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After the discovery of the Standard-Model-like (SM-like) Higgs boson at the Large Hadron Collider (LHC) [1, 2], the high-precision measurements of the properties of the SM-like Higgs boson are the most important tasks at the High-Luminosity LHC (HL-LHC) [3, 4] and future lepton colliders [5]. In other words, all Higgs productions and their decay channels should be probed as precisely as possible at future colliders. From these data, we can verify the SM in higher-energy regions and extract new physics. Among the Higgs decay channels,
H→Zνlˉνl withl=e,μ,τ are of interest with regard to several aspects. First, if one considersZ→νlˉνl in the final state, the decay processes correspond toH→ invisible particles, which have recently studied at the LHC [6]. The search for invisible Higgs-boson decays play a key role in explaining the existence of dark matter. Furthermore, the decay channels contribute to theH→ lepton pair plus missing energy when theZ→ lepton pair is concerned in the final state. These contributions are also useful for precisely evaluating the SM backgrounds for the decay rates of theH→ lepton pair in the final state. For the above reasons, the precise decay rates forH→Zνlˉνl can provide an important tool for testing the SM at higher-energy scales and for probing new physics.One-loop contributions to
H→Zνlˉνl were computed in [7], and those forH→4 fermions were presented in [8–10]. In this study, we evaluate the one-loop contributions for the decay processesH→Zνlˉνl forl=e,μ,τ in the 't Hooft-Veltman gauge. In comparison with the previous calculations, we perform this computation with the following advantages. First, we focus on the analytical calculations for the decay channels and show a clear analytical structure for the one-loop amplitude ofH→Zνlˉνl . As a result, we can explain and extract the dominant contributions to the decay widths when these are necessary (the dominant contributions are from Z-pole diagrams or the diagrams ofH→ZZ∗→Zνlˉνl in the decay channels, as we show in later sections). Furthermore, off-shell Higgs decays are valid in our work. In addition, one can generalize the couplings of Nambu-Goldstone bosons with Higgs bosons, gauge bosons, etc., as shown in our previous work [11]. We can easily extend our results beyond the Standard Model, as Nambu-Goldstone bosons play the same role as the changed Higgs in the extensions of the Standard Model Higgs sector. Last but not least, the signals ofH→Zνlˉνl through Higgs productions at future lepton colliders are studied in our work. In further detail, one-loop form factors are expressed in terms of scalar one-loop Passarino-Veltman functions (called as PV-functions hereafter) in the standard notations ofLoopTools . As a result, one can evaluate the decay rates numerically by using the package. Moreover, the signals ofH→Zνlˉνl through Higgs productions at future lepton colliders, for instance, the processese−e+→ZH∗→Z(Zνlˉνl) with initial beam polarizations, are generated. The Standard Model backgrounds, such ase−e+→νlˉνlZZ , are also included in this analysis. In phenomenological results, we find that one-loop corrections make contributions of approximately 10% to the decay rates. These are sizeable contributions and should be taken into account at future colliders. We show that the signalsH→Zνlˉνl are clearly visible at the center-of-mass energy√s=250 GeV and are difficult to probe in higher-energy regions owing to the dominant backgrounds.The remainder of this paper is organized as follows. In section II, we present the calculations for
H→Zνlˉνl in detail. We then show phenomenological results for the computations. The decay rates for on-shell and off-shell Higgs decay modes are studied, with the unpolarized and longitudinally polarized Z bosons in the final states. The signals ofH→Zνlˉνl via the Higgs productions at future lepton colliders are also presented in this section. Conclusions are presented in section IV. In the appendies, we first summarize all the tensor reduction formulas for one-loop integrals that appear in this work. Numerical checks for the calculations are presented. All self-energy and counter-terms for the decay processes are presented in detail. One-loop Feynman diagrams in the 't Hooft-Veltman gauge for these decay channels are shown in Appendix E. -
We present the calculations for
H(pH)→Z(q1)νl(q2)ˉνl(q3) in detail. For these computations, we are working in the 't Hooft-Veltman gauge. Within the SM framework, all Feynman diagrams can be grouped into several classifications, as shown in Appendix E. In groupG0 , we have tree Feynman diagrams contributing to the decay processes. For groupG1 , we include all one-loop Feynman diagrams correcting to the vertexZνlˉνl . We then list all Z-pole Feynman diagrams in groupG2 and non Z-pole diagrams in groupG3 . The counterterm diagrams for this decay channels are classified into groupG4 .In general, the amplitude for
H(pH)→Z(q1)νl(q2)ˉνl(q3) can be decomposed by the following Lorentz structure:AH→Zνlˉνl={F00gμν+F12qν1qμ2+F13qν1qμ3}×[ˉu(q2)γνPLv(q3)]ε∗μ(q1).
(1) Here,
F00 ,F12 , andF13 are form factors including both tree-level and one-loop diagram contributions. The form factors are functions of the Mandelstam invariants, such assij=(qi+qj)2 fori≠j=1,2,3 and mass-squared in one-loop diagrams. One also verifies thats12+s13+s23=M2H+M2Z . In Eq. (1), projection operatorPL=(1−γ5)/2 is taken into account, and the termε∗μ(q1) is the polarization vector of the final Z boson. Our computations can be summarized as follows. We first write the Feynman amplitude for all the diagrams mentioned above. By usingPackage−X [12], all Dirac traces and Lorentz contractions in d dimensions are performed. The amplitudes are then casted into tensor one-loop integrals. The tensor integrals are next reduced to scalar PV-functions [13, 14]. All the relevant tensor reduction formulas are presented in Appendix A. The PV-functions can be evaluated numerically by usingLoopTools [15].All the form factors are calculated from Feynman diagrams in the 't Hooft-Veltman gauge, and their expressions are presented in this section. For the tree-level diagram, the form factor is given as
F(G0)00(s12,s13,s23)=2παs2Wc3WMWs23−M2Z+iΓZMZ.
(2) Here,
sW(cW) represents the sine (cosine) of the Weinberg angle, andΓZ represents the decay width of the Z boson.At the one-loop level, all form factors take form of
Fij=∑G={G1,⋯,G4}F(G)ij(s12,s13,s23), for ij={00,12,13}.
(3) Here,
{G1,G2,⋯,G4}={group 1,group 2,⋯,group 4} correspond to the groups of Feynman diagrams in Appendix E. By considering each group of Feynman diagrams, analytical results for all the form factors are obtained, and they are presented in the following paragraphs. Taking the attribution from groupG1 , we have one-loop form factors accordingly:F(G1)00(s12,s13,s23)=−α28s4Wc5WMWs23−M2Z+iΓZMZ{−8c4WB0(s23,M2W,M2W)−2[c2W(4s2W−2)+1]B0(s23,0,0)−8c4W[2C00−s23(C1+C2)](0,s23,0,0,M2W,M2W)−4c2W(2s2W−1)[M2WC0+s23C2−2C00]×(s23,0,0,0,0,M2W)+[4C00−2s23C2−2M2ZC0](s23,0,0,0,0,M2Z)+(2c2W+1)}, (4) F(G1)ij(s12,s13,s23)=0,forij={12,13}.
(5) For group
G2 of the Feynman diagrams, the form factors can be divided into the fermion and boson parts as follows:F(G2)00(s12,s13,s23)=α224s4Wc7WMW1(s23−M2Z+iΓZMZ)2[∑fNCfF(G2)00,f+F(G2)00,b]. (6) Here,
NCf represents the color number, which is 3 for quarks and 1 for leptons. For the fermion contributions, we take the top quark loop as an example. The analytical results are as follows:F(G2)00,f=2c2WM2W[8s2W(4s2W−3)+9][A0(m2t)+s23B1(s23,m2t,m2t)−2B00(s23,m2t,m2t)]+2m2tc2W{9M2W−2c2W(M2Z−s23)[4s2W(4s2W−3)+9]}B0(s23,m2t,m2t)+m2tc4W(s23−M2Z){36m2t+[8s2W(4s2W−3)+9](s12+s13)}C0(M2Z,s23,M2H,m2t,m2t,m2t)−m2tc4W(M2Z−s23){(M2H+5M2Z−s23)[8s2W(4s2W−3)+9]+8s2W(3−4s2W)(s12+s13)}C1(M2Z,s23,M2H,m2t,m2t,m2t)−2m2tc4W(M2Z−s23){9M2H+[8s2W(4s2W−3)+9](s12+s13)}C2(M2Z,s23,M2H,m2t,m2t,m2t)+8m2tc4W(M2Z−s23)[8s2W(4s2W−3)+9]C00(M2Z,s23,M2H,m2t,m2t,m2t).
(7) The contribution from the boson part is expressed as
F(G2)00,b=8c6WM2Ws23−6M2Wc2W[3c2W(4c2W−1)+s2W]A0(M2W)−3M2Wc2W[A0(M2Z)+A0(M2H)]+32c4WM2H(M2Z−s23)B0(M2H,M2Z,M2Z)+12M2Ws4Wc4W(M2Z−s23)B0(M2Z,M2W,M2W)+3c4W(M2Z−s23)[c4W(M2H+24M2W)−2M2Hs2Wc2W+M2Hs4W]B0(M2H,M2W,M2W)+12M2Wc2W{(2M2W+5s23)c4W−2M2Ws4W+(M2Z−s23)[s4W−2c2W(c2W+1)]c2W}B0(s23,M2W,M2W)+6M2Wc2W(M2Z−s23)[B0(M2Z,M2H,M2Z)+B0(s23,M2H,M2Z)]−12M4WB0(s23,M2H,M2Z)−4M2Wc2W[40s2W(4s2W−3)+63]B00(s23,0,0)+12M2Wc2WB00(s23,M2H,M2Z)+12M2Wc2W(9c4W−2s2Wc2W+s4W)B00(s23,M2W,M2W)+92c4WM2H(M2Z−s23)B0(M2H,M2H,M2H)+2M2Wc2Ws23[40s2W(4s2W−3)+63]B1(s23,0,0)+24c6WM2Ws23B1(s23,M2W,M2W)−12M2Wc6W(M2Z−s23)[4M2Z+c2W(s12+s13)]C1(M2Z,s23,M2H,M2W,M2W,M2W)+24M2Wc6W(M2Z−s23)(−c2WM2H−s12−s13)C2(M2Z,s23,M2H,M2W,M2W,M2W)−12M2Wc4W(M2Z−s23){2c4W[2M2W+5M2Z−2(s12+s13)]−(M2H+2M2W)s4W+s2Wc2W(M2H+2M2W+s12+s13)}C0(M2Z,s23,M2H,M2W,M2W,M2W)−12c4W(M2Z−s23)[s2W(s2W−2c2W)(M2H+2M2W)+(M2H+18M2W)c4W]C00(M2Z,s23,M2H,M2W,M2W,M2W)+18M2Hc2W(s23−M2Z)[−M2WC0+c2WC00](M2H,s23,M2Z,M2H,M2H,M2Z)+(M2Z−s23)[12M4WC0−6c2W(M2Hc2W+2M2W)C00](M2Z,M2H,s23,M2H,M2Z,M2Z).
(8) Other one-loop form factors follow the same convention:
F(G2)12(s12,s13,s23)=F(G2)13(s13,s12,s23)=−α212s4Wc5WMW1s23−M2Z+iΓZMZ[∑fNCfF(G2)12,f+F(G2)12,b].
(9) Each part in the above equation has the form of (we take the top quark loop as an example for fermion contributions)
F(G2)12,f=9m2tc2WC1(M2Z,s23,M2H,m2t,m2t,m2t)+m2tc2W[8s2W(4s2W−3)+9][C0+4(C2+C12+C22)](M2Z,s23,M2H,m2t,m2t,m2t)
(10) and
F(G2)12,b=−12c2WM2W[(5c4W−2c2Ws2W+s4W)C0+C1](M2Z,s23,M2H,M2W,M2W,M2W)+3c2WM2H[C12(M2Z,M2H,s23,M2H,M2Z,M2Z)−3(C1+C11+C12)(M2H,s23,M2Z,M2H,M2H,M2Z)]+6M2W[C1+C2+C12](M2Z,M2H,s23,M2H,M2Z,M2Z)−6c2W[s2W(s2W−2c2W)(M2H+2M2W)+c4W(M2H+18M2W)]×[C2+C12+C22](M2Z,s23,M2H,M2W,M2W,M2W).
(11) We change to the contributions of all Feynman diagrams in group
G3 . For this group, there are no Z-pole diagrams including in one-loop form factors. However, we have one-loop box diagrams. There are a triple gauge boson vertex and the propagator of leptons or two propagators of leptons in one-loop box diagrams; hence, we have tensor box integrals, for which the highest rank isR=2 in the amplitude. It is explained that the corresponding form factors are expressed in terms of the PV-functions C- and up toD33 -coefficients.F(G3)00=α2MW4s4Wc5W{2c4W[(2s2W−1)C0(M2Z,0,s13,0,0,M2W)+(3c2W+1)C0(0,s23,0,0,M2W,M2W)+C2(0,M2H,s13,0,M2W,M2W)+C2(0,M2H,s12,0,M2W,M2W)]+C0(M2Z,0,s13,0,0,M2Z)+C2(0,M2H,s13,0,M2Z,M2Z)+C2(0,M2H,s12,0,M2Z,M2Z)+8c6W[D00(s12,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)+D00(s13,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)]−2c6W[(2M2Z+s12)D1(s12,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)+(2M2Z+s13)D1(s13,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)]+c4W{[2c2W(3M2H−2s23−3s13)+s2W(s13−M2H)]D3(s13,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)+[s2W(s12−M2H)+2c2W(3M2H−2s23−3s12)]D3(s12,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)}+c4W(3c2W+1)[(M2W−s12)D0(s12,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)+(M2W−s13)D0(s13,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)]+(s12−M2Z)[2c4W(1−2s2W)D2(M2Z,s12,M2H,s13,0,0,0,0,M2W,M2W)−D2(M2Z,s12,M2H,s13,0,0,0,0,M2Z,M2Z)]+s2Wc4W[(M2Z−s13)D2(s13,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)+(M2Z−s12)D2(s12,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)]+(s23+s12)[2c4W(2s2W−1)D3(M2Z,s12,M2H,s13,0,0,0,0,M2W,M2W)+D3(M2Z,s12,M2H,s13,0,0,0,0,M2Z,M2Z)]+[M2ZD0+s12D1−2D00](M2Z,s12,M2H,s13,0,0,0,0,M2Z,M2Z)+2c4W(1−2s2W)[2D00−s12D1−M2WD0](M2Z,s12,M2H,s13,0,0,0,0,M2W,M2W)}.
(12) In addition, we have other form factors, which are expressed as follows:
F(G3)12=α2MW2s4Wc5W{[D2+D12+D23](M2Z,s12,M2H,s13,0,0,0,0,M2Z,M2Z)−4c6W[D3+D13](s13,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)−2c4W(1−2s2W)[D2+D12+D23](M2Z,s12,M2H,s13,0,0,0,0,M2W,M2W)+2c4W[2c2W(D11+D12)+(s2W−c2W)D2](s12,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)},
(13) F(G3)13=α2MW2s4Wc5W{−[D13+D33](M2Z,s12,M2H,s13,0,0,0,0,M2Z,M2Z)−4c6W[D3+D13](s12,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)+2c4W(1−2s2W)[D13+D33](M2Z,s12,M2H,s13,0,0,0,0,M2W,M2W)+2c4W[2c2W(D11+D12)+(s2W−c2W)D2](s13,M2Z,s23,0,0,M2H,0,M2W,M2W,M2W)}.
(14) It is stress that one has the following relation:
F(G3)12(s12,s13,s23)=F(G3)13(s13,s12,s23).
(15) If we apply several transformations for box-functions, we can confirm the relation. The transformations for box-functions are not presented in this subsection. Instead, we verify the relation via numerical checks. One finds that two representations for
F(G3)13 in Eqs. (14) and (16) agree well up to the last digit at several sampling points.With all the form factors, the decay rates can be evaluated as follows:
ΓH→Zνl¯νl=1256π3M3HM2Z(MH−MZ)2∫4m2νlds23smax12∫smin12ds12{(M2Z(2s23−M2H)+s12s13)[|F(G0)00|2+2Re(F(G0),∗00⋅4∑i=1F(Gi)00)]+(M2HM2Z−s12s13)[(M2Z−s12)Re(F(G0),∗00⋅4∑i=1F(Gi)12)+(s12↔s13)]}. (16) Here,
smax,min12=12{M2H+M2Z−s23±√(M2H+M2Z−s23)2−4M2HM2Z}.
(17) The polarized Z boson case is considered next. The longitudinal polarization vectors for Z bosons are defined in the rest frame of the Higgs boson:
εμ(q1,λ=0)=4M2H∗q1,μ−(s23+M2Z)pH,μMZ√λ(s23,4M2H∗,M2Z).
(18) Here, the off-shell Higgs mass is given by
p2H=M2H∗≠M2H . The Kallën function is defined asλ(x,y,z)=(x−y−z)2−4yz . We then arrive atΓH→ZLνl¯νl=1256π3M3H∗M2Z(MH∗−MZ)2∫4m2νlds23smax12∫smin12ds12(s23−4M2H∗+M2Z)(s12s13−M2ZM2H∗)[s23−M2Z−4M2H∗]2−16M2ZM2H∗
×{(s23−4M2H∗+M2Z)[|F(G0)00|2+2Re(F(G0),∗00×4∑i=1F(Gi)00)]+[(s223−M4Z+4M2H∗M2Z)+(s23−4M2H∗+M2Z)s12]×Re(F(G0),∗004∑i=1F(Gi)12)+(s12↔s13)}.
(19) Here,
smin, max12 are obtained as in Eq. (17), in whichMH is replaced with the off-shell Higgs massMH∗ .In the next section, we present phenomenological results for the decay processes. Before generating the data, numerical checks for the calculations are performed. The
UV - finiteness andμ2 -independence of the results are verified. Numerical results for these checks are presented in Appendix B. One finds that the results have good stability over 14 digits. -
For the phenomenological results, we use the following input parameters:
MZ=91.1876 GeV,ΓZ=2.4952 GeV,MW=80.379 GeV,ΓW=2.085 GeV,MH=125.1 GeV, andΓH=4.07⋅10−3 GeV. The lepton masses are given asme=0.00052 GeV,mμ=0.10566 GeV, andmτ=1.77686 GeV. The quark masses aremu=0.00216 GeV,md=0.0048 GeV,mc=1.27 GeV,ms=0.93 GeV,mt=173.0 GeV, andmb=4.18 GeV. We work in the so-calledGμ -scheme, in which the Fermi constant is taken asGμ=1.16638⋅10−5 GeV−2 and the electroweak coupling can be calculated appropriately as follows:α=√2/πGμM2W(1−M2W/M2Z)=1/132.184.
(20) We present the phenomenological results in the following subsections. We first discuss the decay rates for the on-shell Higgs decay
H→Zνlˉνl . In Table 1, the decay rates for on-shell Higgs decay toZνeˉνe are presented. In the first column, the cuts for the invariant mass of the final neutrino-pair are applied. The decay rates for the unpolarized case of the final Z boson are presented in the second column. The results in the last column are the decay rates corresponding to the longitudinal polarization of the final Z boson. Furthermore, in this table, the result for the tree level (full one-loop) decay width is presented on the first (second) line. When we consider all generation of neutrinos, one should add to data by overall factor 3. The one-loop corrections make contributions of ~10% to the tree-level decay rates. We note that one-loop corrections are evaluated as follows:mcutνeˉνe /GeVΓH→Zνeˉνe /keVΓH→ZLνeˉνe /keV0 5.8177 2.2872 6.4174 2.5061 5 5.7014 2.1736 6.2902 2.3818 10 5.3401 1.8515 5.8943 2.0293 20 3.7362 0.8389 4.1305 0.9201 Table 1. Decay rates for on-shell Higgs decay into
Zνeˉνe . The first (second) line corresponds to the tree level (full one-loop) decay width.δ[%]=ΓFull−ΓTreeΓTree×100%.
(21) We next consider the off-shell Higgs decay to
Zνeˉνe . The numerical results are presented in Table 2. In this case, we only consider the unpolarized Z boson in the final state. In the first column, the off-shell Higgs massMH∗ is shown in the range of 200 to 500 GeV. The off-shell decay widths are presented in the second column, where the first (second) line is for the tree-level (full one-loop) decay rate. It is worth mentioning that the results for the off-shell Higgs decays agree well with the decay rates in [16]. This indicates that the main contributions to the decay rates are from the values around the peak of the Z-pole decay toνlˉνl (this explanation will be confirmed later).MH∗ /GeVΓH→Zνeˉνe /GeV200 0.0478 0.0541 300 0.3383 0.3789 400 1.0124 1.1418 500 2.2101 2.4865 Table 2. Decay rates for off-shell Higgs decay into
Zνeˉνe . The first (second) line corresponds to the tree level (full one-loop) decay width.For the experimental analyses, differential decay rates with respect to the invariant mass of the neutrino-pair are of interest. These correspond to the decay rates of Higgs decay to Z plus missing energy. Thus, the data provide the precise backgrounds for the signals of Higgs decay to the lepton-pair when the
Z→ lepton-pair is taken into account. This also contributes to the signals ofH→ invisible particles if the decay of the final Z boson to the neutrino-pair is considered. In Fig. 1, we show for the differential decay rates with respect tomνlˉνl for the case of the unpolarized Z final state. We apply a cut ofmcutνlˉνl≥5 GeV for this study. In the left panel, the triangle points are for the tree-level decay widths, and the rectangle points are for the full one-loop decay widths. In the right panel, the electroweak corrections are plotted. One finds that the corrections make contributions in the range of 9.4% to 10.8%. In Fig. 2, the same distributions are shown in the longitudinal polarization of the final Z boson. We use the same convention as the previous case. We find that the corrections make contributions in the range of 9.4% to 9.8%.Figure 1. Differential decay rates (left panel) and corrections (right panel) with respect to
mνlˉνl for the unpolarized Z boson case. In the left panel, the triangle points are for the tree-level decay widths, and the rectangle points are for the full one-loop decay widths. In the right panel, the electroweak corrections are shown as the rectangle points.Figure 2. Differential decay rates (left panel) and corrections (right panel) with respect to
mνlˉνl in the longitudinal polarization case for the Z boson. In the left panel, the triangle points are for the tree-level decay widths, and the rectangle points are for the full one-loop decay widths. In the right panel, the electroweak corrections are plotted as the rectangle points.The differential decay rates with respect to
mνlˉνl for the off-shell Higgs case atM∗H=500 GeV are presented. In Fig. 3, we observe a peak atmνlˉνl=MZ , which corresponds toZ→νlˉνl . The decay rates exhibit high values around the peak and decrease rapidly beyond the peak. The corrections are from 10% to 25% throughout the range ofmνlˉνl . We note that a cut ofmcutνlˉνl≥5 GeV is employed in the distribution. From the distribution, the main contributions to the off-shell Higgs decay rates come from the corresponding values around the Z-peak, indicating that the off-shell Higgs decay rates in this work agree well with the results in [16]. This supports the previous conclusion regarding the data in Table 2. Additionally, for the entire range of the Higgs mass, we check numerically that the dominant contributions to the decay rates come from the Z-pole diagrams or the diagrams ofH→ZZ∗→Zνlˉνl (from groups 1 and 2) in these decay channels. The same conclusion was drawn in [17].Figure 3. Differential decay rates (left panel) and corrections (right panel) with respect to
mνlˉνl for the off-shell Higgs case. In the left panel, tree-level decay widths are plotted as triangle points, and full one-loop decay widths are shown as rectangle points. In the right panel, the electroweak corrections are presented as the rectangle points.We turn our attention to analyze the signals
H→Zνlˉνl through Higgs productions at future lepton colliders, such ase−e+→ZH∗→Z(Zνlˉνl) , with the initial beam polarizations. The differential cross section with resprect toMH∗ is given as [16]dσe−e+→ZH∗→Z(Zνlˉνl)(√s)dMH∗=(2M2H∗)σe−e+→ZH∗(√s,MH∗)[(M2H∗−M2H)2+Γ2HM2H]×ΓH∗→ZZ(MH∗)π.
(22) The Feynman diagram is shown in Fig. 4. The cross section for
e−e+→ZH∗ can be found in [16]. The total cross section for these processes can be computed as follows:Figure 4. Feynman diagram for the processes
e−e+→Z(Zνl¯νl) at the ILC with the blob representing one-loop corrections toH→Zνl¯νl .σe−e+→ZH∗→Z(Zνlˉνl)=√s−MZ∫MZdMH∗dσe−e+→ZH∗→Z(Zνlˉνl)(√s)dMH∗.
(23) In Table 3, we present the cross sections for the signals of Higgs decay to
Zνlˉνl viae−e+→ZH∗→Z(Zνlˉνl) with the initial beam polarizations (taking all three generations of neutrinos in the data). The second (third) column corresponds to the signals at tree level (full correction) cross sections. The last column is for the SM backgrounds, which are the tree level of the reactionse−e+→ZZνlˉνl . The background processes are generated by using GRACE [18]. For each center-of-mass energy, the first line corresponds to the LR case, and the second line corresponds to the RL polarization case. We show that the signalsH→Zνlˉνl can be probed at the center-of-mass energy√s=250 GeV and that they are difficult to measure in higher-energy regions owing to the dominant backgrounds.√s/GeV σTreesig/fb σFullsig/fb σbkg/fb 250 2.43873 2.69398 0.00309 1.58487 1.74649 0.00016 500 0.68498 0.75668 16.7839 0.44404 0.48932 1.33409 1000 0.26879 0.29692 164.146 0.17424 0.19201 1.16635 Table 3. Total cross section of
e−e+→Z(Zνl¯νl) . The first line presents results for theLR ofe−e+ , and the second line presents results for theRL ofe−e+ . Tree generations for neutrinos are taken into the results.In Fig. 5, we plot the distributions for the cross section as functions of
MH∗ at the center-of-mass energy of√s=500 GeV, considering the initial polarization cases fore−e+ . Cross sections for the LR and RL cases are shown in the left and right panels, respectively. For the signal cross sections, tree-level cross sections are plotted as dashed lines, and full one-loop cross sections are presented as solid lines. The SM backgrounds are shown as dotted points. The off-shell Higgs massMH∗ is varied fromMZ to√s−MZ . It is observed that the cross sections are dominant around the on-shell Higgs massMH∗∼125 GeV. It is well-known that we have another peak that is around the ZH threshold (∼MZ+MH=215 GeV). Owing to the small value of the total decay width of the Higgs boson, the on-shell Higgs mass peak becomes more visible than the later one. In the off-shell Higgs mass region, the cross sections are far smaller (by approximately 2 orders of magnitude) than those around the on-shell Higgs mass peak. We observe that the signals are clearly visible at the on-shell Higgs massMH∗=125 GeV. In the off-shell Higgs mass region, the SM backgrounds are far larger than the signals. These large contributions are mainly attributed to the dominant of t-channel diagrams appear in the background processes.Figure 5. Off-shell Higgs decay rates as a function of
MH∗ at the center-of-mass energy of√s=500 GeV. Three generations for neutrinos are included in the results. Cross sections for the LR and RL cases are shown in the left and right panels, respectively. For the signal cross sections, tree-level cross sections are shown as dashed lines, and full one-loop cross sections are shown as solid lines. The dotted points indicate the SM backgrounds.Full one-loop electroweak corrections to the process
e−e+→ZH and the SM background processes with the initial beam polarizations should be taken into account for the above analyses. The corrections can be generated by using the program [18], and they were recently studied in [19]. Furthermore, by generalizing the couplings of Nambu-Goldstone bosons to Higgs bosons, gauge bosons, etc., as in [11], we can extend our work beyond the SM. These topics will be addressed in our future works. -
Analytical results for one-loop contributions to the decay processes
H→Zνlˉνl forl=e,μ,τ in the 't Hooft-Veltman gauge were presented. The calculations were performed within the Standard Model framework. One-loop form factors are expressed in terms of the Passarino-Veltman functions in the standard conventions ofLoopTools , for which the decay rates can be evaluated numerically. We also studied the signals ofH→Zνlˉνl through Higgs productions at future lepton colliders, such ase−e+→ZH∗→Z(Zνlˉνl) , with the initial beam polarizations. The SM background processes for this analysis were taken into account. Phenomenological results indicated that one-loop corrections make contributions of approximately 10% to the decay rates. These are sizeable contributions and should be taken into account at future colliders. We show that the signalsH→Zνlˉνl are clearly visible at the center-of-mass energy√s=250 GeV and are difficult to probe in higher-energy regions owing to the dominant backgrounds. -
We present all the tensor one-loop reduction formulas applied for this calculation in this appendix. The technique is based on the method in [13]. Tensor one-loop one-, two-, three-, and four-point integrals with rank R are defined as follows:
{A;B;C;D}μ1μ2⋯μR=(μ2)2−d/2∫ddk(2π)dkμ1kμ2⋯kμR{P1;P1P2;P1P2P3;P1P2P3P4}.
Here, the inverse Feynman propagators
Pj (j=1,2,⋯,4 ) are given byPj=(k+qj)2−m2j+iρ.
In this definition, the momenta
qj=j∑i=1pi withpi for the external momenta are taken into account, andmj denotes the internal masses in the loops. The internal masses can be real and complex in the calculation. Following the dimensional regularization method, one-loop integrals are peformed in space-time dimensiond=4−2ε . The renormalization scale is introduced asμ2 in this definition, which helps to track the correct dimension of the integrals in space-time dimension d. If the numerators of one-loop integrands in Eq. (A1) are 1, we have the corresponding scalar one-loop functions (denoted asA0 ,B0 ,C0 , andD0 ). All the reduction formulas for one-loop tensor integrals up to rankR=3 are presented in the following paragraphs. In detail, we have the following reduction expressions for one-loop two-point tensor integrals:Aμ=0,
Aμν=gμνA00,
Aμνρ=0,
Bμ=qμB1,
Bμν=gμνB00+qμqνB11,
Bμνρ={g,q}μνρB001+qμqνqρB111,
The reduction formulas for the one-loop tensor three-point integrals are as follows:
Cμ=qμ1C1+qμ2C2=2∑i=1qμiCi,
Cμν=gμνC00+2∑i,j=1qμiqνjCij,
Cμνρ=2∑i=1{g,qi}μνρC00i+2∑i,j,k=1qμiqνjqρkCijk,
For four-point functions, we have the following reduction expressions:
Dμ=qμ1D1+qμ2D2+qμ3D3=3∑i=1qμiDi,
Dμν=gμνD00+3∑i,j=1qμiqνjDij,
Dμνρ=3∑i=1{g,qi}μνρD00i+3∑i,j,k=1qμiqνjqρkDijk.
We have already used the short notation [13]
{g,qi}μνρ , which is written explicitly as follows:{g,qi}μνρ=gμνqρi+gνρqμi+gμρqνi . All the scalar coefficientsA00,B1,⋯,D333 on the right hand sides of the above reduction formulas are Passarino-Veltman functions [13]. These functions were implemented intoLoopTools [15] for numerical computations. -
With all the neccessary one-loop form factors, we check the computation numerically. We find that
F00 contains theUV -divergence by taking the one-loop counterterm, which corresponds toF(G4)00 . The analytical expressions forF(G4)00 are given in (54), and all the renormalization constants are presented in Appendix D.In Table B1, the checking for the UV-finiteness of the results at a random point in the phase space is presented. Varying the
CUV parameters indicates that the amplitudes have good stability over 14 digits.(CUV,μ2) 2Re {M∗TreeM1-Loop} (0,1) −0.0015130298318390845−0.001513160592122863i (102,105) −0.0015130298318393881−0.001513160592122863i (104,1010) −0.0015130298318233315−0.001513160592122863i Table B1. Checking for the UV-finiteness of the results at an random point in the phase space. The amplitude
M1-Loop is included all one-loop diagrams and counterterm diagrams. -
Each self energy is presented in terms of the PV-functions in the 't Hooft-Veltman gauge.
Self energy A-A
Self-energy photon-photon functions are casted into two fermion and contributions as follows:
ΠAA(q2)=ΠAAT,b(q2)+ΠAAT,f(q2).
The parts are given as follows:
ΠAAT,b(q2)=e2(4π)2{(4M2W+3q2)B0(q2,M2W,M2W)−2(d−2)A0(M2W)}, ΠAAT,f(q2)=e2(4π)2{−2∑fNCfQ2f[4B00(q2,m2f,m2f)+q2B0(q2,m2f,m2f)−2A0(m2f)]}.
Self energy Z-A
Self-energy functions for Z-A mixing are written in the previous form. The parts are given as follows:
ΠZAT,b(q2)=e2(32π2)(d−1)sWcW{2(d−2)[c2W(2d−3)−s2W]A0(M2W)−{4M2W[c2W(3d−4)+(d−2)s2W]+q2[c2W(6d−5)+s2W]}B0(q2,M2W,M2W)},
ΠZAT,f(q2)=e2(32π2)sWcW{2∑fNCfQf(2s2WQf−T3f)[4B00(q2,m2f,m2f)+q2B0(q2,m2f,m2f)−2A0(m2f)]}.
Self energy Z-Z
Self energy functions for Z-Z are presented in terms of scalar one-loop integrals, as follows:
ΠZZT,b(q2)=e2(64π2)(d−1)q2s2Wc4W{2q2c2W(2−d)[c4W(4d−7)+s2W(s2W−2c2W)]A0(M2W)+c2W[M2H−M2Z−(d−2)q2]A0(M2H)+c2W[M2Z−M2H−(d−2)q2]A0(M2Z)+{2q2[c2W(M2H+M2Z)−2M2W(d−1)]−c2W[(M2H−M2Z)2+q4]}B0(q2,M2H,M2Z)+{4M2W[(3c4W−s4W)(2d−3)−2c2Ws2W]+q2[3c4W(4d−3)+(2c2W−s2W)s2W]}c2Wq2B0(q2,M2W,M2W)},
ΠZZT,f(q2)=e2(16π2)s2Wc2W∑fNCf{[(T3f)2(2m2f−q2)+2q2Qfs2W(T3f−Qfs2W)]B0(q2,m2f,m2f)+[4Qfs2W(T3f−Qfs2W)−2(T3f)2][2B00(q2,m2f,m2f)−A0(m2f)]}.
Self energy W-W
Self-energy functions for W-W are presented correspondingly:
ΠWWT,b(q2)=e2(64π2)(d−1)q2s2Wc2W{c2W[M2H−M2W−(d−2)q2]A0(M2H)+c2W[2M2W−M2H−M2Z−2q2(2d−3)(d−2)]A0(M2W)+c2W[4c2W(d−2)+1]×[M2Z−M2W−(d−2)q2]A0(M2Z)+{c2Wq4[4c2W(3d−2)−1]−c2W(M2W−M2Z)2[4c2W(d−2)+1]+2q2M2W[2c4W(3d−5)−2s4W(d−1)+3c2W(2d−3)+1]}B0(q2,M2W,M2Z)+c2W{2q2[(3−2d)M2W+M2H]−(M2H−M2W)2−q4}B0(q2,M2H,M2W)+4c2Ws2W{M2W(2q2−M2W)(d−2)+(3d−2)q4}B0(q2,0,M2W)},
ΠWWT,f(q2)=e2(64π2)s2Wc2W{2c2W∑doubletNCf[(m2f+m2f′−q2)B0(q2,m2f′,m2f)−4B00(q2,m2f′,m2f)+A0(m2f)+A0(m2f′)]}.
Self energy H-H
The expressions for self-energy H-H are as follows:
ΠHHb(q2)=e2(128π2)M2Ws2Wc4W{3M2Hc4W[3M2HB0(q2,M2H,M2H)+A0(M2H)]+2c4W{4M2W[M2W(d−1)−q2]+M4H}B0(q2,M2W,M2W)+{c4WM4H+4M2W[M2W(d−1)−c2Wq2]}B0(q2,M2Z,M2Z)+2c4W[2M2W(d−1)+M2H]A0(M2W)+[c4WM2H+2M2Wc2W(d−1)]A0(M2Z)},
ΠHHf(q2)=e2(128π2)M2Ws2Wc4W{4c4W∑fNCfm2f[(q2−4m2f)B0(q2,m2f,m2f)−2A0(m2f)]}−3δTv.
Here,
v=246 GeV is the vacuum expectation value.Tadpole
The tadpole is calculated as follows:
Tloopb=e(64π2)MWsWc2W{[c2WM2H+2M2W(d−1)]A0(M2Z)+2c2W[2M2W(d−1)+M2H]A0(M2W)+3M2Hc2WA0(M2H)},
Tloopf=−8ec2W(64π2)MWsWc2W∑fNCfm2fA0(m2f).
We then have
δT=−(Tloopb+Tloopf).
In the case of a neutrino, explicit expressions for the self-energy functions
νl -νl are as follows:Σνl(q2)=Kνlγ(q2)q̸+Kνl5γ(q2)q̸γ5
where
Kνlγ(q2)=−Kνl5γ(q2)=−e2128π2s2Wc2W[(2c2W+1)+2B1(q2,0,M2Z)+2c2W∑l(m2lM2W+2)B1(q2,m2l,M2W)].
-
The counterterms of the decay process
H→Zνl¯νl are written asF(G4)00=F(G4)00,Zνl¯νl+F(G4)00,HZZ+F(G4)00,Zχ3+F(G4)00,ZZ,
where
F(G4)00,Zνl¯νl=2παMWs2Wc3W1s−M2Z+iΓZMZ×(δY+δG2+δG3+δZ1/2ZZ+2δZ1/2νlL),
F(G4)00,HZZ=2παMWs2Wc3W1s−M2Z+iΓZMZ×(δY+δG2+δG3+δGZ+2δZ1/2ZZ+δZ1/2H),
F(G4)00,ZZ=2παMWs2Wc3W1(s−M2Z+iΓZMZ)2×(2M2ZδGZ+(M2Z−s)δZ1/2ZZ).
The contribution of
F(G4)00,Zχ3 vanishes owing to the Dirac equation.The renormalization constants are given as follows:
δY=−δZ1/2AA+sWcWδZ1/2ZA,
δG2=δGZ−δH,δG3=δGZ−δGW,
δH=δM2Z−δM2W2(M2Z−M2W),δGZ=δM2Z2M2Z,δGW=δM2W2M2W.
Other renormalization constants are given as
δZ1/2AA=12ddq2ΠAAT(0)=12ddq2ΠAAT(q2)|q2=0,
δZ1/2ZA=−ΠZAT(0)/M2Z=−ΠZAT(q2)/M2Z|q2=0,
δM2W=−Re{ΠWWT(M2W)}=−Re{ΠWWT(q2)|q2=M2W},
δM2Z=−Re{ΠZZT(M2Z)}=−Re{ΠZZT(q2)|q2=M2Z},
δZ1/2ZZ=12Re{ddq2ΠZZT(q2)|q2=M2Z}=12Re{ΠZZ′T(q2)|q2=M2Z},
δZ1/2H=−12Re{ddq2ΠHH(q2)|q2=M2H}=−12Re{ddq2ΠHH(q2)|q2=M2H},
δZ1/2νlL=12Re{Kνl5γ(m2νl)−Kνlγ(m2νl)}.
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All the Feynman diagrams(Figs. E1–E8) contributing to the decay processes
H→Zνlˉνl in the 't Hooft-Veltman are shown in this appendix.Figure E3. Group
G2 : All Z-pole Feynman diagrams contributing to the decay process. We note thatχ± andc± are Nambu-Goldstone bosons and ghost particles, respectively.Figure E4. Group
G2 : All Z-pole Feynman diagrams contributing to the decay process. We note thatχ3 is Nambu-Goldstone boson.Figure E5. Group
G2 : All Z-pole Feynman diagrams contributing to the decay process. We note thatχ± andc± are Nambu-Goldstone bosons and ghost particles, respectively.Figure E6. Group
G2 : All Z-pole Feynman diagrams contributing to the decay process. Here,χ3 is Nambu-Goldstone boson.
One-loop formulas for H → Zνlνl for l = e, µ, τ in 't Hooft-Veltman gauge
- Received Date: 2023-01-16
- Available Online: 2023-05-15
Abstract: In this paper, we present analytical results for one-loop contributions to the decay processes