Top-quark rare decays with flavor violation

  • In the present study, we investigated the decays of the top quark: tcγ, tcg, tcZ, and tch. They are extremely rare processes in the standard model (SM). As the U(1) extension of the minimal supersymmetric standard model (MSSM), the U(1)X SSM features new superfields such as the right-handed neutrinos and three Higgs singlets. We analyzed the effects of different sensitive parameters on the results and made reasonable theoretical predictions, thereby providing a useful reference for future experimental development. Considering the constraint set by the updated experimental data, the numerical results show that the branching ratios of the four processes, i.e., tcγ,cg,cZ,ch, can reach the same order of magnitude as their experimental upper limits. Among them, tanβ has the most evident effect on these processes and is the main parameter; gX, gYX, μ, M2, λH, M2U23, and M2Q23 are also important parameters for the processes, and have effects on the numerical results.
  • Studies on nuclear fission are of considerable research interest [16]. As one of the key and sensitive physical parameters, fission barriers of nuclei are frequently used in nuclear physics [712], reactor physics [13] and nuclear astrophysics [14, 15]. In the synthesis of super-heavy nuclei (SHN) through fusion reactions, the prediction of the evaporation-residue cross section for SHN strongly depends on the fission barrier height of the compound nuclei adopted in the calculations [1620]. An 1-MeV shift of the barrier height may change the calculated cross section of 3n or 4n reactions by 2−3 orders of magnitude [21, 22]. Considering the complexity of a typical fission process, in which not only large-scale collective participation of nucleons is witnessed but also superdeformed shapes of nuclei are encountered, accurate description of the corresponding fission barrier is of great interest but at the same time remains challenging.

    The fission barriers of nuclei can be described with some nuclear mass models, such as macroscopic-microscopic models [2325] and microscopic models based on the Skyrme energy density functionals [2628] or covariant density functionals [2931], in which the model parameters are usually determined by the nuclear properties at the ground state. For unmeasured SHN, the uncertainty of the barrier heights predicted using these different models reaches a few MeV [22, 24]. Considering the strong influence of the barrier height on the prediction of cross section, as mentioned above, it becomes necessary to improve the model accuracy for describing the fission barriers of unstable nuclei.

    Inspired by the Skyrme energy-density functional, the Weizsäcker-Skyrme (WS4) mass model was proposed [32], with which the known masses can be reproduced with an rms error of 0.3 MeV [33] and the known α-decay energies of SHN can be reproduced with deviations smaller than 0.5 MeV [3436]. Therefore, it would be interesting to apply the WS4 model for describing the fission barrier. In this work, we attempt to systematically calculate the fission barrier height based on the WS4 model, considering the shell correction at the ground state and that at the saddle point.

    In the macroscopic-microscopic model, the fission barrier height of a nucleus at zero temperature is expressed as the difference between the energy of the nucleus at saddle point Esad and that at its ground state Egs,

    Bf=EsadEgs=(EmacsadEmacgs)+(UsadUgs)+ΔB.

    (1)

    Here, Emacsad and Emacgs denote the macroscopic energy at the saddle point and that at the ground state, respectively. Usad and Ugs denote the corresponding shell corrections. ΔB denotes the residual correction. With the macroscopic fission barrier height Bmacf=EmacsadEmac0 and the macroscopic deformation energy Bdef=EmacgsEmac0, the fission barrier height can be re-written as

    Bf=BmacfUgs+(UsadBdef)+ΔB.

    (2)

    For spherical nuclei, the barrier height can be estimated as B(0)f=BmacfUgs if neglecting the saddle point shell correction and the residual correction.

    Following Cohen-Swiatecki's formula [1], the macroscopic fission barrier height is expressed as

    Bmacf={0.38(3/4x)Es:1/3<x2/30.88(1x)3Es:2/3<x1

    (3)

    with the ratio x=Ec2Es. Ec=acZ2/A1/3 denotes the Coulomb energy and Es=asA2/3(1κI2) denotes the surface energy with isospin asymmetry I=(NZ)/A. The coefficients ac=0.7092 MeV, as=17.4090 MeV and κ=1.5189 are taken from the WS4 model [32]. Together with the shell corrections Ugs, Usad and the macroscopic deformation energy Bdef also from the WS4 model predictions, the fission barrier heights for all bound heavy nuclei can be calculated as follows:

    BWS4f=BmacfUgs+UsadBdef,

    (4)

    neglecting the residual correction ΔB. The influence of ΔB will be discussed later.

    In this work, the saddle point of a nucleus is determined from the surface of the shell correction U(β2,β4) based on the WS4 calculations in which the Strutinsky shell correction is obtained from single-particle levels of an axially deformed Woods-Saxon potential. As two examples, we show in Fig. 1 the contour plot of the shell correction surface for nuclei 208Pb and 238U. Here, other deformations such as β3 and β6 are neglected in the calculations. The contour plot reveals that the shell correction Usad at the saddle point is approximately 2.2 MeV for 208Pb and 1.0 MeV for 238U. In our calculations, we introduced a truncation for the macroscopic deformation energy, i.e. BdefBmacf, and we neglected the influence of Usad for nuclei with Usad<0.

    Figure 1

    Figure 1.  (color online) Contour plot of the shell corrections for 208Pb and 238U. The dashed curves denote the possible fission paths. The crosses denote the positions of the saddle points.

    In Fig. 2(a), we show the discrepancies between the empirical fission barrier heights Bempf [3] and the model predictions for 71 nuclei with Z82. For actinides, we take the mean value of the inner and the outer barrier height as the value of Bempf in the comparisons. Evidently, with the saddle point shell correction Usad and the macroscopic deformation energy Bdef taken into account, the root-mean-square (rms) deviation with respect to the fission barrier heights is significantly reduced, from 2.410 MeV to 0.873 MeV. We note that, for both spherical and deformed nuclei, the fission barrier heights are generally better described by BWS4f. For doubly-magic nucleus 208Pb, the calculated B(0)f=25.1 MeV, which is smaller than the empirical barrier height by 2.3 MeV. Considering Usad=2.2 MeV for 208Pb, we obtain BWS4f=27.3 MeV, which is very close to the empirical value. For deformed nucleus 238U, the calculated B(0)f=9.2 MeV, which is higher than the empirical barrier by 2.9 MeV. With the macroscopic deformation energy of Bdef=3.4 MeV and Usad=1.0 MeV, we obtain BWS4f=6.8 MeV for 238U, which is comparable to the empirical value. From Fig. 2(a), it is evident that the values of BempfB(0)f can be categorized into two groups: approximately 2 MeV for nuclei with A210 and approximately 3 MeV for A>225. To understand the underlying physics, the macroscopic deformation energies Bdef and the saddle point shell corrections Usad for these nuclei are shown in Fig. 2(b). Evidently, for nuclei with A210, the values of Usad are obviously higher than Bdef, whereas for A>225, Bdef>Usad in general. The values of UsadBdef, therefore, can be categorized into two groups.

    Figure 2

    Figure 2.  (color online) (a) Discrepancies between the empirical fission barrier heights Bempf [3] and the model predictions. The open circles denote the results obtained using B(0)f=BmacfUgs and the solid circles denote the results obtained from Eq. (4). (b) Macroscopic deformation energies Bdef (solid squares) and shell corrections at the saddle points Usad (open squares) for these nuclei.

    To further analyze the influence of the saddle point shell correction, we introduce δU=(UsadUgs)/Ugs to describe the relative value of the shell correction. In Fig. 3, we show the values of BempfBWS4f as a function of δU2. Evidently, the difference between the empirical barrier heights and the model predictions systematically decreases with increasing δU2. Comparing Eq. (2) with Eq. (4), one notes that the residual correction ΔB is neglected in BWS4f. To better describe the fission barriers, we empirically write the residual correction (in MeV) as

    Figure 3

    Figure 3.  (color online) Deviation BempfBWS4f as a function of the ratio square of the shell correction. The error bars denote the difference between the inner barrier height and the corresponding outer barrier height for actinides [3]. The solid curve denotes the results obtained using Eq. (5).

    ΔB2.8+19exp(δU2/0.8).

    (5)

    In Fig. 4, we compare the results obtained using BWS4f+ΔB and those obtained using FRLDM [25]. The rms deviation is further reduced to 0.481 MeV, considering the residual correction given by Eq. (5). We note that the trend of the results obtained using FRLDM is similar to that obtained using WS4, for nuclei with A210 and A>240. We also note that the mean values of the fission barrier heights obtained using the three macroscopic-microscopic approaches, i.e. Bf=(BFRLDMf+BWS4f+BWS4+ΔBf)/3, also agree well with the empirical values, with an rms error of only 0.585 MeV. In the calculations of Bf we set a relatively larger weight for the WS4 model, considering its smaller rms error for describing known masses and empirical Bf. We would like to emphasize that the difference between the inner barrier heights and the outer ones for actinides (Z90) could result in some uncertainties in analyzing the model accuracy. Compared with BWS4f, the rms deviation is reduced from 1.01 to 0.77 MeV for the 45 inner barriers of actinides with ΔB being considered, and the corresponding value is reduced from 0.92 to 0.48 MeV for the outer barriers.

    Figure 4

    Figure 4.  (color online) The same as Fig. 2(a), but with the results of the finite-range liquid-drop (FRLDM) model [25] and BWS4f+ΔB for comparison. The error bars denote the difference between the inner barrier height and the corresponding outer barrier height for actinides [3].

    Using the proposed approach, we systematically studied the fission barrier heights for stable nuclei. In Fig. 5, we show the predicted Bf for even-even nuclei which lie on or are the closest to the β-stability line (Green's expression [37], NZ=0.4A2/(A+200), was arbitrarily adopted). The solid curve denotes the results of the macroscopic fission barrier Bmacf given by Eq.(3). Evidently, the macroscopic barrier height approaches zero for super-heavy nuclei. For nuclei around 208Pb, the fission barrier heights predicted with both FRLDM and WS4 models are significantly higher than those of Bmacf, owing to the strong shell effects. For actinides with A240, the results obtained using WS4 are close to those obtained using FRLDM, with values of approximately 6 MeV. For super-heavy nuclei around 294Cn, the results obtained using FRLDM are higher than those obtained using WS4, by approximately 4 MeV.

    Figure 5

    Figure 5.  (color online) Fission barrier heights for even-even nuclei which lie on or are the closest to the β-stability line (using Green's expression [37]).

    In addition, using the proposed approach we simultaneously investigated the fission barrier heights of unstable nuclei. In Fig. 6, we show the predicted barrier heights for isotopic chains of Pb, Ra, U and Cm. The pink squares denote the empirical barrier heights taken from Ref. [3]. For Pb isotopes, the fission barriers evidently decrease with the increasing distance from the doubly-magic nucleus 208Pb. For Ra and U isotopes, all three approaches predict a peak at the neutron-deficient side with neutron number N=126. For 218U, the predicted barrier height BWS4+ΔBf=5.30 MeV, while the result obtained using FRLDM is 9.67 MeV. Very recently, the fission barrier heights for neutron-deficient nuclei 210Fr and 210Ra have been measured [38], and the reported values were Bf(210Fr) = 10.67 MeV and Bf(210Ra) = 8.54 MeV with uncertainty of 5%. The predicted values of BWS4+ΔBf were 11.50 MeV and 8.78 MeV for 210Fr and 210Ra, respectively. From Fig. 6(b), it is evident that the measured Bf(210Ra) (open circle) can be well reproduced using the WS4+ΔB calculations. For the neutron-rich side, the trend of the fission barrier height is also strongly affected by the shell corrections. In Fig. 7, we show the predicted Bf for nuclei with Z=102, 106, 119 and 120. For No and Sg isotopes, the peaks of the fission barrier heights at N=152 and N=162 can be clearly observed. The abrupt change of α-decay energies at neutron number of 152 and 162 owing to the shell effects can also be clearly observed for heavy and super-heavy nuclei [39].

    Figure 6

    Figure 6.  (color online) Predicted fission barrier heights for isotopic chains of Pb, Ra, U and Cm. The open squares denote the results obtained using FRLDM. The crosses and the solid circles denote the results obtained using WS4 with Eq. (4) and those together with the residual correction ΔB, respectively. The solid curve denotes the mean value of the fission barrier heights Bf obtained using the three approaches. The open circle in (b) denotes the measured Bf for 210Ra taken from Ref. [38].

    Figure 7

    Figure 7.  (color online) The same as Fig. 6, but for heavier nuclei.

    For unknown super-heavy nuclei (SHN) with Z=119 and 120, the predicted fission barrier heights are presented in Fig. 7(c) and (d). Evidently, for the SHN with Z=119 and A=297, the barrier height predicted by the FRLDM is 7.94 MeV, which is higher than that obtained using the WS4 model by 2 MeV. We note that in the study of the fusion reaction 48Ca+238U [40], the negative of the shell correction energy (6.64 MeV) from the finite range droplet model (FRDM) [41] is taken as the fission barrier height of the compound nucleus, but multiplied by 0.7 in order to reproduce the maximal cross section for 283Cn(3n) measured at an excitation energy of 35.0 MeV. The predicted value of BWS4f=4.20 MeV for 286Cn, which is comparable with the result obtained using the FRDM multiplied by 0.7. Considering the reduction factor of 0.7 for the results obtained using the FRLDM, the fission barrier heights obtained using the two models are comparable for the SHN with Z=119 and A=297. For the SHN with Z=120, the largest value of BWS4f=6.23 MeV is located at N=176, which is consistent with the predictions of Warsaw's macroscopic-microscopic calculations [24].

    Based on the WS4 mass model with which the known masses can be reproduced with an rms error of 0.3 MeV and the known α-decay energies of SHN can be reproduced with deviations smaller than 0.5 MeV, the fission barrier heights of heavy and superheavy nuclei were systematically studied. Considering the shell corrections, the macroscopic deformation energy and a phenomenological residual correction, the fission barrier heights for nuclei with Z82 were well described, with an rms error of only 0.481 MeV. We note that in addition to the shell correction at the ground state, the shell correction at the saddle point and its relative value were also important for accurate description of the barrier height. From the predicted fission barriers for isotopic chains of Pb, Ra, No and Sg, we note that the influence of the shell effect on the barrier height was evident. For Ra and U isotopes, all three approaches predicted a peak at the neutron-deficient side with N=126. For No and Sg isotopes, the peaks of the barrier heights at N=152 and N=162 were clearly observed. With the predicted fission barriers, the evaporation residual cross sections in the fusion reactions searching for new neutron-deficient isotopes [42] and the reactions leading to the synthesis of super-heavy nuclei [43] can be analyzed more accurately.

    The table of the fission barriers with the WS4 model is available from http://www.imqmd.com/mass/BfWS4.txt

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    [2] F. Abe et al. (CDF), Phys. Rev. Lett. 74, 2626 (1995) doi: 10.1103/PhysRevLett.74.2626
    [3] G. Aad et al. (ATLAS), JINST 3, S08003 (2008) doi: 10.1088/1748-0221/3/08/S08003
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Ming-Yue Liu, Shu-Min Zhao, Song Gao, Xing-Yu Han and Tai-Fu Feng. The top quark rare decays with flavor violation[J]. Chinese Physics C. doi: 10.1088/1674-1137/ad53bb
Ming-Yue Liu, Shu-Min Zhao, Song Gao, Xing-Yu Han and Tai-Fu Feng. The top quark rare decays with flavor violation[J]. Chinese Physics C.  doi: 10.1088/1674-1137/ad53bb shu
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Top-quark rare decays with flavor violation

    Corresponding author: Shu-Min Zhao, zhaosm@hbu.edu.cn
  • 1. Department of Physics, Hebei University, Baoding 071002, China
  • 2. Hebei Key Laboratory of High-precision Computation and Application of Quantum Field Theory, Baoding 071002, China
  • 3. Hebei Research Center of the Basic Discipline for Computational Physics, Baoding 071002, China
  • 4. Department of Physics, Chongqing University, Chongqing 401331, China

Abstract: In the present study, we investigated the decays of the top quark: tcγ, tcg, tcZ, and tch. They are extremely rare processes in the standard model (SM). As the U(1) extension of the minimal supersymmetric standard model (MSSM), the U(1)X SSM features new superfields such as the right-handed neutrinos and three Higgs singlets. We analyzed the effects of different sensitive parameters on the results and made reasonable theoretical predictions, thereby providing a useful reference for future experimental development. Considering the constraint set by the updated experimental data, the numerical results show that the branching ratios of the four processes, i.e., tcγ,cg,cZ,ch, can reach the same order of magnitude as their experimental upper limits. Among them, tanβ has the most evident effect on these processes and is the main parameter; gX, gYX, μ, M2, λH, M2U23, and M2Q23 are also important parameters for the processes, and have effects on the numerical results.

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    I.   INTRODUCTION
    • The top quark was discovered in 1995 by a set of D0 and CDF experiments conducted at the Fermi National Accelerator Laboratory (Fermilab), located in the United States [1, 2]. This discovery was important for the validation of the Standard Model (SM) and the study of particle physics. The study of the nature and behavior of the top quark helps us understand physical processes such as the origin of the mass of elementary particles, and weak and strong interactions. The existence and properties of the top quark have been experimentally verified several times, including the D0 and CDF experiments at Fermilab, and the ATLAS [3] and CMS [4] experiments at the Large Hadron Collider (LHC) in Geneva, Switzerland. These experiments investigate aspects of the nature, decay modes, and interactions of the top quark through high-energy collisions and particle detection techniques. The next generation of LHC will produce top quarks in large quantities. At the upgraded Fermilab, an integrated luminosity of 10 fb–1 will produce approximately 8×104 top quarks, while at the same luminosity, the LHC will produce approximately 100 times as many [57].

      Top quark decays with flavor violation refer to the decay processes of the top quark that violate the flavor conservation, specifically the violation of the lepton or quark flavor. While the SM predicts that the top quark predominantly decays into a W boson and a bottom quark, extensions beyond the SM allow for additional decay modes that involve different quarks or leptons [8, 9]. It is worth noting that specific details about the nature and extent of flavor violation during top quark decays require more in-depth analysis. The study of heavy particle decays via flavor-changing neutral-currents (FCNC) has played an important role in testing the SM and exploring new physics beyond the SM [1012]. In the SM, branching ratios of the FCNC of the top quarks, tcγ, tcg, tcZ, and tch, are highly suppressed and beyond the detection capabilities of the LHC in the near future [1315]. However, exotic mechanisms from new physics can greatly increase these branching ratios [16], which may be detected in the future. The SM predictions [14] and latest upper bounds on the branching ratios of tcγ, tcg, tcZ, and tch at 95% confidence level (C.L.) [17] are listed in Table 1. Note that the current experimental bounds are much higher than the SM predictions.

      DecayBr(tcγ)Br(tcg)Br(tcZ)Br(tch)
      SM4.6×10144.6×10121×10143×1015
      Upper Limit (95%C.L.)1.8×1042×1045×1041.1×103

      Table 1.  SM predictions and experimental bounds on the decays tcV,ch.

      As the heaviest elementary particle in the SM with mass on the electroweak scale, the top quark is likely to be more sensitive to new physics. Kinematically, it can reach many FCNC decay modes such as tcγ, tcg, tcZ, and tch, where h is the lightest CP-even Higgs boson. In the SM, these FCNC decay modes are highly suppressed by the GIM mechanism, with branching ratios typically of the order of 10151012 [57, 1824], which is a relatively small order of magnitude. The observation of any of such FCNC top-quark decays would be strong evidence of new physics. Therefore, the detection of those top-quark rare decays at the LHC will provide a suitable window to search for new physics beyond the SM. Some theoretical predictions for the branching ratios of top-quark rare decays in new physics extensions are known, such as those from supersymmetric (SUSY) models with R-parity conservation. These branching ratios can reach the following values: Br(tcγ)106, Br(tcg)105, and Br(tcZ)106 [25, 26]. The branching ratios from SUSY without R-parity conservation can reach the following values: Br(tcγ)106, Br(tcg)104, Br(tcZ)107, and Br(tch)104 [27, 28]. The branching ratios in the two Higgs doublet models can reach the following values: Br(tcγ)106, Br(tcg)104, Br(tcZ)107, and Br(tch)103 [2932]. In the extension of the MSSM with additional local U(1)BL gauge symmetry (B-LSSM), the branching ratios can reach the following values: Br(tcγ)5×107, Br(tcg)2×106, Br(tcZ)4×107 , and Br(tch)3×109 [33].

      In this study, we explored top-quark decays with flavor violation under the U(1)X SSM. The U(1)X SSM is an extension of the MSSM that incorporates an extra U(1)X gauge symmetry. Its local gauge group is SU(3)C×SU(2)L×U(1)Y×U(1)X[3436]. Compared to the MSSM, in the U(1)X SSM three new Higgs singlets, ˆη,ˆˉη,ˆS, and three-generation right-handed neutrinos, ˆνi, are added. The right-handed neutrinos generate an extremely small mass for light neutrinos via a see-saw mechanism; light sneutrinos constitute a new dark matter candidate. The presence of right-handed neutrinos, sneutrinos, and additional Higgs singlets alleviates the so-called small hierarchy problem arising in the MSSM, where the μ problem exists. In the U(1)X SSM [37], this problem can be alleviated by the S field after vacuum spontaneous breaking.

      This paper is organized as follows. In Sec. II, we briefly introduce the U(1)X SSM, including its superpotential, general soft breaking terms, and the rotations and interactions of the eigenstates "EWSB". In Sec. III, we provide analytical expressions for the branching ratios of the tcV,ch (V=γ,Z,g) decays in the U(1)X SSM. In Sec. IV, we report on the corresponding parameters and numerical analysis. Finally, in Sec. V, we present a summary of this study.

    II.   U(1)X SSM
    • In this section, we overview the U(1)X SSM. The U(1)X SSM includes a local gauge group of SU(3)C×SU(2)L×U(1)Y with the same gauge group as those of the SM and MSSM. It is a U(1)X extension of the MSSM that has a local gauge group of SU(3)C×SU(2)L×U(1)Y×U(1)X [3840]. In addition to the MSSM, the field spectrum in the U(1)X SSM contains new superfields: the right-handed neutrinos, denoted as ˆνi, and three Higgs singlets: ˆη,ˆˉη,ˆS. Through the see-saw mechanism, the lighter neutrinos gain extremely small masses at the tree level. The formation of the 5×5 mass-squared matrix is due to the mixing of the neutral CP-even parts of Hu, Hd, η, ˉη, and S. To obtain the 125.25 GeV Higgs particle mass [41, 42], loop corrections must be considered. These sneutrinos are decomposed into CP-even sneutrinos and CP-odd sneutrinos, and their mass-squared matrices are both expanded to 6×6.

      The superpotential in the U(1)X SSM is expressed as follows:

      W=lWˆS+μˆHuˆHd+MSˆSˆSYdˆdˆqˆHdYeˆeˆlˆHd+λHˆSˆHuˆHd+Mˆηˆηˆˉη+λCˆSˆηˆˉη+κ3ˆSˆSˆS+YuˆuˆqˆHu+YXˆνˆˉηˆν+YνˆνˆlˆHu.

      (1)

      In Eq. (1), the vacuum expectation value of ˆˉη produces the Majorana mass of the right-handed neutrino through YXˆνˆˉηˆν. The right-handed neutrino mixes with the left-handed neutrino through YνˆνˆlˆHu.

      The vacuum expectation values (VEVs) of the Higgs superfields, i.e., Hu, Hd, η, ˉη, and S, are denoted by vu, vd, vη, vˉη, and vS, respectively. Two angles are defined as tanβ=vu/vd and tanβη=vˉη/vη. The explicit forms of the two Higgs doublets and three Higgs singlets are expressed as follows:

      η=12(vη+ϕ0η+iP0η),ˉη=12(vˉη+ϕ0ˉη+iP0ˉη),S=12(vS+ϕ0S+iP0S),Hu=(H+u12(vu+H0u+iP0u)),Hd=(12(vd+H0d+iP0d)Hd).

      (2)

      The soft SUSY breaking terms of the U(1)X SSM are expressed as follows:

      Lsoft=LMSSMsoftBSS2LSSTκ3S3TλCSηˉη+ϵijTλHSHidHjuTIJXˉη˜νIR˜νJR+ϵijTIJνHiu˜νIR˜lJjm2η|η|2m2ˉη|ˉη|2m2SS2(m2˜νR)IJ˜νIR˜νJR12(MSλ2˜X+2MBBλ˜Bλ˜X)+h.c..

      (3)

      LMSSMsoft are soft breaking terms of the MSSM. The particle content and charge assignments for the U(1)X SSM are listed in Table 2. In a previous study of ours, we showed that the U(1)X SSM is anomaly free [39]. In the U(1)X SSM, U(1)Y and U(1)X are two Abelian groups. We denote the U(1)Y charge by YY and the U(1)X charge by YX. The presence of these two Abelian groups gives rise to a new effect that is not found in the MSSM or other SUSY models with only one Abelian gauge group: the gauge kinetic mixing.

      Superfields ˆqi ˆuci ˆdci ˆli ˆeci ˆνi ˆHu ˆHd ˆη ˆˉη ˆS
      SU(3)C 3 ˉ3 ˉ3 1 1 1 1 1 1 1 1
      SU(2)L 2 1 1 2 1 1 2 2 1 1 1
      U(1)Y 1/6 -2/3 1/3 -1/2 1 0 1/2 -1/2 0 0 0
      U(1)X 0 -1/2 1/2 0 1/2 -1/2 1/2 -1/2 -1 1 0

      Table 2.  Superfields in the U(1)X SSM.

      This effect can be caused by RGEs. AYμ and AXμ denote the gauge fields of U(1)Y and U(1)X, respectively. The form of the covariant derivative of the U(1)X SSM can be expressed as follows:

      Dμ=μi(YY,YX)(gY,gYXgXY,gX)(AYμAXμ).

      (4)

      We redefine the following expression [43, 44]:

      (gY,gYXgXY,gX)RT=(g1,gYX0,gX),R(AYμAXμ)=(AYμAXμ).

      (5)

      Finally, the gauge derivative of the U(1)X SSM is transformed into

      Dμ=μi(YY,YX)(g1,gYX0,gX)(AYμAXμ).

      (6)

      The term gX denotes the gauge coupling constant for the U(1)X group; gYX is the mixed gauge coupling constant for the U(1)Y and U(1)X groups.

      In the U(1)X SSM, the gauge bosons AYμ, AXμ, and V3μ are mixed together at the tree level. The mass matrix of gauge bosons can be found in [39]. We use two mixing angles, θW and θW, to obtain the mass eigenvalues of the matrix; θW is the Weinberg angle whereas θW is the new mixing angle. We define v=v2u+v2d and ξ=v2η+v2ˉη. The new mixing angle is expressed as follows:

      sin2θW=12[(gYX+gX)2g21g22]v2+4g2Xξ22[(gYX+gX)2+g21+g22]2v4+8g2X[(gYX+gX)2g21g22]v2ξ2+16g4Xξ4.

      (7)

      We next derive the eigenvalues of the mass-squared matrix of the neutral gauge bosons. One is the zero mass corresponding to the photon whereas the other two values are Z and Z:

      m2γ=0,m2Z,Z=18((g21+g22+(gYX+gX)2)v2+4g2Xξ2)(g21+g22+(gYX+gX)2)2v4+8((gYX+gX)2g21g22)g2Xv2ξ2+16g2Xξ4.

      (8)

      The mass matrix for the chargino is

      m˜χ=(M212g2vμ12g2vd12λHvS+μ).

      (9)

      This matrix is diagonalized by U and V:

      Um˜χV=mdiag˜χ.

      (10)

      The mass matrix for the neutrino is

      mν=(012vuYTν12vuYν2vˉηYX).

      (11)

      This matrix is diagonalized by UV:

      UV,mνUV,=mdiaν.

      (12)

      Additional mass matrices are required in the calculations [38, 39].

    III.   ANALYTICAL FORMULA
    • In this section, we focus on the theoretical study of the top-quark processes tcγ, tcg, tcZ, and tch with flavor violation under the U(1)X SSM. The relevant Feynman diagrams contributing to tcγ, tcg, tcZ, and tch in the U(1)X SSM are presented in Figs. 1 and 2.

      Figure 1.  Feynman diagrams for the tcγ, tcg, tcZ processes in the U(1)XSSM.

      Figure 2.  Feynman diagrams for the tch process in the U(1)X SSM.

      In the U(1)X SSM, the flavor violating amplitude corresponding to the decay process tcV (V=γ,Z) is expressed as follows:

      MtcV=εμˉuc(p)(AVγμPL+iBVσμνqνPL+(LR))ut(p).

      (13)

      To better explain how the calculations of the above equation and Feynman diagrams in Fig. 1 are done, Fig. 1(1) is selected as an example. The corresponding amplitude can be expressed as follows:

      MtcV=i,j,k,nεμˉuc(p)dDk(2π)Di(ALˉc˜Dkχ±nPL+ARˉc˜Dkχ±nPR)×ipkmχ±ni(ALˉχ±n˜DitPL+ARˉχ±n˜DitPR)ik2m2˜DiiBV˜Di˜Dk×(2kμ+qμ)i(kq)2m2˜Dkut(p).

      (14)

      Here, εμ denotes the polarization vectors of the photon and Z boson; ut and uc denote the wave functions of the top and charm quarks; p is the momentum of the top quark; p is the momentum of the charm quark; q is the momentum of the vector boson; and m˜Di, m˜Dk, and mχ± are the mass eigenvalues from Eq. (9). Correspondingly, ALˉc˜Dχ±, ARˉc˜Dχ±, ALˉχ±˜Dt, ARˉχ±˜Dt, and BV˜D˜D are the coupling vertices [39, 40, 45, 46]. L and R in the subscripts denote the left-handed and right-handed parts, respectively. They can be derived from SARAH.

      Next, we solve the Feynman integral. The formula employed for the integration of the denominator is [47]

      1ABC=10dx102ydy1[(Ax+B(1x))y+C(1y)]3.

      (15)

      Calculating the integral in this manner can greatly increase the efficiency of numerical calculations. According to Eq. (15), we obtain:

      10dx102ydy{([(pk)2m2χ±n]x+(k2m2˜Di)(1x))y+((kq)2m2˜Dk)(1y)}3=10dx102ydy{[kpxyq(1y)]2[pxy+q(1y)]2+(p2m2χ±n)xym2˜Di(1x)y+(q2m2˜Dk)(1y)}3,

      (16)

      where we apply b=pxyq(1y), k=k+b, and J = [p2(xyx2y2)+q2((1y)(1y)2)2pqxy(1y)m2χ±nxym2˜Di(1x)ym2˜Dk(1y)] to obtain the final form of the denominator in Eq. (14):

      10dx102ydy1(k2J)3.

      (17)

      This type of substitution is also performed for the numerator in Eq. (14). We take all the diagrams in Fig. 1 and calculate the Feynman amplitudes for tcγ, tcg, and tcZ. Finally, we calculate the respective mode squares for the three processes.

      In the MSSM, the top quark decay tch is flavor-changing, where h is the lightest CP-even Higgs boson. Note that in Fig. 2, the new contribution of the down-type quarks, the mixing between the Higgs doublet and exotic single-line states ˜η1,2 also affects tch decay channel. We use the following calculation related to Fig. 2(4) as an example. The amplitude can be expressed as follows:

      Mtch=ˉuc(p)dDk(2π)D1[(kq)2m2χ±](k2m2χ±)[(pk)2m2˜Dj],(ALˉcχ±˜DjPL+ARˉcχ±˜DjPR)(kq+mχ±)(ALˉ˜Djχ±tPL+ARˉ˜Djχ±tPR)(k+mχ±)(ALhχ±χ±PL+ARhχ±χ±PR)ut(p).

      (18)

      Other graphs of the tch process can be calculated similarly.

      We use dimensional regularization to treat the divergences with d=42ϵ and the limit d4. To obtain finite results, the divergences are canceled by the modified minimal substraction (¯MS) scheme. The terms proportional to 1ϵγE+log(4π) are deleted. Here, γE0.5772 is an Euler constant.

      Based on the above calculations, the branching ratios of the top-quark rare decays are respectively:

      Br(tcV)=|MtcV|2((mt+mV)2m2c)((m+tmV)2m2c)32πm3tΓtotal,Br(tch)=|Mtch|2((mt+mh)2m2c)((m+tmh)2m2c)32πm3tΓtotal,

      (19)

      where Γtotal = 1.42+0.190.15 GeV [17] is the total decay width of the top quark.

    IV.   NUMERICAL ANALYSIS
    • In this section, we study the numerical results of flavor violation for the top-quark tcV,ch processes. According to the latest LHC data [4852], our values are subject to certain constraints. Thus, we consider the following individual experimental constraints:

      1. The lightest CP-even Higgs mass is approximately 125.25 GeV [17, 5355].

      2. The updated experimental data show that the mass of the Z boson at the 95% confidence level (CL) [56] satisfies MZ> 5.15 TeV. Eq. (15) yields an approximate result of MZ as MZgXξ> 5.15 TeV.

      3. The ratio between MZ and its gauge coupling constant is MZgX6 TeV [57, 58]. Thus, gX is restricted in the region 0<gX0.85.

      4. The new angle βη is constrained by LHC as tanβη<1.5 [59].

      5. The limitations for the particle masses according to the PDG [17] data and the specific contents are as follows. The neutralino mass mandatorily exceeds 116 GeV, the chargino mass mandatorily exceeds 1000 GeV, and the scalar quark mass is greater than 1300 GeV.

      The relevant SM input parameters in the numerical program were selected as follows: mZ = 91.188 GeV, mW = 80.385 GeV, mc = 1.27 GeV, and mt = 172.69 GeV. In conjunction with the aforementioned experimental requirements, we obtained a wealth of data, and used graphs to analyze and process the data. We generally set the values of new particle masses (MBB,MBL) in the order of 103 GeV, which is approximately the energy scale of new physics. TλC and TλH are trilinear coupling coefficients whose values are in the order of magnitude of the mass, and can be varied up or down to the order of 102 104 GeV. M2Uii, M2Qii, M2Dii, BS, and Bμ are all of mass square dimension, and can reach the order of 106 GeV2. The dimensionless parameters λC and λH are generally set to values less than 1. Considering the constraints just described, we set the values of parameters as follows:

      MBB=400GeV,M2Uii=6×106GeV2(i=1,2,3),TλC=100GeV,MBL=1000GeV,λC=0.08,TλH=300GeV,κ=0.1,lW=4×106GeV2,Bμ=BS=1×106GeV2.

      (20)

      We set the non-diagonal elements of the mass matrix to zero unless otherwise specified. In the U(1)X SSM, gYX denotes the mixing gauge coupling constant of the U(1)Y and U(1)X groups; it is the parameter beyond MSSM. The mass matrices of neutralino, down type squark, and up type squark all contain gYX. Furthermore, gYX appears in the vertex and can enlarge its coupling constant. MBB is the mass of the U(1)Y and U(1)X gaugino mixings; it is present in the mass matrix of the neutralino. Moreover, tanβ appears in almost all the mass matrices of fermions, scalars, and Majoranas. It must be a sensitive parameter that affects the masses of particles and vertex couplings by directly influencing vu and vd, MBL is the mass of the new gaugino. It influences the mass matrix of the neutralino. Finally, λH relates to the strength of the self-interaction coupling of the Higgs field, which affects the VEV and Higgs boson mass.

    • A.   Process of tcγ

    • To determine the parameters affecting the top-quark flavor violation, some sensitive parameters need to be studied. To show the numerical results clearly, the parameters were set as follows: M2Dii=6×106GeV2, M2Qii=6×106GeV2 (i = 1,2,3), μ=1000GeV, M1=1200GeV. We next show plots depicting the relationship between Br(tcγ) and different parameters.

      First, we show one-dimensional diagrams of Br(tcγ) versus M2Q23, M2 in Fig. 3. The gray shaded area is the experimental limit satisfied by the Br(tcγ) process. Fig. 3(a) shows Br(tcγ) versus M2Q23, with tanβ=20, M2=1200GeV, gYX=0.2, and λH=0.1. The solid line corresponds to gX = 0.3 whereas the dashed line corresponds to gX = 0.6. Overall, both lines show a decreasing trend in the range of 04×105GeV2 for M2Q23 owing to the fact that the contribution of the lower-type squarks is canceled by the contribution of the charged Higgs boson at the turning point. Then, it is followed by an upward trend, which means that Br(tcγ) increases as M2Q234×105GeV2. From bottom to top in Fig. 3 (a), Br(tcγ) increases as the value of gX increases. Fig. 3 (c) shows the differential distribution of Fig. 3 (a). Figure 3 (c) further evidences the trend and pattern of the values in Fig. 3 (a). Moreover, in Fig. 3 (c), the differential increases linearly, and the speed of variable change is relatively smooth. This means that M2Q23 is a parameter that influences Br(tcγ).

      Figure 3.  (color online) Diagrams of Br(tcγ) affected by different parameters. The gray area represents a reasonable value range where Br(tcγ) is lower than the upper limit. The solid and dashed lines in Fig. 3(a) correspond to gX=0.3 and gX=0.6. The solid and dashed lines in Fig. 3(b) correspond to tanβ=20 and tanβ=25, as MQij=105GeV2 (i=j=1,2,3,ij). Fig. 3(c) shows the differential distribution of (a) and Fig. 3(d) shows the differential distribution of (b).

      Figure 3 (b) represents Br(tcγ) versus M2, with M2Qij=105GeV2 (i,j=1,2,3,ij), gX=0.3, λH=0.1, and gYX=0.2. The solid line corresponds totanβ=20, whereas the dashed line corresponds to tanβ=25. There is a slight bulge in the Br(tcγ) value at M2=1400GeV, followed by a slight downward trend. It can be seen that the overall value satisfies this limit and follows a decreasing trend. As the line in the graph goes from bottom to top, i.e., as tanβ increases, Br(tcγ) also increases gradually. Figure 3 (d) shows the differential distribution of Fig. 3 (b). In Fig. 3 (d), there is a maximum of the differential value at M2 = 1400 GeV; at this point, Br(tcγ) reaches its maximum value. The differential value is negative for M2>1600 GeV. That is to say, Br(tcγ) decreses, but very slightly.

      For a deeper exploration of the parameter space at M2=1200GeV, we scanned some parameters randomly. In particular, in the Br(tcγ) process, we swept some parameters as follows:

      5tanβ50,0.3gX0.7,0.01gYX0.5,0.1λH0.4.

      (21)

      In Fig. 4(a), we set λH=0.1 and gYX=0.2 to explore the effects of tanβ and gX on Br(tcγ). It is clear from this figure that the value of Br(tcγ) increases as tanβ increases. When tanβ reaches its maximum value of 50, Br(tcγ) reaches an order of magnitude of 104, very close to the experimental upper limit. This indicates that tanβ is a crucial parameter. The value of Br(tcγ) becomes large as gX increases; however, the effect of gX on Br(tcγ) is small and hardly noticeable.

      Figure 4.  (color online) (a) Effects of tanβ and gX on Br(tcγ). The horizontal coordinate indicates the range 5tanβ50 whereas the vertical coordinate indicates the range 0.3gX0.7. (b) Effects of gYX and λH on Br(tcγ). The horizontal coordinate indicates the range 0.01gYX0.5 whereas the vertical coordinate indicates 0.1λH0.4. The icons on the right side indicate the colors corresponding to the values of Br(tcγ).

      In Fig. 4(b), we set tanβ=20 and gX=0.3 to explore the effects of λH and gYX on Br(tcγ). Note that both λH and gYX have effects on Br(tcγ). The value of Br(tcγ) decreases with the increase of gYX. The smaller the value of gYX, the closer to the upper limit of Br(tcγ). There is a slight increase in the value of Br(tcγ) with λH, but the impact of λH is relatively small compared to that of gYX. Figure 4(b) shows the presence of a white area in the upper left corner. This is due to the limitation established by the masses of Higgs and other particles.

    • B.   Process of tcg

    • In this section, we continue our exploration of the branching ratio of tcg with respect to certain parameters. In this case, we set M1=1200GeV, M2=1200GeV, M2Dii=6×106GeV2, and M2Qii=6×106GeV2. One-dimensional diagrams of Br(tcg) are shown in Fig. 5. The gray shaded portion indicates the experimental limit that is satisfied by the Br(tcg) process. Figure 5 (a) shows Br(tcg) versus M2U23 for tanβ=20, λH = 0.1, gX=0.3, andgYX=0.2; the solid and dashed lines correspond to μ=1000GeV and μ=1100GeV, respectively. Note that Br(tcg) increases with M2U23 and the value approaches the experimental upper limit as M2U23 further increases. Note also that Br(tcg) decreases as μ increases. Figure 5 (c) shows the differential distribution of Fig. 5 (a). According to Fig. 5 (c), the variation of Fig. 5(a) is mostly regular. Note that tcg increases with M2U23.

      Figure 5.  (color online) Br(tcg) diagrams affected by different parameters. The gray area represents a reasonable value range where Br(tcg) is lower than the upper limit. The solid and dashed lines in Fig. 5(a) correspond to μ=1000GeV and μ=1100GeV. The solid and dashed lines in Fig. 5(b) correspond to tanβ=23 and tanβ=25. Fig. 5(c) shows the differential distribution of (a) and Fig. 5(d) shows the differential distribution of (b).

      Figure 5 (b) shows Br(tcg) versus λH with MQ23=105GeV2, μ=1000GeV, gX=0.3, gYX=0.2, tanβ=23 (solid line), and tanβ=25 (dashed line). Note that the value of Br(tcg) shows a minimum at λH=0.08, which is due to the mixing of several parameters. Its overall value satisfies the experimental limit of the process; it is from five to six orders of magnitude higher than the SM prediction. As tanβ increases from 23 to 25, the Br(tcg) value also increases. However, note that the Br(tcg) values almost coincide at λH=0.07. Figure 5 (d) shows the differential distribution of Fig. 5 (b). In Fig. 5 (d), the differential values are negative for λH<0.08, and Br(tcg) decreases as λH becomes larger. In the range 0.08λH<0.11, the slope is the largest, and Br(tcg) changes more quickly than the others. For λH0.11, the differential values are all positive, but the value variation is small. Moreover, Br(tcg) becomes larger, although the magnitude of the increase is smaller.

      Let us assume that μ=1000GeV and λH=0.1. We randomly scanned the parameters tanβ, gX, gYX as follows:

      5tanβ50,0.3gX0.7,0.01gYX0.5.

      (22)

      In Fig. 6 (a), we set gX=0.3 to explore the effects of tanβ and gYX on Br(tcg). Note that as tanβ increases, Br(tcg) gradually changes from blue to yellow, i.e., a significant increase in Br(tcg) occurs. The larger the value of tanβ, the closer the value of Br(tcg) to the experimental upper limit. Note that gYX has some minor effect on the results, and this effect is hardly noticeable. In Fig. 6 (b), we set tanβ=20 to explore the effects of gX and gYX on Br(tcg); note that the larger the value of gX, the larger the value of Br(tcg). Note also that the larger the value of gYX, the smaller the value of Br(tcg). Br(tcg) is maximized at gX=0.7 and gYX=0.01, and Br(tcg) becomes closer to the upper limit of the experiment. When gYX tends to zero, the dependence of the branching ratio on gX is strong.

      Figure 6.  (color online) (a) Effects of tanβ and gYX on Br(tcg). The horizontal coordinate indicates the range 5tanβ50 whereas the vertical coordinate indicates the range 0.01gYX0.5. (b) Effects of gX and gYX on Br(tcg). The horizontal coordinate indicates the range 0.3gX0.7 whereas the vertical coordinate indicates 0.01gYX0.5. The icons on the right side indicate the colors corresponding to the values of Br(tcg).

    • C.   Process of tcZ

    • The experimental upper bound (5×104) for the Br(tcZ) process is of the same order of magnitude as that for Br(tcγ) and Br(tcg). In this subsection, we analyze the effects of different parameters on the Br(tcZ) branching ratio. In particular, we focus on the effects of the parameters M2U23, M2, gX, gYX, M2Dii, and M2Qii. We set M1=1200GeV and λH=0.1. One-dimensional representations are presented in Fig. 7 whereas multi-dimensional plots are presented in Fig. 8.

      Figure 7.  (color online) Br(tcZ) diagrams affected by different parameters. The gray area indicates a reasonable value range where Br(tcZ) is lower than the upper limit. The solid and dashed lines in Fig. 7(a) correspond to μ=1000GeV and μ=1500GeV. The solid and dashed lines in Fig. 7(b) correspond to tanβ=20 and tanβ=25. Fig. 7(c) shows the differential distribution of (a) and Fig. 7(d) shows the differential distribution of (b).

      Figure 8.  (color online) (a) Effects of gX and gYX on Br(tcZ). The horizontal coordinate indicates the range 0.3gX0.7 whereas the vertical coordinate indicates 0.01gYX0.5. (b) Effects of M2Dii and M2Qii on Br(tcZ). The horizontal coordinate indicates the range 106GeV2M2Dii107GeV2 whereas the vertical coordinate indicates the range 106GeV2M2Qii107GeV2. The icons on the right side indicate the colors corresponding to the values of Br(tcZ).

      Fig. 7(a) represents Br(tcZ) versus M2U23 for M2=1200GeV, tanβ=20, gX=0.3, gYX=0.2, M2Dii=6×106GeV2, and M2Qii=6×106GeV2, with the solid and dashed lines representing μ=1000GeV and μ=1500GeV, respectively. Note that both lines show an increasing trend, i.e., Br(tcZ) increases with M2U23. However, the change is not significant in terms of value. Note also a decrease in Br(tcZ) as μ increases. Both curves are shaded in gray. In Fig. 7 (b), we set μ=1000GeV, gX=0.3, gYX=0.2, M2Dii=6×106GeV2, and M2Qii=6×106GeV2; the figure shows Br(tcZ) versus M2 for tanβ=20 (solid line) and tanβ=25 (dashed line). The two lines are convex and reach a maximum at M2=1150GeV, then exhibit a downward trend and finally level off, i.e., in the range of 1000GeVM21500GeV, M2 has a clear influence on Br(tcZ). The solid and dashed lines run from bottom to top, indicating that tanβ is also a sensitive parameter for Br(tcZ), which increases with tanβ.

      Figure 7(c) shows the differential distribution of Fig. 7 (a). In Fig. 7 (c), the difference values are all positive. When μ=1000GeV and μ=1500GeV, the difference between the values is very small, and the two lines almost coincide. Figure 7 (d) shows the differential distribution of Fig. 7 (b). In Fig. 7 (d), the differential values in most regions are negative when M2<1500GeV; otherwise, they are positive.

      To further explore the effects of different parameters on Br(tcZ), we set μ=1000GeV, M2=1200GeV, and tanβ=20 and performed randomized scans in the following ranges:

      0.01gYX0.5,106GeV2M2Dii107GeV2,0.3gX0.7,106GeV2M2Qii107GeV2(i=1,2,3).

      (23)

      In Fig. 8 (a), we set M2Qii=6×106GeV2, M2Dii=6×106GeV2 to explore the effects of gX and gYX on Br(tcZ). Note that Br(tcZ) has a minimum at gX=0.3 and gYX=0.01. For Br(tcZ), both gX and gYX are sensitive parameters; gYX is a coupling constant that affects the strength of gauge mixing. Furthermore, gX and gYX make a new contribution to Br(tcZ) through ZZ mixing; gX also affects significantlyBr(tcZ) when gYX tends to a minimum. Br(tcZ) increases withgX and gYX. In Fig. 8(a), the white region appears in the upper right corner. We conclude that it is excluded by the experimental upper limit, i.e., Br(tcZ)<5×104.

      In Fig. 8 (b), we set gX=0.3 and gYX=0.2 to explore the effects of M2Qii and M2Dii on Br(tcZ). The values of M2Qii and M2Dii are both in the range of 106107GeV2. Fig. 8 (b) shows that M2Dii has an extremely small effect on Br(tcZ). However, as M2Qii increases, Br(tcZ) changes from yellow to blue, i.e., Br(tcZ) decreases weakly as M2Qii increases.

      In summary, regarding the tcZ process, the main sensitive parameters are M2, gX, gYX, and the off-diagonal element M2U23. The diagonal elements M2Qii (i = 1,2,3) have an effect, but they are not particularly sensitive.

    • D.   Process of tch

    • The experimental upper bound for Br(tch) is 1.1×103. In the U(1)X SSM, Br(tch) can be as high as 104 in some regions of the parameter space. Here, we set M2=1200GeV, M2Qii=6×106GeV2, and M2Dii=6×106GeV2. We studied the effects of M2Q23, μ, M1, and tanβ on Br(tch), as shown in Fig. 9. Figure 9 (a) shows Br(tch) versus M2Q23 for gX=0.4, μ=1000GeV, tanβ=20, gYX=0.2, and λH=0.1. The solid line represents M1=1200GeV whereas the dashed line represents M1=1600GeV. As the dashed and solid lines go from bottom to top, it can be observed that M2 has an effect on Br(tch) as a sensitive parameter, and Br(tch) decreases as M2 increases. Note that Br(tch) increases with M2Q23 almost linearly. Therefore, M2Q23 is also a parameter that notably affects Br(tch). Figure 9 (c) shows the differential distribution of Fig. 9 (a). In Fig. 9(c), the differential values are all positive. The trend of these values is relatively smooth and the regularity is more evident.

      Figure 9.  (color online) Br(tch) diagrams affected by different parameters. The gray area indicates a reasonable value range where Br(tch) is lower than the upper limit. For gX=0.4, the solid and dashed lines in Fig. 9(a) correspond to M1=1200GeV and M1=1600GeV. Setting M2Q23=105GeV2, the solid and dashed lines in Fig. 9(b) correspond to tanβ=20 and tanβ=25. Fig. 9(c) shows the differential distribution of (a) whereas Fig. 9(d) shows the differential distribution of (b).

      Figure 9 (b) shows Br(tch) versus μ for M1=1200GeV, gX=0.3, gYX=0.2, and λH=0.1, with the solid line representing tanβ=20 and the dashed line representing tanβ=25. By analyzing the three previous processes, i.e., tcγ, tcg and tcZ, we conclude that tanβ is one of the sensitive parameters. In the tch process, Fig. 9 (b) shows that tanβ is a more sensitive parameter. When tanβ increases from 20 to 25, Br(tch) increases with tanβ. It implies that Br(tch) reaches a minimum at μ=950GeV. When μ>950GeV, Br(tch) increases as μ increases, but the trend of increase is relatively small. Figure 9 (d) shows the differential distribution of Fig. 9 (b). In Fig. 9 (d), the differential values first decrease and then increase when μ<1050GeV. When μ1050GeV, the tendency of these two lines to decrease becomes progressively weaker.

      To further explore the effect of other parameters on Br(tch), we set M1=1200GeV, μ=1000GeV and performed a randomized scan of gX, gYX, λH, and tanβ:

      0.01gYX0.5,0.3gX0.7,0.1λH0.4,10tanβ50.

      (24)

      Based on the parameters in Eq. (24), we obtained the data and plot depicted in Fig. 10. Figure 10(a) shows the effect of gX (0.3gX0.7) and gYX (0.01gYX0.5) on Br(tch) by setting tanβ=20, λH=0.1. Fig. 10 (b) shows the effect of gX (0.3gX0.7) and λH(0.1λH0.4) on Br(tch) by setting tanβ=20, gYX=0.2. In Fig. 10 (c), we set gX=0.3 and gYX=0.2 to explore the effect of tanβ(10tanβ50) and λH(0.1λH0.4) on Br(tch). Combining the three plots in Fig. 10, we can clearly see that the four parameters, i.e., gX, gYX, λH, and tanβ, affect Br(tch), but they do so differently. Thus, both gX and gYX present clear effects on the numerical results. Br(tch) is a decreasing function of gX and gYX. At the point they both reach their minimum value, the branching ratio of the tch process reaches 104, which is very close to the experimental upper limit. Figs. 10 (b) and (c) show that λH also behaves very sensitively, with Br(tch) increasing as λH increases. Fig. 10 (c) shows that when tanβ>10, tanβ has a weak effect. This occurs because tanβ not only appears in the diagonal sectors of the mass matrix, but also dominates the non-diagonal sectors, leading to the above results.

      Figure 10.  (color online) (a) Effects of gX and gYX on Br(tch). The horizontal coordinate indicates the range 0.3gX0.7 whereas the vertical coordinate indicates 0.01gYX0.5. (b) Effects of gX and λH on Br(tch). The horizontal coordinate indicates the range 0.3gX0.7 whereas the vertical coordinate indicates the range 0.1λH0.4. (c) Effects of tanβ and λH on Br(tch). The horizontal coordinate indicates the range 5tanβ50 whereas the vertical coordinate indicates the range 0.1λH0.4. The icons on the right side indicate the colors corresponding to the values of Br(tcZ).

    V.   CONCLUSIONS
    • In summary, we studied the rare decays tcγ,cg,cZ,ch of the top quark in the U(1)X SSM. Compared to the MSSM, in the U(1)X SSM we added three new Higgs singlets ˆη,ˆˉη,ˆS and three generations of right-handed neutrinos ˆνi. Its local gauge group is SU(3)C×SU(2)L×U(1)Y×U(1)X. Probing with the U(1)X SSM made our study richer and more interesting, establishing a solid basis for the existence of new physics. We started with one-loop diagrams and computed the Feynman amplitude for each process to obtain numerical results for Br(tcγ),Br(tcg),Br(tcZ),Br(tch). We evaluated the effect of various parameters on the branching ratios of each process, selected the most illustrative results, and plotted one-dimensional and multi-dimensional plots for a more comprehensive numerical analysis based on experimental constraints.

      In the considered parameter space, numerical results show that all these processes are very close to the experimental upper limit, reaching even the same order of magnitude as the experimental upper limit at suitable parameter values. Therefore, they may be detected in future high-energy colliders. By analyzing the numerical results in the adopted parameter space, we can conclude that tanβ, gX, gYX, μ, M2, λH, and the off-diagonal parameters M2U23, M2Q23 are sensitive parameters that have a large influence on the branching ratios of the tcγ,cg,cZ,ch processes. Among them, the influence of tanβ is the greatest, being the main parameter of the tcγ,cg,cZ,ch processes. Concerning tanβ, it appears in the mass matrixes of almost all SUSY particles. It is a fact that tanβ affects the numerical results mainly by influencing the particle masses, the corresponding rotational matrices, and the coupling vertexes. Regarding gYX, it is a coupling constant in gauge mixing that is parameterized outside of the MSSM. In couplings where squarks appear, gX and gYX will affect the squark masses and corresponding rotation matrices, resulting in an effect on Br(tcγ,cg,cZ,ch). In addition, for the tcZ process, they generate new contributions via ZZ mixing. Comparing with the data in Table 3, we can see that the maximum value of Br(tcV,ch) obtained in the U(1)X SSM is greater than that achieved in the BLSSM. In particular, for Br(tch), the maximum value is even four orders of magnitude higher than that of the BLSSM. The maximum of Br(tcV,ch) obtained in the U(1)X SSM is already very close to the experimental upper limit, which makes our study more meaningful.

      DecaytcγtcgtcZtch
      Upper limit (95%C.L.)1.8×1042×1045×1041.1×103
      BLSSM [33]5×1072×1064×1073×109
      U(1)X SSM1.5×1045×1051.41×1047.04×105

      Table 3.  Upper limit (95%C.L.), BLSSM and U(1)X SSM bounds on the decays tcV,ch.

      In conclusion, we calculated the rare top-quark decays tcγ,cg,cZ,ch in the U(1)X SSM. They are certainly very interesting and worth exploring. Our study contributes to the understanding of the origin of R-parity and its possible spontaneous violation in super-symmetric models [6062].

    ACKNOWLEDGMENTS
    • The authors thank Xi Wang, Yi-Tong Wang, Xin-Xin Long for participating in the discussion of the numerical results.

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