Associated production of SM Higgs with a photon in type-II seesaw models at the ILC

We consider the production of a single Standard Model (SM) Higgs boson ($h^0$) in association with a photon at the future Linear collider (LC) in the context of a type-II seesaw model. The type-II seesaw model extends the SM particle content by adding one triple Higgs where its Higgs coupling is a key parameter of the scalar potential triggering the electroweak symmetry-breaking mechanism in the SM. It is a well motivated model since it provides neutrino masses and mixing. The LC presents a particularly interesting possibility to probe Higgs couplings due to the clean beams in the initial state. We study the one loop processes $e^+e^- \to h^0\gamma$ and $e^-\gamma \to e^- h^0$, we show that it is possible to correlate the total cross section predictions with the couplings $h^0\gamma\gamma$ and $h^0\gamma Z$ which are sensitive to the presence of singly and doubly charged Higgs. For parameter points allowed by the current experimental constraints, our numerical results show that the effect of $H^\pm$ and $H^{\pm\pm}$ can be as large as $\pm$ 25\% with respect to the SM predictions. For both processes, we also present differential cross section for different center of mass energy.


Introduction
With the discovery of the Higgs-like boson at the Large Hadron Collider (LHC) [1,2], the Standard Model (SM) was finally completed. However, this discovery didn't mark the end of Higgs boson exploration, particularly with regard to mass-generation mechanism for both fermions and gauge bosons. For this purpose, ATLAS and CMS have performed several Higgs coupling measurements, such as h 0 → W + W − , h 0 → ZZ, h 0 → γγ, h 0 → bb and h 0 → τ + τ − with a certain precision which will be improved during the future run of the LHC. Note that all those measurements are well consistent with SM predictions. Therefore, any SM extensions should agree with the above measurements.
However, neutrinos are perhaps the most puzzling among all known particles regarding its masses unexplained within the SM [3]. Moreover, revealing the true neutrino identity could help answer long-standing questions, like whether neutrino and antineutrino are the same particle, and it could even shade more light on the unification of the interactions that exist in nature. One simple way would be to generate a Dirac neutrino mass in a similar manner that the upper quarks get its own, through the Higgs mechanism by introducing right handed neutrinos, i.e. m DνL ν R . Since neutrino masses are at the sub ∼ eV scale, this means that the Yukawa couplings have to be unnaturally small, of the order 10 −12 .
On the other side, if neutrinos happen to coincide with anti-neutrinos, then a non-vanishing dimension five operator 1 Λ L 5 [4,5], constructed from the neutrino and Higgs fields, gives rise to a light Majorana neutrino mass, and leads to leptonic number violation (global symmetries are not sacred). In this case, the large Majorana mass scale Λ that turns out to be quite close to the Grand Unification scale, ends up suppressing the neutrino masses via Seesaw mechanism as v 2 EW /Λ. There are three types of Seesaw mechanisms that provide a comprehensive understanding of the observed sizes of neutrino masses by exchange of 3 different types of heavy particles, known as i) Type-I seesaw where a gauge singlet chiral fermion S = (1, 1, 0) is introduced to the SM sector [6,7,8,9,10,11,12,13], ii)Type-II seesaw in which a SU (2) L weak triplet boson ∆ = (1, 3, 2) is added to the SM Higgs sector [14,15,16,17] and finally iii) the addition of a SU (2) L triplet fermion T = (1, 3, 0) [18] provides the conventional Type-III Seesaw.
So among the previous categories, Seesaw Type-II, also known as the Higgs Triplet Model (HTM), remains the viable option that is made up of the SM Higgs doublet and a triplet of hypercharge of Y = +2. In this context, once the neutral component of the triplet ∆ develops its own vacuum expectation value, the neutrinos acquire Majo-arXiv:1909.07793v3 [hep-ph] 28 Oct 2019 rana mass. In this regards, the most significant attribute of HTM is its minimality regarding the very simple representations of SU (3) × SU (2) × U (1), for both fermions and Higgs sectors.
A close look at the HTM Higgs sector reveals a variety in its spectrum which includes: 2 CP-even Higgs h 0 and H 0 , one CP-odd A 0 , pair of charged Higgs H ± and a pair of doubly charged Higgs H ±± . For more details about HTM spectrum as well as the theoretical constraints, we refer the interested readers to Refs [19,20]. Moreover, a number of detailed phenomenological researchs have already been performed at the LHC [21,22,23,24,25,26,27]. One attractive feature of this model is the presence of the doubly-charged Higgs boson, and its distinguished decay modes which strongly depend on the size of the triplet vev.
At the LHC, ATLAS and CMS already performed the measurement of several Higgs couplings to SM particles with an uncertainty of about 10-20%. These measurements will be further improved by the High Luminosity option of the LHC (HL-LHC) which brings uncertainties down to 2-5% [28]. Moreover, at the e + e − Linear Collider (LC), which would act like a Higgs factory, the uncertainties on the Higgs couplings would be much smaller, reaching 0.6-1.3% for some light fermionic decay channels [29]. It is well known that the precise measurement programs of Higgs properties at the LC and LHC are complementary to each other in many aspects. In addition, the loop-mediated process h 0 → γγ which was a discovery mode for the 125 GeV Higgs-like and is now quite accurately measured. While the other related one-loop decay h 0 → γZ, which is also loop-mediated, is still missing and may show up in the future LHC run when more data is accumulated. At the LC, the one loop mediated process e + e − → γh 0 if measured could also shed some light on h 0 γγ and h 0 γZ couplings. Such process has been investigated in the SM [30,31], and also in many Beyond SM (BSM) scenarios, like SUSY [32,36], extended Higgs sector [33,34], and in the Inert Higgs Model [35].
In this work, we examine the effect of a singly and a doubly charged Higgs bosons in the associated production of the SM Higgs with a photon e + e − → h 0 γ at the LC and also e − γ → h 0 e − which would take place if the e − γ collisions are available at the LC. In Ref [34], the authors study e + e − → γh 0 in the framework of Inert Triplet Model with an exact Z 2 symmetry under which the triplet scalar is odd while all the other SM particles are even which guaranty that the model have a dark matter candidate. Because of Z 2 symmetry, the SM Higgs comes only from the doublet, the couplings h 0 H ± H ∓ and h 0 H ±± H ∓∓ originate only from triplet interaction with SM doublet while in our case there is extra terms that come from the mixing between the doublet and triplet components. In addition, in our study, we will also address the process e − γ → h 0 e − which is not covered in Ref [34].
Study of these processes can be used to shed some light on the couplings h 0 → γγ and h 0 → γZ and their correlation. Clearly, such loop-mediated processes are sensitive to the h 0 γγ and h 0 γZ one loop couplings, and could also be used to disentangle between various BSM models. There-fore, e + e − → h 0 γ and e − γ → h 0 e − would be sensitive to the doubly charged Higgs which contribute to h 0 γγ and h 0 γZ couplings. Moreover, the process e + e − → h 0 γ enjoys a clean final state with a photon and also the handle offered by the SM-like Higgs mass reconstruction at 125 GeV, which is now possible after discovery. We will study the correlation of the diphoton signal strength with the total cross sections of e + e − → h 0 γ and e − γ → h 0 e − and also present some differential cross sections.
The remainder of this paper is organized as follows: we briefly review the basics of the Triplet Higgs Model in Sec. 2. In Sec. 3, we discuss existing experimental constraints. In the subsequent subsections 4.1 and 4.2, we consider in more depth the production cross-sections of e + e − → h 0 γ and e − γ → h 0 e − at the e + e − collider and its e − γ option. We also correlate the production cross section to h 0 → γγ and h 0 → γZ decays. We then present our findings in Sec. 5.

Model framework
In addition to the SM Higgs field Φ ∼ (1, 2, 1/2), the HTM contains an additional SU (2) L triplet Higgs field ∆ ∼ (1, 3, 2) [14,15,16,17]. Both multiplets are represented by After the EWSB, the neutral components φ 0 and δ 0 develop their vev's respectively that read as It's worth mentioning that the gauge bosons get their masses both from the doublet and the triplet and the electroweak scale is fixed from W mass by On the other side, the kinetic and gauge-interaction of the new field ∆ are encoded in the lagrangian term that has the following form where the covariant derivative is given by In the above, c denotes the charge conjugation, while L is the SU (2) L doublets of left-handed leptons. Once ∆ is assigned to carry a non-zero lepton number, L = 2, the cubic µ parameter violates explicitly the lepton number at the Lagrangian level. It's worth mentioning here that the light neutrino mass originate from the above Yukawa lagrangian and is proportional to the triplet vev, The scalar potential of the Higgs fields Φ and ∆ is where µ Φ and µ ∆ are real parameters with dimension of mass, µ is a mass term that controls trilinear couplings between Φ and ∆ and λ 1−4 are dimensionless quartic Higgs couplings. By computing the mass matrices from Eq.(4) taking into account the two minimization conditions, seven physical Higgs states in the mass basis arise and could be written in the weak eigenstate basis. Indeed, in addition to the doubly-charged Higgs bosons, H ±± , the HTM predicts a pair of charged Higgs H ± , that appear together with the charged Goldstone G ± after a unitary rotation R β = {{c β , −s β }, {s β , c β }} with β angle between the non-physical fields φ ± and δ ± , with s x (c x ) stands for sin x (cos x).
The physical masses of the doubly and singly charged Higgs boson H ±± and H ± can be written as The CP-even and CP-odd neutral Higgs bosons h 0 , and H 0 have the physical masses In the above A H , B H and C H are the entries of the CPeven mass matrix, given by, where λ + ij = λ i + λ j , and s 2x stands for sin 2x. Regarding the CP-odd Higgs field, the A 0 has the mass term given by In addition, it should be noted that the previously mentioned mixing angles can be determined in terms of the multiplets vev's and the dimensionless couplings as follows, Furthermore, we consider throughout our analysis a different hierarchy between m H ±± and m H ± , which mainly depends on λ 4 sign (e.g. for positive λ 4 , the H ±± is lighter than H ± ), leading to a splitting that can be expressed by It is worth noting that it is possible to invert these masses to write the quartic couplings λ and λ i 's and µ(or M 2 ∆ ) in terms of the 5 physical scalar masses and the mixing angles as done in [19]. Therefore, in our numerical investigation, to fully describe the scalar sector of HTM, we will take the lightest h 0 as SM-like, and yet use the following set of parameters The following section describes the various direct experimental constraints on the doubly-charged Higgs boson mass and triplet vev.

Theoretical and Experimental Constraints
The parameter space of HTM discussed above is subjected to both theoretical and experimental constraints as we will describe briefly here.
• Perturbativity and Unitarity: The perturbativity translates into the requirement that all quartic couplings of the scalar potential in Eq. (4) obey |λ i | ≤ 8π. Treelevel unitarity can also be imposed by considering a variety of scattering processes: scalar-scalar scattering, gauge boson-gauge boson scattering and scalargauge boson scattering. We impose these unitarity constraints as derived in [19]. • Vacuum Stability: By requiring the HTM to satisfy vacuum stability, we order to maintain the scalar potential V bounded from below, the following constraints on the HTM parameters must be met [19,37] whereλ Furthermore, collider signatures analysis of doubly charged Higgs production could lead to spectacular signature in some cases. Depending on the decay modes of H ±± to either leptonic or bosonic final states, one could have the popular same sign leptons signature. To that end, the triplet vev v ∆ size might be a decisive point. For smaller triplet vev, the H ±± predominantly decays into the samesign leptonic states H ±± → l ± l ± , whereas for larger v ∆ , the gauge boson mode H ±± → W ± W ± becomes dominant [21,22]. A number of studies have been proposed in order to study prospect for doubly charged Higgs production and decay at the LHC [21,22,23,38,39]. Below we discuss the existing constraints on H ±± from collider searches.
-LEP-II: LEP-II detector was used to search for doubly charged Higgs through it decay H ±± → l ± l ± . The limit obtained is m H ±± > 97.3 GeV [40] at 95% C.L.
-LHC: constraints from H ±± pair production and associated production with H ± at the LHC with 13 TeV set a rigorous constraint on m H ±± for v ∆ < 10 −4 GeV through the same-sign dilepton decay H ±± → l ± i l ± j (i, j = e, µ, τ ). In addition, the CMS searches also include the associated production pp → H ±± H ∓ followed by H ± → l ± ν. This combined channel of pairproduction and associated production gives the stringent constraint m H ±± > 820 GeV [41] at 95% C.L for e and µ flavor. The main constraint comes from ATLAS searches through pair-production, which set a lower limit of m H ±± > 870 GeV at 95% C.L [42]. As discussed above, if the triplet vev is larger then H ±± would decay into a pair of gauge bosons [43,44,45], and this would invalidate or, lower the same-sign dileptons limit. Over the past year, the ATLAS experiment has managed in this regard to set a limit for H ±± mass, in such a way that the same-sign W bosons decay mode to be the dominant for doubly-charged Higgs boson. As stipulated by its report, a H ±± boson masses between 200 and 220 GeV are excluded at 95% confidence level [46]. Furthermore, still within the LHC, the golden channel that can give more insights for the doubly-charged Higgs boson is the VBF pp → W * W * → H ±± → W ± W ± . In the HTM, it is well known that once the triplet vev gets larger enough, v ∆ ≥ 10 −4 GeV, the bosonic decay mode H ±± → W ± W ± becomes larger than BR(H ±± → l ± l ± ). At the LHC, CMS with 8 TeV [47] and 13 TeV [48] search for pp → W * W * → H ±± → W ± W ± + X in the framework of Georgi-Machacek (GM) model and set a limit on the doublettriplet mixing angle s H (= sin θ H ) = 2 √ 2v χ /v where v χ is the triplet vev in the GM model. Since in the HTM H ±± W ± W ± = ig 2 v s β / √ 2 and H ±± W ± W ± = ig 2 v s H / √ 2 in the GM, it is clear that the equivalent of s H in the HTM is s β that can be obtained from Eq.(9) as: s β = 2v ∆ /v. Re-interpretation of GM limit on s H imply that s β > 0.18 which can be translated into a limit on the triplet vev. Using Eq.(9), one can 14 GeV which is still far from the stringent bound obtained from δρ constraint.
Note that, for extremely small v ∆ , the mass of the doublycharged Higgs boson is very tightly constrained from pairproduction searches. For a larger triplet vev, this constraint substantially chills out. Indeed, the measured crosssection of the VBF production process probes a quadratically reliance upon the triplet vev and hence, increases for a very large vev. However, the range of v ∆ ∼ 10 −4 − 10 −1 GeV cannot be probed at the 13 TeV LHC in VBF channel, due to the smallness of the production crosssection. Recently, in [49], the authors have looked for pairproduction of doubly charged Higgs H ±± in the case of large v ∆ , and demonstrated that the lighter mass m H ±± ∼ 190 GeV can be probed at the 14 TeV LHC with high luminosity of 3000 fb −1 . In addition, in Ref. [45], by looking to di-lepton decays of H ±± and using LHC 8 TeV run-I data, the limit of m H ±± ≥ 84 GeV have been derived, which is also relevant for large v ∆ .

.1 Processes
In the HTM, at the one-loop level, the processes e + e − → γh 0 and e − γ → e − h 0 are mediated by triangle and selfenergie as well as box diagrams. Hence, they are sensitive to all charged virtual particles inside the loop. We display in Fig.1 the generic Feynman diagrams that effectively contribute to e + e − → γh 0 and e − γ → e − h 0 processes in the HTM.
Our calculation is done in Feynman gauge using dimensional regularization with the help of FeynArts and FormCalc packages [52]. Numerical evaluation of the scalar integrals is done with LoopTools [53]. We have summed up all triangle and boxe diagrams in order to maintain gauge invariance in the final results. As said before, during this calculation we will neglect the electron mass. Since the tree level amplitudes which are suppressed by the electron mass are neglected, Feynman diagrams like Fig. 1-v 2v 3 1 mediated by an off-shell electron are ultraviolet finite because the corresponding counter-terms for h 0 e + e − are proportional to electron mass. We have checked analytically and numerically that the amplitudes are UV finite and independent of the renormalization scale which constitutes a good check of the calculation. In diagrams v1, we depict h 0 γV , V = γ, Z as a generic and the feynman diagrams that contribute are shown in Fig.2. The loop in v4 receives contributions from all SM particles as well as singly and doubly charged Higgs.
In the following, for illustrative purpose and discussions, we introduce the following ratios, which are the total cross sections in the HTM normalized to the SM one. Note that the one-loop amplitudes for h 0 → γγ, γZ, Fig. 2, as well as for the two processes e + e − → γh 0 and e − γ → e − h 0 receive an additional contribution from H ± and H ±± Higgs bosons. We also define the signal strengths R γγ and R γZ as where V = γ or Z These one-loop amplitudes are sensitive to the triple scalar couplings h 0 H ++ H −− and h 0 H + H − which are given in the HTM bȳ If we neglect the terms which contain triplet vev, those couplings are completely fixed by the λ 1 and λ 4 parameters, and depending on their sign; charged Higgs contributions can enhance or suppress e + e − → γh 0 , e − γ → e − h 0 and h 0 → γγ rates, respectively. We also stress that the doubly charged Higgs contribution in the above one-loop amplitudes will enjoy an enhancement by a relative factor four in the amplitudes since H ±± has an electric charge of ±2 units.

Results
We first comment about e + e − → γH in the SM. Like H → γγ and H → γZ, the vertex contribution in e + e − → γH is dominated by the W loops while the top contribution is sub-leading and interfere destructively with the W loops [34]. For center of mass energy ≤ 350 GeV, the SM box contribution is almost of the same order as the vertex and interfere destructively while for higher cm energy ≥ 350 GeV the total cross section is dominated by the boxes and are constructive with the vertex. We start our analysis by emphasizing the impact of the new field ∆. For that, we perform a scan over all the allowed parameters spac, setting h 0 to mimic the observed 125 GeV Higgs boson at the LHC, and taking into account above all theoretical and experimental constraints.
It is worth mentioning that the virtual effects of H ± and H ±± states in h 0 γγ and h 0 γZ couplings bring in a high sensitivity to λ 1 and λ + 14 respectively. This is because the dependence of h 0 H ± H ∓ and h 0 H ±± H ∓∓ triple couplings on λ 1 and λ + 14 comes with the large doublet vev while the  one of λ 2 and λ 3 are associated with the small triplet vev, see eqs. (17) and (18). Therefore, the sensitivity to λ 2,3 in the processes under study is marginal.
In Fig.3 above, we exhibit the allowed range for (λ 1 , λ 4 ) as well as the size of the triple couplingsλ h 0 H + H − ,λ h 0 H ++ H −− . Indeed, the upper panel displays a strong dependency between λ 1,4 couplings and charged Higgs boson masses; m H ± (left) and m H ±± (right). It is clear from this plot the range allowed for −0.4 < λ 1 < 0.8 is rather limited. This is mainly due to the BFB constraints combined with light spectrun m H ± , m H ±± , m A < 280 GeV. It is clear that forλ 1 > 0 and λ 4 < 0, m H ± (resp m H ±± ) takes its larger values which stands below 250 GeV (resp 280 GeV).
The lower panel shows that, according to Eq.(17), the couplingλ h 0 H ±± H ∓∓ is proportional to λ 1 . Such a fact is visible in the left-side where one can see that the sign of λ h 0 H ±± H ∓∓ is completely dictated by λ 1 sign. The situation is quite different forλ h 0 H ± H ∓ which could have both signs for positive or negative λ 1 , see Eq. (18). However, λ h 0 H ± H ∓ coupling have different texture as a function of λ 1 and λ 4 . As it can be seen, for large and negative λ 4 , the couplingλ h 0 H ± H ∓ is maximal and positive and flip sign for a wide range of large and positive λ 4 . Thus, it can be said that λ 1 and λ 4 are important parameters of the model, and more severely restrictions on their values from analysis involving naturalness have been studied in Ref. [54].
In Fig.4 we would like to establish a benchmark for comparing both unpolarized cross section e + e − → h 0 γ and e − γ → e − h 0 as a function of center-of-mass energy √ s with respect to SM one. For this purpose, we also draw the SM values for the cross sections as a function of cm energy. We stress here, as we will see later, the amplitude of the t-channel contribution to e − γ → h 0 e − contains a singularity when cos θ ≈ 1, i.e when the angle between the incoming and outgoing electrons vanish. Therefore, we introduce a cut of 10 • when we evaluate the total cross section for e − γ → h 0 e − . However, in the case of e + e − → γh 0 process, we have checked that the total cross section does not depend on small cut. This is because of a cancelation between t-channel vertices and boxes diagrams.  Fig.4.
+0.2 0.0 As it can be noticed, the cross sections are enhanced near the region √ s ≈ 250 GeV. As far as √ s increases further, the destructive interference between the SM and HTM contributions gets more severe and becomes maximal near the tt threshold, responsible for the dips clearly seen in the figure. After crossing the tt threshold, a constructive or destructive interference with SM contribution depending on the sign of λ 1 which is the same as the sign ofλ h 0 H ±± H ∓∓ . Note that the vertex contribution for e + e − → h 0 γ scales like 1/s and thus drop steeply for large √ s, while for e − γ → e − h 0 which have a t-channel contribution, the drop of the cross section for large √ s is slower than for e + e − → γh 0 .
Concerning the effect of charged Higgses on R γγ (h 0 ) and the cross section σ(e + e − → γ h 0 ) and σ(e − γ → e − h 0 ), we illustrate in Fig.5 the variation of those observable as a function of the parameter λ 1 and the reduced couplingsλ h 0 H ± H ∓ andλ h 0 H ±± H ∓∓ . Hence, the sensitivity to λ 1 < 0 as well asλ h 0 H ± H ∓ < 0 andλ h 0 H ±± H ∓∓ < 0 is particularly striking, as one can see for m H ± above 150 GeV, R γγ is enhanced substantially beyond its SM values. This is due to a constructive interference between the SM contribution dominantly by W + , and that of singly and doubly charged Higgs bosons in h 0 γγ and h 0 γZ couplings. On the other hand, note that both vertices given in Eqs. (18) and (17) contribute to both R γγ and σ(e + e − → γ h 0 ). Therefore, we expect that σ(e + e − → γ h 0 ) would vary in a similar way as R γγ . This fact is clearly seen from the lower panels of Fig.5. Indeed, the cross section can reach values as high as 0.096 fb for negative values of λ 1 , requiring a rather light singly (and/or doubly) charged Higgs bosons in the range [100,200] GeV. Such large enhancement is related to the sensitivity to trilinear reduced couplingsλ h 0 H ± H ∓ andλ h 0 H ±± H ∓∓ , which also depend on λ 1,4 signs. It is, therefore, possible to address a possible correlation between R γ V , V = γ, Z, and R γh 0 (resp. R γ V and R e − h 0 ) as displayed in Fig.6 (resp. Fig.7). Depending on the parameter space, one can predict a positive correlation between these two observable. Thus, it can be seen clearly from these plots that when R γ V (h 0 ) > 1 we almost have σ(e + e − → γ h 0 ) > σ(e + e − → γ H SM ) (resp. σ(e − γ → e − h 0 ) > σ(e − γ → e − H SM )) and vice versa. Further improvement may be achieved, reflecting the charged Higgs masses dependence on these two observable, with regards to λ 1 and 2λ 1 + λ 4 signs, the charged Higgs loops interfere constructively (destructively) with the SM loops. Hence, the lighter the charged Higgs masses are, the larger the enhancement in both the total cross sections σ(e + e − → γ h 0 ), σ(e − γ → e − h 0 ) and the signal strength R γ V as illustrated in the right of Fig.5.
Ultimately it is interesting to understand the differential cross section for both processes e + e − → γh 0 and e − γ → e − h 0 , as well as the structure of the correlation between R γγ and R γ Z for the observed h 0 SM-like. Such correlation is exhibited in Fig.8 (left) for fixed values of µ and v ∆ and a scan over λ 1 , λ 4 , which demonstrate that these two decay modes are generally correlated, and typically an R γγ 1 will be consistent with the model for R γ Z 1. The middle side of Fig.8 shows the distribution for the differential cross section as a function of the transverse momentum of the Higgs boson h 0 (p h 0 T ), such a computation is carried out for various value of √ s = 250, 300, 500 GeV, employing a calculation of the one-loop scattering amplitudes for all relevant partonic channels. It is obvious from the p h 0 T distribution that there is a greater likelihood of producing the h 0 boson with a small transverse momentum. Furthermore, the cross-section is expected to increase as the energy decrease and the increase will be faster at lower p h 0 T values. We also show in Fig.(8) the differential cross section dσ(e − γ → e − h 0 )/d cos θ for three center-of-mass energies √ s = 250, 300 and 500 GeV. Such a differential cross section gets significantly enhanced near the forward direction cos θ ≈ 1, which is due to the t-channel diagram (v 1 ) in Fig.1 as explained below.
Finally, Fig.9 displays differential cross section for e − e + → γh 0 in both SM and HTM for two values of √ s = 250 GeV (left) and 500 GeV. As expected, in the absence of new Lorentz structure in the HTM, the differential cross section in the HTM possess the same shape as in the SM and is slightly shifted up due to the charged Higgses effects.

Conclusions
The LC is expected to play a crucial role in understanding the nature of the Higgs boson, which is just getting    started, and will have a lot to add to whatever the LHC will find out. In this paper, we have studied, in the framework of the HTM, the one-loop processes e + e − → γh 0 and e − γ → e − h 0 in the Feynman gauge using dimensional regularization for the future LC machine, where h 0 is the lightest, neutral, CP-even Higgs boson. We have shown that the singly (-doubly) charged Higgs loops in HTM can modify significantly the cross section compared to the SM predictions, depending on the parameter λ 1 and λ 4 which controls the contribution of the charged Higgs bosons in the loops. We find that such cross sections for the studied processes are quite sensitive to these parameters; so that the observable R γh 0 that we defined for the LC can be away from unity implying the presence of new charged particles in the loops. Such new charged particles would also contribute to the one loop couplings h → γγ and h → γZ. Therefore, we have shown that the correlation between R γh 0 , R e − h 0 and R γγ (h 0 ) can be mainly positive for √ s = 250 GeV depending on the HTM parameter space. We also illustrate on one hand, the transverse momentum distribution for the e + e − → γh 0 which shows an enhancement near p h 0 T ≈ √ s/2 and on the other hand the differential cross section for e + e − → γh 0 for different center of mass energy.