Searching for lepton flavor violating decays in minimal R-symmetric supersymmetric standard model
Abstract
We analyze the lepton flavor violating decays () in the scenario of the minimal R-symmetric supersymmetric standard model. The prediction on the branching ratios BR and BR is affected by the mass insertion parameters and , respectively. These parameters are constrained by the experimental bounds on the branching ratios BR() and BR(). The result shows penguin dominates the prediction on BR() in a large region of the parameter space. The branching ratios for BR() are predicted to be, at least, five orders of magnitude smaller than present experimental bounds and three orders of magnitude smaller than future experimental sensitivities.
pacs:
12.60.Jv, 13.35.DxI Introduction
Searching for lepton flavor violating (LFV) decays is of great importance in probing new physics (NP) beyond the standard model (SM) since the theoretical prediction on these LFV decays is suppressed by small mass of neutrinos in the SM. Much effort has been devoted to searching for LFV decays in experiment and the usually discussed decay channels are , , -e conversion in nuclei, semileptonic decays, and so on. The experimental observation of LFV decays of lepton is one goal of a bunch of excellent dedicated experiments. The first generation of B-factories, that stand for factories too, like BaBar or Belle, have joined in the pursuit of charged LFV decays coming from lepton Cei . All experiments have provided excellent bounds on the hadronic decays of , for the first time Hayasaka ; Belle ; Belle1 , such as , where stands for a pseudoscalar (vector) meson. The study of LFV decays of lepton are also one of main goals of the future SuperKEKB/Belle II project under construction at KEK Belle2 . The present upper bounds on the branching ratios of () are shown in TABLE.1 PDG .
Decay | Bound | Experiment | Decay | Bound | Experiment |
---|---|---|---|---|---|
BELLE BELLEt | BABAR BABARt | ||||
BELLE BELLEt | BELLE BELLEt | ||||
BELLE BELLEt | BELLE BELLEt |
Assuming the integrated luminosity of 50 , the future prospects of BR in Belle II will be extrapolated at the level of - Altmannshofer .
In various extensions of the SM, corrections to BR are enhanced by different LFV sources. There are a few studies within non-SUSY models, such as two Higgs doublet models Li ; Kanemura , 331 model hua , TC2 models yue , littlest Higgs model with T parity Goto , simplest little Higgs model Lami , leptoquark models Carpentier ; Dorsner and unparticle model LiZH . Some models with heavy Dirac/Majorana neutrinos can have BR close to the experimental sensitivity Garcia ; Ilakovac ; Ilakovac3 . In Type III seesaw model, there are tree level flavor changing neutral currents in the lepton sector which can enhance the prediction on BR He1 ; Arhrib . There are also a few studies within SUSY models, such as MSSM Fukuyama ; Sher , unconstrained MSSM brignole , supersymmetric seesaw mechanism model Chen , R-parity violating SUSY Saha , the CMSSM-seesaw and NUHM-seesaw Arganda . Within an effective field theory framework, LFV decays are studied to set constraints on the Wilson coefficients of the LFV operators Black ; cirigliano ; He ; Dorsner ; Cai ; Cai1 ; Gabrielli ; Petrov ; Celis ; Buchmuller ; Grzadkowski .
In this paper, we will study the LFV decays in the minimal R-symmetric supersymmetric standard model (MRSSM) Kribs . The MRSSM has an unbroken global symmetry and provides a new solution to the supersymmetric flavor problem that exists in the MSSM. In this model, R-symmetry forbids the Majorana gaugino masses, term, terms and all left-right squark and slepton mass mixings. The -charged Higgs doublets and are introduced in the MRSSM to yield Dirac mass terms of higgsinos. The additional superfields , and are introduced to yield Dirac mass terms of gauginos. The most unusual characteristic in the MRSSM is that large flavor violation is allowed in the squark and slepton mass matrices. The presence of large flavor violation in the MRSSM means that it is no longer appropriate to discuss stops or selectrons necessarily. The large flavor violation opens the possibility for a wide variety of new signals at the LHC and is worthy of significant study. Studies on phenomenology in the MRSSM can be found in Refs. Die1 ; Die2 ; Die3 ; Die4 ; Die5 ; Die6 ; KSS ; Kumar ; Blechman ; Kribs1 ; Frugiuele ; Jan ; Chakraborty ; Braathen ; Athron ; Alvarado ; sks1 ; sks2 . It is interesting to explore whether BR can be enhanced to be close to the current experiment limits or future experimental sensitivities while the predictions on other LFV processes do not exceed current experiment constraints. Thus, we choose decay channels as an object of the analysis. Similar to the case in the MSSM, LFV decays mainly originate from the off-diagonal entries in slepton mass matrices and . Taking into account the experimental constraints from decay channels and on the off-diagonal parameters, we investigate the branching ratios BR() as a function of the off-diagonal parameters and other model parameters.
The outline of this paper is organized as follows. In Section II, we provide a brief introduction on the MRSSM and present the definitions of the sneutrino mass matrix and slepton mass matrix. Then, we present conventions for the effective operators and the corresponding Wilson coefficients. The existing constraints, benchmark points and the results of our calculation are shown in Section III. In Section IV, the conclusion is drawn. The definitions of mass matrices of scalar and pseudo-scalar Higgs boson, neutralino, -chargino and squarks are listed in Appendix A.
II MRSSM
In this section, we firstly provide a simple overview of the MRSSM in order to fix the notations used in this work. The MRSSM has the same gauge symmetry as the SM and the MSSM. The spectrum of fields in the MRSSM contains the standard MSSM matter, the Higgs and gauge superfields augmented by the chiral adjoints and two -Higgs iso-doublets. The superfields with R-charge in the MRSSM are given in TABLE.2.
Field | Superfield | Boson | Fermion | |||
Gauge vector | 0 | 0 | +1 | |||
Matter | +1 | +1 | 0 | |||
+1 | +1 | 0 | ||||
-Higgs | 0 | 0 | -1 | |||
R-Higgs | +2 | +2 | +1 | |||
Adjoint chiral | 0 | 0 | -1 |
The general form of the superpotential of the MRSSM is given by Die1
(1) |
where and are the MSSM-like Higgs weak iso-doublets, and are the -charged Higgs doublets. The corresponding Dirac higgsino mass parameters are denoted as and . Although R-symmetry forbids the terms of the MSSM, the bilinear combinations of the normal Higgs doublets and with the Higgs doublets and are allowed in Eq.(1). The parameters , , and are Yukawa-like trilinear terms involving the singlet and the triplet .
For the phenomenological studies we take the soft-breaking scalar mass terms Die3
(2) |
All the trilinear scalar couplings involving Higgs bosons to squark and slepton are forbidden in Eq.(2) because the sfermions have an R-charge and these terms are non R-invariant, and this has relaxed the flavor problem of the MSSM Kribs . The Dirac nature is a manifest feature of the MRSSM fermions. The soft-breaking Dirac mass terms of the singlet , triplet and octet take the form as
(3) |
where , and are the usually MSSM Weyl fermions. The R-Higgs bosons do not develop vacuum expectation values (VEVs) since they carry R-charge 2. After electroweak symmetry breaking, the singlet and triplet VEVs effectively modify the and , and the modified parameters are given by
and are vacuum expectation values of and .
There are four complex neutral scalar fields and they can mix. Assuming the vacuum expectation values are real, the real and imaginary components in four complex neutral scalar fields do not mix, and the mass-square matrix breaks into two sub-matrices. In the scalar sector all fields mix and the SM-like Higgs boson is dominantly given by the up-type field. In the pseudo-scalar sector there is no mixing between the MSSM-like states and the singlet-triplet states, and the mass-squared matrix breaks into two submatrices. The number of neutralino degrees of freedom in the MRSSM is doubled compared to the MSSM as the neutralinos are Dirac-type. The number of chargino degrees of freedom in the MRSSM is also doubled compared to the MSSM and these charginos can be grouped to two separated chargino sectors according to their R-charge. The -chargino sector has R-charge 1 electric charge; the -chargino sector has R-charge -1 electric charge. Here, we do not discuss the -chargino sector in detail since it does not contribute to the LFV decays. More information about the -chargino can be found in Ref.Die3 ; Die5 ; sks1 ; KSS . For convenience, we present the tree-level mass matrices for scalar and pseudo-scalar Higgs bosons, neutralinos, charginos and squarks of the MRSSM in Appendix A.
In MRSSM, LFV decays mainly originate from the potential misalignment in slepton mass matrices. In the gauge eigenstate basis , the sneutrino mass matrix and the diagonalization procedure are
(4) |
where the last two terms in mass matrix are newly introduced by MRSSM. The slepton mass matrix and the diagonalization procedure are
(5) |
where
The sources of LFV are the off-diagonal entries of the soft supersymmetry breaking matrices and in Eqs.(4, 5). From Eq.(5) we can see that the left-right slepton mass mixing is absent in the MRSSM, whereas the terms are present in the MSSM. The relevant Feynman diagrams contributing to are presented in FIG.1.

We now focus on the LFV processes . Using the effective Lagrangian method, we present the analytical expression for the decay width of . At the quark level, the interaction Lagrangian for can be written as Flavor
(6) |
where the index (=) denotes the generation of the emitted lepton and . Since only the axial-vector current contributes to , the coefficients in Eq.(6) do not include photon penguin contribution but they include boson and scalar ones. The contribution to the Wilson coefficients and in Eq.(6) can be classified into self-energies, penguins, Higgs penguins and box diagrams, as shown in FIG.1. Now consider the implication of virtual Higgs exchange for . Both the contributions from scalar and pseudo-scalar Higgs sector are considered in this work. However, all the Higgs penguin contribution is negligible since the couplings of scalar and pseudo-scalar Higgs to the light quarks are suppressed by their masses.
Then the decay width for is given by
(7) |
where the averaged squared amplitude can be written as
(8) |
The coefficients and are linear combinations of the Wilson coefficients in Eq.(6),
where is the pion decay constant. The expressions for coefficients , are listed in TABLE.3 Arganda .
1 | |||
---|---|---|---|
- | |||
Here, and denote the masses of the neutral pion and Kaon, and denotes the mixing angle. In addition, = - .
Finally, the MRSSM has been implemented in the Mathematica package SARAH-4.14.3 SARAH ; SARAH1 ; SARAH2 ; Flavor . The masses of the MRSSM particles, mixing matrices and the Wilson coefficients of the corresponding operators in the effective lagrangian are computed by SPheno-4.0.4 SPheno1 ; SPheno2 modules written by SARAH.
III Numerical Analysis
The calculations of BR() in the MRSSM are evaluated within the framework of SARAH-4.14.3 SARAH ; SARAH1 ; SARAH2 ; Flavor and SPheno-4.0.4 SPheno1 ; SPheno2 . The experimental values of the Higgs mass and the W boson mass can impose stringent and nontrivial constraints on the model parameters. The one loop and leading two loop corrections to the lightest (SM-like) Higgs boson in the MRSSM have been computed in Die3 and the new fields and couplings can give large contributions to the Higgs mass even for stop masses of order 1 TeV and no stop mixing. Meanwhile, the new fields and couplings can not give too large contribution to the W boson mass and muon decay in the same regions of parameter space. A better agreement with the latest experimental value for the W boson mass has been investigated in Die6 . It combines all numerically relevant contributions that are known in the SM in a consistent way with all the MRSSM one loop corrections. A set of the updated benchmark point BMP1 is given in Die6 and we display them in Eq.(9) where all the mass parameters are in GeV or GeV2.
(9) |
In the numerical analysis, the default values of the input parameters are set same with those in Eq.(9). The off-diagonal entries of squark mass matrices , , and slepton mass matrices , in Eq.(9) are zero. The large value of is excluded by measurement of the W boson mass because the VEV of the triplet field gives a correction to the W mass through Die1
(10) |
Similarly to the most supersymmetry models, those LFV processes originate from the off-diagonal entries of the soft breaking terms and in the MRSSM, which are parametrized by the mass insertion
(11) |
where . To decrease the number of free parameters involved in our calculation, we assume that the off-diagonal entries of and in Eq.(11) are equal, i.e., = = . The experimental bounds on LFV decays, such as radiative two body decays , leptonic three body decays and -e conversion in nuclei, can give strong constraints on the parameters . In the following, we will use LFV decays and to constrain the parameters . It is noted that has been set zero in following discussion since it has no effect on the prediction of BR(). Current limits on branching ratios of and are listed in TABLE.4 PDG .
Decay | Bound | Experiment | Decay | Bound | Experiment |
---|---|---|---|---|---|
SPEC(2016)MEG | BABAR(2010)BABAR | ||||
BABAR(2010)BABAR | SPEC(1988)SINDRUM | ||||
BELL(2010)BELL | BELL(2010)BELL |


Taking and the parameters in Eq.(9), we plot the predictions of BR versus Log[] in the left panel of FIG.2. Taking and the parameters in Eq.(9), we plot the predictions of BR versus Log[] in the right panel of FIG.2. A linear relationship in logarithmic scale is displayed between BR and the flavor violating parameter (). The actual dependence on or is quadratic. The mentioned linear dependence is due to the fact that both x axis and y axis in FIG.2 are logarithmically scaled. In FIG.2 the following hierarchy is shown, BRBRBR and BRBRBR. The predictions on BR and BR are very close to each other. At = , the prediction on BR is around and this is very close to the current experimental bound. The prediction on BR is around and this is two orders of magnitude below the current experimental bound. The decay channels can set more strong constraint than channels on the flavor violating parameters. The predictions on BR are far below the current experimental bounds. The prediction on BR is around and this is five orders of magnitude below the current experimental bound and three orders of magnitude below the future experimental sensitivity.


Taking , and the parameters in Eq.(9), we plot the predictions of BR from various parts as a function of in the left panel of FIG.3. Taking , and the parameters in Eq.(9), we plot the theoretical predictions of BR from various parts as a function of in the right panel of FIG.3. The lines corresponding to penguin and box diagram indicate the values of BR are given by only the listed contribution with all others set to zero. The total prediction for BR is also indicated. We observe that penguin dominates the prediction on BR in a large region of the parameter space. For larger values of , the prediction from penguin changes slowly, since it is directly proportional to Fok . The contribution from box diagram is not sensitive to and at least two orders of magnitude below penguin. This is because of the small couplings of neutralino/chargino to quark and squark in box diagram.
As mentioned above, the contribution from Higgs penguin is negligible due to the small couplings of the scalar and pseudo-scalar Higgs to the light quarks. However, if the Higgs couplings to the strange components of the and mesons are large enough, which result in large - and - mixing, Higgs-mediated contribution could dominate the predictions on Arganda . Furthermore, it was pointed out in Ref.Celis1 that a one loop Higgs generated gluon operator does not suffer of the light-quark mass suppression and could give a sizeable contribution. The Wilson coefficients and corresponding to the Higgs penguin in Eq.(6) can also contribute to the LFV process -e conversion. In simple formulas, the branching ratios BR() and conversion rate CR(-e, nucleus) are given by
Thus, the predicted CR(-e, nucleus) from Higgs penguin is much larger than BR() though both are negligible compared to the total contribution.


Taking , and the parameters in Eq.(9), we plot the predictions of BR as a function of the diagonal entries in the left panel of FIG.4. Taking , and parameters in Eq.(9), we plot the predictions of BR as a function of the diagonal entries in the right panel of FIG.4. Here, . The prediction on BR is at the level of and this is very close to the future experimental sensitivities Aushev . The prediction on BR is at the level of and this is two orders of magnitude below the future experimental sensitivities Aushev . The predictions on BR, BR and BR in the MRSSM decreas as the slepton mass parameter varies from 1 TeV to 5 TeV.


Taking , and the parameters in Eq.(9), we plot the predictions of BR as a function of the squark mass parameter in the left panel of FIG.5. Taking , and the parameters in Eq.(9), we plot the predictions of BR as a function of the squark mass parameter in the right panel of FIG.5. Here, =. We clearly see that both the predictions on BR() and BR(), which increase slowly as varies from 1 TeV to 5 TeV, are not sensitive to . The off-diagonal entries of the squark mass matrices , and could give additional contributions to BR(). Taking into account the experimental constraints on from low energy B meson physics observables, such as, BR(), BR(), the prediction of BR() takes values along a narrow band. Thus, the prediction of BR is also not sensitive to the off-diagonal entries of the squark mass matrices.
We are also interested to the effect from other parameters on the prediction of BR() in the MRSSM. The predicted BR() decreases slowly along with the increase of the wino-triplino mass parameter . However, the valid region of is constrained by the boundary conditions at the unification scale, and unphysical masses of neutral Higgs and charged Higgs are obtained when above 1 TeV. By scanning over these parameters, which are shown in Eq.(12),
(12) |
the prediction is shown in relation to one input parameter (e.g. or others). The parameters are constrained in a narrow region by the boundary conditions which is close to the benchmark points and can vary in the whole region. The results show that varying those parameters in Eq.(12) have very small effect on the prediction of BR() which takes values along a narrow band.
IV Conclusions
In this work, taking into account the constraints from LFV decays and on the flavor violating parameters, we analyze the LFV decays in the framework of the minimal R-symmetric supersymmetric standard model.
We observe that penguin dominates the prediction on BR, and other contributions are less dominant or negligible. As we all konw the LFV processes can only obtain the dipole contribution from the gamma penguin. The LFV processes and -e conversion can obtain contributions from the gamma penguin (including dipole and non-dipole), penguin, Higgs penguin and box diagram. While, for the LFV processes , contributions from penguin, Higgs penguin and box diagram are included except for the gamma penguin. It is interesting to consider if it is possible to find a parameter region that LFV processes and - conversion are not excluded and which could still give large contribution to . The answer is negative at least in this work. The prediction of BR is two or three orders of magnitude below BR.
In the MRSSM, the prediction on BR and BR is affected by the mass insertions and , respectively. The prediction on BR would be zero if =0 is assumed, and so are the prediction on BR if =0 is assumed. Taking into account the experimental bounds on BR() and BR(), the values of and are constrained around 0.5. The predictions on BR and BR are found to be at the level of -, which are five orders of magnitude below the present experimental upper limits. The processes may be the most competitive LFV semileptonic tau decay channels. The future prospects of BR in Belle II are extrapolated at the level of - Altmannshofer and they are three orders of magnitude above the predictions in the MRSSM. Thus, LFV decays may be out reach of the near future experiments.
Appendix A Mass matrices at tree level in the MRSSM
In the weak basis , the scalar Higgs boson mass matrix and the diagonalization procedure are
(15) |
where the submatrices (, ) are
(18) | |||||
(21) | |||||
(24) |
In the weak basis , the pseudo-scalar Higgs boson mass matrix and the diagonalization procedure are
(29) |
In the weak basis of four neutral electroweak two-component fermions =(,,,) with R-charge 1 and four neutral electroweak two-component fermions =(,,,) with R-charge -1, the neutralino mass matrix and the diagonalization procedure are
(34) |
The mass eigenstates and , and physical four-component Dirac neutralinos are
In the basis =(, ) and =(, ), the -charginos mass matrix and the diagonalization procedure are
(35) |
The mass eigenstates and physical four-component Dirac charginos are
The mass matrix for up squarks and down squarks, and the relevant diagonalization procedure are
(36) |
where
Acknowledgements.
This work has been supported partly by the National Natural Science Foundation of China (NNSFC) under Grants No.11905002 and No.11805140, the Scientific Research Foundation of the Higher Education Institutions of Hebei Province under Grant No. BJ2019210, the Foundation of Baoding University under Grant No. 2018Z01, the Foundation of Department of Education of Liaoning province under Grant No. 2020LNQN14, and the Natural Science Foundation of Hebei province under Grant No. A2020201002.References
- (1) F. Cei and D. Nicolo, Adv. High Energy Phys. 2014, 282915(2014).
- (2) K. Hayasaka and J. Phys. Conf. Ser. 171, 012079(2009).
- (3) Belle, BABAR Collaboration, G. Vasseur, PoS Beauty2014, 041(2015).
- (4) Belle Collaboration, Y. Miyazaki et al., Phys. Lett. B 719, 346(2013).
- (5) Belle-II Collaboration, B. A. Shwartz, Nucl. Part. Phys. Proc. 260, 233(2015).
- (6) M. Tanabashi et al., (Particle Data Group), Phys. Rev. D 98, 030001(2018).
- (7) Y. Miyazaki et al., Belle collaboration, Phys. Lett. B 648, 341(2007).
- (8) B. Aubert et al., BABAR collaboration, Phys. Rev. Lett. 98, 061803(2007).
- (9) W. Altmannshofer et al. (Belle II Collaboration), arXiv:1808.10567.
- (10) W. J. Li, Y. D. Yang and X. D. Zhang, Phys. Rev. D 73, 073005(2006).
- (11) S. Kanemura, T. Ota and K. Tsumura, Phys. Rev. D 73, 016006(2006).
- (12) T. Hua and C.-X. Yue, Commun. Theor. Phys. 62 (2014) 3, 388-392.
- (13) C.-X. Yue, L.-H. Wang and W. Ma, Phys. Rev. D 74, 115018(2006).
- (14) T. Goto, Y. Okada and Y. Yamamoto, Phys. Rev. D 83, 053011(2011).
- (15) A. Lami, J. Portoles and P. Roig, Phys. Rev. D 93, 076008(2016).
- (16) M. Carpentier and S. Davidson, Eur. Phys. J. C 70, 1071(2010).
- (17) I, Dorsner, J. Drobnak, S. Fajfer, J. F. Kamenik and N. Kosnik, J. High Energy Phys. 1111, 002(2011).
- (18) Z.-H. Li, Y. Li and H.-X. Xu, Phys. Lett. B 677, 150(2009).
- (19) A. Ilakovac, Bernd A. Kniehl and A. Pilaftsis, Phys. Rev. D 52, 3993(1995).
- (20) M. C. Gonzalez-Garcia and J. W. F. Valle, Mod. Phys. Lett. A 7, 477(1992).
- (21) A. Ilakovac, Phys. Rev. D 62, 036010(2000).
- (22) X.-G. He and S. Oh, J. High Energy Phys. 0909, 027(2009).
- (23) A. Arhrib, R. Benbrik and C.-H. Chen, Phys. Rev. D 81, 113003(2010).
- (24) M. Sher, Phys. Rev. D 66, 057301(2002).
- (25) T. Fukuyama, A. Ilakovac and T. Kikuchi, Eur. Phys. J. C 56, 125(2008).
- (26) A. Brignole and A. Rossi, Nucl. Phys. B 701, 3(2004).
- (27) C.-H. Chen and C.-Q. Geng, Phys. Rev. D 74, 035010(2006).
- (28) J. P. Saha and A. Kundu, Phys. Rev. D 66, 054021(2002).
- (29) E. Arganda, M.J. Herrero and J. Portoles, J. High Energy Phys. 0806, 079(2008).
- (30) D. Black, T. Han, H. J. He and M. Sher, Phys. Rev. D 66, 053002(2002).
- (31) V. Cirigliano and B. Grinstein, Nucl. Phys. B 752, 18(2006).
- (32) X.-G. He, J. Tandean and G. Valencia, Phys. Lett. B 797, 134842(2019).
- (33) Y. Cai and M. A. Schmidt, J. High Energy Phys. 1602, 176(2016).
- (34) Y. Cai, M. A. Schmidt and G. Valencia, J. High Energy Phys. 1805, 143(2018).
- (35) E. Gabrielli, Phys.Rev. D 62, 055009(2000).
- (36) A. A. Petrov, D. V. Zhuridov, Phys. Rev. D 89, 033005(2014).
- (37) A. Celis, V. Cirigliano and E. Passemar, Phys. Rev. D 89, 095014(2014).
- (38) W. Buchmuller and D. Wyler, Nucl. Phys. B 268, 621(1986).
- (39) B. Grzadkowski, M. Iskrzynski and M. Misiak, J. High Energy Phys. 1010, 085(2010).
- (40) G. D. Kribs, E. Poppitz and N. Weiner, Phys. Rev. D 78, 055010(2008).
- (41) P. Diessner and W. Kotlarski, PoS CORFU 2014, 079(2015).
- (42) P. Diessner, J. Kalinowski, W. Kotlarski and D. Stöckinger, Adv. High Energy Phys. 2015, 760729(2015).
- (43) P. Diessner, J. Kalinowski, W. Kotlarski and D. Stöckinger, J. High Energy Phys. 1412, 124(2014).
- (44) P. Diessner, W. Kotlarski, S. Liebschner and D. Stöckinger, J. High Energy Phys. 1710, 142(2017).
- (45) P. Diessner, J. Kalinowski, W. Kotlarski and D. Stöckinger, J. High Energy Phys. 1603, 007(2016).
- (46) P. Diessner and G. Weiglein, J. High Energy Phys. 1907, 011(2019).
- (47) W. Kotlarski, D. Stöckinger and H. Stöckinger-Kim, J. High Energy Phys. 1908, 082(2019).
- (48) A. Kumar, D. Tucker-Smith and N. Weiner, J. High Energy Phys. 1009, 111(2010).
- (49) A. E. Blechman, Mod. Phys. Lett. A 24, 633(2009).
- (50) G. D. Kribs, A. Martin and T. S. Roy, J. High Energy Phys. 0906, 042(2009).
- (51) C. Frugiuele and T. Gregoire, Phys. Rev. D 85, 015016(2012).
- (52) J. Kalinowski, Acta Phys. Polon. B 47, 203(2016).
- (53) S. Chakraborty, A. Chakraborty and S. Raychaudhuri, Phys. Rev. D 94, 035014(2016).
- (54) J. Braathen, M. D. Goodsell and P. Slavich, J. High Energy Phys. 1609, 045(2016).
- (55) P. Athron, J.-hyeon Park, T. Steudtner, D. Stöckinger and A. Voigt, J. High Energy Phys. 1701, 079(2017).
- (56) C. Alvarado, A. Delgado and A. Martin, Phys. Rev. D 97, 115044(2018).
- (57) K.-S. Sun, J.-B. Chen, X.-Y. Yang and S.-K. Cui, Chin. Phys. C 43, 043101 (2019).
- (58) K.-S. Sun, S.-K. Cui, W Li and H.-B. Zhang, Phys. Rev. D 102, 035029 (2020).
- (59) F. Staub, arXiv:0806.0538.
- (60) F. Staub, Comput. Phys. Commun. 184, 1792(2013).
- (61) F. Staub, Comput. Phys. Commun. 185, 1773(2014).
- (62) W. Porod and F. Staub, A. Vicente, Eur. Phys. J. C 74, 2992(2014).
- (63) W. Porod, Comput. Phys. Commun. 153, 275(2003).
- (64) W. Porod and F. Staub, Comput. Phys. Commun. 183, 2458(2012).
- (65) A. M. Baldini, et al., (MEG Collaboration), Eur. Phys. J. C 76, 434(2016).
- (66) B. Aubert, et.al., (BABAR Collaboration), Phys. Rev. Lett. 104, 021802(2010).
- (67) U. Bellgardt et al., (SINDRUM Collaboration), Nucl. Phys. B 299, 1(1988).
- (68) K. Hayasaka et al., Phys. Lett. B 687, 139(2010).
- (69) R. Fok and G. D. Kribs, Phys. Rev. D 82, 035010(2010).
- (70) A. Celis, V. Cirigliano and E. Passemar, Phys. Rev. D 89, 013008(2014).
- (71) T. Aushev, et al., arXiv:1002.5012.