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CP violation in lepton-number-conserving processes through heavy Majorana neutrinos at future lepton colliders

Zhe Wang wzhe@mail.sdu.edu.cn School of Physics, Shandong University, Jinan, Shandong 250100, China    Xing-Hua Yang yangxinghua@sdut.edu.cn School of Physics and Optoelectronic Engineering, Shandong University of Technology, Zibo, Shandong 255000, China    Xin-Yi Zhang xinyizhang@mail.sdu.edu.cn School of Physics, Shandong University, Jinan, Shandong 250100, China
Abstract

Small neutrino masses confirmed in the neutrino oscillation experiments indicate the need for new physics beyond the standard model. Seesaw mechanism is an interesting way to extend the standard model for explaining the neutrino masses. In a low-scale type-I seesaw mechanism, the tiny masses of neutrinos can be explained by heavy Majorana neutrino masses. Heavy Majorana neutrinos can lead to lepton-number-violating processes and the induced CP violation can contribute to the baryon asymmetry in the Universe. Heavy Majorana neutrinos can also lead to lepton-number-conserving processes and in this paper, we study the CP violation in lepton-number-conserving processes through heavy Majorana neutrinos at future lepton colliders. New possible observations of CP violation can also be connected to evidences of new physics beyond the standard model.

pacs:
14.60.Pq, 14.60.St

I INTRODUCTION

In the standard model (SM), the neutrinos are strictly massless due to the absence of right-handed chiral states and the requirement of SU(2)LSU(2)_{L} gauge invariance and renormalizability. The tiny masses of neutrinos confirmed in neutrino oscillation experiments show that the SM may not be complete. In fact, the SM has some open problems, such as the flavor puzzle, the existence of the dark matter (DM), the baryon asymmetry in the Universe. However, by introducing heavy Majorana neutrinos Canetti:2012vf ; Caputo:2018zky ; Gninenko:2012anz , we can solve some of them. A sector of Majorana neutrinos connected to the SM by mixing with the SM neutrinos could exhibit additional CP violation needed to explain the baryon asymmetry in the Universe. Heavy Majorana neutrinos can be used to explain the tiny masses of neutrinos via the interesting type-I seesaw mechanism Mohapatra:1979ia ; Minkowski:1977sc ; Gell-Mann:1979vob .

In this work, we introduce three generations of right-handed heavy Majorana neutrinos in SM and the Dirac neutrino mass terms will be generated after spontaneous gauge symmetry breaking. The heavy Majorana neutrinos will lead to processes with violation of lepton number by two units ΔL=2\Delta L=2, such as the neutrinoless double-beta decay (0νββ0\nu\beta\betaFurry:1939qr ; Elliott:2004hr . It is an interesting process that the Majorana phase may induce additional CP violation effect. In previous works Lu:2021vzj ; Lu:2022pvw ; Lu:2022wsm , we have studied the lepton-number-violating (LNV) processes with heavy Majorana neutrinos and the induced CP violation. Not only that, the heavy Majorana neutrinos can also lead to lepton-number-conserving (LNC) processes, in this work, we study several interesting LNC processes caused by heavy Majorana neutrinos at future lepton colliders. The CP violation stems from the interference of contributions from different heavy Majorana neutrinos, and even one heavy Majorana neutrino can lead to CP violation in these processes by the intereference of contributions from the ss-channel processes and the tt-channel processes. We also investigate the prospects for searching for these heavy Majorana neutrinos at future lepton colliders like the Muon Collider (MuC) MuonCollider:2022nsa and the International Linear Collider (ILC) Behnke:2013xla . We analyse the processes e+eνe¯Niνe¯eqq¯e^{+}e^{-}\rightarrow\bar{\nu_{e}}N_{i}\rightarrow\bar{\nu_{e}}e^{-}q\bar{q}^{\prime} at e+ee^{+}e^{-} collision with ILC running at 500 GeV, 1000 GeV, 3000 GeV and the processes μ+μνμ¯Niνμ¯μqq¯\mu^{+}\mu^{-}\rightarrow\bar{\nu_{\mu}}N_{i}\rightarrow\bar{\nu_{\mu}}\mu^{-}q\bar{q}^{\prime} at μ+μ\mu^{+}\mu^{-} collision with MuC running at 3000 GeV and 10 TeV, where NiN_{i} represent three generations of heavy Majorana neutrinos N1N_{1}, N2N_{2}, N3N_{3}.

This paper is organized as follows. In Section II, we reviewed the model we used to describe heavy Majorana neutrinos. In Section III, we analyse the CP violation in processes e+eνe¯Niνe¯eqq¯e^{+}e^{-}\rightarrow\bar{\nu_{e}}N_{i}\rightarrow\bar{\nu_{e}}e^{-}q\bar{q}^{\prime} and μ+μνμ¯Niνμ¯μqq¯\mu^{+}\mu^{-}\rightarrow\bar{\nu_{\mu}}N_{i}\rightarrow\bar{\nu_{\mu}}\mu^{-}q\bar{q}^{\prime}. The possibility for measuring CP violation at future lepton colliders is studied in Section IV. Finally, a short summary is given in Section V.

II HEAVY MAJORANA NEUTRINOS BEYOND THE SM

The heavy neutrinos can only interact with the SM through mixing effects, which come from a mass matrix between the electroweak doublet neutrinos and Majorana neutrinos. In this work we extend the standard model with three right-handed heavy Majorana neutrinos. The Lagrangian of the model  Mekala:2022cmm we used in our process is given by:

=SM+N+WN+ZNν+HNν,\mathcal{L}=\mathcal{L}_{SM}+\mathcal{L}_{N}+\mathcal{L}_{WN\ell}+\mathcal{L}_{ZN\nu}+\mathcal{L}_{HN\nu}, (1)

where N\mathcal{L}_{N} is a sum of kinetic and mass terms for heavy Majorana neutrinos:

N=12(Ni¯i/NimNiNi¯Ni),\mathcal{L}_{N}=\frac{1}{2}\left(\bar{N_{i}}i\partial\!\!\!/N_{i}-m_{N_{i}}\bar{N_{i}}N_{i}\right), (2)

where i=1,2,3i=1,2,3, stand for three heavy Majorana neutrinos. The WN\mathcal{L}_{WN\ell} corresponds to heavy neutrino interactions with a WW boson:

WN=g2Wμ+i=13=eτNi¯RiγμPL+h.c.,\displaystyle\mathcal{L}_{WN\ell}=-\frac{g}{\sqrt{2}}W^{+}_{\mu}\sum_{i=1}^{3}\sum_{\ell=e}^{\tau}\bar{N_{i}}R_{\ell i}^{\ast}\gamma^{\mu}P_{L}\ell^{-}+\text{h.c.}, (3)

The ZNν\mathcal{L}_{ZN\nu} to interactions with a ZZ boson:

ZNν=g2cosθWZμi=13=eτNi¯RiγμPLνl+h.c.,\mathcal{L}_{ZN\nu}=-\frac{g}{2\text{cos}\theta_{W}}Z_{\mu}\sum_{i=1}^{3}\sum_{\ell=e}^{\tau}\bar{N_{i}}R_{\ell i}^{\ast}\gamma^{\mu}P_{L}\nu_{l}+\text{h.c.}, (4)

then the HNν\mathcal{L}_{HN\nu} to interactions with a Higgs boson:

HNν=gmN2MWhi=13=eτNi¯RiPLνl+h.c.,\displaystyle\mathcal{L}_{HN\nu}=-\frac{gm_{N}}{2M_{W}}h\sum_{i=1}^{3}\sum_{\ell=e}^{\tau}\bar{N_{i}}R_{\ell i}^{\ast}P_{L}\nu_{l}+\text{h.c.}, (5)

Finally we write the weak charged-current interaction Lagrangian as:

cc=g2Wμ+m=13=eτVmνm¯γμPLg2Wμ+i=13=eτNi¯RiγμPL+h.c.,\displaystyle\mathcal{L}_{\rm cc}=-\frac{g}{\sqrt{2}}W^{+}_{\mu}\sum_{m=1}^{3}\sum_{\ell=e}^{\tau}V_{\ell m}^{\ast}\overline{\nu_{m}}\gamma^{\mu}P_{L}\ell^{-}-\frac{g}{\sqrt{2}}W^{+}_{\mu}\sum_{i=1}^{3}\sum_{\ell=e}^{\tau}\bar{N_{i}}R_{\ell i}^{\ast}\gamma^{\mu}P_{L}\ell^{-}+\text{h.c.},\; (6)

Here VmV_{\ell m} is the neutrino mixing matrix that can be measured from the neutrino oscillation experiments. The RiR_{\ell i} indicates the mixing between heavy Majorana neutrinos and charged-leptons, which can be parameterized as Xing:2007zj .

Ri=|Ri|eiϕi,=e,μ,τ,i=1,2,3.R_{\ell i}=\left|R_{\ell i}\right|e^{i\phi_{\ell i}},~{}~{}~{}\ell=e,\mu,\tau,~{}~{}~{}i=1,2,3\;. (7)

The mixing between heavy Majorana neutrinos and ZZ boson is different from those between heavy neutrinos and WW bosons, so the phases ϕi\phi_{\ell i} should be set to different values. In this work we have at least 6 different phases as free parameters. For convenience, we set the phases between heavy neutrinos and ZZ boson to ϕi=0\phi_{\ell i}=0, then we will set three free parameters of phases ϕ1=ϕa,ϕ2=ϕb,ϕ3=ϕc\phi_{\ell 1}=\phi_{a},\phi_{\ell 2}=\phi_{b},\phi_{\ell 3}=\phi_{c} which are from mixing between heavy neutrinos and WW bosons to study each process and induced CP violation at ILC and MuC.

Now we give the mixing relations between the neutrino flavor eigenstates and mass eigenstates as followsAtre:2009rg :

νL=m=13VmνmL+i=13RiNiLc.\nu_{\ell L}=\sum_{m=1}^{3}V_{\ell m}\nu_{mL}+\sum_{i=1}^{3}R_{\ell i}N^{c}_{iL}\;. (8)

In this work, we consider the case that the heavy Majorana neutrinos are nearly degenerate, so we set ΓN1ΓN2ΓN3\Gamma_{N_{1}}\approx\Gamma_{N_{2}}\approx\Gamma_{N_{3}}, mN2=mN1+ΓN1/2,mN3=mN2+ΓN1/2m_{N_{2}}=m_{N_{1}}+\Gamma_{N_{1}}/2,m_{N_{3}}=m_{N_{2}}+\Gamma_{N_{1}}/2 and we set mN1m_{N_{1}} in the range of 300 GeV-3000 GeV for ILC, 300 GeV-10 TeV for MuC according to Ref. Mekala:2022cmm and Ref. Li:2023tbx , for these ranges, at ILC, the parameters of the mixing between heavy neutrinos and leptons are set as |Rei|2=|Rμi|2=|Rτi|2=0.0003\left|R_{ei}\right|^{2}=\left|R_{\mu i}\right|^{2}=\left|R_{\tau i}\right|^{2}=0.0003, and at MuC, the mixing parameters |Rμi|2\left|R_{\mu i}\right|^{2} are obviously dependent on mN1m_{N_{1}}, we set the values of |Rμi|2\left|R_{\mu i}\right|^{2} according to the constraint in Fig.10 in Ref. Li:2023tbx .

We simplify the widths of heavy Majorana neutrinos ΓN1,ΓN2,ΓN3\Gamma_{N_{1}},\Gamma_{N_{2}},\Gamma_{N_{3}} according to Refs.Si:2008jd ; Atre:2009rg in expression:

ΓNi{18(GF2mNi5192π3)Σ=e,μ,τ|Ri|2,mNi<MW𝒜(GFmNi382π)Σ=e,μ,τ|Ri|2,𝒜=2(3)[4],mNi>MW(MZ)[MH]\Gamma_{N_{i}}\simeq\left\{\begin{aligned} &18\left(\frac{G_{F}^{2}m_{N_{i}}^{5}}{192\pi^{3}}\right)\Sigma_{\ell=e,\mu,\tau}\left|R_{\ell i}\right|^{2},m_{N_{i}}<M_{W}\\ &{\cal A}\left(\frac{G_{F}m_{N_{i}}^{3}}{8\sqrt{2}\pi}\right)\Sigma_{\ell=e,\mu,\tau}\left|R_{\ell i}\right|^{2},{\cal A}=2(3)[4],m_{N_{i}}>M_{W}(M_{Z})[M_{H}]\\ \end{aligned}\right. (9)

In the range of the mass mN1m_{N_{1}} we consider, we take 𝒜=4{\cal A}=4, so that the widths can be simplified as:

ΓNiGFmNi322πΣ=e,μ,τ|Ri|2\Gamma_{N_{i}}\simeq\frac{G_{F}m_{N_{i}}^{3}}{2\sqrt{2}\pi}\Sigma_{\ell=e,\mu,\tau}\left|R_{\ell i}\right|^{2} (10)

We set the Cabibbo-Kobayashi-Maskawa (CKM) matrix as diagonal with unit entries for simplicity in our calculation. We put all these parameters in the model with FEYNRULES\text{F}_{\text{EYN}}\text{R}_{\text{ULES}} Alloul:2013bka , the MATHEMATICA\text{M}_{\text{ATHEMATICA}} package to calculate Feynman rules associated with the Lagrangian of a given model, and use the model to generate the cross sections of the process with MadGraph5_aMC@NLO Alwall:2014hca .

III CP VIOLATION IN LEPTON-NUMBER-CONSERVING PROCESSES CONTRIBUTED BY HEAVY MAJORANA NEUTRINOS

The Feynman diagrams for our process are given in Fig. 1,

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Figure 1: Feynman diagrams for process +ν¯Niν¯qq¯\ell^{+}\ell^{-}\rightarrow\bar{\nu_{\ell}}N_{i}\rightarrow\bar{\nu_{\ell}}\ell^{-}q\bar{q}^{\prime}

where ±=e±,μ±\ell^{\pm}=e^{\pm},\mu^{\pm}. We can see there are two main diagrams, one is an ss-channel diagram with ZZ boson rare decay and the other one is a tt-channel diagram with WW boson exchange. The NiN_{i} respect three heavy Majorana neutrinos N1,N2,N3N_{1},N_{2},N_{3}. We take q,q=c,sq,q^{\prime}=c,s or u,du,d. The total cross section of this process can be expressed as

σ+ν¯qq¯=12s|+ν¯qq¯|2¯𝑑ips4\sigma_{\ell^{+}\ell^{-}\rightarrow\bar{\nu_{\ell}}\ell^{-}q\bar{q\prime}}=\frac{1}{2s}\int\overline{\left|{\cal M}_{\ell^{+}\ell^{-}\rightarrow\bar{\nu_{\ell}}\ell^{-}q\bar{q\prime}}\right|^{2}}d{\cal L}_{ips4} (11)

where the |+ν¯qq¯|2¯\overline{\left|{\cal M}_{\ell^{+}\ell^{-}\rightarrow\bar{\nu_{\ell}}\ell^{-}q\bar{q\prime}}\right|^{2}} represents the squared matrix elements averaged (summed) over the initial (final) particles for the process with dips4d{\cal L}_{ips4} being the Lorentz invariant phase space of the four final particles. The ss-channel process is dominant at the ZZ-pole (around the mass of the ZZ boson), while for center-of-mass energy above the ZZ-pole, which belongs to the range we choose in this work, the WW exchange contribution is more important. The diagrams with heavy Majorana neutrinos N1N_{1}, N2N_{2} and N3N_{3} will give CP phase ϕa\phi_{a}, ϕb\phi_{b} and ϕc\phi_{c} in their ss-channel diagrams which cause the CP violation of the total process +ν¯jj\ell^{+}\ell^{-}\rightarrow\bar{\nu_{\ell}}\ell^{-}jj, and this CP phase does not exist in the tt-channel diagrams. The total cross section is shown as the function of the center-of-mass energys s\sqrt{s} in Fig. 2. The results in Fig. 2 represent the case at ILC, and the results in Fig. 2 corresponding to the case at MuC. They show that the total cross sections go up as the s\sqrt{s} increase, it means the contributions from tt-channel are more important.

The results for the total cross sections as the function of heavy Majorana neutrino mass mN1m_{N_{1}} at ILC and MuC are shown in Fig. 3 and Fig. 3 respectively.

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Figure 2: The total cross sections for (a) e+eνe¯eqq¯e^{+}e^{-}\rightarrow\bar{\nu_{e}}e^{-}q\bar{q}^{\prime} and (b) μ+μνμ¯μqq¯\mu^{+}\mu^{-}\rightarrow\bar{\nu_{\mu}}\mu^{-}q\bar{q}^{\prime} as versus the center-of-mass energy s\sqrt{s} with all CP phase set to ϕa=ϕb=ϕc=0\phi_{a}=\phi_{b}=\phi_{c}=0 and the Majorana neutrino mass set to mN1=300m_{N_{1}}=300 GeV, and we set |RμN|2=1×105\left|R_{\mu N}\right|^{2}=1\times 10^{-5} in (b).
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Figure 3: The total cross sections for (a) e+eνe¯eqq¯e^{+}e^{-}\rightarrow\bar{\nu_{e}}e^{-}q\bar{q}^{\prime} at s=500\sqrt{s}=500 GeV, s=1000\sqrt{s}=1000 GeV, s=3000\sqrt{s}=3000 GeV and (b) μ+μνμ¯μqq¯\mu^{+}\mu^{-}\rightarrow\bar{\nu_{\mu}}\mu^{-}q\bar{q}^{\prime} at s=3000\sqrt{s}=3000 GeV, s=10\sqrt{s}=10 TeV versus the Majorana neutrino mass mN1m_{N_{1}}. We set |RμN|2=5×106\left|R_{\mu N}\right|^{2}=5\times 10^{-6} in (b).

In Fig. 3, the dashed line represents the case s=500\sqrt{s}=500 GeV at ILC, and the dash-dotted line represents s=1000\sqrt{s}=1000 GeV, full line represents s=3\sqrt{s}=3 TeV. In Fig. 3, the dash-dotted line represents the case s=3\sqrt{s}=3 TeV at MuC, and the full line represents s=10\sqrt{s}=10 TeV. We can see that the cross section decrease quickly as the mN1m_{N_{1}} increase. The difference between the rates of +ν¯qq¯\ell^{+}\ell^{-}\rightarrow\bar{\nu_{\ell}}\ell^{-}q\bar{q\prime} and +ν+q¯q\ell^{-}\ell^{+}\rightarrow\nu_{\ell}\ell^{+}\bar{q}q\prime, where =e,μ\ell=e,\mu may induce the CP asymmetry, which can be defined as

𝒜CP=σ+ν¯qq¯σ+ν+q¯qσ+ν¯qq¯+σ+ν+q¯q,{\cal A}_{CP}=\frac{\sigma_{\ell^{+}\ell^{-}\rightarrow\bar{\nu_{\ell}}\ell^{-}q\bar{q\prime}}-\sigma_{\ell^{-}\ell^{+}\rightarrow\nu_{\ell}\ell^{+}\bar{q}q\prime}}{\sigma_{\ell^{+}\ell^{-}\rightarrow\bar{\nu_{\ell}}\ell^{-}q\bar{q\prime}}+\sigma_{\ell^{-}\ell^{+}\rightarrow\nu_{\ell}\ell^{+}\bar{q}q\prime}}, (12)

As mentioned before, we have three CP phases ϕa,ϕb,ϕc\phi_{a},\phi_{b},\phi_{c} as free parameters, they will cause CP violation in the processes +ν¯qq¯\ell^{+}\ell^{-}\rightarrow\bar{\nu_{\ell}}\ell^{-}q\bar{q\prime}, for the case that if there is only one generation of heavy neutrinos, its ss-channel diagram will give a CP phase but the tt-channel diagram will not, so that this heavy Majorana neutrino will cause CP violation in this proces. We study the CP violation for cases that there is only one heavy Majorana neutrino, two generations of heavy Majorana neutrinos, and three generations of heavy Majorana neutrinos respectively. The results are in following pictures.

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Figure 4: CP violation for (a),(b) e+eνe¯eqq¯e^{+}e^{-}\rightarrow\bar{\nu_{e}}e^{-}q\bar{q}^{\prime} and (c),(d) μ+μνμ¯μqq¯\mu^{+}\mu^{-}\rightarrow\bar{\nu_{\mu}}\mu^{-}q\bar{q}^{\prime} with only one generation of heavy Majorana neutrino N1N_{1} versus CP phase ϕa\phi_{a} and Majorana neutrino mass mN1m_{N_{1}} where in (a) and (c) we set mN1=300m_{N_{1}}=300 GeV. In (a),(b) we set s=1000\sqrt{s}=1000 GeV, |Rμi|2=3×104\left|R_{\mu i}\right|^{2}=3\times 10^{-4}. In (c), (d) we set s=3000\sqrt{s}=3000 GeV, and we set |Rμi|2=1×105\left|R_{\mu i}\right|^{2}=1\times 10^{-5} in (c), |Rμi|2=4×106\left|R_{\mu i}\right|^{2}=4\times 10^{-6} in (d).

We show the results of CP violation as functions of mass mN1m_{N_{1}} and CP phase ϕa\phi_{a} for case with only one generation of heavy Majorana neutrino here. Fig. 4 and Fig. 4 represent ILC case, Fig. 4 and Fig. 4 represent MuC case. We set mN1=300m_{N_{1}}=300 GeV, s=1000\sqrt{s}=1000 GeV when we study the CP violation as the function of CP phases for e+ee^{+}e^{-} case in Fig. 4, and for μ+μ\mu^{+}\mu^{-} case, we set |Rμi|2=1×105\left|R_{\mu i}\right|^{2}=1\times 10^{-5} in Fig. 4. When we study the CP violation as the function of mN1m_{N_{1}}, as the mixing parameter |Rμi|2\left|R_{\mu i}\right|^{2} is obviously dependent on mN1m_{N_{1}} in μ+μ\mu^{+}\mu^{-} case, we set |Rμi|2=4×106\left|R_{\mu i}\right|^{2}=4\times 10^{-6} for μ+μ\mu^{+}\mu^{-} case in Fig. 4 and |Rμi|2=3×104\left|R_{\mu i}\right|^{2}=3\times 10^{-4} in Fig. 4 at the range 300 GeV <mN1<<m_{N_{1}}< 3000 GeV for convenience in this paper. From Fig. 4 and Fig. 4, we can find that the CP violation is independent of the heavy Mjaorana neutrino mass mN1m_{N_{1}}, in Fig. 4 and Fig. 4 we can see that the CP violation is related to CP phase, and the maximum value can reach near 1.25×1041.25\times 10^{-4} at ϕa=±π/2\phi_{a}=\pm\pi/2. This shows that only one generation of Majorana neutrino can lead to CP violation in LNC process even though it is small, which is different from that in LNV process, and the results for μ+μ\mu^{+}\mu^{-} case is not the same as that in e+ee^{+}e^{-} case, the function have the same shape but the values in μ+μ\mu^{+}\mu^{-} case are much smaller than those in e+ee^{+}e^{-}, the differences come from the different value of mixing |Rμi|2\left|R_{\mu i}\right|^{2} we take at ILC and MuC.

The results with two generations of Majorana neutrinos N1N_{1} and N2N_{2} are shown in Fig. 5.

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Figure 5: CP violation for (a),(b) e+eνe¯eqq¯e^{+}e^{-}\rightarrow\bar{\nu_{e}}e^{-}q\bar{q}^{\prime} and (c),(d) μ+μνμ¯μqq¯\mu^{+}\mu^{-}\rightarrow\bar{\nu_{\mu}}\mu^{-}q\bar{q}^{\prime} with two generations of heavy Majorana neutrinos N1,N2N_{1},N_{2} versus CP phase ϕa,ϕb\phi_{a},\phi_{b} and Majorana neutrino mass mN1m_{N_{1}}. In (a) and (c) we set mN1=300m_{N_{1}}=300 GeV. In (a),(b) s=1000\sqrt{s}=1000 GeV, |RμNi|2=3×104\left|R_{\mu_{N_{i}}}\right|^{2}=3\times 10^{-4}. In (c), (d) we set s=3000\sqrt{s}=3000 GeV, and we set |RμNi|2=1×105\left|R_{\mu_{N_{i}}}\right|^{2}=1\times 10^{-5} in (c), |RμNi|2=4×106\left|R_{\mu_{N_{i}}}\right|^{2}=4\times 10^{-6} in (d).

Fig. 5 and Fig. 5 show that the influences on CP violation from different CP phase ϕa\phi_{a} and ϕb\phi_{b}, and when there are two generations of heavy Majorana neutrinos, the maxium value of CP violation will reach the order of magnitude of 1×1031\times 10^{-3}. However, from Fig. 5 and Fig. 5 we can see when there are two heavy Majorana neutrinos, the CP violation will be influenced by mN1m_{N_{1}}.

Finally, the results of the total CP violation with the case that there are three heavy Majorana neutrinos are shown in Fig. 6.

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Figure 6: CP violation for (a),(b) e+eνe¯eqq¯e^{+}e^{-}\rightarrow\bar{\nu_{e}}e^{-}q\bar{q}^{\prime} and (c),(d) μ+μνμ¯μqq¯\mu^{+}\mu^{-}\rightarrow\bar{\nu_{\mu}}\mu^{-}q\bar{q}^{\prime} with three generations of heavy Majorana neutrinos N1,N2,N3N_{1},N_{2},N_{3} versus CP phase ϕa,ϕb,ϕc\phi_{a},\phi_{b},\phi_{c} and Majorana neutrino mass mN1m_{N_{1}} where in (a) and (c) we set mN1=300m_{N_{1}}=300 GeV. In (a),(b) we set s=1000\sqrt{s}=1000 GeV, |RμNi|2=3×104\left|R_{\mu_{N_{i}}}\right|^{2}=3\times 10^{-4}. In (c), (d) we set s=3000\sqrt{s}=3000 GeV, and we set |RμNi|2=1×105\left|R_{\mu_{N_{i}}}\right|^{2}=1\times 10^{-5} in (c), |RμNi|2=4×106\left|R_{\mu_{N_{i}}}\right|^{2}=4\times 10^{-6} in (d).

Fig. 6 and Fig. 6 show that the influence from ϕa\phi_{a}, ϕb\phi_{b} and ϕc\phi_{c} are different, and the CP violation caused by ϕb\phi_{b} are obviously smaller than those from ϕa\phi_{a} and ϕc\phi_{c} when there are three heavy neutrinos, and in this situation, the maximum value of total CP violation is nearly the same with that when there are two heavy neutrinos but a little bit higher.

The results show that the feature of CP violation caused by heavy Majorana neutrinos in LNV processes which we studied in previous works Lu:2021vzj ; Lu:2022pvw ; Lu:2022wsm are different from those in the LNC processes, CP violation in LNC processes are obviously smaller but nonzero. In LNV processes, the CP violation is obviously independent on mass of heavy Majorana neutrinos mN1m_{N_{1}}, but in LNC process, when there are more than one generation of heavy Majorana neutrino, the CP violation will be influenced by mN1m_{N_{1}}, it will decrease as the mN1m_{N_{1}} goes up. In LNV processes, the CP violation exists when there are at least two generations of heavy Majorana neutrinos, but in LNC process, only one generation of heavy Majorana neutrino will cause nozero CP violation though it is small. For the case there are three heavy Majorana neutrinos, we search for the maximum value of CP violation when we running all CP phase ϕa,ϕb,ϕc\phi_{a},\phi_{b},\phi_{c} from π-\pi to +π+\pi where we take the interval of each point as π/10\pi/10, and the maximum value of total CP violation will reach 3.82×1033.82\times 10^{-3} at ϕa=π/2,ϕb=π/2,ϕc=3/5π\phi_{a}=-\pi/2,\phi_{b}=\pi/2,\phi_{c}=3/5\pi in ILC case, and it will reach 7.43×1047.43\times 10^{-4} at ϕa=3/5π,ϕb=π/5,ϕc=π/2\phi_{a}=-3/5\pi,\phi_{b}=\pi/5,\phi_{c}=\pi/2 in MuC case.

IV SEARCH FOR HEAVY MAJORANA NEUTRINOS AT FUTURE LEPTON COLLIDERS

After analysing the CP violation, now we are interested in the prospect of searching for heavy Majorana neutrinos at future lepton colliders, so we analyse the signals and backgrounds at 500 GeV, 1000 GeV, 3000 GeV ILC and 3000 GeV, 10 TeV MuC. In order to identify the isolated lepton or jet, we indentify isolated jets and leptons by angular separation, which can be defined as

ΔRij=Δϕij2+Δηij2,\Delta R_{ij}=\sqrt{\Delta\phi_{ij}^{2}+\Delta\eta_{ij}^{2}}, (13)

where Δϕij(Δηij)\Delta\phi_{ij}(\Delta\eta_{ij}) is the azimuthal angle (rapidity) difference of the corresponding particles. We apply some basic acceptance cuts (referred as cut-I)

pT>10GeV,|η|<2.5,pTj>20GeV,|ηj|<3.0,0.4<ΔRij<3.0p_{T}^{\ell}>10~{}\text{GeV},~{}\left|\eta^{\ell}\right|<2.5,~{}p_{T}^{j}>20~{}\text{GeV},~{}\left|\eta^{j}\right|<3.0,~{}0.4<\Delta R_{ij}<3.0 (14)

In order to purify the signal, the missing transverse energy is required to satisfy (referred as cut-II)

E/T<60 GeVE\!\!\!/_{T}<60\text{~{}GeV} (15)

There are too much diagrams of backgrounds in the SM for this process, so we simulate all of them with the SM model by MadGraph5_aMC@NLO, we also simulate the signals via MadGraph5_aMC@NLO with the New Physics model generated by FEYNRULES\text{F}_{\text{EYN}}\text{R}_{\text{ULES}}. The parton shower and hadronization are performed with Pythia-8.2 Sjostrand:2006za . We also give another cut for our signal process, a WW boson will decay hadronically, and we can reconstructed it from the two jets (j1,j2j_{1},j_{2}). Their invariant mass should be closest to mWm_{W}. This leads to a new cut (referred as cut-III):

|Mj1j2mW|<50GeV,\left|M_{j_{1}j_{2}}-m_{W}\right|<50~{}\text{GeV}, (16)

where j1,j2j_{1},j_{2} are the two jets decayed by WW boson.

In this process, for a better cut at background the transverse momentum of jets HT\text{H}_{\text{T}} is required to satisfy (referred as cut-IV)

HT>200GeV,\text{H}_{\text{T}}>200~{}\text{GeV}, (17)

After all the cuts on the backgrounds and signals, we get the results of statistical significance S/B\sqrt{B} as function of mN1m_{N_{1}} at 500 GeV, 1000 GeV in Fig. 7 and Fig. 7. Here, we set all phases to zero.

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Figure 7: The statistical significance S/BS/\sqrt{B} as a function of mN1m_{N_{1}} with (a) the center-of-mass energy of s=500\sqrt{s}=500 GeV, the integrated luminosity of =1600{\cal L}=1600 fb-1, (b) s=1000\sqrt{s}=1000 GeV, =3200{\cal L}=3200 fb-1, (c) s=3000\sqrt{s}=3000 GeV, =4000{\cal L}=4000 fb-1 at ILC, where all CP phases ϕa,ϕb,ϕc\phi_{a},\phi_{b},\phi_{c} are set to zero.

It is clear that at 500 GeV ILC, a 3σ3\sigma discovery can be made for near 440 GeV mN1\leq m_{N_{1}}\leq 450 GeV with =1600{\cal L}=1600 fb-1, at 1000 GeV ILC, a 5σ5\sigma discovery can be made for near 650 GeV mN1\leq m_{N_{1}}\leq 950 GeV with =3200{\cal L}=3200 fb-1, a 5σ5\sigma discovery can be made for near 2650 mN1\leq m_{N_{1}}\leq 2950 GeV with =4000{\cal L}=4000 fb-1. It’s hard to have a 3σ3\sigma discovery at 3 TeV, 10 TeV MuC, the results are too small that we don’t put the results in this paper. Finally, we give the total cross sections for signal processes in Table. 1.

Table 1: Total cross sections for +ν¯qq¯\ell^{+}\ell^{-}\rightarrow\bar{\nu_{\ell}}\ell^{-}q\bar{q}^{\prime} at 500 GeV, 1000 GeV, 3000 GeV ILC with the integrated luminosity of 1.61.6ab,13.2{}^{-1},3.2ab,14{}^{-1},4ab-1 respectively and at 3000 GeV, 10 TeV MuC with the integrated luminosity of 11ab,110{}^{-1},10ab-1 respectively where all the CP phases ϕa,ϕb,ϕc\phi_{a},\phi_{b},\phi_{c} are set to zero.
σtotal[fb]\sigma_{total}[\text{fb}] at ILC
=1.6ab1{\cal L}=1.6\text{ab}^{-1},s=500\sqrt{s}=500 GeV 3.48
e+eνe¯eqq¯e^{+}e^{-}\rightarrow\bar{\nu_{e}}e^{-}q\bar{q}^{\prime} =3.2ab1{\cal L}=3.2\text{ab}^{-1},s=1000\sqrt{s}=1000 GeV 5.47
=4ab1{\cal L}=4\text{ab}^{-1},s=3000\sqrt{s}=3000 GeV 6.16
=1ab1{\cal L}=1\text{ab}^{-1},s=3000\sqrt{s}=3000 GeV 1.01×1021.01\times 10^{-2}
μ+μνμ¯μqq¯\mu^{+}\mu^{-}\rightarrow\bar{\nu_{\mu}}\mu^{-}q\bar{q}^{\prime} =10ab1{\cal L}=10\text{ab}^{-1},s=10\sqrt{s}=10 TeV 0.241

V SUMMARY

The small neutrino masses show that we need to expand the SM for explaining the tiny neutrino masses. An interesting model is the type-I seesaw mechanism which introduced heavy Majorana neutrinos that can lead to the CP violation in LNV process, the CP violation can give a new source to explain the baryon asymmetry in the Universe via leptogenesis. We have studied the heavy Majorana neutrinos in LNV process and there shold be at least two generations of heavy Majorana neutrinos to generate CP violation by the interference of contributions from different heavy Majorana neutrinos.

In this work, we investigate the heavy Majorana neutrinos in an interesting LNC process, and find that only one generation of heavy Majorana neutrino can lead to CP violation, and several features of CP violation in the LNC process are different from that in LNV process. The CP violation in the LNC process is caused by the interference of contributions from different generations of heavy Majorana neutrinos and from the interference of contribution of the ss-channel diagram and tt-channel diagram. We consider three generations of heavy Majorana neutrinos N1,N2,N3N_{1},N_{2},N_{3}, and the possibility for searching it at future lepton colliders is studied at future lepton colliders 500,1000,3000 GeV ILC, and 3000 GeV,10 TeV MuC. The results show that there are great chances to explore the CP violation effects at future lepton colliders, and the exploring of CP violation can be a probe for studying the underlying new physics.

ACKNOWLEDGEMENTS

Z. Wang, X. H. Yang and X. Y. Zhang thank the members of the Institute of theoretical physics of Shandong University for their helpful discussions. This work is supported in part by National Natural Science Foundation of China (Grants No. 12235008, 12305106) and Natural Science Foundation of Shandong Province (Grant No. ZR2021QA040).

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