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QCD Corrections to e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} in Type-I THDM at Electron Positron Colliders

Qiang Yang State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China Department of Modern Physics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China    Ren-You Zhang [email protected] State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China Department of Modern Physics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China    Ming-Ming Long State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China Department of Modern Physics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China    Shao-Ming Wang Department of Physics, Chongqing University, Chongqing 401331, People’s Republic of China    Wen-Gan Ma State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China Department of Modern Physics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China    Jian-Wen Zhu State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China Department of Modern Physics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China    Yi Jiang State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China Department of Modern Physics, University of Science and Technology of China, Hefei 230026, Anhui, People’s Republic of China
Abstract

We investigate in detail the charged Higgs production associated with a WW boson at electron-positron colliders within the framework of the Type-I two-Higgs-doublet model (THDM). We calculate the integrated cross section at the LO and analyze the dependence of the cross section on the THDM parameters and the colliding energy in a benchmark scenario of the input parameters of Higgs sector. The numerical results show that the integrated cross section is sensitive to the charged Higgs mass, especially in the vicinity of mH±184GeVm_{H^{\pm}}\simeq 184~{}{\rm GeV} at a 500GeV500~{}{\rm GeV} e+ee^{+}e^{-} collider, and decreases consistently as the increment of tanβ\tan\beta in the low tanβ\tan\beta region. The peak in the colliding energy distribution of the cross section arises from the resonance of loop integrals and its position moves towards low colliding energy as the increment of mH±m_{H^{\pm}}. We also study the two-loop NLO QCD corrections to both the integrated cross section and the angular distribution of the charged Higgs boson, and find that the QCD relative correction is also sensitive to the charged Higgs mass and strongly depends on the final-state phase space. For tanβ=2\tan\beta=2, the QCD relative correction at a 500GeV500~{}{\rm GeV} e+ee^{+}e^{-} collider varies in the range of [10%, 11%][-10\%,\,11\%] as mH±m_{H^{\pm}} increases from 150150 to 400GeV400~{}{\rm GeV}.

keywords

two-loop QCD correction, Type-I THDM, charged Higgs boson

I Introduction

In July 2012, the 125GeV125~{}{\rm GeV} Higgs boson has been discovered by ATLAS and CMS collaborations at CERN Large Hadron Collider (LHC) Aad et al. (2012); Chatrchyan et al. (2012). In addition to measuring the 125GeV125~{}{\rm GeV} Higgs boson precisely, great efforts have been made to search for exotic Higgs bosons in various scenarios beyond the standard model (SM). Among all the extensions of the SM, the two-Higgs-doublet model (THDM) is an appealing one. It provides rich phenomena such as charged Higgs bosons, explicit and spontaneous 𝒞𝒫\mathcal{CP}-violation, and the candidate for dark matter, since the Higgs sector of the THDM is composed of two complex scalar doublets Lee (1973); Gunion et al. (2000); Gunion and Haber (2003); Branco et al. (2012). In the THDM, there are five Higgs bosons: two neutral 𝒞𝒫\mathcal{CP}-even Higgs bosons hh and HH (mh<mHm_{h}<m_{H}), two charged Higgs bosons H±H^{\pm} and a neutral 𝒞𝒫\mathcal{CP}-odd Higgs boson AA. Although both of the two 𝒞𝒫\mathcal{CP}-even scalars can be interpreted as the 125GeV125~{}{\rm GeV} Higgs boson in the alignment limit, we assume that the lighter scalar hh is the 125GeV125~{}{\rm GeV} Higgs boson in this paper. Since the flavor changing neutral currents (FCNCs) can be induced in THDM which have not been observed, an additional Z2Z_{2} symmetry is imposed to eliminate FCNCs at the tree level. Depending on the types of the Yukawa interactions between fermions and the two Higgs doublets, one can introduce several different types of THDMs (Type-I, Type-II, lepton-specific, and flipped) Branco et al. (2012). The most investigated THDMs are the Type-I and Type-II THDMs. In the Type-I THDM, all the fermions only couple to one of the two Higgs doublets, while in the Type-II THDM, the up-type and down-type fermions couple to the two Higgs doublets, respectively.

The THDMs have been widely studied in many different aspects in previous works. Since it is possible to introduce the spontaneous 𝒞𝒫\mathcal{CP}-violation in THDM, it has been considered as a solution to the problem of baryogenesis in Refs.Turok and Zadrozny (1991); Davies et al. (1994); Fromme et al. (2006). In Refs.Deshpande and Ma (1978); Dolle and Su (2009), the neutral scalar in the inert THDM is interpreted as the candidate for dark matter. The existence of charged Higgs boson is one important characteristic of new physics beyond the SM. Therefore, searching for charged Higgs boson in various aspects is a high priority of experiments. At the LHC Run II, the charged Higgs boson has been probed in various channels, such as H±tb,τντandWZH^{\pm}\rightarrow tb,\,\tau\nu_{\tau}~{}\text{and}~{}WZ Sirunyan et al. (2017, 2020); Aaboud et al. (2018a, b).

To match the precise experimental data, the theoretical predictions on kinematic observables should be calculated with high precision. The renormalization of the THDM has been detailedly studied in different renormalization schemes in Refs.Santos and Barroso (1997); Degrande (2015); Krause et al. (2016); Denner et al. (2016); Altenkamp et al. (2017). The production mechanisms and decay modes of the charged Higgs boson have been investigated at one-loop level in the THDM. The Drell-Yan production of charged Higgs pair has been studied at NLO in Refs.Arhrib and Moultaka (1999); Heinemeyer and Schappacher (2016). The full one-loop contributions for the charged Higgs production associated with a vector boson were given in Refs.Zhu ; Arhrib et al. (2000); Kanemura (2000a); Heinemeyer and Schappacher (2016). The dominant decays of the charged Higgs boson into tbtb and τντ\tau\nu_{\tau} have been studied in Refs.Drees and Roy (1991); Roy (1999), and the loop-induced decay modes H±W±γH^{\pm}\to W^{\pm}\gamma and H±W±ZH^{\pm}\to W^{\pm}Z have also been investigated in Refs.Capdequi Peyranere et al. (1991); Kanemura (2000b); Hernandez-Sanchez et al. (2004); Arhrib et al. (2007). In this work, we focus on the H±WH^{\pm}W^{\mp} associated production at electron-positron colliders in the Type-I THDM. This production channel is a loop-induced process at the lowest order due to the absence of tree-level H±WγH^{\pm}W^{\mp}\gamma and H±WZH^{\pm}W^{\mp}Z couplings, and has been investigated at one-loop level in the THDM as well as the minimal supersymmetric standard model Farris et al. (2004); Kanemura et al. (2011); Logan and Su (2002, 2003). In order to test the THDM via H±WVH^{\pm}W^{\mp}V couplings precisely, we study in detail the two-loop QCD corrections to the e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} process, provide the NLO QCD corrected integrated and differential cross sections, and discuss the dependence on the THDM parameters and the e+ee^{+}e^{-} colliding energy.

The rest of this paper is organized as follows. In Sec.II, we give a brief review of the Type-I THDM and provide the benchmark scenario that we adopt. The methods and details of our LO and NLO calculations are presented in Sec.III. In Sec.IV, the numerical results for both integrated and differential cross sections and some discussions are provided. Finally, a short summary is given in Sec.V.

II Two-Higgs-Doublet model

The Higgs sector of the THDM is composed of two complex scalar doublets Φ1=(ϕ1+,ϕ10)T\Phi_{1}=(\phi_{1}^{+},\phi_{1}^{0})^{T} and Φ2=(ϕ2+,ϕ20)T\Phi_{2}=(\phi_{2}^{+},\phi_{2}^{0})^{T}, which are both in the (𝟏,𝟐,𝟏)(\mathbf{1},\mathbf{2},\mathbf{1}) representation of the SU(3)CSU(2)LU(1)YSU(3)_{C}\otimes SU(2)_{L}\otimes U(1)_{Y} gauge group. In this paper, we consider only the 𝒞𝒫\mathcal{CP}-conserving THDM with a discrete Z2Z_{2} symmetry of the form Φ1Φ1\Phi_{1}\rightarrow-\Phi_{1}. Then the renormalizable and gauge invariant scalar potential is given by

𝒱scalar\displaystyle\mathcal{V}_{\text{scalar}} =m112Φ1Φ1+m222Φ2Φ2[m122Φ1Φ2+h.c.]+12λ1(Φ1Φ1)2+12λ2(Φ2Φ2)2\displaystyle=m_{11}^{2}\Phi_{1}^{\dagger}\Phi_{1}+m_{22}^{2}\Phi_{2}^{\dagger}\Phi_{2}-\left[m_{12}^{2}\Phi_{1}^{\dagger}\Phi_{2}+\text{h.c.}\right]+\frac{1}{2}\lambda_{1}\left(\Phi_{1}^{\dagger}\Phi_{1}\right)^{2}+\frac{1}{2}\lambda_{2}\left(\Phi_{2}^{\dagger}\Phi_{2}\right)^{2} (1)
+λ3(Φ1Φ1)(Φ2Φ2)+λ4(Φ1Φ2)(Φ2Φ1)+12[λ5(Φ1Φ2)2+h.c.].\displaystyle+\lambda_{3}\left(\Phi_{1}^{\dagger}\Phi_{1}\right)\left(\Phi_{2}^{\dagger}\Phi_{2}\right)+\lambda_{4}\left(\Phi_{1}^{\dagger}\Phi_{2}\right)\left(\Phi_{2}^{\dagger}\Phi_{1}\right)+\frac{1}{2}\left[\lambda_{5}\left(\Phi_{1}^{\dagger}\Phi_{2}\right)^{2}+\text{h.c.}\right].

Since the parameter m12m_{12} has the mass-dimension 11, the terms of this kind only break the Z2Z_{2} symmetry softly which can be retained. The parameters m11,m22,λ1,λ2,λ3,λ4m_{11},\,m_{22},\,\lambda_{1},\,\lambda_{2},\,\lambda_{3},\,\lambda_{4} have to be real since the Lagrangian must be real. Though the parameters m12m_{12} and λ5\lambda_{5} can be complex, the imaginary parts of these two parameters would induce explicit 𝒞𝒫\mathcal{CP} violation that we do not consider in this paper. So we assume all the parameters in Eq.(1) are real. The minimization of the potential in Eq.(1) gives two minima Φ1\langle\Phi_{1}\rangle and Φ2\langle\Phi_{2}\rangle of the form

Φ1=(0v1/2),Φ2=(0v2/2),\left\langle\Phi_{1}\right\rangle=\left(\begin{array}[]{c}{0}\\ {v_{1}/\sqrt{2}}\end{array}\right),\quad\left\langle\Phi_{2}\right\rangle=\left(\begin{array}[]{c}{0}\\ {v_{2}/\sqrt{2}}\end{array}\right), (2)

where v1v_{1} and v2v_{2} are the vacuum expectation values of the neutral components of the two Higgs doublets Φ1\Phi_{1} and Φ2\Phi_{2}, respectively. With respect to the convention in Ref.Eriksson et al. (2010), we define v1=vcosβv_{1}=v\cos\beta and v2=vsinβv_{2}=v\sin\beta, where v=(2GF)1/2246GeVv=(\sqrt{2}G_{F})^{-1/2}\approx 246~{}{\rm GeV}. Expanding at the minima, the two complex Higgs doublets Φ1,2\Phi_{1,2} can be expressed as

Φ1=(ϕ1+(v1+ρ1+iη1)/2),Φ2=(ϕ2+(v2+ρ2+iη2)/2).\Phi_{1}=\left(\begin{array}[]{c}{\phi_{1}^{+}}\\ {(v_{1}+\rho_{1}+i\eta_{1})/\sqrt{2}}\end{array}\right),\quad\Phi_{2}=\left(\begin{array}[]{c}{\phi_{2}^{+}}\\ {(v_{2}+\rho_{2}+i\eta_{2})/\sqrt{2}}\end{array}\right). (3)

The mass eigenstates of the Higgs fields are given by Branco et al. (2012); Altenkamp et al. (2017)

(Hh)=(cosαsinαsinαcosα)(ρ1ρ2),\left(\begin{array}[]{c}{H}\\ {h}\end{array}\right)=\left(\begin{array}[]{cc}{\cos\alpha}&{\sin\alpha}\\ {-\sin\alpha}&{\cos\alpha}\end{array}\right)\left(\begin{array}[]{c}{\rho_{1}}\\ {\rho_{2}}\end{array}\right), (4)
(G0A)=(cosβsinβsinβcosβ)(η1η2),\left(\begin{array}[]{c}{G^{0}}\\ {A}\end{array}\right)=\left(\begin{array}[]{cc}{\cos\beta}&{\sin\beta}\\ {-\sin\beta}&{\cos\beta}\end{array}\right)\left(\begin{array}[]{c}{\eta_{1}}\\ {\eta_{2}}\end{array}\right), (5)
(G±H±)=(cosβsinβsinβcosβ)(ϕ1±ϕ2±),\left(\begin{array}[]{c}{G^{\pm}}\\ {H^{\pm}}\end{array}\right)=\left(\begin{array}[]{cc}{\cos\beta}&{\sin\beta}\\ {-\sin\beta}&{\cos\beta}\end{array}\right)\left(\begin{array}[]{c}{\phi_{1}^{\pm}}\\ {\phi_{2}^{\pm}}\end{array}\right), (6)

where α\alpha is the mixing angle of the neutral 𝒞𝒫\mathcal{CP}-even Higgs sector. After the spontaneous electroweak symmetry breaking, the charged and neutral Goldstone fields G±G^{\pm} and G0G^{0} are absorbed by the weak gauge bosons W±W^{\pm} and ZZ, respectively. Thus, the THDM predicts the existence of five physical Higgs bosons: two neutral 𝒞𝒫\mathcal{CP}-even Higgs bosons hh and HH, one neutral 𝒞𝒫\mathcal{CP}-odd Higgs boson AA, and two charged Higgs bosons H±H^{\pm}. The masses of these physical Higgs bosons are given by

mA2\displaystyle m_{A}^{2} =m122sinβcosβv2λ5,\displaystyle=\frac{m_{12}^{2}}{\sin\beta\cos\beta}-v^{2}\lambda_{5}, (7)
mH±2\displaystyle m_{H^{\pm}}^{2} =m122sinβcosβv22(λ4+λ5),\displaystyle=\frac{m_{12}^{2}}{\sin\beta\cos\beta}-\frac{v^{2}}{2}\left(\lambda_{4}+\lambda_{5}\right),
mH,h2\displaystyle m_{H,h}^{2} =12[112+222±(112222)2+4(122)2],\displaystyle=\frac{1}{2}\left[\mathcal{M}_{11}^{2}+\mathcal{M}_{22}^{2}\pm\sqrt{\left(\mathcal{M}_{11}^{2}-\mathcal{M}_{22}^{2}\right)^{2}+4\left(\mathcal{M}_{12}^{2}\right)^{2}}\right],

where 2\mathcal{M}^{2} is the mass matrix of the neutral 𝒞𝒫\mathcal{CP}-even Higgs sector. The explicit form of 2\mathcal{M}^{2} is expressed as

2=mA2(sin2βsinβcosβsinβcosβcos2β)+v22,\mathcal{M}^{2}=m_{A}^{2}\left(\begin{array}[]{cc}{\sin^{2}\beta}&{-\sin\beta\cos\beta}\\ {-\sin\beta\cos\beta}&{\cos^{2}\beta}\end{array}\right)+v^{2}\mathcal{B}^{2}, (8)

where

2=(λ1cos2β+λ5sin2β(λ3+λ4)sinβcosβ(λ3+λ4)sinβcosβλ2sin2β+λ5cos2β).\mathcal{B}^{2}=\left(\begin{array}[]{cc}{\lambda_{1}\cos^{2}\beta+\lambda_{5}\sin^{2}\beta}&{\left(\lambda_{3}+\lambda_{4}\right)\sin\beta\cos\beta}\\ {\left(\lambda_{3}+\lambda_{4}\right)\sin\beta\cos\beta}&{\lambda_{2}\sin^{2}\beta+\lambda_{5}\cos^{2}\beta}\end{array}\right). (9)

The SM Higgs is the combination of the two neutral 𝒞𝒫\mathcal{CP}-even Higgs bosons as

hSM\displaystyle h^{SM} =ρ1cosβ+ρ2sinβ\displaystyle=\rho_{1}\cos\beta+\rho_{2}\sin\beta (10)
=hsin(βα)+Hcos(βα).\displaystyle=h\sin(\beta-\alpha)+H\cos(\beta-\alpha).

Thus, the lighter neutral 𝒞𝒫\mathcal{CP}-even scalar hh can be identified as the SM-like Higgs boson in the so-called alignment limit of sin(βα)1\sin(\beta-\alpha)\rightarrow 1. In this paper, we consider the lighter 𝒞𝒫\mathcal{CP}-even Higgs hh as the SM-like Higgs boson discovered at the LHC.

The input parameters for the Higgs sector of the THDM are chosen as

{mh,mH,mA,mH±,m12,sin(βα),tanβ},\left\{m_{h},\,m_{H},\,m_{A},\,m_{H^{\pm}},\,m_{12},\,\sin(\beta-\alpha),\,\tan\beta\right\}, (11)

which are implemented as the “physical basis” in 2HDMC Eriksson et al. (2010). We adopt the following benchmark scenario,

mh=125.18GeV,\displaystyle m_{h}=125.18~{}{\rm GeV}, (12)
mH=mA=mH±,\displaystyle m_{H}=m_{A}=m_{H^{\pm}},
m122=mA2sinβcosβ,\displaystyle m_{12}^{2}=m_{A}^{2}\sin\beta\cos\beta,
sin(βα)=1,\displaystyle\sin(\beta-\alpha)=1,
mH±[150,400]GeV,\displaystyle m_{H^{\pm}}\in[150,400]~{}{\rm GeV},
tanβ[1,5],\displaystyle\tan\beta\in[1,5],

which satisfies the theoretical constraints from perturbative unitarity Grinstein et al. (2016), stability of vacuum Nie and Sher (1999), and tree-level unitarity Akeroyd et al. (2000). The Z2Z_{2} soft-breaking parameter m122m_{12}^{2} is chosen as mA2sinβcosβm_{A}^{2}\sin\beta\cos\beta in order to satisfy the perturbative unitarity for tanβ[1,5]\tan\beta\in[1,5]. Considering the constraints from experiments at the 13TeV13~{}{\rm TeV} LHC in Ref.Sirunyan et al. (2019), cos(βα)\cos(\beta-\alpha) is very closed to 0. So we apply the alignment limit in our benchmark scenario to set sin(βα)=1\sin(\beta-\alpha)=1. As to the mH±m_{H^{\pm}} and tanβ\tan\beta parameters, we concentrate on the region with low mass and small tanβ\tan\beta.

III Descriptions of calculation

In this section, we present in detail the calculation procedure for the e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} process at one- and two-loop levels. The Feynman diagrams and the amplitudes are generated by FeynArts-3.11 Hahn (2001), using the Feynman rules of THDM in Ref.Altenkamp et al. (2017). The evaluation of Dirac trace and the contraction of Lorentz indices are performed by the FeynCalc-9.3 package Mertig et al. (1991); Shtabovenko et al. (2016). In order to reduce the Feynman integrals into the combinations of a small set of integrals called the master integrals (MIs), we utilize the KIRA-1.2 package Maierhöfer et al. (2018), which adopts the integration-by-parts (IBP) method with Laporta’s algorithm Laporta (2000). One can get the numerical results of amplitudes after evaluating the MIs which is the main difficulty of multi-loop calculation.

In this paper, we calculate the MIs by using the ordinary differential equations (ODEs) method Liu et al. (2018). A LL-loop Feynman integral can be expressed as

({a1,,an},D,η)=j=1LdDljk=1n1(Ek+iη)ak,\mathcal{I}(\left\{a_{1},\ldots,a_{n}\right\},\,D,\,\eta)=\int\prod_{j=1}^{L}d^{D}l_{j}\prod_{k=1}^{n}\frac{1}{(E_{k}+i\eta)^{a_{k}}}, (13)

where D42ϵD\equiv 4-2\epsilon and Ek=qk2mk2E_{k}=q_{k}^{2}-m_{k}^{2} are the denominators of Feynman propagators in which the qkq_{k} are the linear combinations of loop momenta and external momenta. The physical results of the Feynman integrals are obtained by taking η0+\eta\rightarrow 0^{+}, i.e.,

({a1,,an},D, 0)=limη0+({a1,,an},D,η).\mathcal{I}(\left\{a_{1},\ldots,a_{n}\right\},\,D,\,0)=\lim_{\eta\to 0^{+}}\mathcal{I}(\left\{a_{1},\ldots,a_{n}\right\},\,D,\,\eta). (14)

One can construct the ODEs with respect to η\eta,

(η)η=(η).(η),\frac{\partial\vec{\mathcal{I}}(\eta)}{\partial\eta}=\mathcal{M}(\eta).\vec{\mathcal{I}}(\eta), (15)

where \vec{\mathcal{I}} is a complete set of MIs. The boundary conditions of these ODEs are chosen at η=\eta=\infty which are the simple vacuum integrals. The analytical expressions for the vacuum integrals up to three-loop order can be found in Refs.Davydychev and Tausk (1993); Broadhurst (1999); Kniehl et al. (2017). To solve these ODEs numerically, we utilize the odeint package Ahnert et al. (2011) to evaluate ODEs from an initial point ηi\eta_{i} to a target point ηj\eta_{j}. To perform the asymptotic expansion in the domain nearby η=0\eta=0, we transform the coefficient matrix into normalized fuchsian form with the help of the epsilon package Prausa (2017).

III.1 Calculation at LO

For the LO calculation, we adopt the ’t Hooft-Feynman gauge with the on-shell renormalization scheme at one-loop order mentioned in Ref.Altenkamp et al. (2017). Some representative Feynman diagrams for the e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} process at the LO are shown in Fig.1, where SS and VV in the loops represent the Higgs/Goldstone and weak gauge bosons, respectively. Due to the tiny mass of electron, the contribution from the diagrams involving Higgs Yukawa coupling to electron is ignored. The diagrams with VSV-S mixing are also not shown in Fig.1, because these diagrams can induce a factor of mem_{e} via Dirac equation. The last diagram in Fig.1 is a vertex counterterm diagram induced by the renormalization constant δZG±H±\delta Z_{G^{\pm}H^{\pm}} at one-loop level. In the on-shell renormalization scheme, the renormalization constant δZG±H±\delta Z_{G^{\pm}H^{\pm}} is given by

δZG±H±=2Re~W±H±(mH±2)mW,\delta Z_{G^{\pm}H^{\pm}}=-\frac{2\widetilde{Re}\sum^{W^{\pm}H^{\pm}}(m_{H^{\pm}}^{2})}{m_{W}}, (16)

where W±H±(mH±2)\sum^{W^{\pm}H^{\pm}}(m_{H^{\pm}}^{2}) is the transition of W±H±W^{\pm}-H^{\pm} at p2=mH±2p^{2}=m_{H^{\pm}}^{2}, and Re~\widetilde{Re} means to take the real parts of the loop integrals in the transition. It is worth mentioning that Eq.(16) is valid at both 𝒪(α)\mathcal{O}(\alpha) and 𝒪(ααs)\mathcal{O}(\alpha\alpha_{s}).

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Figure 1: Representative Feynman diagrams for e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} at LO.

III.2 Calculation at QCD NLO

There are 2424 two-loop and counterterm diagrams for e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} at the QCD NLO. Some representative ones of them are depicted in Fig.2. At the QCD NLO, all the two-loop Feynman diagrams are generated from the LO quark triangle loop diagram (i.e., the first diagram in Fig.1). The cross in the quark loop diagrams represents the renormalization constant of quark mass at 𝒪(αs)\mathcal{O}(\alpha_{s}), while the circle cross displayed in the last counterterm diagram represents the renormalization constant δZG±H±\delta Z_{G^{\pm}H^{\pm}} at 𝒪(ααs)\mathcal{O}(\alpha\alpha_{s}). The quark mass renormalization constant used in NLO QCD calculation is given by Bernreuther et al. (2005)

δmq=mqαs2πC(ϵ)(μ2mq2)ϵCF2(32ϵ)ϵ(12ϵ),\delta_{m_{q}}=-m_{q}\frac{\alpha_{s}}{2\pi}C(\epsilon)\left(\frac{\mu^{2}}{m_{q}^{2}}\right)^{\epsilon}\frac{C_{F}}{2}\frac{(3-2\epsilon)}{\epsilon(1-2\epsilon)}, (17)

where C(ϵ)=(4π)ϵΓ(1+ϵ)C(\epsilon)=(4\pi)^{\epsilon}\Gamma(1+\epsilon) and CF=43C_{F}=\dfrac{4}{3}. The lowest order for e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} is one-loop order, therefore, the renormalization should be dealt with carefully in NLO QCD calculation. As shown in Figs.1 and 2, the wave-function renormalization constant δZG±H±\delta Z_{G^{\pm}H^{\pm}} is involved in both NLO and LO amplitudes. Since the self-energy W±H±(mH±2)\sum^{W^{\pm}H^{\pm}}(m_{H^{\pm}}^{2}) is nonzero at 𝒪(ααs)\mathcal{O}(\alpha\alpha_{s}), i.e. δZG±H±\delta Z_{G^{\pm}H^{\pm}} is nonzero at 𝒪(ααs)\mathcal{O}(\alpha\alpha_{s}), the contribution from the last diagram in Fig.2 should be included in NLO QCD calculation. The typical Feynman diagrams for H±W±H^{\pm}-W^{\pm} transition at 𝒪(ααs)\mathcal{O}(\alpha\alpha_{s}) are shown in Fig.3. After taking into account all the contributions at 𝒪(ααs)\mathcal{O}(\alpha\alpha_{s}) in DD-dimensional spacetime, both 1ϵ2\dfrac{1}{\epsilon^{2}} and 1ϵ\dfrac{1}{\epsilon} singularities are all canceled.

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Figure 2: Representative Feynman diagrams for e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} at NLO in QCD.
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Figure 3: Representative Feynman diagrams contributing to W±H±W^{\pm}-H^{\pm} transition at 𝒪(ααs)\mathcal{O}(\alpha\alpha_{s}).

IV Numerical results and discussion

Besides the input parameters for the Higgs sector of the THDM specified in benchmark scenario in Eq.(12), the following SM input parameters are adopted in our numerical calculation Tanabashi et al. (2018):

GF=1.1663787×105GeV2,αs(mZ)=0.118,\displaystyle G_{F}=1.1663787\times 10^{-5}~{}{\rm GeV^{-2}},\quad\alpha_{s}(m_{Z})=0.118, (18)
mt=173GeV,mb=4.78GeV,\displaystyle m_{t}=173~{}{\rm GeV},\quad m_{b}=4.78~{}{\rm GeV},
mW=80.379GeV,mZ=91.1876GeV,\displaystyle m_{W}=80.379~{}{\rm GeV},\quad m_{Z}=91.1876~{}{\rm GeV},

where GFG_{F} is the Fermi constant. The fine structure constant α\alpha is fixed by

α=2GFπmW2(mZ2mW2)mZ2.\alpha=\frac{\sqrt{2}G_{F}}{\pi}\frac{m_{W}^{2}(m_{Z}^{2}-m_{W}^{2})}{m_{Z}^{2}}. (19)

IV.1 LO

In Fig.4, we display the LO cross section for e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} as a function of mH±m_{H^{\pm}} and tanβ\tan\beta in the benchmark scenario in Eq.(12) at s=500GeV\sqrt{s}=500~{}{\rm GeV} (left) and 1000GeV1000~{}{\rm GeV} (right), respectively. From the left plot, we can see clearly that the LO cross section for H±WH^{\pm}W^{\mp} production at a 500GeV500~{}{\rm GeV} e+ee^{+}e^{-} collider peaks at mH±184GeVm_{H^{\pm}}\simeq 184~{}{\rm GeV} due to the resonance effect of loop integrals. The cross section is sensitive to the mass of charged Higgs boson, it can exceed 3fb3~{}{\rm fb} in the vicinity of mH±184GeVm_{H^{\pm}}\simeq 184~{}{\rm GeV} at small tanβ\tan\beta. In the region of mH±<180GeVm_{H^{\pm}}<180~{}{\rm GeV}, the cross section increases slowly as the increment of mH±m_{H^{\pm}}, while it drops rapidly when mH±>184GeVm_{H^{\pm}}>184~{}{\rm GeV}. As the increment of tanβ\tan\beta from 11 to 55, the cross section decreases consistently due to the decline of the H+t¯bH^{+}\bar{t}b Yukawa coupling strength in the low tanβ\tan\beta region. Comparing the two plots in Fig.4, we can see that the cross section at s=1000GeV\sqrt{s}=1000~{}{\rm GeV} is much smaller than that at s=500GeV\sqrt{s}=500~{}{\rm GeV} because of the ss-channel suppression. As the increasing of the e+ee^{+}e^{-} colliding energy from 500500 to 1000GeV1000~{}{\rm GeV}, the peak position of the cross section as a function of mH±m_{H^{\pm}} moves towards high mH±m_{H^{\pm}} and the mH±m_{H^{\pm}} dependence of the cross section is reduced significantly. Moreover, the production cross section at s=1000GeV\sqrt{s}=1000~{}{\rm GeV} also decreases quickly as the increment of tanβ\tan\beta in the plotted tanβ\tan\beta region.

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Figure 4: Contours of LO cross section for e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} at s=500GeV\sqrt{s}=500~{}{\rm GeV} (left) and 1000GeV1000~{}{\rm GeV} (right) on the mH±tanβm_{H^{\pm}}-\tan\beta plane.

In Fig.5, we present the dependence of the LO cross section for e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} on the e+ee^{+}e^{-} colliding energy for some typical values of mH±m_{H^{\pm}} and tanβ\tan\beta. As shown in this figure, the behaviors of the production cross section as a function of the colliding energy at different values of tanβ\tan\beta are quite similar. For mH±=160GeVm_{H^{\pm}}=160~{}{\rm GeV}, the cross section increases sharply in the range of s<360GeV\sqrt{s}<360~{}{\rm GeV}, reaches its maximum at s360GeV\sqrt{s}\simeq 360~{}{\rm GeV}, and then decreases slowly as the increment of s\sqrt{s}. The existence of the peak at s360GeV\sqrt{s}\simeq 360~{}{\rm GeV} can be attributed to the competition between the phase-space enlargement and the ss-channel suppression as the increasing of s\sqrt{s}. The maximum value of the cross section can exceed 1fb1~{}{\rm fb} for tanβ=1\tan\beta=1 and decreases to about 0.3fb0.3~{}{\rm fb} and 0.1fb0.1~{}{\rm fb} for tanβ=2\tan\beta=2 and tanβ=3\tan\beta=3, respectively. Comparing the upper two plots of Fig.5, we can see that the s\sqrt{s} dependence of the cross section for mH±=180GeVm_{H^{\pm}}=180~{}{\rm GeV} is very close to that for mH±=160GeVm_{H^{\pm}}=160~{}{\rm GeV}, but there is a small peak at s630GeV\sqrt{s}\simeq 630~{}{\rm GeV} for mH±=180GeVm_{H^{\pm}}=180~{}{\rm GeV}. Such resonance induced by loop integrals only occurs above the threshold of H+tb¯H^{+}\rightarrow t\bar{b}, i.e., mH±>mt+mbm_{H^{\pm}}>m_{t}+m_{b}. As the increment of mH±m_{H^{\pm}}, this resonance effect becomes more considerable and the peak position moves towards low s\sqrt{s}. As shown in the bottom-left plot of Fig.5, the resonance peak for mH±=185GeVm_{H^{\pm}}=185~{}{\rm GeV} is located at s490GeV\sqrt{s}\simeq 490~{}{\rm GeV}, and is more distinct compared to that for mH±=180GeVm_{H^{\pm}}=180~{}{\rm GeV}. As to the s\sqrt{s} dependence of the H±WH^{\pm}W^{\mp} production cross section for mH±=200GeVm_{H^{\pm}}=200~{}{\rm GeV} shown in the bottom-right plot of Fig.5, it looks quite different from those for mH±=160, 180m_{H^{\pm}}=160,\,180 and 185GeV185~{}{\rm GeV}. There is a sharp peak at s390GeV\sqrt{s}\simeq 390~{}{\rm GeV} for each value of tanβ{1,2,3}\tan\beta\in\{1,2,3\} which was also mentioned in previous works Zhu ; Kanemura (2000a); Heinemeyer and Schappacher (2016). This peak is a consequence of competition among the phase-space enlargement, ss-channel suppression and the resonance induced by loop integrals. We can see that the peak cross section can reach about 4fb4~{}{\rm fb} for tanβ=1\tan\beta=1, and will decrease to around 1fb1~{}{\rm fb} and 0.4fb0.4~{}{\rm fb} when tanβ\tan\beta increases to 22 and 33, respectively. In the region of s<350GeV\sqrt{s}<350~{}{\rm GeV}, the cross section increases quickly as the increment of s\sqrt{s} due to the enlargement of phase space, while in the region s>450GeV\sqrt{s}>450~{}{\rm GeV}, it is close to the result of ss-channel suppression, especially at high s\sqrt{s}.

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Figure 5: LO cross section for e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} as a function of e+ee^{+}e^{-} colliding energy for some typical values of mH±m_{H^{\pm}} and tanβ\tan\beta.

IV.2 NLO QCD

In this subsection, we calculate the e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} process at the QCD NLO, and discuss the dependence of the integrated cross section on the e+ee^{+}e^{-} colliding energy and the charged Higgs mass as well as the angular distribution of the final-state charged Higgs boson.

The LO, NLO QCD corrected integrated cross sections and the corresponding QCD relative correction for e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} as functions of the e+ee^{+}e^{-} colliding energy s\sqrt{s} are depicted in Fig.6, where mH±=200GeVm_{H^{\pm}}=200~{}{\rm GeV} and tanβ=2\tan\beta=2. As shown in the upper panel of this figure, the NLO QCD corrected integrated cross section peaks at s375GeV\sqrt{s}\simeq 375~{}{\rm GeV}, it increases sharply when s<375GeV\sqrt{s}<375~{}{\rm GeV} and decreases approximately linearly in the region of s>500GeV\sqrt{s}>500~{}{\rm GeV} as the increment of s\sqrt{s}. From the lower panel of Fig.6, we can see that the QCD relative correction increases rapidly from about 9%9\% to above 60%60\% as the increment of s\sqrt{s} from 300300 to 345GeV345~{}{\rm GeV} and then decreases back to about 3%3\% as s\sqrt{s} increases to 385GeV385~{}{\rm GeV}. The variation of QCD relative correction with s\sqrt{s} in the region of s>385GeV\sqrt{s}>385~{}{\rm GeV} is also plotted in the inset in the upper panel of Fig.6 for clarity. It clearly shows that the QCD relative correction decreases approximately linearly from about 3%3\% to around 4%-4\% as the increment of s\sqrt{s} from 385385 to 1000GeV1000~{}{\rm GeV}. In Table 1 we list the LO, NLO QCD corrected cross sections and the corresponding QCD relative corrections at some specific colliding energies. At s=340GeV\sqrt{s}=340~{}{\rm GeV} which can be reached by both the International Linear Collider (ILC) Behnke et al. (2013) and the Future Circular Electron-Positron Collider (FCC-ee) Abada et al. (2019), the cross section is about 0.235fb0.235~{}{\rm fb} at the QCD NLO. At the ILC with s=500\sqrt{s}=500 and 1000GeV1000~{}{\rm GeV}, the NLO QCD corrected cross sections reach about 0.1930.193 and 0.0778fb0.0778~{}{\rm fb}, respectively, and the corresponding relative corrections are 0.26%0.26\% and 4.27%-4.27\%.

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Figure 6: LO, NLO QCD corrected integrated cross sections and the corresponding QCD relative correction for e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} as functions of e+ee^{+}e^{-} colliding energy for mH±=200GeVm_{H^{\pm}}=200~{}{\rm GeV} and tanβ=2\tan\beta=2.
s\sqrt{s} [GeV] 300300 320320 340340 400400 500500 600600 700700 800800 900900 10001000
σLO\sigma_{\textrm{LO}} [fb] 0.045920.04592 0.078680.07868 0.17120.1712 0.38700.3870 0.19200.1920 0.14810.1481 0.12300.1230 0.10540.1054 0.091960.09196 0.081260.08126
σNLO\sigma_{\textrm{NLO}} [fb] 0.050040.05004 0.091630.09163 0.23530.2353 0.39630.3963 0.19250.1925 0.14660.1466 0.12060.1206 0.10240.1024 0.088650.08865 0.077790.07779
δ\delta [%] 8.978.97 16.416.4 37.437.4 2.402.40 0.2600.260 1.01-1.01 1.95-1.95 2.85-2.85 3.60-3.60 4.27-4.27
Table 1: LO, NLO QCD corrected cross sections and the corresponding QCD relative corrections for e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} at some specific colliding energies. (mH±=200GeVm_{H^{\pm}}=200~{}{\rm GeV} and tanβ=2\tan\beta=2)

In order to study the mH±m_{H^{\pm}} dependence of the QCD correction, we plot the NLO QCD corrected cross section, as well as the LO cross section, and the QCD relative correction as functions of mH±m_{H^{\pm}} in Fig.7 with tanβ=2\tan\beta=2 and s=500GeV\sqrt{s}=500~{}{\rm GeV}. The numerical results for some typical values of mH±m_{H^{\pm}} are also given in Table 2. From Fig.7, we can see that the LO and NLO QCD corrected cross sections increase from about 0.18fb0.18~{}{\rm fb} to around 0.290.29 and 0.32fb0.32~{}{\rm fb}, respectively, as mH±m_{H^{\pm}} increases from 150150 to 184GeV184~{}{\rm GeV}, and drop to less than 0.01fb0.01~{}{\rm fb} when mH±=400GeVm_{H^{\pm}}=400~{}{\rm GeV}. Similarly, there is also a notable spike at mH±184GeVm_{H^{\pm}}\simeq 184~{}{\rm GeV} for QCD relative correction, as shown in the lower panel of Fig.7. The QCD relative correction is less than 0.5%0.5\% and thus can be neglected when mH±=150GeVm_{H^{\pm}}=150~{}{\rm GeV}, while it is expected to increase to about 11%11\% as mH±m_{H^{\pm}} increases to 184GeV184~{}{\rm GeV}. When mH±>185GeVm_{H^{\pm}}>185~{}{\rm GeV}, the QCD relative correction decreases slowly down to about 10%-10\% as mH±m_{H^{\pm}} increases to 400GeV400~{}{\rm GeV}.

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Figure 7: LO, NLO QCD corrected cross sections and the corresponding QCD relative correction for H±WH^{\pm}W^{\mp} associated production at a s=500GeV\sqrt{s}=500~{}{\rm GeV} e+ee^{+}e^{-} collider as functions of charged Higgs mass for tanβ=2\tan\beta=2.
mH±m_{H^{\pm}} [GeV] 150150 160160 170170 180180 190190 200200 250250 300300 350350 400400
σLO\sigma_{\textrm{LO}} [fb] 0.18280.1828 0.18760.1876 0.19510.1951 0.21400.2140 0.22300.2230 0.19200.1920 0.10900.1090 0.056990.05699 0.025530.02553 0.0075950.007595
σNLO\sigma_{\textrm{NLO}} [fb] 0.18360.1836 0.18960.1896 0.19900.1990 0.22490.2249 0.22400.2240 0.19250.1925 0.10620.1062 0.053760.05376 0.023430.02343 0.0068170.006817
δ\delta [%] 0.4380.438 1.071.07 2.002.00 5.095.09 0.4480.448 0.2600.260 2.57-2.57 5.67-5.67 8.22-8.22 10.24-10.24
Table 2: LO, NLO QCD corrected cross sections and the corresponding QCD relative corrections for H±WH^{\pm}W^{\mp} production at a s=500GeV\sqrt{s}=500~{}{\rm GeV} e+ee^{+}e^{-} collider for some typical values of mH±m_{H^{\pm}}. (tanβ=2\tan\beta=2)

The LO, NLO QCD corrected angular distributions of the final-state charged Higgs boson and the corresponding QCD relative corrections for H+WH^{+}W^{-} associated production at a 500GeV500~{}{\rm GeV} e+ee^{+}e^{-} collider for tanβ=2\tan\beta=2 and mH±=200m_{H^{\pm}}=200 and 300GeV300~{}{\rm GeV} are depicted in Fig.8, where θ\theta denotes the scattering angle of H+H^{+} with respect to the electron beam direction. Due to the 𝒞𝒫\mathcal{CP} conservation, the distribution of the scattering angle of HH^{-} with respect to the positron beam direction for e+eHW+e^{+}e^{-}\rightarrow H^{-}W^{+} is the same as the angular distribution of H+H^{+} for e+eH+We^{+}e^{-}\rightarrow H^{+}W^{-}. From this figure, we can see that the charged Higgs boson is mostly produced in transverse direction for both mH±=200m_{H^{\pm}}=200 and 300GeV300~{}{\rm GeV}. For mH+=200GeVm_{H^{+}}=200~{}{\rm GeV}, the QCD relative correction decreases rapidly from 10%10\% to nearly 0%0\% as the increment of cosθ\cos\theta from 1-1 to 0.5-0.5, and is steady at around 0%0\% in the region of 0.5<cosθ<1-0.5<\cos\theta<1. It implies that the NLO QCD correction can be neglected in most of the phase space region except when θπ\theta\rightarrow\pi. For mH±=300GeVm_{H^{\pm}}=300~{}{\rm GeV}, the LO differential cross section is suppressed by the NLO QCD correction in the whole phase space region. The corresponding QCD relative correction decreases from about 0.8%-0.8\% to 7.5%-7.5\% as cosθ\cos\theta increases from 1-1 to 11. This QCD correction should be taken into consideration for precision study of the H±WH^{\pm}W^{\mp} production at lepton colliders.

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Figure 8: Angular distributions of charged Higgs boson for H+WH^{+}W^{-} associated production at a 500GeV500~{}{\rm GeV} e+ee^{+}e^{-} collider for tanβ=2\tan\beta=2 and mH±=200m_{H^{\pm}}=200 (left) and 300GeV300~{}{\rm GeV} (right).

V Summary

Searching for exotic Higgs boson and studying its properties are important tasks at future lepton colliders. In this work, we study in detail the H±WH^{\pm}W^{\mp} associated production at future electron-positron colliders within the framework of the Type-I THDM. We calculate the e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp} process at the LO, and investigate the dependence of the production cross section on the THDM parameters (mH±m_{H^{\pm}} and tanβ\tan\beta) and the e+ee^{+}e^{-} colliding energy. The numerical results show that the cross section is very sensitive to the charge Higgs mass in the vicinity of mH±184GeVm_{H^{\pm}}\simeq 184~{}{\rm GeV} at a 500GeV500~{}{\rm GeV} e+ee^{+}e^{-} collider, and decreases consistently with the increment of tanβ\tan\beta in the low tanβ\tan\beta region. The existence of a peak in the colliding energy distribution of the cross section is explained by the resonance effect induced by loop integrals. This resonance occurs only above the threshold of H+tb¯H^{+}\rightarrow t\bar{b}, and the peak position moves towards low colliding energy as the increment of mH±m_{H^{\pm}}. We also calculate the two-loop NLO QCD corrections to e+eH±We^{+}e^{-}\rightarrow H^{\pm}W^{\mp}, and provide some numerical results for the NLO QCD corrected integrated cross section and the angular distribution of the final-state charged Higgs boson. For s=500GeV\sqrt{s}=500~{}{\rm GeV} and tanβ=2\tan\beta=2, the QCD relative correction varies smoothly in the range of [10%, 3%][-10\%,\,3\%] as the increment of mH±m_{H^{\pm}} from 150150 to 400GeV400~{}{\rm GeV}, except in the vicinity of mH±184GeVm_{H^{\pm}}\simeq 184~{}{\rm GeV}. The QCD relative correction is sensitive to the charged Higgs mass and strongly depends on the final-state phase space. For mH±=300GeVm_{H^{\pm}}=300~{}{\rm GeV} and tanβ=2\tan\beta=2, the QCD relative correction to the H+WH^{+}W^{-} production at a 500GeV500~{}{\rm GeV} e+ee^{+}e^{-} collider increases from about 7.5%-7.5\% to 0.8%-0.8\% as the scattering angle of H+H^{+} increases from 0 to π\pi. Compared to hadron colliders, the measurement precision of Higgs associated production at future high-energy electron-positron colliders is much higher. The expected experimental error of Higgs production in association with a weak gauge boson at high-energy electron-positron colliders is less than 1%1\% through the recoil mass of the associated vector boson. For example, the measurement precision of HZHZ production at s=240GeV\sqrt{s}=240~{}{\rm GeV} FCC-ee and s=250GeV\sqrt{s}=250~{}{\rm GeV} CEPC can reach about 0.4%0.4\% and 0.7%0.7\%, respectively Peskin ; Bicer et al. (2014); Ruan (2016). Due to the high WW-tagging efficiency at e+ee^{+}e^{-} colliders, the measurement precision of H±WH^{\pm}W^{\mp} production at a high-energy e+ee^{+}e^{-} collider can be also less than 1%1\%. Thus, the two-loop QCD correction should be taken into consideration in precision study of the H±WH^{\pm}W^{\mp} associated production at future lepton colliders.

VI Acknowledgements

This work is supported in part by the National Natural Science Foundation of China (Grants No. 11775211 and No. 11535002) and the CAS Center for Excellence in Particle Physics (CCEPP).

References