chi_{\text{nr}}^{c} are the X2X_{2} couplings to the neutral (0) and charged (c)(c) charmed mesons, while the subscript “nr” stands for “nonrelativistic”. As we know, there is a slight difference between the neutral and charged meson masses that leads to an isospin-breaking effect. However, according to Refs. [17, 27], this effect is small so that the couplings χnr0\chi_{\rm nr}^{0} and χnrc\chi_{\rm nr}^{c} are approximately the same. In addition, the relative size of X2X_{2} is much smaller compared to the Bohr radius of a ground-state hadronic atom, made out of the charged D+D^{*+} and DD^{*-} mesons, so that the electromagnetic effects can be ignored in such a scenario. Therefore, we follow Ref. [46] and set χnr0=χnrc=χnr\chi_{\text{nr}}^{0}=\chi_{\text{nr}}^{c}=\chi_{\text{nr}}. The X2DD¯X_{2}D^{*}\bar{D}^{*} vertex is then

ΓμναβX2=iχnrgμαgνβ.\displaystyle\Gamma_{\mu\nu\alpha\beta}^{X_{2}}=i\chi_{\text{nr}}\,g_{\mu\alpha}\,g_{\nu\beta}\,. (4)

Next, the interaction vertex between the ψ\psi and charmed D()D^{(*)} and D¯()\bar{D}^{(*)} mesons can be extracted from

ψ=\displaystyle{\cal L}_{\psi}= g2ψμ(D¯ννD+μD¯νμDνD¯μνD)νg2ψμD¯μD\displaystyle\,g_{2}\psi_{\mu}\left({\bar{D}}^{*{\dagger}}{}^{\nu}\overleftrightarrow{\partial}_{\nu}D^{*{\dagger}}{}^{\mu}+{\bar{D}}^{*{\dagger}}{}^{\mu}\overleftrightarrow{\partial}_{\nu}D^{*{\dagger}}{}^{\nu}-{\bar{D}}^{*{\dagger}}{}^{\nu}\overleftrightarrow{\partial}^{\mu}D^{*{\dagger}}{}_{\nu}\right)-g_{2}\psi_{\mu}{\bar{D}}^{{\dagger}}\overleftrightarrow{\partial}^{\mu}D^{{\dagger}}
ig2ϵμναβψμvα(D¯βνDD¯βD)ν+h.c.,\displaystyle-ig_{2}\epsilon^{\mu\nu\alpha\beta}\psi_{\mu}v_{\alpha}\left({\bar{D}}^{*{\dagger}}{}_{\nu}\overleftrightarrow{\partial}_{\beta}D^{{\dagger}}-{\bar{D}}^{{\dagger}}\overleftrightarrow{\partial}_{\beta}D^{*{\dagger}}{}_{\nu}\right)+\text{h.c.}, (5)

encoding HQSS [51, 52]. In Eq. (5), vαv_{\alpha} is the four-velocity of the charmed meson. By defining the four-momentum as pα=mD()vα+kαp_{\alpha}=m_{D^{(*)}}v_{\alpha}+k_{\alpha}, with kαk_{\alpha} a residual momentum of 𝒪(ΛQCD)\mathcal{O}(\Lambda_{\text{QCD}}), and recalling that v2=1v^{2}=1, we can write vαv_{\alpha} as

vα=pαmD()𝒪(kαmD()),v_{\alpha}=\frac{p_{\alpha}}{m_{D^{(*)}}}-{\cal O}\left(\frac{k_{\alpha}}{m_{D^{(*)}}}\right)\,, (6)

where mD()m_{D^{(*)}} is the charmed meson mass. Furthermore, we can write the coupling constant g2g_{2} in terms of the relativistic couplings gDD¯,gDD¯g_{D\bar{D}},g_{D\bar{D}^{*}}, and gDD¯g_{D^{*}\bar{D}^{*}} as given in Refs. [52, 49, 46], that is

gD¯D=g2mDmψ,gD¯D=2g2mDmψmD,gD¯D=g2mDmψ,\displaystyle g_{{\bar{D}}D}=g_{2}m_{D}\sqrt{m_{\psi}},\quad g_{{\bar{D}}^{*}D}=2g_{2}\sqrt{\frac{m_{D}m_{\psi}}{m_{D^{*}}}},\quad g_{{\bar{D}}^{*}D^{*}}=g_{2}m_{D^{*}}\sqrt{m_{\psi}}, (7)

where mψm_{\psi} is the mass of the ψ\psi meson. From Eq. (5) we extract the interaction vertices ψμ(p)D¯ν(k1)D(k2)\psi_{\mu}(p)\to\bar{D}^{*}_{\nu}(k_{1})D(-k_{2}) and ψμ(p)D¯α(k1)Dβ(k2)\psi_{\mu}(p)\to\bar{D}^{*}_{\alpha}(k_{1})D^{*}_{\beta}(-k_{2}), which are

Γμν(D¯D)\displaystyle\Gamma^{({\bar{D}}^{*}D)}_{\mu\nu} =i2g2mDϵμναβk1αk2β,\displaystyle=-i\frac{2g_{2}}{m_{D^{*}}}\epsilon_{\mu\nu\alpha\beta}\,k_{1}^{\alpha}\,k_{2}^{\beta}, (8)
Γμαβ(D¯D)\displaystyle\Gamma^{({\bar{D}}^{*}D^{*})}_{\mu\alpha\beta} =g2[(k1+k2)αgμβ+(k1+k2)βgμα(k1+k2)μgαβ].\displaystyle=g_{2}\left[(k_{1}+k_{2})_{\alpha}\,g_{\mu\beta}+(k_{1}+k_{2})_{\beta}\,g_{\mu\alpha}-(k_{1}+k_{2})_{\mu}\,g_{\alpha\beta}\right]. (9)

Now, we move on to the interaction between the charmed mesons and the photon. In this case, we have two couplings corresponding to the electric and magnetic interactions. The former is obtained by gauging the kinetic term associated with the charged D()D^{(*)} mesons, which is

e=\displaystyle{\cal L}_{e}= μDμDmD2DD+ieQDAμ(μDDDμD)+e2QD2AμAμDD12DμνDμν\displaystyle\,\partial_{\mu}D^{{\dagger}}\partial^{\mu}D-m_{D}^{2}D^{{\dagger}}D+ie\text{Q}_{D}A_{\mu}\left(\partial^{\mu}D^{{\dagger}}D-D^{{\dagger}}\partial^{\mu}D\right)+e^{2}\text{Q}_{D}^{2}A_{\mu}A^{\mu}D^{{\dagger}}D-\frac{1}{2}D^{*{\dagger}}_{\mu\nu}D^{*}{}^{\mu\nu}
+mD2DμD+μieQDAμ(DνμD+ννDDμνDννD)μ\displaystyle+m_{D^{*}}^{2}D^{*{\dagger}}_{\mu}D^{*}{}^{\mu}+ie\text{Q}_{D^{*}}A_{\mu}\left(D^{*{\dagger}}_{\nu}~{}\overleftrightarrow{\partial}^{\mu}D^{*}{}^{\nu}+\partial_{\nu}D^{*{\dagger}}{}^{\mu}D^{*}{}^{\nu}-D^{*{\dagger}}{}^{\nu}\partial_{\nu}D^{*}{}^{\mu}\right)
e2QD2(AμAμDνDνAμAνDDν)μ,\displaystyle-e^{2}\text{Q}_{D^{*}}^{2}\left(A_{\mu}A^{\mu}D^{*{\dagger}}_{\nu}D^{*}{}^{\nu}-A_{\mu}A_{\nu}D^{*{\dagger}}{}^{\nu}D^{*}{}^{\mu}\right), (10)

with eQD()e\text{Q}_{D^{(*)}} standing for the electric charge of the heavy D()D^{(*)} meson, and Dμν=μDννDμD^{*}_{\mu\nu}=\partial_{\mu}D^{*}_{\nu}-\partial_{\nu}D^{*}_{\mu}. The Dμ(k1)±Dα(k2)±γβ(q)D^{*}_{\mu}{}^{\pm}(k_{1})\to D^{*}_{\alpha}{}^{\pm}(k_{2})\gamma_{\beta}(q) vertex reads

Γμαβ(e)\displaystyle\Gamma^{(e)}_{\mu\alpha\beta} =ie|QD|[(k1+k2)βgμαk1gμβαk2gαβμ].\displaystyle=ie|\text{Q}_{D^{*}}|\left[(k_{1}+k_{2})_{\beta}g_{\mu\alpha}-k_{1}{}_{\alpha}g_{\mu\beta}-k_{2}{}_{\mu}g_{\alpha\beta}\right]. (11)

Note that this vertex satisfies the Ward-Takahashi identity, as discussed in Ref. [46]. Besides, after gauging the vertex of Eq. (9), a four-point vertex for ψμ(p)γν(q)Dα(k1)Dβ+(k2)\psi_{\mu}(p)\gamma_{\nu}(q)\to D^{*-}_{\alpha}(k_{1})D^{*+}_{\beta}(-k_{2}), see the diagram in Fig. 1 (e), reads

Γμναβ(e)=2e|QD|g2(gμβgνα+gμαgνβgμνgαβ).\displaystyle\Gamma^{(e)}_{\mu\nu\alpha\beta}=2e|\text{Q}_{D^{*}}|g_{2}\left(g_{\mu\beta}g_{\nu\alpha}+g_{\mu\alpha}g_{\nu\beta}-g_{\mu\nu}g_{\alpha\beta}\right). (12)

On the other hand, the magnetic vertices are extracted from the Lagrangian [53]

m=\displaystyle{\cal L}_{m}= ieFμν(DμDνDνDμ)(Qβ2Q2mc)+eϵμναβFμνvα(DDβ+DβD)(Qβ2+Q2mc)\displaystyle-ieF^{\mu\nu}\left(D^{*{\dagger}}_{\mu}D^{*}_{\nu}-D^{*{\dagger}}_{\nu}D^{*}_{\mu}\right)\left(\frac{Q\beta^{\prime}}{2}-\frac{Q^{\prime}}{2m_{c}}\right)+e\epsilon^{\mu\nu\alpha\beta}F_{\mu\nu}v_{\alpha}\left(D^{{\dagger}}D^{*}_{\beta}+D^{*{\dagger}}_{\beta}D\right)\left(\frac{Q\beta^{\prime}}{2}+\frac{Q^{\prime}}{2m_{c}}\right)
+ieFμν(D¯μD¯νD¯νD¯μ)(Qβ2Q2mc)+eϵμναβFμνvα(D¯D¯β+D¯βD¯)(Qβ2+Q2mc),\displaystyle+ieF^{\mu\nu}\left({\bar{D}}^{*{\dagger}}_{\mu}{\bar{D}}^{*}_{\nu}-{\bar{D}}^{*{\dagger}}_{\nu}{\bar{D}}^{*}_{\mu}\right)\left(\frac{Q\beta^{\prime}}{2}-\frac{Q^{\prime}}{2m_{c}}\right)+e\epsilon^{\mu\nu\alpha\beta}F_{\mu\nu}v_{\alpha}\left({\bar{D}}^{{\dagger}}{\bar{D}}^{*}_{\beta}+{\bar{D}}^{*{\dagger}}_{\beta}{\bar{D}}\right)\left(\frac{Q\beta^{\prime}}{2}+\frac{Q^{\prime}}{2m_{c}}\right), (13)

where Q=Diag(2/3,1/3)Q=\text{Diag}(2/3,-1/3) is the light quark charge matrix, and Q=2/3Q^{\prime}=2/3 corresponds to the charge of the charm quark, while the FμνF_{\mu\nu} stands for the electromagnetic field tensor. In addition, mcm_{c} is the charm quark mass, and the parameter β\beta^{\prime} is discussed in Ref. [54]. From Eq. (13) the vertices Dμ(k1)γν(q)D(k2)D^{*}_{\mu}(k_{1})\to\gamma_{\nu}(q)D(k_{2}), Dμ(k1)γβ(q)Dα(k2)D^{*}_{\mu}(k_{1})\to\gamma_{\beta}(q)D^{*}_{\alpha}(k_{2}), D¯μ(k1)γν(q)D¯(k2){\bar{D}}^{*}_{\mu}(k_{1})\to\gamma_{\nu}(q){\bar{D}}(k_{2}) and D¯μ(k1)γβ(q)D¯α(k2){\bar{D}}^{*}_{\mu}(k_{1})\to\gamma_{\beta}(q){\bar{D}}^{*}_{\alpha}(k_{2}) are

Γμν(m)DDγ\displaystyle\Gamma^{(m)D^{*}D\gamma}_{\mu\nu} =eϵμναβvαqβ(βQ+Qmc),\displaystyle=e\epsilon_{\mu\nu\alpha\beta}v_{\alpha}q_{\beta}\left(\beta^{\prime}Q+\frac{Q^{\prime}}{m_{c}}\right), (14)
Γμαβ(m)DDγ\displaystyle\Gamma^{(m)D^{*}D^{*}\gamma}_{\mu\alpha\beta} =ie(qαgμβqμgαβ)(βQQmc),\displaystyle=ie(q_{\alpha}g_{\mu\beta}-q_{\mu}g_{\alpha\beta})\left(\beta^{\prime}Q-\frac{Q^{\prime}}{m_{c}}\right), (15)
Γμν(m)D¯D¯γ\displaystyle\Gamma^{(m){\bar{D}}^{*}{\bar{D}}\gamma}_{\mu\nu} =eϵμναβvαqβ(βQ+Qmc),\displaystyle=e\epsilon_{\mu\nu\alpha\beta}v_{\alpha}q_{\beta}\left(\beta^{\prime}Q+\frac{Q^{\prime}}{m_{c}}\right), (16)
Γμαβ(m)D¯D¯γ\displaystyle\Gamma^{(m){\bar{D}}^{*}{\bar{D}}^{*}\gamma}_{\mu\alpha\beta} =ie(qαgμβqμgαβ)(βQQmc).\displaystyle=-ie(q_{\alpha}g_{\mu\beta}-q_{\mu}g_{\alpha\beta})\left(\beta^{\prime}Q-\frac{Q^{\prime}}{m_{c}}\right). (17)

As in Eq. (11), these vertices also satisfy the appropriate Ward identity.

II.2 The amplitude X2γψX_{2}\rightarrow\gamma\psi

Once we have all the vertices in the loop diagrams in Fig. 1, we are able to write the amplitude for the X2γψX_{2}\to\gamma\psi decay. Namely,

i=ieχnrg2ϵ(X2)μνϵβ(γ)ϵσ(ψ)μνβσ,i{\cal M}=ie\,\chi_{\text{nr}}\,g_{2}\,\epsilon^{*}{}^{\mu\nu}(X_{2})\epsilon^{\beta}(\gamma)\epsilon^{\sigma}(\psi)\,{\cal M}_{\mu\nu\beta\sigma}, (18)

with ε(X2)μν,εβ(γ)\varepsilon^{*}{}^{\mu\nu}(X_{2}),\varepsilon^{\beta}(\gamma), and εσ(ψ)\varepsilon^{\sigma}(\psi) the polarization vectors for the X2X_{2} state, the photon, and ψ\psi mesons (ψ\psi^{\prime}, and J/ψJ/\psi), respectively. The tensor structure μνβσ{\cal M}_{\mu\nu\beta\sigma} in Eq. (18) encodes the contributions of all the diagrams in Fig. 1, and it is written as

μνβσ=\displaystyle{\cal M}_{\mu\nu\beta\sigma}= mX2mψd4k(2π)4Sνρ(k)Sμα(kp)\displaystyle\,\sqrt{m_{X_{2}}m_{\psi}}\int\frac{d^{4}k}{(2\pi)^{4}}S_{\nu}^{\rho}(k)S_{\mu}^{\alpha}(k-p)
(Jαρβσ(a)m(k)+Jαρβσ(a)e(k)+Jαρβσ(b)m(k)+Jαρβσ(c)m(k)+Jαρβσ(c)e(k)+Jαρβσ(d)m(k)+Jαρβσ(e)e(k)),\displaystyle\left(J_{\alpha\rho\beta\sigma}^{(a)m}(k)+J_{\alpha\rho\beta\sigma}^{(a)e}(k)+J_{\alpha\rho\beta\sigma}^{(b)m}(k)+J_{\alpha\rho\beta\sigma}^{(c)m}(k)+J_{\alpha\rho\beta\sigma}^{(c)e}(k)+J_{\alpha\rho\beta\sigma}^{(d)m}(k)+J_{\alpha\rho\beta\sigma}^{(e)e}(k)\right), (19)

where the superscripts (a)-(e) match the labels of each individual diagram in Fig. 1. Yet, the contributions in Eq. (19) with the labels mm and ee corresponds to the magnetic and electric couplings, respectively. Explicitly, each contribution in Eq. (19) reads

Jαρβσ(a)m(k)=\displaystyle J_{\alpha\rho\beta\sigma}^{(a)m}(k)= i3mD3Sξγ(kp+q)[(2kp+q)σgρξ(2kp+q)ρgσξ(2kp+q)ξgρσ]\displaystyle\frac{i}{3}m_{D^{*}}^{3}S^{\xi\gamma}(k-p+q)\left[(2k-p+q)_{\sigma}g_{\rho\xi}-(2k-p+q)_{\rho}g_{\sigma\xi}-(2k-p+q)_{\xi}g_{\rho\sigma}\right]
(qαgγβqγgαβ)(β4mc),\displaystyle(q_{\alpha}g_{\gamma\beta}-q_{\gamma}g_{\alpha\beta})\left(\beta^{\prime}-\frac{4}{m_{c}}\right), (20)
Jαρβσ(a)e(k)=\displaystyle J_{\alpha\rho\beta\sigma}^{(a)e}(k)= imD2Sξγ(kp+q)[(2kp+q)σgρξ(2kp+q)ρgσξ(2kp+q)ξgρσ]\displaystyle im_{D^{*}}^{2}S^{\xi\gamma}(k-p+q)\left[(2k-p+q)_{\sigma}g_{\rho\xi}-(2k-p+q)_{\rho}g_{\sigma\xi}-(2k-p+q)_{\xi}g_{\rho\sigma}\right]
[(2k2p+q)βgαγ(kp+q)αgγβ(kp)γgαβ],\displaystyle\left[(2k-2p+q)_{\beta}g_{\alpha\gamma}-(k-p+q)_{\alpha}g_{\gamma\beta}-(k-p)_{\gamma}g_{\alpha\beta}\right], (21)
Jαρβσ(b)m(k)=\displaystyle J_{\alpha\rho\beta\sigma}^{(b)m}(k)= 2i3mDS(kp+q)ϵσργδkγ(kp+q)δϵαβξη(kp)ξqη(β+4mc),\displaystyle-\,\frac{2i}{3}m_{D^{*}}S(k-p+q)\epsilon_{\sigma\rho\gamma\delta}k^{\gamma}(k-p+q)^{\delta}\epsilon_{\alpha\beta\xi\eta}(k-p)^{\xi}q^{\eta}\left(\beta^{\prime}+\frac{4}{m_{c}}\right), (22)
Jαρβσ(c)m(k)=\displaystyle J_{\alpha\rho\beta\sigma}^{(c)m}(k)= i3mD3Sξγ(kq)[(2kpq)σgαξ(2kpq)ξgσα(2kpq)αgσξ]\displaystyle-\,\frac{i}{3}m_{D^{*}}^{3}S^{\xi\gamma}(k-q)\left[(2k-p-q)_{\sigma}g_{\alpha\xi}-(2k-p-q)_{\xi}g_{\sigma\alpha}-(2k-p-q)_{\alpha}g_{\sigma\xi}\right]
(qγgρβqρgβγ)(β4mc),\displaystyle(q_{\gamma}g_{\rho\beta}-q_{\rho}g_{\beta\gamma})\left(\beta^{\prime}-\frac{4}{m_{c}}\right), (23)
Jαρβσ(c)e(k)=\displaystyle J_{\alpha\rho\beta\sigma}^{(c)e}(k)= imD2Sξγ(kq)[(2kpq)σgαξ(2kpq)ξgσα(2kpq)αgσξ]\displaystyle im_{D^{*}}^{2}S^{\xi\gamma}(k-q)\left[(2k-p-q)_{\sigma}g_{\alpha\xi}-(2k-p-q)_{\xi}g_{\sigma\alpha}-(2k-p-q)_{\alpha}g_{\sigma\xi}\right]
[(2kq)βgργkγgρβ(kq)ρgγβ],\displaystyle\left[(2k-q)_{\beta}g_{\rho\gamma}-k_{\gamma}g_{\rho\beta}-(k-q)_{\rho}g_{\gamma\beta}\right], (24)
Jαρβσ(d)m(k)=\displaystyle J_{\alpha\rho\beta\sigma}^{(d)m}(k)= 2i3mDS(kq)ϵρβξηkξqηϵσαγδ(kq)γ(kp)δ(β+4mc),\displaystyle\frac{2i}{3}m_{D}S(k-q)\epsilon_{\rho\beta\xi\eta}k^{\xi}q^{\eta}\epsilon_{\sigma\alpha\gamma\delta}(k-q)^{\gamma}(k-p)^{\delta}\left(\beta^{\prime}+\frac{4}{m_{c}}\right), (25)
Jαρβσ(e)(k)=\displaystyle J_{\alpha\rho\beta\sigma}^{(e)}(k)=  2mD2(gασgβρ+gσρgαβgαρgβσ),\displaystyle\,2m_{D^{*}}^{2}\left(g_{\alpha\sigma}g_{\beta\rho}+g_{\sigma\rho}g_{\alpha\beta}-g_{\alpha\rho}g_{\beta\sigma}\right)\,, (26)

with SS and SμνS_{\mu\nu} the propagator for the heavy fields DD and DD^{*}, respectively, given by

S(p~)\displaystyle S(\tilde{p}) =ip~2mD2+iϵ,\displaystyle=\frac{i}{\tilde{p}^{2}-m_{D}^{2}+i\epsilon},
Sμν(p~)\displaystyle S_{\mu\nu}(\tilde{p}) =ip~2mD+iϵ(gμν+p~μp~νmD2).\displaystyle=\frac{i}{\tilde{p}^{2}-m_{D^{*}}+i\epsilon}\left(-g_{\mu\nu}+\frac{\tilde{p}_{\mu}\tilde{p}_{\nu}}{m_{D^{*}}^{2}}\right). (27)

The factor mX2mψ\sqrt{m_{X_{2}}\,m_{\psi}} in Eq. (19) accounts for the normalization of the heavy meson fields.222Except for the electric coupling in Eq. (11), we use the nonrelativistic normalization for the heavy mesons (including the charmonium, charmed mesons, and X2X_{2}), which differs from the traditional relativistic normalization by a factor mH\sqrt{m_{H}}. It is worth noticing that, as a consistency check, the loop amplitude in Eq. (19) is gauge invariant, as we must expect.

The loop amplitude defined in Eq. (19) is a UV divergent integral. In order to have a well-defined amplitude from which we can get consistent results, we add a X2γψX_{2}\gamma\psi counterterm amplitude like the case for the X(3872)γψX(3872)\to\gamma\psi [46], depicted in Fig. 1(f), to the one given in Eq. (19). Specifically, it is

icont=\displaystyle i{\cal M}^{\text{cont}}= iλ1ϵμν(X2)ϵμ(γ)ϵν(ψ)+iλ2qμqνϵμν(X2)pϵ(γ)qϵ(ψ)\displaystyle\,i\lambda_{1}\epsilon^{*}_{\mu\nu}(X_{2})\epsilon^{\mu}(\gamma)\epsilon^{\nu}(\psi)+i\lambda_{2}q^{\mu}q^{\nu}\epsilon^{*}_{\mu\nu}(X_{2})p\cdot\epsilon(\gamma)q\cdot\epsilon(\psi)
+iλ3qμϵν(ψ)ϵμνpϵ(γ)+iλ4qμϵν(γ)ϵμνpϵ(ψ)+iλ5qμqνϵμνϵ(γ)ϵ(ψ),\displaystyle+i\lambda_{3}q^{\mu}\epsilon^{\nu}(\psi)\epsilon^{*}_{\mu\nu}p\cdot\epsilon(\gamma)+i\lambda_{4}q^{\mu}\epsilon^{\nu}(\gamma)\epsilon^{*}_{\mu\nu}p\cdot\epsilon(\psi)+i\lambda_{5}q^{\mu}q^{\nu}\epsilon^{*}_{\mu\nu}\epsilon(\gamma)\cdot\epsilon(\psi), (28)

which is straightforward to see its manifest gauge invariance. These terms are defined such that λr\lambda_{r} (r=1,...,5r=1,\,.\,.\,.,5), which is subject to renormalization, absorbs the UV divergence from the loops in Eq. (19), as done in Ref. [46]. On the one hand, the counterterm defined in Ref. [46] has only one parameter λ\lambda; on the other hand, in our case, Eq. (28) has five terms with each one having its strength λr\lambda_{r}. However, for our purposes, we do not consider relations among them.

The X2γψX_{2}\to\gamma\psi two-body decay width is given by the following formula

ΓX2=\displaystyle\Gamma_{X_{2}}= e2χnr2g22polarizations15q8πmX22|ϵ(X2)μνϵβ(γ)ϵσ(ψ)μνβσ|2\displaystyle\,e^{2}\chi_{\text{nr}}^{2}g_{2}^{2}\sum_{\text{polarizations}}\frac{1}{5}\frac{q}{8\pi m_{X_{2}}^{2}}\left|\epsilon^{*}{}^{\mu\nu}(X_{2})\epsilon^{\beta}(\gamma)\epsilon^{\sigma}(\psi){\cal M}_{\mu\nu\beta\sigma}\right|^{2}
=\displaystyle= e2χnr2g22q40πmX22μνβσμνβσg¯σσ(pq,mψ)gββP(2)(p,mX2)μνμν,\displaystyle-\frac{e^{2}\chi_{\text{nr}}^{2}g_{2}^{2}~{}{q}}{40\pi m_{X_{2}}^{2}}{\cal M}_{\mu\nu\beta\sigma}\,{\cal M}_{\mu^{\prime}\nu^{\prime}\beta^{\prime}\sigma^{\prime}}^{*}\bar{g}^{\sigma\sigma^{\prime}}(p-q,m_{\psi})g^{\beta\beta^{\prime}}P^{(2)}{}^{\mu\nu\mu^{\prime}\nu^{\prime}}(p,m_{X_{2}}), (29)

where q=|q|q=|\vec{q\,}| stands for the momentum of the final states (γ\gamma or ψ\psi) in the center-of-mass frame,

q=mX22mψ22mX2.\displaystyle q=\frac{m_{X_{2}}^{2}-m_{\psi}^{2}}{2m_{X_{2}}}. (30)

Furthermore, Pμνμν(2)(p,mX2)P^{(2)}_{\mu\nu\mu^{\prime}\nu^{\prime}}(p,m_{X_{2}}) in Eq. (29) is the projection operator corresponding to the summation over the polarizations of X2X_{2}, which is given by [55]

Pμνμν(2)(p,mX2)=\displaystyle P^{(2)}_{\mu\nu\mu^{\prime}\nu^{\prime}}(p,m_{X_{2}})= polarizationsϵμν(p,mX2)ϵμν(p,mX2)\displaystyle\sum_{\text{polarizations}}\epsilon_{\mu\nu}(p,m_{X_{2}})\epsilon_{\mu^{\prime}\nu^{\prime}}(p,m_{X_{2}})
=\displaystyle= 12[g¯μμ(p,mX2)g¯νν(p,mX2)+g¯μν(p,mX2)g¯νμ(p,mX2)]\displaystyle\,\frac{1}{2}\left[\bar{g}_{\mu\mu^{\prime}}(p,m_{X_{2}})\bar{g}_{\nu\nu^{\prime}}(p,m_{X_{2}})+\bar{g}_{\mu\nu^{\prime}}(p,m_{X_{2}})\bar{g}_{\nu\mu^{\prime}}(p,m_{X_{2}})\right]
13g¯μν(p,mX2)g¯μν(p,mX2),\displaystyle-\frac{1}{3}\bar{g}_{\mu\nu}(p,m_{X_{2}})\bar{g}_{\mu^{\prime}\nu^{\prime}}(p,m_{X_{2}}), (31)

where g¯αβ\bar{g}_{\alpha\beta} denotes the summation over the polarization vectors

g¯αβ(p,m)=\displaystyle\bar{g}_{\alpha\beta}(p,m)= gαβ+pαpβm2,\displaystyle-g_{\alpha\beta}+\frac{p_{\alpha}p_{\beta}}{m^{2}}, (32)

with four-momentum pp and mass mm.

In the next subsection, we shall discuss the parameters used in our numerical analysis, which will be presented later in Section III.

II.3 The parameters

In order to numerically calculate the radiative decay widths of X2X_{2}, we should fix the values for the parameters used. The values for the meson masses are [43]

mD=1867.25MeV,mD=2008.56MeV,mX2=4014.3MeV,m_{D}=1867.25~{}\text{MeV},~{}m_{D^{*}}=2008.56~{}\text{MeV},~{}m_{X_{2}}=4014.3~{}\text{MeV},
mJ/ψ=3096.90MeV,mψ(2S)=3686.10MeV,m_{J/\psi}=3096.90~{}\text{MeV},~{}m_{\psi(2S)}=3686.10~{}\text{MeV},

where mDm_{D} (mDm_{D^{*}}) is the average mass between the neutral and charged DD (DD^{*}) mesons, and the X2X_{2} mass is taken from Ref. [35]. The charm quark mass and the parameter related to the magnetic coupling are fixed by the partial electromagnetic widths for D0γD0D^{*0}\to\gamma D^{0} and D+γD+D^{*+}\to\gamma D^{+} [54],

β1=379MeV,mc=1863MeV.\displaystyle\beta^{\prime-1}=379~{}\text{MeV},~{}m_{c}=1863~{}\text{MeV}. (33)

The coupling constant for X2X_{2} to the charged and neutral charmed mesons is extracted from the binding energy of X2X_{2} [56, 57],

χnr0={λ216πμ02EBμ0[1+𝒪(2μ0EBr)]}1/2,\displaystyle\chi^{0}_{\text{nr}}=\left\{\lambda^{2}\frac{16\pi}{\mu_{*0}}\sqrt{\frac{2E_{B}}{\mu_{*0}}}\left[1+{\cal O}(\sqrt{2\mu_{*0}E_{B}}r)\right]\right\}^{1/2}, (34)

where EBE_{B} and μ0\mu_{*0} are the binding energy of X2X_{2} relative to the D0D¯0D^{*0}\bar{D}^{*0} threshold and the D0D¯0D^{*0}\bar{D}^{*0} reduced mass, respectively. rr is identified with the range of forces, where 1/r2μ0EB1/r\gg\sqrt{2\mu_{*0}E_{B}} in the weak binding limit [58]. We assume that the X2X_{2} is a pure DD¯D^{*}\bar{D}^{*} bound state, λ2=1\lambda^{2}=1, and then we obtain the coupling constant χnr=1.31.3+1.0GeV1/2\chi_{\text{nr}}=1.3^{+1.0}_{-1.3}~{}\text{GeV}^{-1/2}, where the uncertainty is derived from the uncertainties of D0D^{*0} (D¯0\bar{D}^{*0}) and X2X_{2} masses. Besides, gg and gg^{\prime} denote the J/ψJ/\psi and ψ(2S)\psi(2S) couplings to the charmed mesons, respectively.

We evaluate the loop integrals in Fig. 1 by using the dimensional regularization method. In particular, we adopt the MS¯\overline{\text{MS}} subtraction scheme. As for the strength of the interaction corresponding to the counterterms, denoted by the λr\lambda_{r} parameters, following the idea in Ref. [46], we set to zero the contribution of the finite part of the counterterms in Eq. (28) and vary the energy scale in a large range, 1.5–7.0 GeV, in the UV divergent loop integrals. We define the ratios

rχ|χnrχ¯nr|,rχ|χnrχ¯nr|,rg|g2g20|,rg|g2g20|,\displaystyle r_{\chi}\equiv\left|\frac{\chi_{\text{nr}}}{\bar{\chi}_{\text{nr}}}\right|,\quad r^{\prime}_{\chi}\equiv\left|\frac{\chi^{\prime}_{\text{nr}}}{\bar{\chi}^{\prime}_{\text{nr}}}\right|,\quad r_{g}\equiv\left|\frac{g_{2}}{g^{0}_{2}}\right|,\quad r^{\prime}_{g}\equiv\left|\frac{g^{\prime}_{2}}{g^{0}_{2}}\right|, (35)

where g2g_{2} (g2g^{\prime}_{2}) is the coupling constant between J/ψJ/\psi (ψ(2S)\psi(2S)) and charmed mesons in Eq. (7). We take χ¯nr=1.3GeV1/2\bar{\chi}_{\text{nr}}=1.3~{}\text{GeV}^{-1/2} and g20=2.0GeV3/2g_{2}^{0}=2.0~{}\text{GeV}^{-3/2} with the latter from the model-dependent estimates discussed in Refs. [52, 49]. The X(3872)X(3872) coupling to DD¯D\bar{D}^{*} is denoted as χnr\chi^{\prime}_{\text{nr}}, and its benchmark value is set to χ¯nr=0.97GeV1/2\bar{\chi}^{\prime}_{\text{nr}}=0.97~{}\text{GeV}^{-1/2} [59].

In what follows, we present the numerical results for the X2X_{2} radiative decays into γψ\gamma\psi. In order to perform the numerical analysis, we have used the following Mathematica packages: FeynCalc [60], FeynHelpers [61], and Package-X [62].

III Numerical results

In Table 2, we show our numerical results for the partial decays X2γψX_{2}\to\gamma\psi with ψ=ψ(2S)\psi=\psi(2S) and J/ψJ/\psi as given in Eq. (29), along with the corresponding ratio RX2R_{X_{2}}. These observables depend on the products among the quantities defined in Eq. (35). In order to fix those quantities, we have to make assumptions on the coupling constants g2g_{2} and g2g_{2}^{\prime} since their values are not well established in the literature. Besides, we have also to fix the contribution from the contact terms, that is, to fix the size of λr\lambda_{r}’s in Eq. (28), which is unknown; however, as discussed Ref. [46], we may estimate their size by noticing that any change in μ\mu must also change the counterterms accordingly so that the overall result does not depend on the renormalization scale μ\mu. Thus, we set λr=0\lambda_{r}=0 and vary the scale μ\mu within a large range from 1.51.5 GeV up to 2mX22m_{X_{2}}, with mX2m_{X_{2}} the X2X_{2} mass, as mentioned above. In Table 2, we can see such behavior in the partial decays under consideration by noticing their corresponding changes as μ\mu varies. In other words, such variation in each partial decay width we are concerned with may be considered a measure of the size of λr\lambda_{r}’s.

Table 2: Decay widths and their ratio RR for the process XγψX\rightarrow\gamma\psi with X=X(3872),X2X=X(3872),X_{2} and ψ=J/ψ,ψ(2S)\psi=J/\psi,\psi(2S). Γψ\Gamma^{\prime}_{\psi} and Γψ\Gamma_{\psi} denote the decay width for X(3872)ψγX(3872)\to\psi\gamma and X2ψγX_{2}\to\psi\gamma, respectively. The first row is the energy scale in the MS¯\overline{\text{MS}} subtraction scheme, g2g_{2} (g2g^{\prime}_{2}) is the coupling constant in Eq. (7), and rχr^{\prime}_{\chi}, rgr_{g}, and rgr_{g}^{\prime} are defined in Eq. (35). In the last row, Nmin(X2γJ/ψ)N_{\text{min}}(X_{2}\to\gamma J/\psi) denotes the lower limit of the X2X_{2} signal yield in the J/ψγ+γJ/\psi\gamma\to\ell^{+}\ell^{-}\gamma (=e,μ\ell=e,\mu) mode for the two-photon process at Belle.
μ\mu (GeV) 1.5 2.0 4.0 7.0
ΓJ/ψ\Gamma^{\prime}_{J/\psi} (keV) 162 (rχrg)2(r^{\prime}_{\chi}r_{g})^{2} 176 (rχrg)2(r^{\prime}_{\chi}r_{g})^{2} 212 (rχrg)2(r^{\prime}_{\chi}r_{g})^{2} 244 (rχrg)2(r^{\prime}_{\chi}r_{g})^{2}
Γψ(2S)\Gamma^{\prime}_{\psi(2S)} (keV) 17.5 (rχrg)2(r^{\prime}_{\chi}r_{g}^{\prime})^{2} 18.4 (rχrg)2(r^{\prime}_{\chi}r_{g}^{\prime})^{2} 20.8 (rχrg)2(r^{\prime}_{\chi}r_{g}^{\prime})^{2} 22.7 (rχrg)2(r^{\prime}_{\chi}r_{g}^{\prime})^{2}
ΓJ/ψ\Gamma_{J/\psi} (keV) 139 (rχrg)2(r_{\chi}r_{g})^{2} 161 (rχrg)2(r_{\chi}r_{g})^{2} 224 (rχrg)2(r_{\chi}r_{g})^{2} 284 (rχrg)2(r_{\chi}r_{g})^{2}
Γψ(2S)\Gamma_{\psi(2S)} (keV) 25.0 (rχrg)2(r_{\chi}r_{g}^{\prime})^{2} 27.1 (rχrg)2(r_{\chi}r_{g}^{\prime})^{2} 32.7 (rχrg)2(r_{\chi}r_{g}^{\prime})^{2} 37.6 (rχrg)2(r_{\chi}r_{g}^{\prime})^{2}
RX(3872)R_{X(3872)} 0.11 (g2/g2)2(g_{2}^{\prime}/g_{2})^{2} 0.10 (g2/g2)2(g_{2}^{\prime}/g_{2})^{2} 0.10 (g2/g2)2(g_{2}^{\prime}/g_{2})^{2} 0.09 (g2/g2)2(g_{2}^{\prime}/g_{2})^{2}
RX2R_{X_{2}} 0.18 (g2/g2)2(g_{2}^{\prime}/g_{2})^{2} 0.17 (g2/g2)2(g_{2}^{\prime}/g_{2})^{2} 0.15 (g2/g2)2(g_{2}^{\prime}/g_{2})^{2} 0.13 (g2/g2)2(g_{2}^{\prime}/g_{2})^{2}
RX2/RX(3872)R_{X_{2}}/R_{X(3872)} 1.67 1.61 1.49 1.43
Nmin(X2γJ/ψ)N_{\text{min}}(X_{2}\to\gamma J/\psi) 35 36 39 41

As for the ratio RX2R_{X_{2}}, we set the finite part of the counterterm to zero and RX2R_{X_{2}} will depend only on the ratio g2/g2g_{2}^{\prime}/g_{2} at a given scale. In order to fix this latter ratio, we consider some model-dependent estimates. If g2/g2g_{2}^{\prime}/g_{2} is assumed to equal to unity, for the X(3872)X(3872) case the γψ(2S)\gamma\psi(2S) channel is relatively suppressed [46]. Similarly, in our case, by considering g2/g2=1g_{2}^{\prime}/g_{2}=1, we find that the γψ(2S)\gamma\psi(2S) channel is also suppressed. In Ref. [63], the ratio was fixed to g2/g2=1.67g_{2}^{\prime}/g_{2}=1.67 by modeling the couplings in a vector-meson dominance picture [52]; in this case, the γψ(2S)\gamma\psi(2S) channel is still suppressed relatively to the γJ/ψ\gamma J/\psi channel. Alternatively, we can fix g2/g2g_{2}^{\prime}/g_{2} by using the upper limit for the ratio RX(3872)R_{X(3872)} corresponding to the X(3872)γψ(2S)X(3872)\to\gamma\psi(2S) and γJ/ψ\gamma J/\psi, reported by BESIII in Ref. [47]. The X(3872)X(3872) radiative decays are discussed in Ref. [46] (see Appendix A which updates a couple of expressions in Ref. [46]). The results for the X(3872)X(3872) state are also shown in Table 2. Note that, in this case, the RX(3872)R_{X(3872)} barely changes as we vary the scale μ\mu. Thus, we can choose one specific value for μ\mu, for instance, μ=1.5\mu=1.5 GeV, and then, by using the BESIII measurement for RX(3872)<0.59R_{X(3872)}<0.59, we obtain from Table 2

g2/g2<2.34.g_{2}^{\prime}/g_{2}<2.34. (36)
Refer to caption
Refer to caption
Figure 2:  Scale dependence of the ratios RX(3872)R_{X(3872)} and RX2R_{X_{2}}, where μ\mu is the energy scale in the MS¯\overline{\text{MS}} subtraction scheme of the dimensional regularization method used to regularize the loops in Fig. 1. g2/g2=2.34g_{2}^{\prime}/g_{2}=2.34 is the upper bound given in Eq. (36), derived from the BESIII measurement RX(3872)<0.59R_{X(3872)}<0.59 [47], and g2/g2=1.67g_{2}^{\prime}/g_{2}=1.67 is the model value used in Ref. [63].

As a matter of checking, in Fig. 2, we show the plots for both ratios RX(3872)R_{X(3872)} and RX2R_{X_{2}} as a function of the scale μ\mu. As we can see, within the range 1.5GeVμ2mX1.5~{}\text{GeV}\leqslant\mu\leqslant 2m_{X}, those ratios are, to a good approximation, independent of μ\mu, as we expect.

As discussed above, both ratios RX(3872)R_{X(3872)} and RX2R_{X_{2}} depend on g2/g2g_{2}^{\prime}/g_{2} value, whose value is not fixed and model dependent. However, we can determine RX2R_{X_{2}} independently of the couplings g2g_{2}^{\prime} and g2g_{2}, using the experimental information for RX(3872)<0.59R_{X(3872)}<0.59, measured by BESIII in Ref. [47], as an input. Specifically, in Fig. 3 we show the double ratio RX2/RX(3872)R_{X_{2}}/R_{X(3872)} as a function of μ\mu. Note that this observable only slightly decreases from 1.671.67 to 1.431.43 as the renormalization scale μ\mu varies within the large range [1.5GeV,2mX2][1.5~{}\text{GeV},2\,m_{X_{2}}]. This flat variation indicates that we can set any value within that range for RX2/RX(3872)R_{X_{2}}/R_{X(3872)}, and then use the upper boundary RX(3872)<0.59R_{X(3872)}<0.59 provided by BESIII such that we obtain an upper limit for RX2R_{X_{2}}:

RX21.0.R_{X_{2}}\lesssim 1.0. (37)
Refer to caption
Figure 3: Scale dependence of the double ratio RX2/RX(3872)R_{X_{2}}/R_{X(3872)}.

Next, we shall estimate the number of events of X2X_{2} that can be collected in the γJ/ψ\gamma J/\psi final state of the two-photon process at the Belle experiment. The signal yield of X2X_{2} in such a process is given by

N(X2γψ)=ΓγγBr[X2]Br[ψ]ϵF(s,J)Ltot ,N(X_{2}\rightarrow\gamma\psi)=\Gamma_{\gamma\gamma}\operatorname{Br}\left[X_{2}\right]\operatorname{Br}[\psi]\epsilon F(\sqrt{s},J)L_{\text{tot }}, (38)

where Γγγ\Gamma_{\gamma\gamma} is the two-photon decay width of X2X_{2}, Br[X2]\textrm{Br}[X_{2}] is the branching fraction for X2γψ(ψ=J/ψ,ψ(2S))X_{2}\to\gamma\psi(\psi=J/\psi,\psi(2S)), ϵ\epsilon is the efficiency, and Ltot L_{\text{tot }} is the total integrated luminosity of the Belle data sample. In addition, for the ψ(2S)\psi(2S) reconstructed from J/ψπ+πJ/\psi\pi^{+}\pi^{-} as done in Ref. [35] and J/ψJ/\psi from the +\ell^{+}\ell^{-} lepton pairs (=e,μ\ell=e,\mu), one has Br[ψ(2S)]=Br[ψ(2S)π+πJ/ψ]Br[J/ψ+]\textrm{Br}[\psi(2S)]=\textrm{Br}\left[\psi(2S)\to\pi^{+}\pi^{-}J/\psi\right]\textrm{Br}\left[J/\psi\rightarrow\ell^{+}\ell^{-}\right] and Br[J/ψ]=\textrm{Br}[J/\psi]= Br[J/ψ+]\textrm{Br}\left[J/\psi\to\ell^{+}\ell^{-}\right]. The factor F(s,J)F(\sqrt{s},J) is related to the two-photon luminosity function LγγL_{\gamma\gamma} [64, 35]

F(s,J)=4π2(2J+1)Lγγ(s)/s,F(\sqrt{s},J)=4\pi^{2}(2J+1)L_{\gamma\gamma}(\sqrt{s})/s, (39)

with the effective energy of the two-photon collision s\sqrt{s} and the spin JJ for X2X_{2}. Since the two-photon decay width Γγγ\Gamma_{\gamma\gamma}, the efficiency ϵ\epsilon, the total integrated luminosity Ltot L_{\text{tot }} and the factor F(s,J)F(\sqrt{s},J) are the same for N(X2γJ/ψ)N\left(X_{2}\to\gamma J/\psi\right) and N(X2γψ(2S))N\left(X_{2}\to\gamma\psi(2S)\right), the signal yield of X2X_{2} in the γJ/ψ\gamma J/\psi with J/ψ+J/\psi\to\ell^{+}\ell^{-} is given by

N(X2γJ/ψ)=N(X2γψ(2S))RX2Br[ψ(2S)π+πJ/ψ].N(X_{2}\to\gamma J/\psi)=\frac{N(X_{2}\to\gamma\psi(2S))}{R_{X_{2}}\textrm{Br}[\psi(2S)\to\pi^{+}\pi^{-}J/\psi]}\,. (40)

The signal yield of X2X_{2} is 19±719\pm 7 in Ref. [35], and the branching fraction for ψ(2S)π+πJ/ψ\psi(2S)\to\pi^{+}\pi^{-}J/\psi is (34.68±0.30)%(34.68\pm 0.30)\% [43]. As discussed above, for μ=1.5\mu=1.5 GeV we have RX21.0R_{X_{2}}\lesssim 1.0, the yield of X2X_{2} is

N(X2γJ/ψ)35.N\left(X_{2}\rightarrow\gamma J/\psi\right)\gtrsim 35. (41)

Therefore, we estimate that the signal yield of X2X_{2} observed in the γJ/ψ\gamma J/\psi invariant mass distribution is at least about 35 for the two-photon collision at Belle. Besides, the minimal yields of X2X_{2} estimated with other energy scales are listed in Table 2. The prediction can be checked with the Belle data.

IV Summary

By assuming the existence of a tensor state X2X_{2}, that, according to HQSS, is a spin partner of the X(3872)X(3872) state in the hadronic molecular model, as predicted in Refs. [17, 18, 23], we have evaluated its radiative decays into γψ(2S)\gamma\,\psi(2S) and γJ/ψ\gamma\,J/\psi channels. Although with low statistics, a candidate of such a state was recently observed by the Belle Collaboration in Ref. [35], with mass and width in accordance with the corresponding values predicted in Refs. [17, 18, 23].

In particular, in our case, the decays we are concerned with proceed through hadronic loops with charmed mesons as intermediate particles. These loops are UV divergent, requesting an introduction of additional counterterm amplitude, in which the strength of that contact interaction absorbs the infinities after renormalization. However, with the available theoretical information, it is impossible to determine the contribution from the counterterms precisely. Notwithstanding, we estimated their contributions by varying the renormalization scale, as done in Ref. [46] for the X(3872)X(3872) case, such that the changes in the partial decay widths encode the size of the counterterm.

Moreover, we have used effective Lagrangians to describe the X2X_{2} couplings to the charmed DD^{*} and D¯\bar{D}^{*} mesons, and the couplings of those mesons with the charmonia ψ(2S)\psi(2S) and J/ψJ/\psi. Since these latter set of couplings are not well-determined in literature, we have written the partial decays X2γψ(2S)X_{2}\to\gamma\,\psi(2S) and X2γJ/ψX_{2}\to\gamma\,J/\psi in terms of ratios involving those couplings, that allows us to draw conclusions based on the relations among them.

According to our findings, for values of g2/g2g_{2}^{\prime}/g_{2} close to one, we always find suppression of the γψ(2S)\gamma\,\psi(2S) channel against the γJ/ψ\gamma\,J/\psi one. On the other hand, as g2/g2g_{2}^{\prime}/g_{2} increases the ratios RX(3872)R_{X(3872)} and RX2R_{X_{2}} increase accordingly. We have fixed the range of g2/g2g_{2}^{\prime}/g_{2} to be <2.34<2.34 using input from the BESIII measurement of RX(3872)<0.59R_{X(3872)}<0.59. Consequently, we found RX21.0R_{X_{2}}\lesssim 1.0. As a matter of comparison, RX2R_{X_{2}} estimated using the quark model assuming the X2X_{2} to be the χc2(2P)\chi_{c2}(2P) meson leads to a value about 4, as displayed in Table 1, significantly larger than the one we obtained in the hadronic molecular picture. In principle, future experimental measurements of the observable RX2R_{X_{2}} may shed light on the internal structure of X2X_{2}.

Finally, we predict the signal yield of X2X_{2} in the γJ/ψ\gamma\,J/\psi spectrum from the two-photon process based on our findings for RX2R_{X_{2}}, and also the yields of X2X_{2} in the γγγψ(2S)\gamma\,\gamma\to\gamma\,\psi(2S) reaction reported by the Belle Collaboration [35]. As a result, we expect that the yield of X2X_{2} in the γJ/ψγ+\gamma\,J/\psi\to\gamma\ell^{+}\ell^{-} final states (=e,μ)(\ell=e,\mu) should be at least about 3535, that is larger than the number of events observed by the Belle collaboration in Ref. [35].

Acknowledgements.
We would like to thank Alexey Nefediev for valuable discussions. This work is partly supported by the Chinese Academy of Sciences under Grant No. XDB34030000; by the National Natural Science Foundation of China (NSFC) under Grants No. 12125507, No. 11835015, and No. 12047503; and by the NSFC and the Deutsche Forschungsgemeinschaft (DFG) through the funds provided to the Sino-German Collaborative Research Center “Symmetries and the Emergence of Structure in QCD” (NSFC Grant No. 12070131001, DFG Project-ID 196253076 - TRR110).

Appendix A X(3872)X(3872) radiative decays into γψ(2S)\gamma\,\psi(2S) and γJ/ψ\gamma\,J/\psi channels

The X(3872)X(3872) radiative decays into the γψ(2S)\gamma\,\psi(2S) and γJ/ψ\gamma\,J/\psi channels have been evaluated in Ref. [46], adopting a molecular picture as the quark configuration for the X(3872)X(3872) state. The findings reported in Ref. [46] are in line with the experimental ratio RX(3872)R_{X(3872)} measured by the BESIII Collaboration [47]. In particular, it is stressed in Ref. [46] that those specific decays take place through hadron loops involving charmed mesons plus short-distance contributions in the form of a counterterm. For pure hadronic molecular states the hadron loops are the leading order contribution and play an important role in such processes. However, the charged conjugated diagrams in the loops are not considered in Ref. [46]; these contributions will lead to a factor of 2 for all the loop contributions but does not affect the ratio RX(3872)R_{X(3872)} which was the main concern in Ref. [46]. In addition, pαp^{\alpha} in Eq. (24) and pγp^{\gamma} in Eq. (28) in Ref. [46] should be changed to kαk^{\alpha} and (kp)γ(k-p)^{\gamma}, respectively, which has also been noticed in Ref. [30]. That is because the four-velocity of heavy mesons with respect to the magnetic vertices in Eqs. (14) and (16) are related to the charmed-meson momentum inside the loop, instead of the X(3872)X(3872) four-velocity. The updated expressions of Eqs.(24)-(29) in Ref. [46] for the individual contributions to the process Xσ(p)γλ(q)ψμ(pq)X_{\sigma}(p)\to\gamma_{\lambda}(q)\psi_{\mu}(p-q) are (we use the same notation as in Ref. [46])

Jμνλ(a)m(k)=\displaystyle J_{\mu\nu\lambda}^{(a)m}(k)= 23m(β+4mc)ϵνλαβkαqβ(2kpq)μ(kq)2m2,\displaystyle\,\frac{2}{3}m\left(\beta+\frac{4}{m_{c}}\right)\epsilon_{\nu\lambda\alpha\beta}k^{\alpha}q^{\beta}\frac{(2k-p-q)_{\mu}}{(k-q)^{2}-m^{2}},
Jμνλ(b)e(k)=\displaystyle J_{\mu\nu\lambda}^{(b)e}(k)=  4ϵμραβ(kp)α(kq)β(kq)2m2[(2kq)λgνρ(kq)νgλρkρgνλ],\displaystyle\,4\epsilon_{\mu\rho\alpha\beta}\frac{(k-p)^{\alpha}(k-q)^{\beta}}{(k-q)^{2}-m_{*}^{2}}\left[(2k-q)_{\lambda}g^{\rho}_{\nu}-(k-q)_{\nu}g^{\rho}_{\lambda}-k^{\rho}g_{\nu\lambda}\right],
Jμνλ(b)m(k)=\displaystyle J_{\mu\nu\lambda}^{(b)m}(k)= 43m(β4mc)ϵμραβ(kp)α(kq)β(kq)2m2[qνgλρqρgνλ],\displaystyle\,\frac{4}{3}m_{*}\left(\beta-\frac{4}{m_{c}}\right)\epsilon_{\mu\rho\alpha\beta}\frac{(k-p)^{\alpha}(k-q)^{\beta}}{(k-q)^{2}-m_{*}^{2}}\left[q_{\nu}g^{\rho}_{\lambda}-q^{\rho}g_{\nu\lambda}\right],
Jμνλ(c)e(k)=\displaystyle J_{\mu\nu\lambda}^{(c)e}(k)=  4ϵμναβ(kp+q)αkβ(2k2p+q)λ(kp+q)2m2,\displaystyle\,4\epsilon_{\mu\nu\alpha\beta}(k-p+q)^{\alpha}k^{\beta}\frac{(2k-2p+q)_{\lambda}}{(k-p+q)^{2}-m^{2}},
Jμνλ(d)m(k)=\displaystyle J_{\mu\nu\lambda}^{(d)m}(k)= 23m(β+4mc)[(2kp+q)μgβν(2kp+q)βgμν(2kp+q)νgβμ]ϵαλγδ(kp)γqδ(kp+q)2m2\displaystyle\,\frac{2}{3}m_{*}\left(\beta+\frac{4}{m_{c}}\right)\left[(2k-p+q)_{\mu}g_{\beta\nu}-(2k-p+q)_{\beta}g_{\mu\nu}-(2k-p+q)_{\nu}g_{\beta\mu}\right]\frac{\epsilon_{\alpha\lambda\gamma\delta}(k-p)^{\gamma}q^{\delta}}{(k-p+q)^{2}-m_{*}^{2}}
(gαβ+(kp+q)α(kp+q)βm2),\displaystyle\left(-g^{\alpha\beta}+\frac{(k-p+q)^{\alpha}(k-p+q)^{\beta}}{m_{*}^{2}}\right),
Jμνλ(e)e(k)=\displaystyle J_{\mu\nu\lambda}^{(e)e}(k)= 4ϵμνλαpα,\displaystyle-4\epsilon_{\mu\nu\lambda\alpha}p^{\alpha}, (42)

where mm and mm_{*} are the masses of DD and DD^{*} mesons, respectively, and the magnetic coupling parameter β\beta is the β\beta^{\prime} in Eq. (33).

Table 3: Decay widths X(3872)γψX(3872)\to\gamma\psi with ψ=J/ψ,ψ(2S)\psi=J/\psi,\psi(2S) and their ratio RX(3872)R_{X(3872)}. The second row displays the results for X(3872)γψX(3872)\to\gamma\psi with ψ=J/ψ,ψ(2S)\psi=J/\psi,~{}\psi(2S) calculated in Ref. [46], while the updated results are shown in the third row.
μ\mu ΓJ/ψ\Gamma^{\prime}_{J/\psi} [keV] Γψ(2S)\Gamma^{\prime}_{\psi(2S)} [keV] RX(3872)R_{X(3872)}
Ref. [46] mX(3872)m_{X(3872)} 23.5 (rχrg)2(r^{\prime}_{\chi}r_{g})^{2} 4.9 (rχrg)2(r^{\prime}_{\chi}r^{\prime}_{g})^{2} 0.21 (g2/g2)2(g_{2}^{\prime}/g_{2})^{2}
Updated mX(3872)m_{X(3872)} 211 (rχrg)2(r^{\prime}_{\chi}r_{g})^{2} 20.6 (rχrg)2(r^{\prime}_{\chi}r^{\prime}_{g})^{2} 0.10 (g2/g2)2(g_{2}^{\prime}/g_{2})^{2}

The updated numerical results for the partial decay widths of X(3872)γψ(2S)X(3872)\to\gamma\,\psi(2S) and γJ/ψ\gamma\,J/\psi are shown in Table 3, where we have kept the results from Ref. [46] for a comparison. As can be seen, they are much larger than the ones in Ref. [46]. As for the ratio RX(3872)R_{X(3872)}, the new result is about half of the previous one. Nevertheless, the conclusion in Ref. [46], that is the hadronic molecular picture of the X(3872)X(3872) is compatible with the measured ratio RX(3872)R_{X(3872)}, is not altered.

References