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Phenomenological studies on ˉB0[Kπ+]S/V[π+π]V/SKπ+π+π decay

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1. Yan, D.-C., Rui, Z., Yan, Y. et al. Study of four-body decays B(s)→ (ππ) (ππ) in the perturbative QCD approach[J]. European Physical Journal C, 2023, 83(10): 974. doi: 10.1140/epjc/s10052-023-12152-z
2. Liang, H.-Q., Yu, X.-Q. Study of the four-body decays BS0 →ππππ in the perturbative QCD approach[J]. Physical Review D, 2022, 105(9): 096018. doi: 10.1103/PhysRevD.105.096018
3. Yan, D.-C., Rui, Z., Xiao, Z.-J. et al. Study of B (s)0 →φφ → (K+K-) (K+K-) decays in the perturbative QCD approach[J]. Physical Review D, 2022, 105(9): 093001. doi: 10.1103/PhysRevD.105.093001
4. Giacosa, F., Okopińska, A., Shastry, V. A simple alternative to the relativistic Breit–Wigner distribution[J]. European Physical Journal A, 2021, 57(12): 336. doi: 10.1140/epja/s10050-021-00641-2
5. Li, Y., Yan, D.-C., Rui, Z. et al. Study of B(s)→ (ππ) (Kπ) decays in the perturbative QCD approach[J]. European Physical Journal C, 2021, 81(9): 806. doi: 10.1140/epjc/s10052-021-09608-5
6. Rui, Z., Li, Y., Li, H.-N. Four-body decays B(s) → (Kπ)S/P(Kπ)S/P in the perturbative QCD approach[J]. Journal of High Energy Physics, 2021, 2021(5): 82. doi: 10.1007/JHEP05(2021)082

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Jing-Juan Qi, Zhen-Yang Wang, Zhu-Feng Zhang and Xin-Heng Guo. Phenomenological studies on the ˉB0[Kπ+]S/V[π+π]V/SKπ+π+π decay[J]. Chinese Physics C. doi: 10.1088/1674-1137/abeb06
Jing-Juan Qi, Zhen-Yang Wang, Zhu-Feng Zhang and Xin-Heng Guo. Phenomenological studies on the ˉB0[Kπ+]S/V[π+π]V/SKπ+π+π decay[J]. Chinese Physics C.  doi: 10.1088/1674-1137/abeb06 shu
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Phenomenological studies on ˉB0[Kπ+]S/V[π+π]V/SKπ+π+π decay

    Corresponding author: Zhen-Yang Wang, wangzhenyang@nbu.edu.cn
    Corresponding author: Xin-Heng Guo, xhguo@bnu.edu.cn
  • 1. Junior College, Zhejiang Wanli University, Zhejiang 315101, China
  • 2. Physics Department, Ningbo University, Zhejiang 315211, China
  • 3. College of Nuclear Science and Technology, Beijing Normal University, Beijing 100875, China

Abstract: Within the quasi-two-body decay model, we study the localized CP violation and branching fraction of the four-body decay ˉB0[Kπ+]S/V[π+π]V/SKπ+ππ+ when the Kπ+ and ππ+ pair invariant masses are 0.35<mKπ+<2.04GeV and 0<mππ+<1.06GeV, with the pairs being dominated by the ˉK0(700)0, ˉK(892)0, ˉK(1410)0, ˉK0(1430) and ˉK(1680)0, and f0(500), ρ0(770), ω(782) and f0(980) resonances, respectively. When dealing with the dynamical functions of these resonances, f0(500), ρ0(770), f0(980) and ˉK0(1430) are modeled with the Bugg model, Gounaris-Sakurai function, Flatté formalism and LASS lineshape, respectively, while the others are described by the relativistic Breit-Wigner function. Adopting the end point divergence parameters ρA[0,0.5] and ϕA[0,2π], our predicted results are ACP(ˉB0Kπ+π+π)[0.365,0.447] and B(ˉB0Kπ+π+π)[6.11,185.32]×108, based on the hypothetical qˉq structures for the scalar mesons in the QCD factorization approach. Meanwhile, we calculate the CP violating asymmetries and branching fractions of the two-body decays ˉB0SV(VS) and all the individual four-body decays ˉB0SV(VS)Kπ+ππ+, respectively. Our theoretical results for the two-body decays ˉB0ˉK(892)0f0(980), ˉB0ˉK0(1430)0ω(782), ˉB0ˉK(892)0f0(980), ˉB0ˉK0(1430)0ρ, and ˉB0ˉK0(1430)0ω are consistent with the available experimental data, with the remaining predictions await testing in future high precision experiments.

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    I.   INTRODUCTION
    • Four-body decays of heavy mesons are hard to investigate because of their complicated phase spaces and relatively small branching fractions. This leads to much less research on four-body decays than on two- and three- body decays [1-11]. We have discussed localized CP violation and branching fractions of the four-body decays ˉB0Kπ+ππ+ in Ref. [12], focusing on the ππ and Kπ invariant masses near the masses of the f0(500) and K0(700)o mesons. The more resonance states there are, the more abundant physical mechanisms are available to us. We now further expand our research to include more contributions from different resonances in our study of CP violation and branching fractions in ˉB0 four-body decays. Specifically, the invariant mass of the Kπ+ pair lies in the range 0.35<mKπ+<2.04GeV, which is dominated by the ˉK0(700)0, ˉK(892)0, ˉK(1410)0, ˉK0(1430) and ˉK(1680)0 resonances, and that of the ππ+ pair is in the range 0<mππ+<1.06GeV, which includes the f0(500), ρ0(770), ω(782) and f0(980) resonances. Meanwhile, studying the multibody decays can provide rich information about their intermediate resonances, especially about the compositions of scalar mesons, which are still unclear. The basic structure of the scalar meson is not well established because it is very difficult to identify experimentally [13, 14]. In the Bf0(980)K channel, B decay into a scalar meson was first observed and updated in Ref. [15], and confirmed by BaBar [16]. In Refs. [17, 18], there are two typical scenarios for scalar mesons based on their mass spectra and strong or electromagnetic decays. In Scenario 1 (S1), the light scalar mesons (such as f0(500), ˉK0(700)0, f0(980) and a0(980) mesons) are regarded as the lowest-lying qˉq states, and some others (their masses near 1.5 GeV, including a0(1450), K0(1430), f0(1370) and f0(1500) [19-21]) are treated as the first corresponding excited states. In Scenario 2 (S2), the heavier nonet mesons are regarded as the ground states of qˉq, while the lighter nonet mesons are not regular mesons and might be four-quark states. To further improve our understanding of the QCD mechanism and quark confinement, it is necessary for us to study the structural composition of the scalar mesons and related content.

      In 2019, the LHCb collaboration studied the B0ρ(770)0K(892)0 decay within a quasi-two-body decay mode, B0(π+π)(K+π) [22]. In our work, we adopt this mechanism to study the four-body decay ˉB0Kπ+ππ+, i.e. ˉB0ˉκρKπ+ππ+, ˉB0ˉκωKπ+ππ+, ˉB0ˉK(892)0σKπ+ππ+, ˉB0ˉK(892)0f0(980)\rightarrowKπ+ππ+, ˉB0ˉB0ˉK(1410)0σ\rightarrowKπ+ππ+, ˉB0ˉK(1410)0f0(980)Kπ+ππ+, ˉB0ˉK0(1430)0ρKπ+ππ+,ˉB0ˉK0(1430)0ωKπ+ππ+, ˉB0ˉK(1680)0σKπ+ππ+ and ˉB0ˉK(1680)0f0(980)Kπ+ππ+, where the scalar mesons will be treated using S1 as mentioned above. We can then calculate the localized CP violations and branching fractions of the four-body decay ˉB0Kπ+ππ+. We can also calculate the CP violations and branching fractions of the two-body decays ˉB0SV(VS) and all the individual four-body decays ˉB0SV(VS)Kπ+ππ+. In fact, with the further development of the LHCb and Belle II experiments, more and more decay modes involving one or two scalar states in the B and D meson decays are expected to be measured with high precision in the future.

      The remainder of this paper is organized as follows. Our theoretical framework is presented in Sect. II. In Sect. III, we give our numerical results. We summarize our work in Sect. IV. Appendix A collects the explicit formulas for all the four-body decay amplitudes. The dynamical functions for the corresponding resonances are summarized in Appendix B. We also consider the f0(500)f0(980) mixing in Appendix C. Related theoretical parameters are listed in Appendix D.

    II.   THEORETICAL FRAMEWORK

      A.   B decay in the QCD factorization approach

    • In the framework of the QCD factorization approach [4, 23], the effective Hamiltonian matrix elements can be written as

      M1M2|Heff|B=p=u,cλ(D)pM1M2|TpA+TpB|B,

      (1)

      where Heff is the effective weak Hamiltonian, λ(D)p=VpbVpD, Vpb and VpD are the CKM matrix elements, and TpA and TpB describe the contributions from non-annihilation and annihilation amplitudes, respectively; they can be expressed in terms of api and bpi.

      Generally, api includes the contributions from naive factorization, vertex correction, penguin amplitude and spectator scattering, and can be expressed as follows [4]:

      api(M1M2)=(ci+ci±1Nc)Ni(M2)+ci±1NcCFαs4π×[Vi(M2)+4π2NcHi(M1M2)]+Ppi(M2),

      (2)

      where ci are the Wilson coefficients, Ni(M2) is the leading-order coefficient, and Vi(M2), Hi(M1M2) and Ppi(M1M2) are one-loop vertex corrections, hard spectator interactions with a hard gluon exchange between the emitted meson and the spectator quark of the B meson, and penguin contractions, respectively. CF=(N2c1)/2Nc, with Nc=3 [4].

      The weak annihilation contributions can be expressed in terms of bi and bi,EW, which are:

      b1=CFN2cc1Ai1,b2=CFN2cc2Ai1,bp3=CFN2c[c3Ai1+c5(Ai3+Af3)+Ncc6Af3],bp4=CFN2c[c4Ai1+c6Ai2],bp3,EW=CFN2c[c9Ai1+C7(Ai3+Af3)+Ncc8Af3],bp4,EW=CFN2c[c10Ai1+c8Ai2],

      (3)

      where the subscripts 1, 2, 3 of Ai,fn(n=1,2,3) stand for the annihilation amplitudes induced from (VA)(VA), (VA)(V+A), and (SP)(S+P) operators, respectively, and the superscripts i and f refer to gluon emission from the initial- and final-state quarks, respectively. The explicit expressions for Ai,fn can be found in Ref. [24].

      In the expressions for the spectator and annihilation corrections, there are end-point divergences X=10dx/(1x), which can be parametrized as [17]

      XH,A=(1+ρH,AeiϕH,A)lnmBΛh,

      (4)

      with Λh being a typical scale of order 500 MeV, ρA,H an unknown real parameter and ϕA,H the free strong phase in the range [0,2π].

    • B.   Four-body decay amplitudes

    • For the four-body decay ˉB0Kπ+ππ+, we consider the two-body cascade decay mode ˉB0[Kπ+]S/V[ππ+]V/SKπ+ππ+. Within the QCDF framework in Ref. [4], we can deduce the two-body weak decay amplitudes of ˉB0[Kπ+]S/V[ππ+]V/S, which are:

      M(ˉB0ˉK00iρ)=iGFp=u,cλ(s)p{[δpuα2(ˉK00iρ)+32αp3,EW(ˉK00iρ)]fρmρερpBFˉB0ˉK00i1(m2ρ)+[αp4(ρˉK00i)12αp4,EW(ρˉK00i)]ˉfˉK00imρερpBAˉB0ρ0(m2ˉK00i)+[12bp3(ρˉK00i)14bp3,EW(ρˉK00i)]fˉB0fρˉfˉK00i},

      (5)

      M(ˉB0ˉK00iω)=iGFp=u,cλ(s)p{[δpuα2(ˉK00iω)+2αp3(ˉK00iω)+12αp3,EW(ˉK00iω)]fωmωεωpBFˉB0ˉK00i1(m2ω)+[12αp4,EW(ωˉK00i)αp4(ωˉK00i)]ˉfˉK00imωεωpBAˉB0ω0(m2ˉK00i)+[14bp3,EW(ωˉK00i)12bp3(ωˉK00i)]fˉB0fρˉfˉK00i},

      (6)

      with ˉK00i=ˉK0(700)0,ˉK0(1430)0 corresponding to i=1,2, respectively, and

      M(ˉB0ˉK0if0j)=iGFp=u,cλ(s)p{[δpuα2(ˉK0if0j)+2αp3(ˉK0if0j)+12αp3,EW(ˉK0if0j)]×ˉffn0jmˉK0iεˉK0ipBAˉB0ˉK0i0(m2f0j)+[2αp3(ˉK0if0j)+2αp4(ˉK0if0j)12αp3,EW(ˉK0if0j)12αp4,EW(ˉK0if0j)]ˉffs0jmˉK0iεˉK0ipBAˉB0ˉK0i0(m2f0j)+[12αp4,EW(f0jˉK0i)αp4(f0jˉK0i)]fˉK0imˉK0iεˉK0ipBFˉB0f0j1(m2ˉK0i)+[12bp3(ˉK0if0j)122bp3,EW(ˉK0if0j)]fˉB0fˉK0iˉfsf0j+[12bp3(f0jˉK0i)14bp3,EW(f0jˉK0i)]fˉB0fˉK0iˉfnf0j},

      (7)

      with ˉK0i=ˉK(892)0,ˉK(1410)0,ˉK(1680)0 corresponding to i=1,2,3, respectively, and f0j=f0(500), f0(980) when j=1,2, respectively. In Eqs. (5)-(7), FˉB0S1(m2V) and AˉB0V0(m2S) are the form factors for ˉB0 to scalar and vector meson transitions, respectively, fV, ˉfS, and fˉB0 are the decay constants of the vector, scalar, and ˉB0 mesons, respectively, ˉfsf0j and ˉfnf0j are the decay constants of the f0j mesons coming from the up and strange quark components, respectively.

      In the framework of the two two-body decays, the four-body decay can be factorized into three pieces as follows:

      M(ˉB0[Kπ+]S[ππ+]VKπ+ππ+)=SV|Heff|ˉB0Kπ+|HSKπ+|Sππ+|HVππ+|VsSsV,

      (8)

      and

      M(ˉB0[Kπ+]V[ππ+]SKπ+ππ+)=VS|Heff|ˉB0Kπ+|HVKπ+|Vππ+|HSππ+|SsVsS,

      (9)

      where Heff is the effective weak Hamiltonian, M1M2|Hs|V=gVM1M2(pM1pM2)ϵV and M1M2|Hs|S=gSM1M2, gVM1M2 and gSM1M2 are the strong coupling constants of the corresponding vector and scalar mesons decays, and sS/V are the reciprocals of the dynamical functions TS/V for the corresponding resonances. The specific kinds and expressions of TS/V are given in the fifth column of Table 1 and Appendix C, respectively.

      ResonanceMass/MeVWidth/MeVJPModel
      σ475±75550±1500+BUGG
      ρ775.26±0.25149.1±0.81GS
      ω782.65±0.128.49±0.081RBW
      f0(980)990±2065±450+FLATTˊE
      ˉκ824±30478±500+RBW
      ˉK(892)0895.5±0.2047.3±0.51RBW
      ˉK(1410)01421±9236±181RBW
      ˉK0(1430)01425±50270±800+LASS
      ˉK(1680)01718±18322±1101RBW

      Table 1.  Masses, widths and decay models of the intermediate resonances [25].

      When considering the contributions from the ˉB0[Kπ+]S[ππ+]V\rightarrowKπ+ππ+ and ˉB0[Kπ+]V[ππ+]SKπ+ππ+ channels as listed in Eqs. (8) and (9), the total decay amplitude of the ˉB0Kπ+π+π decay can be written as (As for the relative strong phase δ between these two interference amplitudes, we set δ=0 as in Refs. [5, 30, 31])

      M=M(ˉB0[Kπ+]S[ππ+]VKπ+ππ+)+M(ˉB0[Kπ+]V[ππ+]SKπ+ππ+).

      (10)
    • C.   Kinematics of the four-body decay and localized CP violation

    • One can use the five variables sππ, sKπ, ϕ, θπ and θK to describe the kinematics of the four-body decay ˉB0K(p1)π+(p2)π(p3)π+(p4) [26-29], where sππ and sKπ are the invariant mass squared of the ππ system and Kπ system, respectively, ϕ is the angle between the ππ and Kπ planes, and θπ (or θK) is the angle of the π+ (or K) in the ππ (or Kπ) center-of-mass system with respect to the ππ (or Kπ) line of flight in the ˉB0 rest frame. Their specific physical ranges can be found in detail in Refs. [12, 26-29].

      For presentation and calculation, it is more convenient to replace the individual momenta p1, p2, p3, p4 with the following kinematic variables:

      P=p1+p2,Q=p1p2,L=p3+p4,N=p3p4.

      (11)

      Using the above formula, we can get:

      P2=sKπ,Q2=2(p2K+p2π)sKπ,L2=sππ,PL=12(m2ˉB0sKπsππ),PN=Xcosθπ,LQ=σ(sKπ)XcosθK,

      (12)

      where

      σ(sKπ)=1(m2K+m2π)/sKπ.

      (13)

      With the decay amplitude, one can get the decay rate of the four-body decay [32],

      d5Γ=14(4π)6m3ˉB0σ(sππ)X(sππ,sKπ)spins|M|2dΩ,

      (14)

      where σ(sππ)=14m2π/sππ, and Ω represents the phase space with dΩ=dsππdsKπdcosθπdcosθKdϕ.

      The differential CP asymmetry parameter and the localized integrated CP asymmetry take the following forms:

      ACP=|M|2|ˉM|2|M|2+|ˉM|2,

      (15)

      and

      AΩCP=dΩ(|M|2|ˉM|2)dΩ(|M|2+|ˉM|2),

      (16)

      respectively.

    III.   NUMERICAL RESULTS
    • When dealing with the scalar mesons, we adopt Scenario 1 in Ref. [17], in which those with masses below or near 1 GeV (σ, f0(980), κ) and near 1.5 GeV (K0(1430)) are suggested as the lowest-lying qˉq states and the first excited state, respectively. For the decay constants of the f0j mesons, we consider the f0(500)f0(980) mixing with the mixing angle |φm|=170 (see Appendix A for details). For the decay constants and Gegenbauer moments of the ˉK(1410)0 and the ˉK(1680)0 mesons, we assume they have the same central values as that of ˉK(892)0 and assign their uncertainties to be ±0.1 [33]. With the QCDF approach, we have obtained the amplitudes of the two-body decays ˉB0SV and ˉB0VS, which are listed in Eqs. (5)-(7). Generally, the end-point divergence parameter ρA is constrained in the range [0,1] and ϕA is treated as a free strong phase. The experimental data for B two-body decays can provide important information to restrict the ranges of these two parameters. In fact, compared with the BPV/VP/PP decays, there is much less experimental data for the BVS/PS and BSV/SP decays, so the values of ρA and ϕA for these decays are not well-determined. Therefore, we adopt ρA,H<0.5 and 0, as in Refs. [17, 24]. With more experimental data, both of these could be defined in small regions in the future.

      Substituting Eqs. (5)-(7) into Eq. (15), we obtain the CP -violating asymmetries of the two-body decays \bar{B}^0\rightarrow SV and \bar{B}^0\rightarrow VS with the parameters given in Table 1 and Appendix F, which are listed in Table 2. From Table 2, one can see our theoretical results for the CP asymmetries of \bar{B}^0\rightarrow \bar{K}^*(892)^0 f_0(980) and \bar{B}^0\rightarrow \bar{K}^*_0(1430)^0 \omega are consistent with the data from the BaBar collaboration. However, the predicted central values of the CP asymmetries of \bar{B}^0\rightarrow \bar{K}^*_0(1430)^0 \rho and \bar{B}^0\rightarrow \bar{K}^*_0(1430)^0\omega are larger than those in Ref. [18]. The main difference between our work and Ref. [18] is the structure of the \bar{K}^*_0(1430)^0 meson, which is explored in S1 in our work and S2 in Ref. [18]. Furthermore, we predict the CP asymmetries of some other decay channels. We find the signs of the CP asymmetries are negative in \bar{B}^0\rightarrow \bar{\kappa}\rho , \bar{B}^0\rightarrow \bar{K}^*(1410)^0 f_0(980) and \bar{B}^0\rightarrow \bar{K}^*(1680)^0 f_0(980) decays, with the first of these being one order of magnitude larger than the other two. For the positive values of the CP asymmetries in our work, those for the \bar{B}^0\rightarrow\bar{\kappa}\omega and \bar{B}^0\rightarrow\bar{K}^*(892)^0\sigma decays are also one order of magnitude larger than the others. We have also calculated the branching fractions of the two-body decays \bar{B}^0\rightarrow SV and \bar{B}^0\rightarrow VS which are listed in Table 3. Our results are consistent with the available experimental data for the \bar{B}^0\rightarrow \bar{K}^*(892)^0f_0(980) , \bar{B}^0\rightarrow \bar{K}^*_0(1430)^0\rho and \bar{B}^0\rightarrow\bar{K}^*_0(1430)^0\omega decays. Meanwhile, we find the magnitudes of the branching fractions are of order 10^{-5} for \bar{B}^0\rightarrow\bar{K}^*(892)^0f_0(980) , \bar{B}^0\rightarrow\bar{K}^*(1410)^0\sigma and \bar{B}^0\rightarrow \bar{K}^*(1410)^0f_0(980) , but of order 10^{-6} for \bar{B}^0\rightarrow\bar{\kappa}\rho , \bar{B}^0\rightarrow\bar{\kappa}\omega , \bar{B}^0\rightarrow\bar{K}^*_0(1430)^0\rho and \bar{B}^0\rightarrow\bar{K}^*_0(1430)^0\omega . We note that the predicted branching fraction of \bar{B}^0\rightarrow\bar{K}^*(892)^0 \sigma is the smallest, of the order of 10^{-7} .

      Decay modeBaBarPDG [25][18]This work
      \bar{\kappa}\rho-10.66\pm3.14
      \bar{\kappa}\omega17.43\pm6.53
      \bar{K}^*(892)^0\sigma25.57\pm10.42
      \bar{K}^*(892)^0f_0(980)7\pm10\pm27\pm109.31\pm1.04
      \bar{K}^*(1410)^0\sigma0.43\pm0.13
      \bar{K}^*(1410)^0f_0(980)-2.01\pm0.19
      \bar{K}^*_0(1430)^0\rho0.54^{+0.45+0.02+3.76}_{-0.46-0.02-1.80}6.03\pm0.97
      \bar{K}^*_0(1430)^0\omega-7\pm9\pm20.03^{+0.37+0.01+0.29}_{-0.35-0.01-3.00}-9.53\pm3.88
      \bar{K}^*(1680)^0\sigma3.03\pm0.77
      \bar{K}^*(1680)^0f_0(980)-2.76\pm0.20

      Table 2.  Direct CP violations (in units of 10^{-2} ) of the two-body decays \bar{B}^0\rightarrow [K^-\pi^+]_{S/V}[\pi^+\pi^-]_{V/S} . The experimental branching fractions are taken from Ref. [34]. The theoretical errors come from the uncertainties of the form factors, decay constants, Gegenbauer moments and divergence parameters.

      For different intermediate resonance states, we use different models to deal with their dynamical functions. These are listed in detail in Table 1 and Appendix D; \sigma , \rho^0(770) , f_0(980) and \bar{K}^*_0(1430) are modeled with the Bugg model [37], Gounaris-Sakurai function [38], Flatté formalism [39] and LASS lineshape [40-42], respectively, while the others are described by the relativistic Breit-Wigner function [43]. Inserting Eqs. (A1)-(A3) into Eqs. (16) and (14), we can directly obtain the CP asymmetries and branching fractions of all the individual four-body decay channels \bar{B}^0\rightarrow [K^-\pi^+]_{S/V}[\pi^+\pi^-]_{V/S} \rightarrow K^-\pi^+\pi^+\pi^- by integrating the phase space of Eq. (14), both of which are summarized in Table 4. From this table, we can conclude that the ranges of these CP asymmetries and branching fractions are about [-7.03, 24.33]\times10^{-2} and [0.11, 27.3]\times 10^{-6} , respectively. Considering the contributions from all the four-body decays listed in Table 4, we can obtain the localized integrated CP asymmetries and branching fractions of the \bar{B}^0\rightarrow K^-\pi^+\pi^+\pi^- decay by integrating the phase space. Our results are in the ranges \mathcal{A_{CP}}(\bar{B}^0\rightarrow K^-\pi^+\pi^+\pi^-) = [-0.365, 0.447] and \mathcal{B}(\bar{B}^0\rightarrow K^-\pi^+\pi^+\pi^-) = [6.11,185.32]\times10^{-8} when the invariant masses of K^-\pi^+ and \pi^-\pi^+ are in the ranges 0.35<m_{K^-\pi^+}<2.04 \, \mathrm{GeV} and 0<m_{\pi^-\pi^+}<1.06\; \mathrm{GeV} , where the K\pi channel is dominated by the \kappa , \bar{K}^*(892)^0 , \bar{K}^*(1410)^0 , \bar{K}^*_0(1430) and \bar{K}^*(1680)^0 resonances, the \pi\pi channel is dominated by the \sigma , \rho^0(770) , \omega(782) and f_0(980) resonances, and the ranges of \rho_A and \phi_A are taken as [0,0.5] and [0,2\pi] , respectively. Both of them are expected to be tested experimentally in the near future.

      Decay modeBaBarBelleLHCb [24]PDG [25]QCDF [18]pQCD [35, 36]This work
      \bar{\kappa}\rho1.35\pm0.47
      \bar{\kappa}\omega3.87\pm1.65
      \bar{K}^*(892)^0\sigma0.11\pm0.04
      \bar{K}^*(892)^0f_0(980)11.4\pm1.4<4.47.8^{+4.2}_{-3.6}9.1^{+1.0+1.0+5.3}_{-0.4-0.5-0.7}11.2\sim13.79.48\pm2.88
      \bar{K}^*(1410)^0\sigma25.41\pm9.13
      \bar{K}^*(1410)^0f_0(980)14.39\pm4.22
      \bar{K}^*_0(1430)^0\rho27\pm4\pm2\pm310.0^{+2.4+0.5+12.1}_{-2.0-0.4-3.1}27.0\pm6.04.1^{+1.1+0.2+2.6}_{-1.0-0.2-0.1}4.8^{+1.1+1.0+0.3}_{-0.0-1.0-0.3}8.13\pm2.03
      \bar{K}^*_0(1430)^0\omega6.4^{+1.4+0.3+4.0}_{-1.2-0.2-0.9}16.0\pm3.49.3^{+2.7+0.3+3.9}_{-2.2-0.3-1.3}9.3^{+2.1+3.6+1.2}_{-2.0-2.9-1.0}5.02\pm1.06
      \bar{K}^*(1680)^0\sigma27.64\pm8.59
      \bar{K}^*(1680)^0f_0(980)21.76\pm8.33

      Table 3.  Branching fractions (in units of 10^{-6} ) of the two-body decays \bar{B}^0\rightarrow [K^-\pi^+]_{S/V}[\pi^+\pi^-]_{V/S} . We have used \mathcal{B}(f_0(980)\rightarrow \pi^+\pi^-) = 0.5 to obtain the experimental branching fractions for f_0(980)V . The theoretical errors come from the uncertainties of the form factors, decay constants, Gegenbauer moments and divergence parameters.

      Decay modeCP asymmetriesBranching fractions
      \bar{\kappa}\rho(\rightarrow K^-\pi^+\pi^+\pi^-)-10.03\pm5.011.46\pm0.51
      \bar{\kappa}\omega (\rightarrow K^-\pi^+\pi^+\pi^-)18.34\pm5.174.10\pm0.63
      \bar{K}^*(892)^0\sigma (\rightarrow K^-\pi^+\pi^+\pi^-)24.33\pm9.010.11\pm0.05
      \bar{K}^*(892)^0f_0(980) (\rightarrow K^-\pi^+\pi^+\pi^-)-3.85\pm1.019.22\pm4.15
      \bar{K}^*(1410)^0\sigma (\rightarrow K^-\pi^+\pi^+\pi^-)0.41\pm0.5321.18\pm6.32
      \bar{K}^*(1410)^0f_0(980)(\rightarrow K^-\pi^+\pi^+\pi^-)-2.38\pm0.4916.01\pm4.04
      \bar{K}^*_0(1430)^0\rho (\rightarrow K^-\pi^+\pi^+\pi^-)-7.03\pm2.472.03\pm0.41
      \bar{K}^*_0(1430)^0\omega (\rightarrow K^-\pi^+\pi^+\pi^-)10.39\pm3.422.55\pm0.87
      \bar{K}^*(1680)^0\sigma (\rightarrow K^-\pi^+\pi^+\pi^-)8.05\pm3.0127.30\pm7.05
      \bar{K}^*(1680)^0f_0(980)(\rightarrow K^-\pi^+\pi^+\pi^-)-5.03\pm0.6219.89\pm4.01

      Table 4.  Direct CP violations (in units of 10^{-2} ) and branching fractions (in units of 10^{-6} ) of the four-body decays \bar{B}^0\rightarrow [K^-\pi^+]_{S/V}[\pi^+\pi^-]_{V/S} \rightarrow K^-\pi^+\pi^+\pi^- . The theoretical errors come from the uncertainties of the form factors, decay constants, Gegenbauer moments and divergence parameters.

    IV.   SUMMARY
    • In this work, we have revisited the four-body decay \bar{B}^0\rightarrow K^-\pi^+\pi^-\pi^+ in the framework of the two two-body decays. We have considered more contributions from different resonances. We have also updated the model when dealing with the dynamical function for the \rho resonance. The most important thing is that we have added the relevant calculations to further test the rationality of the two-quark model for scalar mesons in the two-body decay of the \bar{B}^0 meson. In this analysis, we first calculated the direct CP -violating asymmetries and branching fractions of the two-body decays \bar{B}^0\rightarrow [K^-\pi^+]_{S/V}[\pi^+\pi^-]_{V/S} within the QCDF approach, as listed in Table 2 and Table 3, respectively. From these two tables, we can see that our theoretical results are consistent with the available experimental data for the CP asymmetries of the \bar{B}^0\rightarrow \bar{K}^*(892)^0 f_0(980) and \bar{B}^0\rightarrow \bar{K}^*_0(1430)^0 \omega decays and the branching fractions of the \bar{B}^0\rightarrow \bar{K}^*(892)^0f_0(980) , \bar{B}^0\rightarrow\bar{K}^*_0(1430)^0\rho and \bar{B}^0\rightarrow\bar{K}^*_0(1430)^0\omega decays. Because of different structures of the \bar{K}^*_0(1430)^0 meson, our predicted central values for the CP asymmetries are larger than those given in Ref. [18] for the \bar{B}^0\rightarrow \bar{K}^*_0(1430)^0 \rho and \bar{B}^0\rightarrow \bar{K}^*_0(1430)^0\omega decays. It is found that the signs of the CP asymmetries are negative for the \bar{B}^0\rightarrow \bar{\kappa}\rho , \bar{B}^0\rightarrow \bar{K}^*(1410)^0 f_0(980) and \bar{B}^0\rightarrow \bar{K}^*(1680)^0 f_0(980) decays and are positive for other decays. The magnitudes of the branching fractions for the two-body decays considered, \bar{B}^0\rightarrow [K^-\pi^+]_{S/V}[\pi^+\pi^-]_{V/S} , are of orders 10^{-7}\sim10^{-5} . Then, under the assumption of the quasi-two-body decay mode, we regard the \bar{B}^0\rightarrow K^-\pi^+\pi^-\pi^+ decay as happening through \bar{B}^0\rightarrow [K^-\pi^+]_{S/V}[\pi^+\pi^-]_{V/S}\rightarrow K^-\pi^+\pi^-\pi^+ and calculate the direct CP asymmetries and branching fractions of all the individual four-body decay channels \bar{B}^0\rightarrow [K^-\pi^+]_{S/V}[\pi^+\pi^-]_{V/S} \rightarrow K^-\pi^+\pi^+\pi^- . Their ranges are about [-7.03, 24.33]\times10^{-2} and [0.11, 27.3]\times10^{-6} , respectively. Finally, considering the contributions from all these decay channels, we obtain the localized integrated CP asymmetries and the branching fraction of \bar{B}^0\rightarrow K^-\pi^+\pi^-\pi^+ when 0.35<m_{K^-\pi^+}<2.04 \, \mathrm{GeV} and 0<m_{\pi^-\pi^+}<1.06\; \mathrm{GeV} , which are dominated by the \bar{K}^*_0(700)^0 , \bar{K}^*(892)^0 , \bar{K}^*(1410)^0 , \bar{K}^*_0(1430) and \bar{K}^*(1680)^0 , and f_0(500) , \rho^0(770) , \omega(782) and f_0(980) resonances, respectively. The predicted results are \mathcal{A_{CP}}(\bar{B}^0\rightarrow K^-\pi^+\pi^+\pi^-) = [-0.365,0.447] and \mathcal{B}(\bar{B}^0\rightarrow K^-\pi^+\pi^+\pi^-) = [6.11,185.32]\times10^{-8} . In our analysis, the errors come from the uncertainties of the form factors, decay constants, Gegenbauer moments and divergence parameters. These theoretical predictions await testing in future high-precision experiments. If our predictions are confirmed, the viewpoint that scalars have a q\bar{q} composition may be supported. However, to exclude other possible structures, more investigations will be needed due to uncertainties from both theory and experiments.

    APPENDIX A: FOUR-BODY DECAY AMPLITUDES
    • Considering the related weak and strong decays, one can obtain the four-body decay amplitudes of the \bar{B}^0\rightarrow [K^-\pi^+]_{S/V}[\pi^+\pi^-]_{V/S} \rightarrow K^-\pi^+\pi^+\pi^- channels as follows:

      \tag{A1} \begin{aligned}[b] \mathcal{M}(\bar{B}^0\rightarrow \bar{K}^{*0}_{0i}\rho\rightarrow K^-\pi^+\pi^+\pi^- ) =& \frac{{\rm i}G_Fg_{\bar{K}^{*0}_{0i}K\pi}g_{\rho\pi\pi}}{S_{\bar{K}^{*0}_{0i}}S_\rho }\bigg[(P\cdot N)+(L\cdot N)+\frac{1}{m_{\rho}^2}(L\cdot P+L^2)(L\cdot N)\bigg]\\ &\times\sum_{p = u,c}\lambda_p^{(s)}\bigg\{\bigg[\delta_{pu}\alpha_2(\bar{K}^{*0}_{0i}\rho) +\frac{3}{2}\alpha_{3,EW}^p(\bar{K}^{*0}_{0i}\rho)\bigg] f_\rho m_{\bar{B}^0}p_cF_1^{\bar{B}^0 \bar{K}^{*0}_{0i}}(m_{\rho}^2)\\& +\bigg[\alpha_4^p(\rho\bar{K}^{*0}_{0i})-\frac{1}{2}\alpha_{4,EW}^p(\rho\bar{K}^{*0}_{0i})\bigg] \bar{f}_{\bar{K}^{*0}_{0i}}m_{\bar{B}^0}p_cA_0^{\bar{B}^0\rho}(m_{\bar{K}^{*0}_{0i}}^2)\\& +\bigg[\frac{1}{2}b_3^p(\rho\bar{K}^{*0}_{0i})-\frac{1}{4}b_{3,EW}^p(\rho\bar{K}^{*0}_{0i})\bigg] \frac{f_{\bar{B}^0}f_\rho \bar{f}_{\bar{K}^{*0}_{0i}}m_{\bar{B}^0}p_c}{m_\rho}\bigg\},\end{aligned}

      \tag{A2} \begin{aligned}[b] \mathcal{M}(\bar{B}^0\rightarrow \bar{K}^{*0}_{0i}\omega\rightarrow K^-\pi^+\pi^+\pi^- ) =& \frac{{\rm i}G_Fg_{\bar{K}^{*0}_{0i}K\pi}g_{\omega\pi\pi}}{S_{\bar{K}^{*0}_{0i}}S_\omega}\bigg[(P\cdot N)+(L\cdot N)+\frac{1}{m_{\omega}^2}(L\cdot P+L^2)(L\cdot N)\bigg]\\& \times\sum_{p = u,c}\lambda_p^{(s)}\bigg\{\bigg[\delta_{pu}\alpha_2(\bar{K}^{*0}_{0i}\omega)+2\alpha_3^p(\bar{K}^{*0}_{0i}\omega) +\frac{1}{2}\alpha_{3,EW}^p(\bar{K}^{*0}_{0i}\omega)\bigg]\\& \times f_\omega m_{\bar{B}^0}p_cF_1^{\bar{B}^0 \bar{K}^{*0}_{0i}}(m_{\omega}^2) +\bigg[\frac{1}{2}\alpha_{4,EW}^p(\omega\bar{K}^{*0}_{0i})-\alpha_4^p(\omega\bar{K}^{*0}_{0i})\bigg]\bar{f}_{\bar{K}^{*0}_{0i}}m_{\bar{B}^0}p_c\\& \times A_0^{\bar{B}^0\omega}(m_{\bar{K}^{*0}_{0i}}^2) +\bigg[\frac{1}{4}b_{3,EW}^p(\omega\bar{K}^{*0}_{0i})-\frac{1}{2}b_3^p(\omega\bar{K}^{*0}_{0i})\bigg] \frac{f_{\bar{B}^0}f_\rho \bar{f}_{\bar{K}^{*0}_{0i}}m_{\bar{B}^0}p_c}{m_\omega}\bigg\},\end{aligned}

      and

      \tag{A3} \begin{aligned}[b] \mathcal{M}(\bar{B}^0\rightarrow \bar{K}^{*0}_if_{0j}\rightarrow K^-\pi^+\pi^+\pi^-) = &-\frac{{\rm i}G_Fg_{\bar{K}^{*0}_iK\pi}g_{f_{0j}\pi\pi}}{S_{\bar{K}^{*0}_i}S_{f_{0j}}} \bigg[-(P\cdot Q)-(L\cdot Q)+\frac{1}{{m_{\bar{K}^{*0}_i}}^2}(P^2+P\cdot L)(P\cdot Q)]\bigg]\\&\times \sum_{p = u,c}\lambda_p^{(s)}\bigg\{\bigg[\delta_{pu}\alpha_2(\bar{K}^{*0}_if_{0j})+2\alpha_3^p(\bar{K}^{*0}_if_{0j}) +\frac{1}{2}\alpha_{3,EW}^p(\bar{K}^{*0}_if_{0j})\bigg]\\& \times \bar{f}_{f_{0j}^n} m_{\bar{B}^0}p_cA_0^{\bar{B}^0 \bar{K}^{*0}_i}(m_{f_{0j}}^2)+\bigg[\sqrt{2}\alpha_3^p(\bar{K}^{*0}_if_{0j})+\sqrt{2}\alpha_4^p(\bar{K}^{*0}_if_{0j})\\ &-\frac{1}{\sqrt{2}}\alpha_{3,EW}^p(\bar{K}^{*0}_i\sigma)-\frac{1}{\sqrt{2}}\alpha_{4,EW}^p(\bar{K}^{*0}_i\sigma)\bigg]\bar{f}_{\sigma^s} m_{\bar{B}^0}p_cA_0^{\bar{B}^0\bar{K}^{*0}_i}(m_{f_{0j}}^2)\\& +\bigg[\frac{1}{2}\alpha_{4,EW}^p(f_{0j}\bar{K}^{*0}_i)-\alpha_4^p(f_{0j}\bar{K}^{*0}_i)\bigg]f_{\bar{K}^{*0}_i}m_{\bar{B}^0}p_c F_1^{\bar{B}^0f_{0j}}(m_{\bar{K}^{*0}_i}^2)\\& +\bigg[\frac{1}{\sqrt{2}}b_3^p(\bar{K}^{*0}_if_{0j})-\frac{1}{2\sqrt{2}}b_{3,EW}^p(\bar{K}^{*0}_if_{0j})\bigg] \frac{f_{\bar{B}^0}f_{\bar{K}^{*0}_i}\bar{f}_{f_{0j}}^s m_{\bar{B}^0}p_c}{m_{\bar{K}^{*0}_i}}\\& +\bigg[\frac{1}{2}b_3^p(f_{0j}\bar{K}^{*0}_i)-\frac{1}{4}b_{3,EW}^p(f_{0j}\bar{K}^{*0}_i)\bigg]\frac{f_{\bar{B}^0}f_{\bar{K}^{*0}_i}\bar{f}_{f_{0j}}^nm_{\bar{B}^0}p_c}{m_{\bar{K}^{*0}_i}}\bigg\}.\end{aligned}

    APPENDIX B: DYNAMICAL FUNCTIONS FOR THE CORRESPONDING RESONANCES

      B.1.   BUGG MODEL

    • We adopt the Bugg model [37] to parameterize the \sigma resonance:

      \tag{B1} T_R(m_{\pi\pi}) = 1/[M^2-s_{\pi\pi}-g_1^2(s_{\pi\pi})\frac{s_{\pi\pi}-s_A}{M^2-s_A}z(s_{\pi\pi})-{\rm i}M\Gamma_{\mathrm{tot}}(s_{\pi\pi})],

      where z(s_{\pi\pi}) = j_1(s_{\pi\pi})-j_1(M^2) with j_1(s_{\pi\pi}) = \dfrac{1}{\pi}\bigg[2+ \rho_1 \times \ln\bigg(\dfrac{1-\rho_1}{1+\rho_1}\bigg)\bigg], \Gamma_{\mathrm{tot}}(s_{\pi\pi}) = \displaystyle\sum\limits _{i = 1}^4 \Gamma_i(s_{\pi\pi}) with:

      \tag{B2} \begin{aligned}[b] M\Gamma_1(s_{\pi\pi}) =& g_1^2(s_{\pi\pi})\frac{s_{\pi\pi}-s_A}{M^2-s_A}\rho_1(s_{\pi\pi}),\\ M\Gamma_2(s_{\pi\pi}) =& 0.6g_1^2(s_{\pi\pi})(s_{\pi\pi}/M^2)\mathrm{exp}(-\alpha|s_{\pi\pi}-4m_K^2|)\rho_2(s_{\pi\pi}),\\ M\Gamma_3(s_{\pi\pi}) =& 0.2g_1^2(s_{\pi\pi})(s_{\pi\pi}/M^2)\mathrm{exp}(-\alpha|s_{\pi\pi}-4m_\eta^2|)\rho_3(s_{\pi\pi}),\\ M\Gamma_4(s_{\pi\pi}) =& Mg_4\rho_{4\pi}(s_{\pi\pi})/\rho_{4\pi}(M^2), \end{aligned}

      and:

      \tag{B3} \begin{aligned}[b] g_1^2(s_{\pi\pi}) =& M(b_1+b_2s)\mathrm{exp}[-(s_{\pi\pi}-M^2)/A],\\ \rho_{4\pi}(s_{\pi\pi}) =& 1.0/[1+\mathrm{exp}(7.082-2.845s_{\pi\pi})].\end{aligned}

      In the above two formulas, the relevant parameters are specifically fixed as M = 0.953\;\mathrm{GeV} , g_{4\pi} = 0.011\; \mathrm{GeV} , s_A = 0.14m_\pi^2 , A = 2.426\; \mathrm{GeV}^2 , b_1 = 1.302 \;\mathrm{GeV}^2 , and b^2 = 0.340 in Ref. [37]. The phase-space factor parameters \rho_1 , \rho_2 and \rho_3 have the following forms:

      \tag{B4} \rho_i(s_{\pi\pi}) = \sqrt{1-4\frac{m_i^2}{s_{\pi\pi}}},

      with m_1 = m_\pi , m_2 = m_K and m_3 = m_\eta .

    • B.2.   GOUNARIS-SAKURAI FUNCTION

    • In the framework of the Gounaris-Sakurai model, which includes an analytic dispersive term, the propagator of the \rho^0(770) resonance can be expressed as [38]

      \tag{B5} T_R(m_{\pi\pi}) = \frac{1+D\Gamma_0/m_0}{m_0^2-s_{\pi\pi}+f(m_{\pi\pi})-{\rm i}m_0\Gamma(m_{\pi\pi})},

      where m_0 and \Gamma_0 are the the mass and decay width of the \rho^0(770) meson, respectively, and f(m_{\pi\pi}) is given by

      \tag{B6} f(m_{\pi\pi}) = \Gamma_0\frac{m_0^2}{q_0^3}\left[q^2\left[h(m_{\pi\pi})-h(m_0)\right]+(m_0^2-m_{\pi\pi}^2)q^2_0\frac{\mathrm{d}h}{\mathrm{d}m_{\pi\pi}^2}\bigg|_{m_0}\right],

      where q_0 is the value of q = |\vec{q}| when the mass of the \pi\pi pair satisfies m_{\pi\pi} = m_{\rho^0(770)} , with:

      \tag{B7} h(m_{\pi\pi}) = \frac{2}{\pi}\frac{q}{m_{\pi\pi}}\log\bigg(\frac{m_{\pi\pi}+2q}{2m_\pi}\bigg),

      \tag{B8} \frac{\mathrm{\rm d}h}{\mathrm{\rm d}m_{\pi\pi}^2}\bigg|_{m_0} = h(m_0)\left[(8q_0^2)^{-1}-(2m_0^2)^{-1}\right]+(2\pi m_0^2)^{-1}.

      In Eq. (B5), the concrete form of the constant parameter D is

      \tag{B9} D = \frac{3}{\pi}\frac{m_\pi^2}{q_0^2}\log\bigg(\frac{m_0+2q_0}{2m_\pi}\bigg)+\frac{m_0}{2\pi q_0}-\frac{m_\pi^2 m_0}{\pi q_0^3}.

    • B.3.   FLATTÉ MODEL

    • In Refs. [39, 44], when studying the f_0(980) resonance, we can use the Flatté model to deal with it, which has the following form:

      \tag{B10} T_R(m_{\pi\pi}) = \frac{1}{m_R^2-s_{\pi\pi}-{\rm i}m_R(g_{\pi\pi}\rho_{\pi\pi}+g_{KK}F_{KK}^2\rho_{KK})},

      where m_R is the mass of the f_0(980) meson, and g_{\pi\pi} (or g_{KK} )is the coupling constant of the f_0(980) resonance decay to a \pi^+\pi^- (or K^+K^- ) pair. Within the Lorentz-invariant phase space, the phase-space \rho factors are given by:

      \tag{B11} \begin{aligned}[b] \rho_{\pi\pi} =& \frac{2}{3}\sqrt{1-\frac{4m_{\pi^\pm}^2}{s_{\pi\pi}}}+\frac{1}{3}\sqrt{1-\frac{4m_{\pi^0}^2}{s_{\pi\pi}}},\\ \rho_{KK} =& \frac{1}{2}\sqrt{1-\frac{4m_{K^\pm}^2}{s_{\pi\pi}}}+\frac{1}{2}\sqrt{1-\frac{4m_{K^0}^2}{s_{\pi\pi}}}.\end{aligned}

      Compared to the normal Flatté function, a form factor F_{KK} = \mathrm{exp}(-\alpha k^2) in Eq. (B10) is introduced above the KK threshold and serves to reduce the \rho_{KK} factor as s_{\pi\pi} increases, where k is the momentum of each kaon in the KK rest frame, and \alpha = (2.0\pm0.25)\;\mathrm{GeV}^{-2} [44]. This parametrization slightly decreases the f_0(980) width above the KK threshold. The parameter \alpha is fixed to be 2.0 \;\mathrm{GeV}^{-2} , which is not very sensitive to the fit.

    • B.4.   LASS MODEL

    • Generally, the LASS model can describe the low mass of the K^+\pi^- resonance. It has been used widely in theories and experiments [40-42], and has been written as

      \tag{B12} \begin{aligned}[b] T(m_{K\pi}) =& \frac{m_{K\pi}}{|\vec{q}|\cot\delta_B-{\rm i}|\vec{q}|}\\&+{\rm e}^{2{\rm i}\delta_B}\dfrac{m_0\Gamma_0\frac{m_0}{|q_0|}}{m_0^2-s_{K\pi}^2-{\rm i}m_0\Gamma_0\dfrac{|\vec{q}|}{m_{K\pi}}\dfrac{m_0}{|q_0|}},\end{aligned}

      where m_0 and \Gamma_0 are the mass and width of the K_0^*(1430) state, respectively, |\vec{q_0}| is the value of |\vec{q}| when m_{K\pi} = m_{K_0^*(1430)} , |\vec{q}| is the momentum vector of the resonance decay product measured in the resonance rest frame, and \cot\delta_B has two terms, \cot\delta_B = \dfrac{1}{a|\vec{q}|}+\dfrac{1}{2}r|\vec{q}| , with a = (3.1\pm1.0)\,\mathrm{GeV}^{-1} and r = (7.0\pm2.3)\,\mathrm{GeV}^{-1} being the scattering length and effective range [42], respectively.

    • B.5.   RELATIVISTIC BREIT-WIGNER

    • We adopt the relativistic Breit-Wigner function to describe the distributions of the \bar{K}^*_0(700)^0 , \bar{K}^*(892)^0 , \bar{K}^*(1410)^0 and \bar{K}^*(1680)^0 resonances [43],

      \tag{B13} T_R(m_{K\pi}) = \frac{1}{M_R^2-s_{K\pi}-{\rm i}M_R\Gamma_{K\pi}} \quad\quad\quad(R = \bar{\kappa},\bar{K}^*),

      with

      \tag{B14} \Gamma_{K\pi} = \Gamma_0^R\bigg(\frac{p_{K\pi}}{p_R}\bigg)^{2J+1}\bigg(\frac{M_R}{m_{K\pi}}\bigg)F^2_R,

      where M_R and \Gamma_0^R are the mass and width, respectively, m_{K\pi} is the invariant mass of the K\pi pair, p_{K\pi}(p_R) is the momentum of either daughter in the K\pi (or R) rest frame, and F_R is the Blatt-Weisskopf centrifugal barrier factor [45], which is listed in Table B1 and depends on a single parameter R_r , which can be taken as R_r = 1.5\;\mathrm{GeV}^{-1} [46].

      Spin F_R
      0 1
      1 \dfrac{\sqrt{1+(R_r p_R)^2} }{\sqrt{1+(R_r p_{AB})^2} }

      Table B1.  Summary of the Blatt-Weisskopf penetration form factors.

    APPENDIX C: f_0(500)-f_0(980) MIXING
    • Analogous to the \eta-\eta' mixing, using a 2 \times 2 rotation matrix, the f_0(500)-f_0(980) mixing can be parameterized as

      \tag{C1} \left( \begin{array}{cc} f_0(980)\\ f_0(500)\\ \end{array} \right) = \left( \begin{array}{cc} \cos\varphi_m& \sin\varphi_m \\ -\sin\varphi_m& \cos\varphi_m \end{array} \right ) \left( \begin{array}{cc} f_s\\ f_q\\ \end{array} \right ),

      where f_s\equiv s\bar{s} and f_q\equiv \dfrac{u\bar{u}+d\bar{d}}{\sqrt{2}} , and \varphi_m is the mixing angle, which has been summarized in Refs. [18, 47]. However, based on the measurement by the LHCb collaboration, the range of \varphi_m is |\varphi_m|<31^0 [48]. In our calculation, we adopt |\varphi_m| = 17^0 [18].

    APPENDIX D: THEORETICAL INPUT PARAMETERS
    • The predictions obtained in the QCDF approach depend on many input parameters. The values of the Wolfenstein parameters are taken from Ref. [49]: \bar{\rho} = 0.117\pm0.021 , \bar{\eta} = 0.353\pm0.013 .

      For the masses used in the \bar{B}^0 decays, we use the following values, except for those listed in Table 1 (in \mathrm{GeV} ) [49]:

      \tag{D1} \begin{aligned}[b]& m_u = m_d = 0.0035,\quad m_s = 0.119, \quad m_b = 4.2,\\& m_{\pi^\pm} = 0.14,\quad m_{K^-} = 0.494,\quad m_{\bar{B}^0} = 5.28,\end{aligned}

      while for the widths we shall use (in units of \mathrm{GeV} ) [49]:

      \tag{D2} \begin{aligned}[b]& \Gamma_{\rho\rightarrow\pi\pi} = 0.149,\quad\Gamma_{\omega\rightarrow\pi\pi} = 0.00013,\quad\Gamma_{\sigma\rightarrow\pi\pi} = 0.3,\\& \Gamma_{f_0(980)\rightarrow \pi\pi} = 0.33,\quad \Gamma_{\bar{K}^*(892)^0\rightarrow K\pi} = 0.0487,\\&\Gamma_{\bar{K}^*(1410)^0\rightarrow K\pi} = 0.015,\quad \Gamma_{\bar{K}^*(1680)^0\rightarrow K\pi} = 0.10,\\& \Gamma_{K^*_0(1430)\rightarrow K\pi} = 0.251.\end{aligned}

      The Wilson coefficients used in our calculations are taken from Refs. [50-53]:

      \tag{D3}\begin{aligned}[b]&c_1 = -0.3125, \quad c_2 = 1.1502, \quad c_3 = 0.0174,\\& c_4 = -0.0373,\quad c_5 = 0.0104,\quad c_6 = -0.0459,\\& c_7 = -1.050\times10^{-5},\quad c_8 = 3.839\times10^{-4}, \\& c_9 = -0.0101,\quad c_{10} = 1.959\times10^{-3}. \end{aligned}

      The following relevant decay constants (in \mathrm{GeV} ) are used [17, 54, 55]:

      \tag{D4} \begin{aligned}[b]& f_{\pi^\pm} = 0.131,\quad f_{\bar{B}^0} = 0.21\pm0.02, \quad f_{K^-} = 0.156\pm0.007, \\& \bar{f}^s_{\sigma} = -0.21\pm0.093,\quad \bar{f}_{\sigma}^u = 0.4829\pm0.076,\\& \bar{f}_{\bar{\kappa}} = 0.34\pm0.02,\quad f_{\rho} = 0.216\pm0.003,\\& f_{\rho}^\perp = 0.165\pm0.009,\quad f_{\omega} = 0.187\pm0.005,\\& f_{\omega}^\perp = 0.151\pm0.009,\quad f_{\bar{K}^*(892)^0} = 0.22\pm0.005,\\&f_{\bar{K}^*(892)^0}^\perp = 0.185\pm0.010,\quad \bar{f}_{\bar{K}^*_0(1430)^0} = -0.300\pm0.030. \\& \bar{f}^s_{f_0(980)} = 0.325\pm0.016,\quad \bar{f}_{f_0(980)}^u = 0.1013\pm0.005.\end{aligned}

      As for the form factors, we use [17, 33, 55, 56]:

      \tag{D5} \begin{aligned}[b]& F_0^{\bar{B}^0\rightarrow K}(0) = 0.35\pm0.04,\quad F_0^{\bar{B}^0\rightarrow \sigma}(0) = 0.45\pm0.15,\quad F^{\bar{B}^0\rightarrow\kappa}(0) = 0.3\pm0.1,\\ &A_0^{\bar{B}^0\rightarrow \bar{K}^*(892)^0}(0) = 0.374\pm0.034, \quad F_0^{\bar{B}^0\rightarrow \pi}(0) = 0.25\pm0.03, \quad F_0^{\bar{B}^0\rightarrow \bar{K}^*_0(1430)^0}(0) = 0.21,\\& A_0^{\bar{B}^0\rightarrow \bar{K}^*(1410)^0}(0) = 0.26\pm0.0275, \quad A_0^{\bar{B}^0\rightarrow \bar{K}^*(1680)^0}(0) = 0.2154\pm0.0281 \quad A_0^{\bar{B}^0\rightarrow \rho}(0) = 0.303\pm0.029,\end{aligned}

      The values of the Gegenbauer moments at \mu = 1\; \mathrm{GeV} are taken from [17, 54, 55]:

      \tag{D6}\begin{aligned}[b]& \alpha_1^\rho = 0,\quad \alpha_2^\rho = 0.15\pm0.07, \quad \alpha_{1,\perp}^\rho = 0,\quad \alpha_{2,\perp}^\rho = 0.14\pm0.06, \quad \alpha_1^\omega = 0,\quad \alpha_2^\omega = 0.15\pm0.07, \quad \alpha_{1,\perp}^\omega = 0,\quad \alpha_{2,\perp}^\omega = 0.14\pm0.06, \\& \alpha_1^{\bar{K}^*(892)^0} = 0.03\pm0.02,\quad \alpha_{1,\perp}^{\bar{K}^*(892)^0} = 0.04\pm0.03,\quad \alpha_2^{\bar{K}^*(892)^0} = 0.11\pm0.09,\quad \alpha_{2,\perp}^{\bar{K}^*(892)^0} = 0.10\pm0.08,\\& B_{1,\sigma}^u = -0.42\pm0.074,\quad B_{3,\sigma}^u = -0.58\pm0.23,\quad B_{1,\sigma}^s = -0.35\pm0.061,\quad B_{3,\sigma}^s = -0.43\pm0.18,\\& B_{1,f_0(980)}^u = -0.92\pm0.08,\quad B_{3,f_0(980)}^u = -0.74\pm0.064,\quad B_{1,f_0(980)}^s = -1\pm0.05,\quad B_{3,f_0(980)}^s = -0.8\pm0.04,\\& B_{1,\bar{\kappa}} = -0.92\pm0.11,\quad B_{3,\bar{\kappa}} = 0.15\pm0.09,\quad B_{1,\bar{K}^*_0(1430)^0} = 0.58\pm0.07,\quad B_{3,\bar{K}^*_0(1430)^0} = -1.20\pm0.08.\end{aligned}

Reference (56)

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