Pair production of the singlet vector-like B quark at the CLIC
Abstract
Vector-like quarks (VLQs) are a common feature of many scenarios of new physics beyond the Standard Model (SM), which generally decay into a SM third-generation quark with a SM gauge boson, or a Higgs boson. The presence of a new exotic decay mode of VLQs will reduce the branching ratios of these standard decay modes and thus relax the current mass exclusion limits from LHC experiments. Based on a model-independent framework, we investigate the prospect of discovering the pair production of the weak-singlet VLQ- at the future 3-TeV Compact Linear Collider (CLIC), by focusing on the final states including one boson and four -jets via two types of modes: and . By performing a rapid detector simulation of the signal and background events, and considering the initial state radiation and beamstrahlung effects, the exclusion limit at the 95% confidence level and the discovery prospects are respectively obtained on the branching ratio of and the VLQ- masses at the future 3-TeV CLIC with an integrated luminosity of 5 ab-1.
I Introduction
New heavy quarks appear in a variety of new physics models beyond the Standard Model (SM), formulated to obtain an answer to the problem of the naturalness of the electroweak (EW) scale DeSimone:2012fs ; ArkaniHamed:2002qy ; Han:2003wu ; Chang:2003vs ; Agashe:2004rs ; He:1999vp ; Wang:2013jwa ; He:2001fz ; He:2014ora . Vector-like quarks (VLQs) are spin 1/2 particles characterized by having left- and right-handed components defined by the same color and EW quantum numbers Aguilar-Saavedra:2013qpa , and thus could still be viable under the present searches. However, an extra fourth generation of SM-like quarks He:2001tp ; Chen:2012wz should be much heavier due to the EW precision constraints, and thus a certain non-perturbative method is needed to reliably analyze the strongly coupled Yukawa sector of these extra heavy chiral quarks. VLQs can have different charge assignments under the SM EW gauge group . Hence, there exists the possibility of having multiple VLQs, including electroweak singlet [, ], electroweak doublets [ or ], or electroweak triplets [ or ]. It is generally assumed that the VLQs decay into a SM third-generation quark with a SM gauge boson or a Higgs boson, therefore providing a rich phenomenology at future high-energy colliders Atre:2011ae ; Cacciapaglia:2011fx ; Nutter:2012an ; Okada:2012gy ; Buchkremer:2013bha ; Yang:2014usa ; Matsedonskyi:2014mna ; Backovic:2014uma ; Barducci:2017xtw ; Cacciapaglia:2018lld ; Cacciapaglia:2018qep ; Liu:2017sdg ; Moretti:2017qby ; Liu:2019jgp ; Buckley:2020wzk ; Deandrea:2021vje ; Tian:2021oey ; Tian:2021nmj ; Yang:2021btv ; Han:2022npb ; Han:2022jcp ; Han:2023jzm ; Alves:2023ufm .
For a vector-like -quark (VLQ-) with electric charge -(1/3)e, direct searches generally assume three standard decay channels: , , and . Very recently, ATLAS and CMS collaborations primarily focus on the quantum chromodynamics (QCD)-induced pair production modes of VLQs and lead to lower bounds on the VLQ masses of approximately 1-1.5 TeV ATLAS:2018tnt ; ATLAS:2018ziw ; CMS:2018zkf ; CMS:2019eqb ; CMS:2020ttz ; ATLAS:2021ibc . Using Run 2 data with a total integrated luminosity of 137 fb-1, the CMS Collaboration recently presented a search for VLQ- pair production in the fully hadronic final state CMS:2020ttz , and excluded their masses up to 1.57 and 1.39 TeV for 100% and 100% , respectively. The ATLAS Collaboration presented a search for the pair production of VLQs optimized for decays into a boson and a third-generation SM quark ATLAS:2022hnn . The lower limits on the masses of VLQ- are 1.20 TeV for the weak-isospin singlet model and 1.42 TeV for 100% cases. However, these bounds would be relaxed if such VLQs were to have non-standard decay channels. Recently, exotic decays of the VLQs in different set-ups with different collider signatures have been considered in the literature Aguilar-Saavedra:2017giu ; Das:2018gcr ; Benbrik:2019zdp ; Cacciapaglia:2019zmj ; Aguilar-Saavedra:2019ghg ; Zhou:2020byj ; Wang:2020ips ; Corcella:2021mdl ; Cacciapaglia:2021uqh ; Cui:2022hjg ; Banerjee:2022izw ; Banerjee:2022xmu ; Bhardwaj:2022wfz ; Bhardwaj:2022nko ; Bardhan:2022sif .
Compared with the complicated QCD background at the hadron colliders, the future high-energy linear collider is a precision machine with which the properties of such new VLQs can be measured precisely Kong:2007uu ; Senol:2011nm ; Guo:2014piv ; Liu:2014pts . In particular, the final stage of Compact Linear Collider (CLIC) will operate at energy of 3 TeV CLICDetector:2013tfe , and any such new particles can be produced with sizable rate up to the kinematic limit of 1.5 TeV, and in some cases up to 3 TeV, via single production mechanisms Franceschini:2019zsg . Recently, the single production processes of VLQs at the CLIC have been widely studied via different decay modes Qin:2021cxl ; Han:2021kcr ; Han:2021lpg ; Qin:2022mru ; Han:2022exz ; Han:2022zgw ; Han:2022rxy ; Yang:2023wnv . Unlike the single production mode, the production of VLQs pairs is model-independent, i.e., their cross sections depend only on their masses Qin:2023zoi . In this paper we will focus on the illustrative examples of VLQ- pairs interacting with the third generation of SM quarks, and we will analyze their pair production signatures via the standard decay channels at the future 3-TeV CLIC. Furthermore, we will estimate the reach for discovering (or excluding) VLQ- in which it is assumed that the exotic decay mode is possible and take the branching ratio (BR) of as a free parameter.
This paper is organized as follows: in Sec. II, we briefly describe the couplings of the singlet VLQ- with the SM particles in the simplified model and the direct LHC constraints on its mass and the branching ratio of . In section III, we discuss the pair production process at the 3-TeV CLIC, and perform a detailed collider analysis of the relevant signals and backgrounds. Finally, we provide a summary in Sec. IV.
II Singlet VLQ- in the simplified model
A generic parameterization of an effective Lagrangian for the singlet VLQ- is given by 333 Details are provided on the URL http://feynrules.irmp.ucl.ac.be/wiki/VLQ_bsingletvl.
(1) | |||||
where is the gauge coupling constant, and there are two free parameters: the VLQ- quark mass and the coupling strength to SM quarks in units of standard couplings, .
Assuming an almost degenerate VLQ mass hierarchy, they are generally assumed to decay into a third-generation quark and either a boson or a Higgs boson. For a heavy weak-isospin singlet VLQ-, the relationship of the BRs of three standard decay modes is
(2) |
which is a good approximation as expected from the Goldstone boson equivalence theorem He:1992nga ; He:1993yd ; He:1994br ; He:1996rb ; He:1996cm . With the introduction of the new decay modes , the sum of the above three standard decay modes changes to
(3) |
where is the BR for the new exotic decay channel, such as (an additional scalar or pseudoscalar particle Bhardwaj:2022nko ; Bardhan:2022sif ). A smaller BR in the new mode implies larger BRs in the SM modes. Based on Eqs. (2-3), we can obtain
(4) |
In this case, it is instructive to analyze the current constraints from direct searches of VLQ-. Very recently, Refs. Bhardwaj:2022nko ; Bardhan:2022sif recast the current LHC searches to put mass exclusion bounds on VLQ- as a function of the branching ratio in the new decay mode. In Fig. 1, we show the exclusion mass limits on VLQ- as a function of according to Eq. (4) and the results in the literature Bhardwaj:2022nko , where they recast the relevant limits from the available exclusive CMS:2019eqb ; CMS:2020ttz and inclusive ATLAS:2021ibc searches to select the strongest one. From the rescaled VLQ- limits in Fig 1, one can see the VLQ- mass could be smaller than 1.3 TeV for the smaller BR of the standard decay mode , which implies that the VLQ- could be pair produced at the future 3-TeV CLIC.
III Collider simulation and analysis
In order to make a prediction for the signal, we calculate the production cross section for the process at leading order (LO). Note that here the effects of initial state radiation (ISR) and beamstrahlung are also considered at the 3-TeV CLIC in MadGraph5_aMC_v3.3.2 mg5 by adding the following commands in the run_card:
set lpp1 +3 set lpp2 -3 set pdlabel clic3000ll
In Fig. 2, we show the dependence of the cross sections as a function of with (without) ISR and beamstrahlung effects. One can see that the cross sections can be changed with ISR and beamstrahlung effects compared with those without ISR and beamstrahlung effects. In the region of [1000, 1490] GeV, the ratios of cross sections with and without ISR and beamstrahlung effects are changed from 0.96 to 0.43; thus, it is necessary to consider these effects at the future 3-TeV CLIC, especially for the high VLQ- masses. For TeV, the cross section can reach about 3.94 (1.29) fb with ISR and beamstrahlung effects.
Under the narrow-width approximation (NWA), it is possible to separate and factorize production and decay of the heavy quarks, thus allowing for a model-independent analysis of the results Moretti:2016gkr . For the processes and , their cross sections can be written as
Assuming the relationship of , we will take as a free parameter in the remainder of this article.
We demand that a pair-produced VLQ- event should have at least one boson and four -jets, whith one pair of -jets decaying from a boson or a Higgs boson,
(5) |
In the next section, we will perform the Monte Carlo simulation and explore the discovery potentiality of VLQ- through the subsequent leptonic decay channel and the invisible decay channel , respectively. To generate events for each signal benchmark, we pick model parameters such that and while ensuring that the NWA remains valid for VLQ-.
Monte Carlo event simulations for the signal and SM background are interfaced to Pythia 8.20 pythia8 for fragmentation and showering. All event samples are fed into the Delphes 3.4.2 program deFavereau:2013fsa with the CLIC detector card designed for 3 TeV Leogrande:2019qbe . In our analysis, jets are clustered with the Valencia Linear Collider (VLC) algorithm Boronat:2014hva ; Boronat:2016tgd in exclusive mode with a fixed number of jets ( where corresponds to the number of partons expected in the final state) and fixed-size parameter . The -tagging efficiency is taken as the loose working points with 90% b-tagging efficiency in order not to excessively reduce the signal efficiency. Finally, event analysis is performed by using MadAnalysis 5 ma5 .
III.1 The decay channel
In this subsection, we analyze the signal and background events at the 3-TeV CLIC through the () decay channel:
(6) |
For this channel, the typical signal is two opposite-sign same-flavor (OSSF) leptons coming from one boson and four -tagged jets, with a pair of -tagged jets coming from a boson or a Higgs boson. The dominant SM backgrounds come from the SM processes and . Note that the contributions from the processes , , and are also included with the decay modes , , and .
To identify objects, we choose the basic cuts at parton level for the signals and SM backgrounds as follows:
(7) |
where denotes the separation in the rapidity-azimuth plane, and are the transverse momentum of leptons, -jets, and light jets.
In Fig. 3, we plot differential distributions for signals and SM backgrounds, including the invariant mass distribution for the boson (), the transverse momentum distributions of the leading and sub-leading leptons (), the transverse momentum distributions of the leading and sub-leading -jets (), the invariant mass distribution for the boson or Higgs boson (), and the separations . For the signal, the leptons and are two OSSF leptons that are assumed to be the product of the boson decay, and at least two -tagged jets are assumed to be the product of one boson or a Higgs boson decay. Based on these kinematic distributions, we can impose the following set of cuts:
-
•
Cut-1: There are exactly two isolated leptons (), and the invariant mass of the boson is required to have , and the transverse momenta of two leptons are required .
-
•
Cut-2: There are exactly four -tagged jets (), and the transverse momenta of the leading and sub-leading -jet are required and .
-
•
Cut-3: The invariant masses of the boson or the Higgs boson are required to have with .
Cuts | Signals | Backgrounds | ||||
---|---|---|---|---|---|---|
1200 GeV | 1300 GeV | 1400 GeV | ||||
Basic | 0.031 | 0.024 | 0.015 | 0.005 | 0.004 | |
Cut-1 | 0.023 | 0.018 | 0.012 | 0.0025 | 0.0021 | |
Cut-2 | 0.012 | 0.009 | 0.006 | 0.0012 | 0.00055 | |
Cut-3 | 0.0043 | 0.0036 | 0.0026 | 0.00026 | 0.00015 |
We present the cross sections of three typical signals ( GeV) and the relevant backgrounds after imposing the cuts in Table 1. One can see that all the SM backgrounds are suppressed very efficiently, while the signals still have relatively good efficiency at the end of the cut flow. The cross section of the total SM background is about fb.
III.2 The decay channel
In this subsection, we analyze the signal and background events through the decay channel of the invisible decays :
(8) |
For this channel, the main SM backgrounds come from the processes and with the cross sections of 21.7 fb and 2.5 fb, respectively. Note that the contributions from the processes , , , , , , , and are also included with the decay modes , , and .
Obviously, the signal events should contain large missing transverse energy from the boosted boson. Furthermore, at least two -tagged jets are coming from the boson or Higgs boson decay. In order to obtain some hint of further cuts for reducing the SM backgrounds, we analyzed the normalized distributions of the missing transverse energy , the transverse momentum distributions of the leading and sub-leading -jets , the separations , the invariant mass distribution , and the scalar sum of the transverse energy of all final-state jets for signals and SM backgrounds as shown in Fig. 4. Based on these kinematic distributions, a set of further cuts are given as:
-
•
Cut-1: The transverse missing energy is required .
-
•
Cut-2: Any electrons and muons are forbidden () and there are exactly four -tagged jets (). Furthermore, the transverse momenta of the leading and sub-leading -jets are required and . The invariant masses of the remaining two -tagged jets are required to have with .
-
•
Cut-3: The scalar sum of the transverse energy of all final-state jets .
Cuts | Signals | Backgrounds | ||||
---|---|---|---|---|---|---|
1200 GeV | 1300 GeV | 1400 GeV | ||||
Basic | 0.093 | 0.071 | 0.044 | 2.44 | 4.51 | |
Cut-1 | 0.085 | 0.066 | 0.042 | 0.44 | 1.36 | |
Cut-2 | 0.016 | 0.013 | 0.0093 | 0.0044 | 0.011 | |
Cut-3 | 0.015 | 0.013 | 0.0088 | 0.0019 | 0.0037 |
We summarize the cross sections of three typical signals ( GeV) and the relevant backgrounds after imposing the cuts in Table 2. One can see that the total SM backgrounds are suppressed very efficiently, with a cross section of about fb.
III.3 Discovery and exclusion significance
In order to analyze the observability, we use the median significance to estimate the expected discovery and exclusion significance Cowan:2010js :
(9) | ||||
where , and are the numbers of signal and background events at a given luminosity, respectively, and is the percentage systematic error on the SM background estimate. In the limit of , these expressions can be simplified as
(10) | ||||
It is instructive to acknowledge systematic uncertainties at the experiment which can effect our results. To show this, we include a 10% systematic uncertainty alongside the null systematic uncertainty results.
In Fig. 5, we plot the 95% CL exclusion limit and sensitivity reaches for as a function of at the 3-TeV CLIC with an integrated luminosity of 5 ab-1 for two decay channels with the aforementioned two systematic error cases of and . We find that with a realistic 10% systematic error, the sensitivities are slightly weaker than those without any systematic error. For the decay channel, the VLQ- quark can be excluded in the region of and [1000, 1490] GeV at the 3-TeV CLIC with an integrated luminosity of 5 ab-1, while the discover region can reach and [1000, 1420] GeV. For the decay channel, the VLQ- quark can be excluded in the region of and [1000, 1490] GeV, and the discover region can reach and [1000, 1430] GeV at the 3-TeV CLIC with an integrated luminosity of 5 ab-1.
Next, we combine the significance with by using the results from the above two decay channels with . One can see that the singlet VLQ- can be excluded in the regions of and [1000, 1490] GeV at the 3-TeV CLIC with integrated luminosity of 5 ab-1, while the discover regions can reach and [1000, 1450] GeV. For comparison, we also present the observed 95% CL exclusion limits at the 13-TeV LHC and the predicted exclusions at the future HL-LHC with an integrated luminosity of 3000 fb-1. For simplicity, the exclusion limits for the HL-LHC are obtained by scaling the current LHC limits with the increased luminosity. We can observe that the future CLIC with and an integrated luminosity of 5 ab-1 could provide better sensitivity than that reported in current experimental searches, and even better sensitivity than the future HL-LHC in some mass regions of VLQ-B (e.g., 1200-1500 GeV).
IV Conclusion
In this work, we have concentrated on the pair production of the singlet VLQ- at the future 3 TeV CLIC in a simplified model. With the increasing branching in the extra decay mode, the existing limits on VLQs can be relaxed, so we first reinterpret the latest mass-exclusion limits for VLQ- in terms of . Then we perform a full simulation for the signals and the relevant SM backgrounds on the final states including one boson and four -jets via two types of modes: and . We present the 95% CL exclusion limits and discovery prospects in the parameter plane of the two variables and the VLQ- masses at the future 3-TeV CLIC with an integrated luminosity of 5 ab-1. The results show that the VLQ- quark can be excluded in the region of and [1000, 1490] GeV at the 3- TeV CLIC with integrated luminosity of 5 ab-1, while the discover region can reach and [1000, 1450] GeV. We therefore expect that the signatures studied here will provide complementary information for detecting such VLQ-, including non-standard decay modes, at the future 3-TeV CLIC.
Acknowledgements.
The work is supported by the Project of Innovation and Entrepreneurship Training for College Students in Henan Province (202310478033).References
- (1) A. De Simone, O. Matsedonskyi, R. Rattazzi, and A. Wulzer, JHEP 04, 004 (2013).
- (2) N. Arkani-Hamed, A. G. Cohen, E. Katz, and A. E. Nelson, JHEP 07, 034 (2002).
- (3) T. Han, H. E. Logan, B. McElrath and L. T. Wang, Phys. Rev. D 67, 095004 (2003).
- (4) S. Chang and H. J. He, Phys. Lett. B 586, 95-105 (2004).
- (5) K. Agashe, R. Contino, and A. Pomarol, Nucl. Phys. B719 165 (2005).
- (6) H. J. He, T. M. P. Tait and C. P. Yuan, Phys. Rev. D 62, 011702(R) (2000).
- (7) X. F. Wang, C. Du and H. J. He, Phys. Lett. B 723, 314 (2013).
- (8) H. J. He, C. T. Hill and T. M. P. Tait, Phys. Rev. D 65, 055006 (2002).
- (9) H. J. He and Z. Z. Xianyu, J. Cosmol. Astropart. Phys. 10 019 (2014).
- (10) J. A. Aguilar-Saavedra, R. Benbrik, S. Heinemeyer, and M. Pérez-Victoria,, Phys. Rev. D 88, 094010 (2013).
- (11) H. J. He, N. Polonsky and S. f. Su, Phys. Rev. D 64, 053004 (2001).
- (12) N. Chen and H. J. He, JHEP 04, 062 (2012).
- (13) A. Atre, G. Azuelos, M. Carena, T. Han, E. Ozcan, J. Santiago, and G. Unel, JHEP 08, 080 (2011).
- (14) G. Cacciapaglia, A. Deandrea, L. Panizzi, N. Gaur, D. Harada and Y. Okada, JHEP 03, 070 (2012).
- (15) J. W. Nutter, R. Schwienhorst, D. G. E. Walker and J. H. Yu, Phys. Rev. D 86, 094006 (2012).
- (16) Y. Okada and L. Panizzi, Adv. High Energy Phys. 2013, 364936 (2013).
- (17) M. Buchkremer, G. Cacciapaglia, A. Deandrea, and L. Panizzi, Nucl. Phys. B 876, 376-417 (2013).
- (18) S. Yang, J. Jiang, Q. S. Yan and X. Zhao, JHEP 09, 035 (2014).
- (19) O. Matsedonskyi, G. Panico and A. Wulzer, JHEP 12, 097 (2014).
- (20) M. Backović, T. Flacke, S. J. Lee and G. Perez, JHEP 09, 022 (2015).
- (21) D. Barducci and L. Panizzi, JHEP 12 057 (2017).
- (22) G. Cacciapaglia, A. Deandrea, N. Gaur, D. Harada, Y. Okada and L. Panizzi, JHEP 11, 055 (2018).
- (23) G. Cacciapaglia, A. Carvalho, A. Deandrea, T. Flacke, B. Fuks, D. Majumder, L. Panizzi, and H. S. Shao, Phys. Lett. B 793, 206 (2019).
- (24) Y. B. Liu and Y. Q. Li, Eur. Phys. J. C 77, 654 (2017).
- (25) S. Moretti, D. O’Brien, L. Panizzi, and H. Prager, Phys. Rev. D 96, 035033 (2017).
- (26) Y. B. Liu and S. Moretti, Phys. Rev. D 100, 015025 (2019).
- (27) A. Buckley, J.M. Butterworth, L. Corpe, D. Huang, and P. Sun, SciPost Phys. 9, 069 (2020).
- (28) A. Deandrea, T. Flacke, B. Fuks, L. Panizzi, and H.S. Shao, JHEP 08, 107 (2021).
- (29) X.Y. Tian, L.F. Du, and Y.B. Liu, Nucl. Phys. B 965, 115358 (2021).
- (30) X.Y. Tian, L.F. Du and Y.B. Liu, Eur. Phys. J. C 81, 594 (2021).
- (31) B. Yang, M. Wang, H. Bi, and L. Shang, Phys. Rev. D 103, 036006 (2021).
- (32) J.Z. Han, J. Yang, S. Xu, H.K. Wang, Nucl. Phys. B 975, 115672 (2022).
- (33) J.Z. Han, Y.B. Liu, L.Xing and S. Xu, Chin. Phys. C 46, 103103 (2022)
- (34) J.Z. Han, S. Xu, W.J. Mao and H.Q. Song, Nucl. Phys. B 992, 116235 (2023).
- (35) J.M. Alves, G.C. Branco, A.L. Cherchiglia, J.T. Penedo, P.M.F. Pereira, C.C. Nishi, M.N. Rebelo and J.I. Silva-Marcos, arXiv:2304.10561 [hep-ph].
- (36) M. Aaboud et al. [ATLAS], Phys. Rev. D 98, no.11, 112010 (2018).
- (37) M. Aaboud et al. [ATLAS], Phys. Rev. Lett. 121, no.21, 211801 (2018).
- (38) A.M. Sirunyan et al. [CMS], JHEP 08, 177 (2018).
- (39) A.M. Sirunyan et al. [CMS], Phys. Rev. D 100, no.7, 072001 (2019).
- (40) A.M. Sirunyan et al. [CMS], Phys. Rev. D 102, 112004 (2020).
- (41) [ATLAS], ATLAS-CONF-2021-024.
- (42) G. Aad et al. [ATLAS], Phys. Lett. B 843, 138019 (2023).
- (43) J.A. Aguilar-Saavedra, D.E. López-Fogliani and C. Muñoz, JHEP 06, 095 (2017).
- (44) K. Das, T. Mondal and S.K. Rai, Phys. Rev. D 99, 115002 (2019).
- (45) R. Benbrik, E.B. Kuutmann, D. Buarque Franzosi, V. Ellajosyula, R. Enberg, G. Ferretti, M. Isacson, Y.B. Liu, T. Mandal, T. Mathisen, et al. JHEP 05, 028 (2020).
- (46) G. Cacciapaglia, T. Flacke, M. Park and M. Zhang, Phys. Lett. B 798, 135015 (2019).
- (47) J.A. Aguilar-Saavedra, J. Alonso-González, L. Merlo and J.M. No, Phys. Rev. D 101, 035015 (2020).
- (48) H. Zhou and N. Liu, Phys. Rev. D 101, 115028 (2020).
- (49) D. Wang, L. Wu and M. Zhang, Phys. Rev. D 103, 115017 (2021).
- (50) G. Corcella, A. Costantini, M. Ghezzi, L. Panizzi, G.M. Pruna and J. Šalko, JHEP 10, 108 (2021).
- (51) G. Cacciapaglia, T. Flacke, M. Kunkel and W. Porod, JHEP 02, 208 (2022).
- (52) X.M. Cui, Y.Q. Li and Y.B. Liu, Phys. Rev. D 106, 115025 (2022).
- (53) A. Banerjee, D.B. Franzosi and G. Ferretti, JHEP 03, 200 (2022).
- (54) A. Banerjee, D.B. Franzosi, G. Cacciapaglia, A. Deandrea, G. Ferretti, T. Flacke, B. Fuks, M. Kunkel, L. Panizzi and W. Porod, et al. arXiv:2203.07270 [hep-ph].
- (55) A. Bhardwaj, K. Bhide, T. Mandal, S. Mitra and C. Neeraj, Phys. Rev. D 106, no.7, 075024 (2022).
- (56) A. Bhardwaj, T. Mandal, S. Mitra and C. Neeraj, Phys. Rev. D 106, no.9, 095014 (2022).
- (57) J. Bardhan, T. Mandal, S. Mitra and C. Neeraj, Phys. Rev. D 107, no.11, 115001 (2023).
- (58) K. Kong and S.C. Park, JHEP 08, 038 (2007).
- (59) A. Senol, A.T. Tasci and F. Ustabas, Nucl. Phys. B 851, 289-297 (2011).
- (60) L. Guo, W. Liu, W.G. Ma, R.Y. Zhang, W.J. Zhang and M.A. B., Commun. Theor. Phys. 62, 824-832 (2014).
- (61) Y.B. Liu and Z.J. Xiao, Nucl. Phys. B 892, 63-82 (2015).
- (62) H. Abramowicz et al. [CLIC Detector and Physics Study], arXiv:1307.5288 [hep-ex].
- (63) R. Franceschini, Int. J. Mod. Phys. A 35, 2041015 (2020).
- (64) X. Qin and J.F. Shen, Nucl. Phys. B 966, 115388 (2021).
- (65) L. Han and J.F. Shen, Eur. Phys. J. C 81, no.5, 463 (2021).
- (66) J.Z. Han, J. Yang, S. Xu and H.K. Wang, Phys. Rev. D 105, 015005 (2022).
- (67) X. Qin, L.F. Du, and J.F. Shen, Nucl. Phys. B 979, 115784 (2022).
- (68) L. Han, L.F. Du and Y.B. Liu, Phys. Rev. D 105, 115032 (2022).
- (69) L. Han, J.F. Shen and Y.B. Liu, Eur. Phys. J. C 82, 637 (2022)
- (70) J.Z. Han, S. Xu, H.Q. Song and Y.J. Wang, Nucl. Phys. B 985, 116030 (2022).
- (71) B. Yang, S. Wang, X. Sima and L. Shang, Commun. Theor. Phys. 75, 035202 (2023).
- (72) X. Qin and C. Wang, Nucl. Phys. B 992, 116248 (2023).
- (73) H.J. He, Y.P. Kuang, and X.Y. Li, Phys. Rev. Lett. 69, 2619 (1992).
- (74) H.J. He, Y.P. Kuang, and X.Y. Li, Phys. Rev. D 49, 4842 (1994).
- (75) H. J. He, Y. P. Kuang, and C. P. Yuan, Phys. Rev. D 51, 6463 (1995).
- (76) H.J. He, Y.P. Kuang, and C.P. Yuan, Phys. Rev. D 55, 3038 (1997).
- (77) H.J. He and W.B. Kilgore, Phys. Rev. D 55, 1515 (1997).
- (78) J. Alwall, R. Frederix, S. Frixione, V. Hirschi, F. Maltoni, O. Mattelaer, H.-S. Shao, T. Stelzer, P. Torrielli, and M. Zaro, JHEP 07, 079 (2014).
- (79) S. Moretti, D. O’Brien, L. Panizzi, and H. Prager, Phys. Rev. D 96, 075035 (2017).
- (80) T. Sjöstrand, S. Ask, J. R. Christiansen et al., Comput. Phys. Commun. 191, 159 (2015).
- (81) J. de Favereau et al. (DELPHES 3 Collaboration), JHEP 02, 057 (2014).
- (82) E. Leogrande, P. Roloff, U. Schnoor and M. Weber, arXiv:1909.12728 [hep-ex].
- (83) M. Boronat, J. Fuster, I. Garcia, E. Ros and M. Vos, Phys. Lett. B 750, 95-99 (2015).
- (84) M. Boronat, J. Fuster, I. Garcia, P. Roloff, R. Simoniello and M. Vos, Eur. Phys. J. C 78, 144 (2018).
- (85) E. Conte, B. Fuks, and G. Serret, Comput. Phys. Commun. 184, 222 (2013).
- (86) G. Cowan, K. Cranmer, E. Gross, and O. Vitells, Eur. Phys. J. C 71, 1554 (2011) [erratum: Eur. Phys. J. C 73, 2501 (2013)].