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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 [5−7].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 [10−12]. In the SM, branching ratios of the FCNC of the top quarks,
t→cγ ,t→cg ,t→cZ , andt→ch , are highly suppressed and beyond the detection capabilities of the LHC in the near future [13−15]. 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 oft→cγ ,t→cg ,t→cZ , andt→ch 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.Decay Br(t→cγ) Br(t→cg) Br(t→cZ) Br(t→ch) SM 4.6×10−14 4.6×10−12 1×10−14 3×10−15 Upper Limit (95%C.L.) 1.8×10−4 2×10−4 5×10−4 1.1×10−3 Table 1. SM predictions and experimental bounds on the decays
t→cV,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
t→cγ ,t→cg ,t→cZ , andt→ch , 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 of10−15−10−12 [5−7, 18−24], 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(t→cγ)∼10−6 ,Br(t→cg)∼10−5 , andBr(t→cZ)∼10−6 [25, 26]. The branching ratios from SUSY without R-parity conservation can reach the following values:Br(t→cγ)∼10−6 ,Br(t→cg)∼10−4 ,Br(t→cZ)∼10−7 , andBr(t→ch)∼10−4 [27, 28]. The branching ratios in the two Higgs doublet models can reach the following values:Br(t→cγ)∼10−6 ,Br(t→cg)∼10−4 ,Br(t→cZ)∼10−7 , andBr(t→ch)∼10−3 [29−32]. In the extension of the MSSM with additional localU(1)B−L gauge symmetry (B-LSSM), the branching ratios can reach the following values:Br(t→cγ)∼5×10−7 ,Br(t→cg)∼2×10−6 ,Br(t→cZ)∼4×10−7 , andBr(t→ch)∼3×10−9 [33].In this study, we explored top-quark decays with flavor violation under the
U(1)X SSM. TheU(1)X SSM is an extension of the MSSM that incorporates an extraU(1)X gauge symmetry. Its local gauge group isSU(3)C×SU(2)L×U(1)Y×U(1)X [34−36]. Compared to the MSSM, in theU(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 theU(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 thet→cV,ch (V=γ,Z,g ) decays in theU(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. -
In this section, we overview the
U(1)X SSM. TheU(1)X SSM includes a local gauge group ofSU(3)C×SU(2)L×U(1)Y with the same gauge group as those of the SM and MSSM. It is aU(1)X extension of the MSSM that has a local gauge group ofSU(3)C×SU(2)L×U(1)Y×U(1)X [38−40]. In addition to the MSSM, the field spectrum in theU(1)X SSM contains new superfields: the right-handed neutrinos, denoted asˆνi , 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 the5×5 mass-squared matrix is due to the mixing of the neutral CP-even parts ofHu ,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 to6×6 .The superpotential in the
U(1)X SSM is expressed as follows:W=lWˆS+μˆHuˆHd+MSˆSˆS−YdˆdˆqˆHd−YeˆeˆlˆHd+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 throughYXˆνˆˉηˆν . The right-handed neutrino mixes with the left-handed neutrino throughYνˆνˆlˆHu .The vacuum expectation values (VEVs) of the Higgs superfields, i.e.,
Hu ,Hd , η,ˉη , and S, are denoted byvu ,vd ,vη ,vˉη , andvS , respectively. Two angles are defined astanβ=vu/vd andtanβη=vˉη/vη . The explicit forms of the two Higgs doublets and three Higgs singlets are expressed as follows:η=1√2(vη+ϕ0η+iP0η),ˉη=1√2(vˉη+ϕ0ˉη+iP0ˉη),S=1√2(vS+ϕ0S+iP0S),Hu=(H+u1√2(vu+H0u+iP0u)),Hd=(1√2(vd+H0d+iP0d)H−d).
(2) The soft SUSY breaking terms of the
U(1)X SSM are expressed as follows:Lsoft=LMSSMsoft−BSS2−LSS−Tκ3S3−TλCSηˉη+ϵijTλHSHidHju−TIJXˉη˜ν∗IR˜ν∗JR+ϵijTIJνHiu˜νI∗R˜lJj−m2η|η|2−m2ˉη|ˉη|2−m2SS2−(m2˜νR)IJ˜νI∗R˜νJR−12(MSλ2˜X+2MBB′λ˜Bλ˜X)+h.c..
(3) LMSSMsoft are soft breaking terms of the MSSM. The particle content and charge assignments for theU(1)X SSM are listed in Table 2. In a previous study of ours, we showed that theU(1)X SSM is anomaly free [39]. In theU(1)X SSM,U(1)Y andU(1)X are two Abelian groups. We denote theU(1)Y charge byYY and theU(1)X charge byYX . 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.
A′Yμ andA′Xμ denote the gauge fields ofU(1)Y andU(1)X , respectively. The form of the covariant derivative of theU(1)X SSM can be expressed as follows:Dμ=∂μ−i(YY,YX)(gY,g′YXg′XY,g′X)(A′YμA′Xμ).
(4) We redefine the following expression [43, 44]:
(gY,g′YXg′XY,g′X)RT=(g1,gYX0,gX),R(A′YμA′Xμ)=(AYμAXμ).
(5) Finally, the gauge derivative of the
U(1)X SSM is transformed intoDμ=∂μ−i(YY,YX)(g1,gYX0,gX)(AYμAXμ).
(6) The term
gX denotes the gauge coupling constant for theU(1)X group;gYX is the mixed gauge coupling constant for theU(1)Y andU(1)X groups.In the
U(1)X SSM, the gauge bosonsA′Yμ ,A′Xμ , andV3μ are mixed together at the tree level. The mass matrix of gauge bosons can be found in [39]. We use two mixing angles,θW andθ′W , to obtain the mass eigenvalues of the matrix;θW is the Weinberg angle whereasθ′W is the new mixing angle. We definev=√v2u+v2d andξ=√v2η+v2ˉη . The new mixing angle is expressed as follows:sin2θ′W=12−[(gYX+gX)2−g21−g22]v2+4g2Xξ22√[(gYX+gX)2+g21+g22]2v4+8g2X[(gYX+gX)2−g21−g22]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)2−g21−g22)g2Xv2ξ2+16g2Xξ4.
(8) The mass matrix for the chargino is
m˜χ−=(M21√2g2vμ1√2g2vd1√2λHvS+μ).
(9) This matrix is diagonalized by U and V:
U∗m˜χ−V†=mdiag˜χ−.
(10) The mass matrix for the neutrino is
mν=(01√2vuYTν1√2vuYν√2vˉηYX).
(11) This matrix is diagonalized by
UV :UV,∗mνUV,†=mdiaν.
(12) Additional mass matrices are required in the calculations [38, 39].
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In this section, we focus on the theoretical study of the top-quark processes
t→cγ ,t→cg ,t→cZ , andt→ch with flavor violation under theU(1)X SSM. The relevant Feynman diagrams contributing tot→cγ ,t→cg ,t→cZ , andt→ch in theU(1)X SSM are presented in Figs. 1 and 2.In the
U(1)X SSM, the flavor violating amplitude corresponding to the decay processt→cV (V=γ,Z ) is expressed as follows:Mt→cV=εμˉuc(p′)(AVγμPL+iBVσμνqνPL+(L→R))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:
Mt→cV=∑i,j,k,nεμˉuc(p′)∫dDk(2π)Di(ALˉc˜Dkχ±nPL+ARˉc˜Dkχ±nPR)×i⧸p−⧸k−mχ±ni(ALˉχ±n˜DitPL+ARˉχ±n˜DitPR)ik2−m2˜DiiBV˜Di˜Dk×(−2kμ+qμ)i(k−q)2−m2˜Dkut(p).
(14) Here,
εμ denotes the polarization vectors of the photon and Z boson;ut anduc 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; andm˜Di ,m˜Dk , andmχ± are the mass eigenvalues from Eq. (9). Correspondingly,ALˉc˜Dχ± ,ARˉc˜Dχ± ,ALˉχ±˜Dt ,ARˉχ±˜Dt , andBV˜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=∫10dx∫102ydy1[(Ax+B(1−x))y+C(1−y)]3.
(15) Calculating the integral in this manner can greatly increase the efficiency of numerical calculations. According to Eq. (15), we obtain:
∫10dx∫102ydy{([(⧸p−⧸k)2−m2χ±n]x+(k2−m2˜Di)(1−x))y+((⧸k−⧸q)2−m2˜Dk)(1−y)}−3=∫10dx∫102ydy{[k−pxy−q(1−y)]2−[pxy+q(1−y)]2+(p2−m2χ±n)xy−m2˜Di(1−x)y+(q2−m2˜Dk)(1−y)}−3, (16) where we apply
⧸b=−⧸pxy−⧸q(1−y) ,⧸k′=⧸k+⧸b , and J =−[p2(xy−x2y2)+q2((1−y)−(1−y)2)−2p⋅qxy(1−y)−m2χ±nxy− m2˜Di(1−x)y−m2˜Dk(1−y)] to obtain the final form of the denominator in Eq. (14):∫10dx∫102ydy1(k′2−J)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
t→cγ ,t→cg , andt→cZ . Finally, we calculate the respective mode squares for the three processes.In the MSSM, the top quark decay
t→ch 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 affectst→ch decay channel. We use the following calculation related to Fig. 2(4) as an example. The amplitude can be expressed as follows:Mt→ch=−ˉuc(p′)∫dDk(2π)D1[(k−q)2−m2χ±](k2−m2χ±)[(p−k)2−m2˜Dj],⋅(ALˉcχ±˜DjPL+ARˉcχ±˜DjPR)(⧸k−⧸q+mχ±)(ALˉ˜D†jχ±tPL+ARˉ˜D†jχ±tPR)⋅(⧸k+mχ±)(ALhχ±χ±PL+ARhχ±χ±PR)ut(p).
(18) Other graphs of the
t→ch process can be calculated similarly.We use dimensional regularization to treat the divergences with
d=4−2ϵ and the limitd→4 . To obtain finite results, the divergences are canceled by the modified minimal substraction(¯MS) scheme. The terms proportional to1ϵ−γE+log(4π) are deleted. Here,γE≈0.5772 is an Euler constant.Based on the above calculations, the branching ratios of the top-quark rare decays are respectively:
Br(t→cV)=|MtcV|2√((mt+mV)2−m2c)((m+t−mV)2−m2c)32πm3tΓtotal,Br(t→ch)=|Mtch|2√((mt+mh)2−m2c)((m+t−mh)2−m2c)32πm3tΓtotal,
(19) where
Γtotal =1.42+0.19−0.15 GeV [17] is the total decay width of the top quark. -
In this section, we study the numerical results of flavor violation for the top-quark
t→cV,ch processes. According to the latest LHC data [48−52], 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, 53−55].
2. The updated experimental data show that the mass of the
Z′ boson at the 95% confidence level (CL) [56] satisfiesMZ′> 5.15 TeV. Eq. (15) yields an approximate result ofMZ′ asMZ′≈gXξ> 5.15 TeV.3. The ratio between
MZ′ and its gauge coupling constant isMZ′gX⩾ 6TeV [57, 58]. Thus,gX is restricted in the region 0<gX⩽ 0.85.4. The new angle
βη is constrained by LHC astanβη<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 = 91.188GeV ,mW = 80.385GeV ,mc = 1.27GeV , andmt = 172.69GeV . 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 of103 GeV, which is approximately the energy scale of new physics.TλC andTλH 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 of102 ∼ 104 GeV.M2Uii ,M2Qii ,M2Dii ,BS , andBμ are all of mass square dimension, and can reach the order of106 GeV2 . The dimensionless parametersλC andλH 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 theU(1)Y andU(1)X groups; it is the parameter beyond MSSM. The mass matrices of neutralino, down type squark, and up type squark all containgYX . Furthermore,gYX appears in the vertex and can enlarge its coupling constant.MBB′ is the mass of theU(1)Y andU(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 influencingvu andvd ,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. -
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(t→cγ ) and different parameters.First, we show one-dimensional diagrams of
Br(t→cγ) versusM2Q23 ,M2 in Fig. 3. The gray shaded area is the experimental limit satisfied by theBr(t→cγ) process. Fig. 3(a) showsBr(t→cγ) versusM2Q23 , withtanβ=20 ,M2=1200GeV ,gYX=0.2 , andλH=0.1 . The solid line corresponds togX = 0.3 whereas the dashed line corresponds togX = 0.6. Overall, both lines show a decreasing trend in the range of0−4×105GeV2 forM2Q23 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 thatBr(t→cγ) increases asM2Q23≥4×105GeV2 . From bottom to top in Fig. 3 (a),Br(t→cγ) increases as the value ofgX 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 thatM2Q23 is a parameter that influencesBr(t→cγ) .Figure 3. (color online) Diagrams of Br(
t→cγ ) affected by different parameters. The gray area represents a reasonable value range where Br(t→cγ ) is lower than the upper limit. The solid and dashed lines in Fig. 3(a) correspond togX=0.3 andgX=0.6 . The solid and dashed lines in Fig. 3(b) correspond totanβ=20 andtanβ=25 , asMQij=105GeV2 (i=j=1,2,3,i≠j) . Fig. 3(c) shows the differential distribution of (a) and Fig. 3(d) shows the differential distribution of (b).Figure 3 (b) represents
Br(t→cγ) versusM2 , withM2Qij=105GeV2 (i,j=1,2,3,i≠j) ,gX=0.3 ,λH=0.1 , andgYX=0.2 . The solid line corresponds totanβ=20 , whereas the dashed line corresponds totanβ=25 . There is a slight bulge in theBr(t→cγ) value atM2=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., astanβ increases,Br(t→cγ) 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 atM2 = 1400 GeV; at this point,Br(t→cγ) reaches its maximum value. The differential value is negative forM2> 1600 GeV. That is to say,Br(t→cγ) decreses, but very slightly.For a deeper exploration of the parameter space at
M2=1200GeV , we scanned some parameters randomly. In particular, in theBr(t→cγ) process, we swept some parameters as follows:5≤tanβ≤50,0.3≤gX≤0.7,0.01≤gYX≤0.5,0.1≤λH≤0.4.
(21) In Fig. 4(a), we set
λH=0.1 andgYX=0.2 to explore the effects oftanβ andgX onBr(t→cγ) . It is clear from this figure that the value ofBr(t→cγ) increases astanβ increases. Whentanβ reaches its maximum value of 50,Br(t→cγ) reaches an order of magnitude of10−4 , very close to the experimental upper limit. This indicates thattanβ is a crucial parameter. The value ofBr(t→cγ) becomes large asgX increases; however, the effect ofgX onBr(t→cγ) is small and hardly noticeable.Figure 4. (color online) (a) Effects of
tanβ andgX onBr(t→cγ) . The horizontal coordinate indicates the range5≤tanβ≤50 whereas the vertical coordinate indicates the range0.3≤gX≤0.7 . (b) Effects ofgYX andλH onBr(t→cγ) . The horizontal coordinate indicates the range0.01≤gYX≤0.5 whereas the vertical coordinate indicates0.1≤λH≤0.4 . The icons on the right side indicate the colors corresponding to the values ofBr(t→cγ) .In Fig. 4(b), we set
tanβ=20 andgX=0.3 to explore the effects ofλH andgYX onBr(t→cγ) . Note that bothλH andgYX have effects onBr(t→cγ) . The value ofBr(t→cγ) decreases with the increase ofgYX . The smaller the value ofgYX , the closer to the upper limit ofBr(t→cγ) . There is a slight increase in the value ofBr(t→cγ) withλH , but the impact ofλH is relatively small compared to that ofgYX . 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. -
In this section, we continue our exploration of the branching ratio of
t→cg with respect to certain parameters. In this case, we setM1=1200GeV ,M2=1200GeV ,M2Dii=6×106GeV2 , andM2Qii=6×106GeV2 . One-dimensional diagrams of Br(t→cg ) are shown in Fig. 5. The gray shaded portion indicates the experimental limit that is satisfied by the Br(t→cg ) process. Figure 5 (a) shows Br(t→cg ) versusM2U23 fortanβ=20 ,λH = 0.1,gX=0.3 , andgYX=0.2 ; the solid and dashed lines correspond toμ=1000GeV andμ=1100GeV , respectively. Note that Br(t→cg ) increases withM2U23 and the value approaches the experimental upper limit asM2U23 further increases. Note also that Br(t→cg ) 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 thatt→cg increases withM2U23 .Figure 5. (color online) Br(
t→cg ) diagrams affected by different parameters. The gray area represents a reasonable value range where Br(t→cg ) is lower than the upper limit. The solid and dashed lines in Fig. 5(a) correspond toμ=1000GeV andμ=1100GeV . The solid and dashed lines in Fig. 5(b) correspond totanβ=23 andtanβ=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(
t→cg ) versusλH withMQ23=105GeV2 ,μ=1000GeV ,gX=0.3 ,gYX=0.2 ,tanβ=23 (solid line), andtanβ=25 (dashed line). Note that the value of Br(t→cg ) shows a minimum atλH=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. Astanβ increases from 23 to 25, the Br(t→cg ) value also increases. However, note that the Br(t→cg ) values almost coincide atλH=0.07 . Figure 5 (d) shows the differential distribution of Fig. 5 (b). In Fig. 5 (d), the differential values are negative forλH< 0.08, and Br(t→cg ) decreases asλH becomes larger. In the range0.08≤λH<0.11 , the slope is the largest, and Br(t→cg ) changes more quickly than the others. ForλH≥ 0.11, the differential values are all positive, but the value variation is small. Moreover, Br(t→cg ) becomes larger, although the magnitude of the increase is smaller.Let us assume that
μ=1000GeV andλH=0.1 . We randomly scanned the parameterstanβ ,gX ,gYX as follows:5≤tanβ≤50,0.3≤gX≤0.7,0.01≤gYX≤0.5.
(22) In Fig. 6 (a), we set
gX=0.3 to explore the effects oftanβ andgYX onBr(t→cg) . Note that astanβ increases,Br(t→cg) gradually changes from blue to yellow, i.e., a significant increase inBr(t→cg) occurs. The larger the value oftanβ , the closer the value ofBr(t→cg) to the experimental upper limit. Note thatgYX has some minor effect on the results, and this effect is hardly noticeable. In Fig. 6 (b), we settanβ=20 to explore the effects ofgX andgYX onBr(t→cg) ; note that the larger the value ofgX , the larger the value ofBr(t→cg) . Note also that the larger the value ofgYX , the smaller the value ofBr(t→cg) .Br(t→cg) is maximized atgX=0.7 andgYX=0.01 , andBr(t→cg) becomes closer to the upper limit of the experiment. WhengYX tends to zero, the dependence of the branching ratio ongX is strong.Figure 6. (color online) (a) Effects of
tanβ andgYX onBr(t→cg) . The horizontal coordinate indicates the range5≤tanβ≤50 whereas the vertical coordinate indicates the range0.01≤gYX≤0.5 . (b) Effects ofgX andgYX onBr(t→cg) . The horizontal coordinate indicates the range0.3≤gX≤0.7 whereas the vertical coordinate indicates0.01≤gYX≤0.5 . The icons on the right side indicate the colors corresponding to the values ofBr(t→cg) . -
The experimental upper bound (
5×10−4 ) for theBr(t→cZ) process is of the same order of magnitude as that forBr(t→cγ) andBr(t→cg) . In this subsection, we analyze the effects of different parameters on theBr(t→cZ) branching ratio. In particular, we focus on the effects of the parametersM2U23 ,M2 ,gX ,gYX ,M2Dii , andM2Qii . We setM1=1200GeV andλH=0.1 . One-dimensional representations are presented in Fig. 7 whereas multi-dimensional plots are presented in Fig. 8.Figure 7. (color online) Br(
t→cZ ) diagrams affected by different parameters. The gray area indicates a reasonable value range whereBr(t→cZ) is lower than the upper limit. The solid and dashed lines in Fig. 7(a) correspond toμ=1000GeV andμ=1500GeV . The solid and dashed lines in Fig. 7(b) correspond totanβ=20 andtanβ=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 andgYX onBr(t→cZ) . The horizontal coordinate indicates the range0.3≤gX≤0.7 whereas the vertical coordinate indicates0.01≤gYX≤0.5 . (b) Effects ofM2Dii andM2Qii onBr(t→cZ) . The horizontal coordinate indicates the range106GeV2≤M2Dii≤107GeV2 whereas the vertical coordinate indicates the range106GeV2≤M2Qii≤107GeV2 . The icons on the right side indicate the colors corresponding to the values ofBr(t→cZ) .Fig. 7(a) represents
Br(t→cZ) versusM2U23 forM2=1200GeV ,tanβ=20 ,gX=0.3 ,gYX=0.2 ,M2Dii=6×106GeV2 , andM2Qii=6×106GeV2 , with the solid and dashed lines representingμ=1000GeV andμ=1500GeV , respectively. Note that both lines show an increasing trend, i.e.,Br(t→cZ) increases withM2U23 . However, the change is not significant in terms of value. Note also a decrease inBr(t→cZ) as μ increases. Both curves are shaded in gray. In Fig. 7 (b), we setμ=1000GeV ,gX=0.3 ,gYX=0.2 ,M2Dii=6×106GeV2 , andM2Qii=6×106GeV2 ; the figure showsBr(t→cZ) versusM2 fortanβ=20 (solid line) andtanβ=25 (dashed line). The two lines are convex and reach a maximum atM2=1150GeV , then exhibit a downward trend and finally level off, i.e., in the range of1000GeV≤M2≤1500GeV ,M2 has a clear influence onBr(t→cZ) . The solid and dashed lines run from bottom to top, indicating thattanβ is also a sensitive parameter forBr(t→cZ) , which increases withtanβ .Figure 7(c) shows the differential distribution of Fig. 7 (a). In Fig. 7 (c), the difference values are all positive. When
μ=1000GeV andμ=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 whenM2<1500GeV ; otherwise, they are positive.To further explore the effects of different parameters on
Br(t→cZ) , we setμ=1000GeV ,M2=1200GeV , andtanβ=20 and performed randomized scans in the following ranges:0.01≤gYX≤0.5,106GeV2≤M2Dii≤107GeV2,0.3≤gX≤0.7,106GeV2≤M2Qii≤107GeV2(i=1,2,3).
(23) In Fig. 8 (a), we set
M2Qii=6×106GeV2 ,M2Dii=6×106GeV2 to explore the effects ofgX andgYX onBr(t→cZ) . Note thatBr(t→cZ) has a minimum atgX=0.3 andgYX=0.01 . ForBr(t→cZ) , bothgX andgYX are sensitive parameters;gYX is a coupling constant that affects the strength of gauge mixing. Furthermore,gX andgYX make a new contribution toBr(t→cZ) throughZ−Z′ mixing;gX also affects significantlyBr(t→cZ) whengYX tends to a minimum.Br(t→cZ) increases withgX andgYX . 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(t→cZ)<5×10−4 .In Fig. 8 (b), we set
gX=0.3 andgYX=0.2 to explore the effects ofM2Qii andM2Dii onBr(t→cZ) . The values ofM2Qii andM2Dii are both in the range of106−107GeV2 . Fig. 8 (b) shows thatM2Dii has an extremely small effect onBr(t→cZ) . However, asM2Qii increases,Br(t→cZ) changes from yellow to blue, i.e.,Br(t→cZ) decreases weakly asM2Qii increases.In summary, regarding the
t→cZ process, the main sensitive parameters areM2 ,gX ,gYX , and the off-diagonal elementM2U23 . The diagonal elementsM2Qii (i = 1,2,3) have an effect, but they are not particularly sensitive. -
The experimental upper bound for
Br(t→ch) is1.1×10−3 . In theU(1)X SSM,Br(t→ch) can be as high as10−4 in some regions of the parameter space. Here, we setM2=1200GeV ,M2Qii=6×106GeV2 , andM2Dii=6×106GeV2 . We studied the effects ofM2Q23 , μ,M1 , andtanβ onBr(t→ch) , as shown in Fig. 9. Figure 9 (a) showsBr(t→ch) versusM2Q23 forgX=0.4 ,μ=1000GeV ,tanβ=20 ,gYX=0.2 , andλH=0.1 . The solid line representsM1=1200GeV whereas the dashed line representsM1=1600GeV . As the dashed and solid lines go from bottom to top, it can be observed thatM2 has an effect onBr(t→ch) as a sensitive parameter, andBr(t→ch) decreases asM2 increases. Note thatBr(t→ch) increases withM2Q23 almost linearly. Therefore,M2Q23 is also a parameter that notably affectsBr(t→ch) . 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(
t→ch ) diagrams affected by different parameters. The gray area indicates a reasonable value range whereBr(t→ch) is lower than the upper limit. ForgX=0.4 , the solid and dashed lines in Fig. 9(a) correspond toM1=1200GeV andM1=1600GeV . SettingM2Q23=105GeV2 , the solid and dashed lines in Fig. 9(b) correspond totanβ=20 andtanβ=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(t→ch) versus μ forM1=1200GeV ,gX=0.3 ,gYX=0.2 , andλH=0.1 , with the solid line representingtanβ=20 and the dashed line representingtanβ=25 . By analyzing the three previous processes, i.e.,t→cγ ,t→cg andt→cZ , we conclude thattanβ is one of the sensitive parameters. In thet→ch process, Fig. 9 (b) shows thattanβ is a more sensitive parameter. Whentanβ increases from 20 to 25,Br(t→ch) increases withtanβ . It implies thatBr(t→ch) reaches a minimum atμ=950GeV . Whenμ>950GeV ,Br(t→ch) 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 whenμ<1050GeV . Whenμ≥1050GeV , the tendency of these two lines to decrease becomes progressively weaker.To further explore the effect of other parameters on
Br(t→ch) , we setM1=1200GeV ,μ=1000GeV and performed a randomized scan ofgX ,gYX ,λH , andtanβ :0.01≤gYX≤0.5,0.3≤gX≤0.7,0.1≤λH≤0.4,10≤tanβ≤50.
(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 (0.3≤gX≤0.7 ) andgYX (0.01≤gYX≤0.5 ) onBr(t→ch) by settingtanβ=20 ,λH=0.1 . Fig. 10 (b) shows the effect ofgX (0.3≤gX≤0.7 ) andλH(0.1≤λH≤0.4) onBr(t→ch) by settingtanβ=20 ,gYX=0.2 . In Fig. 10 (c), we setgX=0.3 andgYX=0.2 to explore the effect oftanβ(10≤tanβ≤50) andλH(0.1≤λH≤0.4) onBr(t→ch) . Combining the three plots in Fig. 10, we can clearly see that the four parameters, i.e.,gX ,gYX ,λH , andtanβ , affectBr(t→ch) , but they do so differently. Thus, bothgX andgYX present clear effects on the numerical results.Br(t→ch) is a decreasing function ofgX andgYX . At the point they both reach their minimum value, the branching ratio of thet→ch process reaches10−4 , which is very close to the experimental upper limit. Figs. 10 (b) and (c) show thatλH also behaves very sensitively, withBr(t→ch) increasing asλH increases. Fig. 10 (c) shows that whentanβ>10 ,tanβ has a weak effect. This occurs becausetanβ 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 andgYX onBr(t→ch) . The horizontal coordinate indicates the range0.3≤gX≤0.7 whereas the vertical coordinate indicates0.01≤gYX≤0.5 . (b) Effects ofgX andλH onBr(t→ch) . The horizontal coordinate indicates the range0.3≤gX≤0.7 whereas the vertical coordinate indicates the range0.1≤λH≤0.4 . (c) Effects oftanβ andλH onBr(t→ch) . The horizontal coordinate indicates the range5≤tanβ≤50 whereas the vertical coordinate indicates the range0.1≤λH≤0.4 . The icons on the right side indicate the colors corresponding to the values ofBr(t→cZ) . -
In summary, we studied the rare decays
t→cγ,cg,cZ,ch of the top quark in theU(1)X SSM. Compared to the MSSM, in theU(1)X SSM we added three new Higgs singletsˆη,ˆˉη,ˆS and three generations of right-handed neutrinosˆνi . Its local gauge group isSU(3)C×SU(2)L×U(1)Y×U(1)X . Probing with theU(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 forBr(t→cγ),Br(t→cg),Br(t→cZ),Br(t→ch) . 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 parametersM2U23 ,M2Q23 are sensitive parameters that have a large influence on the branching ratios of thet→cγ,cg,cZ,ch processes. Among them, the influence oftanβ is the greatest, being the main parameter of thet→cγ,cg,cZ,ch processes. Concerningtanβ , it appears in the mass matrixes of almost all SUSY particles. It is a fact thattanβ affects the numerical results mainly by influencing the particle masses, the corresponding rotational matrices, and the coupling vertexes. RegardinggYX , it is a coupling constant in gauge mixing that is parameterized outside of the MSSM. In couplings where squarks appear,gX andgYX will affect the squark masses and corresponding rotation matrices, resulting in an effect onBr(t→cγ,cg,cZ,ch) . In addition, for thet→cZ process, they generate new contributions viaZ−Z′ mixing. Comparing with the data in Table 3, we can see that the maximum value ofBr(t→cV,ch) obtained in theU(1)X SSM is greater than that achieved in the B− LSSM. In particular, forBr(t→ch) , the maximum value is even four orders of magnitude higher than that of the B− LSSM. The maximum ofBr(t→cV,ch) obtained in theU(1)X SSM is already very close to the experimental upper limit, which makes our study more meaningful.Decay t→cγ t→cg t→cZ t→ch Upper limit (95%C.L.) 1.8×10−4 2×10−4 5×10−4 1.1×10−3 B−L SSM [33]5×10−7 2×10−6 4×10−7 3×10−9 U(1)X SSM1.5×10−4 5×10−5 1.41×10−4 7.04×10−5 Table 3. Upper limit (95%C.L.),
B−L SSM andU(1)X SSM bounds on the decayst→cV,ch. In conclusion, we calculated the rare top-quark decays
t→cγ,cg,cZ,ch in theU(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 [60−62]. -
The authors thank Xi Wang, Yi-Tong Wang, Xin-Xin Long for participating in the discussion of the numerical results.
