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Eur. Phys. J. C (2016) 76:454 DOI 10.1140/epjc/s10052-016-4306-3

Regular Article - Theoretical Physics

D-wave charmonia ηc2(11D2), ψ2(13D2), and ψ3(13D3) in Bc decays

Qiang Lia, Tianhong Wangb, Yue Jiangc, Han Yuand, Guo-Li Wange

Department of Physics, Harbin Institute of Technology, Harbin 150001, People’s Republic of China

Received: 11 July 2016 / Accepted: 1 August 2016 / Published online: 12 August 2016 © The Author(s) 2016. This article is published with open access at Springerlink.com

Abstract We study the semileptonic and nonleptonic de- cays of Bc meson to D-wave charmonia, namely, ηc2(11D2), ψ2(13D2), and ψ3(13D3). In our calculations, the instan- taneous Bethe–Salpeter method is applied to obtain the hadronic matrix elements. This method includes relativis- tic corrections which are important especially for the higher orbital excited states. For the semileptonic decay channels with electron as the final lepton, we get the branching ratios B[Bc → ηc2eν̄e] = 5.9−0.8+1.0 × 10−4, B[Bc → ψ2eν̄e] = 1.5−0.2+0.3 × 10−4, and B[Bc → ψ3eν̄e] = 3.5−0.6+0.8 × 10−4. The transition form factors, forward–backward asymmetries, and lepton spectra in these processes are also presented. For the nonleptonic decay channels, those with ρ as the lighter meson have the largest branching ratios, B[Bc → ηc2ρ] = 8.1−1.0+1.0 × 10−4, B[Bc → ψ2ρ] = 9.6−1.0+1.0 × 10−5, and B[Bc→ψ3ρ] = 4.1−0.7+0.8 × 10−4.

1 Introduction

In 2013, the Belle Collaboration reported the evidence of a new resonance X (3823) in the B decay channel B±→X (→ χc1γ )K± with a statistical significance of 3.8σ [1]. And very recently, the BESIII Collaboration verified its existence with a statistical significance of 6.2σ [2]. Both groups got a similar mass and ratio of the partial decay widths for this particle. On one hand, this state has a mass of 3821.7 ± 1.3(stat) ± 0.7(syst) MeV/c2, which is very near the mass value of the 13D2 charmonium predicted by potential models [3,4]; on the other hand, the electromagnetic decay channels χc1γ and χc2γ are observed while the later one is suppressed, which means the 11D2 and 13D3 charmonia cases are excluded.

a e-mail: lrhit@protonmail.com b e-mail: thwang@hit.edu.cn c e-mail: jiangure@hit.edu.cn d e-mail: hanyuan@hit.edu.cn e e-mail: gl_wang@hit.edu.cn

To confirm the above experimental results and compare with other theoretical predictions, studying the properties of D-wave charmonia in a different approach is relevant. In this work we study the ψ2(13D2) and its two partners ηc2(11D2) and ψ3(13D3) in the weak decays of the Bc meson which has attracted lots of attention since its discovery by the CDF Collaboration at Fermilab [5]. Unlike the charmonia and bot- tomonia, which are hidden-flavor bound states, the Bc meson, which consists of a bottom quark and a charm quark, is open- flavor. Besides that, it is the ground state, which means it cannot decay through strong or electromagnetic interaction. So the Bc meson provides an ideal platform to study the weak interaction.

The semileptonic and nonleptonic transitions of the Bc meson into charmonium states are important processes. Experimentally, only those with J/ψ or ψ(2S) as the final charmonium have been detected [6]. As the LHC accumu- lates more and more data, the weak decay processes of the Bc meson to charmonia with other quantum numbers will have more possibilities to be detected. That is to say, this is an alter- native way to study the charmonia, especially those have not yet been discovered, such as ηc2(11D2) and ψ3(13D3). Theo- retically, the semileptonic and nonleptonic transitions of the Bc meson into S-wave charmonium states are studied widely by several phenomenological models, such as the relativis- tic constituent quark model [7–12], the non-relativistic con- stituent quark model [13], the technique of hard and soft factorization [14] and QCD factorization [15], QCD sum rules [16], Light-cone sum rules [17], the perturbative QCD approach [18–21], and NRQCD [22,23]. There are also some theoretical models to study the processes of Bc decay to a P- wave charmonium [8,24–28], while we lack the information of Bc decay to a D-wave charmonium.

Here we will use the Bethe–Salpeter (BS) method to inves- tigate the exclusive semileptonic and nonleptonic decays of the Bc meson to the D-wave charmonium. This method has been used to study processes with P-wave charmo- nium [24,28]. As is well known, the BS equation [29] is

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454 Page 2 of 13 Eur. Phys. J. C (2016) 76 :454

a relativistic two-body bound state equation. To solve BS equation of D-wave mesons and get the corresponding wave function and mass spectra, we use the instantaneous approx- imation, that is, we solve the Salpeter equations [30] which has been widely used for bound states decay problems [31– 34].

This paper is organized as follows. In Sect. 2 we present the general formalism for semileptonic and nonleptonic decay widths of Bc into D-wave charmonia. In Sect. 3 we give the analytic expressions of the corresponding form fac- tors given by the BS method. In Sect. 4, the numerical results are obtained and we compare our results with others’, also the theoretical uncertainties and lepton spectra are presented in this section. Section 5 is a short summary of this work. Some bulky analytical expressions are presented in the appendix.

2 Formalisms of semileptonic and nonleptonic decays

In this section we will derive the general formalism for the calculations of both semileptonic and nonleptonic decay widths of Bc meson.

2.1 The semileptonic decay

The semileptonic decays of the Bc meson into D-wave char- monia are three-body decay processes. We consider the neu- trinos as massless fermions. The differential form of the three-body decay width can be written as

d = 1 (2π)3

1

32M3 |M|2dm212dm223, (1)

where M is the mass of Bc; m12 is the invariant mass of final cc̄meson and neutrino which is defined asm212 = (PF+pν)2; m23 is the invariant mass of final neutrino and charged lepton, which is defined as m223 = (pν + p )2. Here we have used PF , pν , and p to denote the 4-momentum of final cc̄ meson, neutrino, and charged lepton, respectively.M is the invariant amplitude of this process. In the above equation we have summed over the polarizations of final states.

2.1.1 Form factors

The Feynman diagram involved in the semileptonic decays of Bc meson in the tree level is showed in Fig. 1. The invariant amplitude M can be written directly as

M = GF√ 2 Vcb〈cc̄|hμ|Bc〉ū (p ) μvν(pν), (2)

where GF is the Fermi constant; Vcb is the CKM matrix element for the b→c transition; 〈cc̄|hμ|Bc〉 is the hadronic matrix element; hμ = c̄ μb is the weak charged current and μ = γ μ(1 − γ 5). The general form of the hadronic matrix

B−c , P

b cp1

m1

p1

m1

2S+1DJ , PF

c̄ c̄

p2

m2

p2

m2

−

ν̄

Fig. 1 Feynman diagram of the semileptonic decay of Bc into D-wave charmonia. P and PF are the momenta of initial and final mesons, respectively. S, D, and J are quantum numbers of spin, orbital angu- lar momentum and total angular momentum for the final cc̄ system, respectively

element 〈cc̄|hμ|Bc〉 depends on the total angular momentum J of the final meson. For ηc2, J = 2, the transition matrix can be written as

〈cc̄|hμ|Bc〉 = eαβ Pα(s1Pβ Pμ + s2Pβ PμF + s3gβμ + is4 μβPPF ), (3)

where gβμ is the Minkowski metric tensor. We have used the definition μνPPF ≡ μναβ PαPβF ; μναβ is the totally anti- symmetric tensor; eαβ is the polarization tensor of the char- monium with J = 2; s1, s2, s3, and s4 are the form factors for the 1D2 state; for 3D2 state the relation between 〈cc̄|hμ|Bc〉 and form factors ti (i = 1, 2, 3, 4)has the same form with 1D2 just si replaced with ti . For the J = 3 meson, the hadronic matrix element can be described by the form factors hi :

〈cc̄|hμ|Bc〉 = eαβγ PαPβ(h1Pγ Pμ + h2Pγ PμF + h3gγμ + ih4 μγ PPF ), (4)

where eαβγ is the polarization tensor for the meson with J = 3. The expressions of these form factors are given in the next section.

The squared transition matrix element with the summed polarizations of final states (see Eq. (1)) has the form

|M|2 = G 2 F

2 |Vcb|2LμνHμν. (5)

In the above equation Lμν is the leptonic tensor

Lμν = ∑

s ,sν

[ū (p ) μvν(pν)][ū (p ) νvν(pν)]†

= 8(pμ pνν + pμν pν − p · pνgμν − i μνp pν ), (6) and Hμν is the hadronic tensor, which can be written as

Hμν = N1PμPν + N2(PμPF ν + Pν PFμ) + N4PFμPFν + N5gμν + iN6 μνPPF , (7)

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Eur. Phys. J. C (2016) 76 :454 Page 3 of 13 454

where Ni (i = 1, 2, 4, 5, 6) is described by form factors s j , t j or h j ( j = 1, 2, 3, 4) (see Appendix A). By using Eqs. (6) and (7), we can write LμνHμν as follows:

LμνHμν = 8N1(2P · p P · pν − M2 pν · p ) + 16N2(P · p PF · pν + PF · p P · pν − pν · p P ·PF ) + 8N4(2PF · p PF · pν − M2F pν · p ) − 16N5 pν · p + 16N6(PF · p P · pν −P · p PF · pν), (8)

where MF stands for the mass of final charmonium meson.

2.1.2 Angular distribution and lepton spe

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