Modular flavor symmetric models 111The contribution to a special book dedicated to the memory of Professor Harald Fritzsch
We review the modular flavor symmetric models of quarks and leptons focusing on our works. We present some flavor models of quarks and leptons by using finite modular groups and discuss the phenomenological implications. The modular flavor symmetry gives interesting phenomena at the fixed point of modulus. As a representative, we show the successful texture structure at the fixed point . We also study CP violation, which occurs through the modulus stabilization. Finally, we study SMEFT with modular flavor symmetry by including higher dimensional operators. )
1 Introduction
One of important mysteries in particle physics is the origin of the flavor structure, i.e., fermion mass hierarchies, their mixing angles, and CP violation. Various studies have been done to understand their origin. One of traditional approaches is the texture zeros proposed by Weinberg and Fritzsch, where zero entries are put in the fermion mass matrices [1, 2]. Indeed, the Fritzsch Ansatz [3, 4] gave significant prediction power for the flavor mixing although the origin of zeros are unclear. This approach leads to the texture zero analysis where some elements of mass matrices are required to be zero to reduce the degrees of freedom in mass matrices. Some famous works have been made in the texture zeros [5, 6, 7, 8, 9]. Those zeros can be related with certain symmetries.
Flavor symmetries are interesting approaches to attack the origin of fermion mass hierarchies and mixing angles. Froggatt-Nielsen have taken the symmetry to explain the observed masses and mixing angles for quarks [10]. Furthermore, the symmetry was used for quark mass matrices [11, 12]. It was also discussed to understand the large mixing angle [13] in the oscillation of atmospheric neutrinos [14]. For the last twenty years, non-Abelian discrete flavor symmetries have been developed, that is motivated by the precise observation of flavor mixing angles of leptons [15, 16, 17, 19, 20, 21, 22, 23, 24, 18, 25].
The standard model (SM) is the low-energy effective field theory from the viewpoint of underlying theory, and it is referred to as the SM effective field theory (SMEFT) [26, 27, 28]. The SMEFT includes many higher dimensional operators, and they contribute to flavor changing processes and muon . Flavor symmetries are useful not only to derive realistic fermion masses and their mixing angles, but to control higher dimensional operators in the SMEFT. Indeed, the and symmetries control the SMEFT operators [29]. The symmetry [30] allows us to apply the Minimal Flavor Violation (MFV) hypothesis [31, 32], which is the most restrictive hypothesis consistent with the SMEFT. In the symmetry [33, 34, 35], it retains most of the MFV virtues and allows us to have a much richer structure as far as the dynamics of third family is concerned. Thus, flavor symmetries are useful to connect between the low-energy physics and high-energy physics such as superstring theory.
Superstring theory is a promising candidate for unified theory of all the interactions including gravity and matters such as quarks and leptons, and Higgs modes. Superstring theory must have six-dimensional (6D) compact space in addition to four-dimensional (4D) space times. Geometrical symmetries of 6D compact space control 4D effective field theory. For example, in certain compactifications there appears non-Abelian discrete symmetries such as and [36, 37, 38, 39, 40].
The modular symmetry is a geometrical symmetry of and , and corresponds to change of their cycle basis. Matter modes transform non-trivially under the modular symmetry. (See for hetetrotic string theory on orbifolds Refs. [41, 42, 43, 44] and magnetized D-brane models Refs. [45, 46, 47, 48, 49, 50, 51] . 222Calai-Yau manifolds have larger symplectic modular symmetries of many moduli [52, 53, 54, 55] .) That is, the modular symmetry is a flavor symmetry. Indeed, finite modular groups include , , , , which have been used in 4D flavor models so far, while and are also included as subgroups.
The well-known finite groups , , and are isomorphic to the finite modular groups for , respectively[56]. The lepton mass matrices have been presented in terms of modular forms [57]. Modular forms have also been obtained for [58], [59] and [60, 61], respectively. By using them, the viable lepton mass matrices have been obtained for [59], and then [60, 61].
The 4D CP symmetry can be embedded into a proper Lorentz symmetry in higher dimensional theory such as superstring theory [62, 63, 64, 65, 66, 67]. From this viewpoint, CP violation in 4D effective field theory would originate from the compactification, that is, the moduli stabilization. (See for early studies on the CP violation through the moduli stabilization Refs. [68, 69, 70, 71] .) Recently, the spontaneous breaking of the CP symmetry was studied through the moduli stabilization due to 3-form fluxes Refs. [72, 54]. In modular flavor symmetric models, the CP symmetry is combined with the modular symmetry as well as other symmetries, and is enlarged [73, 74, 75, 76, 77, 55] 333See for the CP symmetry in the Calabi-Yau compactification Refs. [54, 55, 78] .. The CP-invariant vacua and CP-preserving modulus values increase by the modular symmetry. It is important to study the CP violation in such models with the enlarged symmetry [79, 80].
Higher dimensional operators can be computed within the framework of superstring theory. Allowed couplings are controlled by stringy symmetries and -point couplings are written by products of 3-point couplings. The modular flavor symmetry also control these higher dimensional operators [81, 82, 83].
In addition to the above aspects, the modular flavor symmetries were recently extended to models for dark matter [84, 85], soft supersymmetry breaking terms [86, 87, 88], matter parity [89], the strong CP problem[90], etc.
The paper is organized as follows. In section 2, we give a brief review on modular symmetry. In section 3, we study modular flavor symmetric models. As an illustrating example, we explain modular symmetric models. In section 4, we study texture structure at the fixed point . In section 5, we study CP violation in modular symmetric models. In section 6, we study SMEFT with modular flavor symmetry. Section 7 is devoted to conclusion. In Appendix A, we review modular forms of . In Appendix B, the tensor product decomposition is given in the group.
2 Modular Symmetry
The modular symmetry is a geometrical symmetry of the two-dimensional torus, . The two-dimensional torus is constructed as division of the two-dimensional Euclidean space by a lattice , . Instead of , one can use the one-dimensional complex plane. As shown in Fig. 1, the lattice is spanned by two basis vectors, and as , where and are integer. Their ratio,
(1) |
in the complex plane, represents the shape of , and the parameter is called the modulus.

The same lattice can be spanned by other basis vectors such as
(8) |
where are integer satisfying . That is the .
Under the above transformation, the modulus transforms as follows,
(9) |
That is the modular symmetry [91, 92, 93, 94]. For the element in ,
(12) |
the modulus is invariant, . Thus, the modular group is . It is sometimes called the inhomogeneous modular group. On the other hand, the group, is called the homogeneous modular group or the full modular group.
The generators of are written by and ,
(17) |
They satisfy the following algebraic relations,
(18) |
Note that
(19) |
On , they satisfy
(20) |
These relations are also confirmed explicitly by the following transformations:
(21) |


In addition to the above algebraic relations of , we can require , i.e.
(22) |
They can correspond to finite groups such as for . In practice, we define the principal congruence subgroup as
(29) |
It includes , but not or . Then, we define the quotient , where the above algebraic relations are satisfied. It is found that with are isomorphic to , respectively [56].
We define by
(32) |
where denotes integers modulo . The group is isomorphic to for , while is isomorphic to , because in .
Similar to , we can define , and it is the double cover of . That is, the groups for are isomorphic to the double covering groups of , i.e. , respectively, although is isomorphic to .
The upper half-plane of the modulus space is mapped onto itself. For example, does not include the basis change. , i.e. . In practice, we find
(33) |
Thus, the modular group is represented on the upper half-plane of . Obviously one can map any value of on the upper half-plane into the region, by . Furthermore, by the modular transformation one can map any value of on the upper half-plane into the following region:
(34) |
which is called the fundamental domain. Suppose that is a maximum value among all of for a fixed value of . If , we map it by , and we find
(35) |
That is inconsistent with the assumption that is a maximum value among all of . That is, we find . Thus, we can map on the upper half-plane into the fundamental region by the modular transformation. The point is the fixed point under because , where symmetry remains. Similarly, the point is the fixed point under , where symmetry remains.
Modular forms of weight are the holomorphic functions of and transform as
(36) |
under the modular symmetry, where is a unitary matrix under .
Under the modular transformation, chiral superfields ( denotes flavors) with weight transform as [95]
(37) |
We study global SUSY models. The superpotential which is built from matter fields and modular forms is assumed to be modular invariant, i.e., to have a vanishing modular weight. For given modular forms, this can be achieved by assigning appropriate weights to the matter superfields.
The kinetic terms are derived from a Kähler potential. The Kähler potential of chiral matter fields with the modular weight is given simply by
(38) |
where the superfield and its scalar component are denoted by the same letter, and after taking vacuum expectation value (VEV) of . The canonical form of the kinetic terms is obtained by changing the normalization of parameters. The general Kähler potential consistent with the modular symmetry possibly contains additional terms [96]. However, we consider only the simplest form of the Kähler potential.
3 Modular flavor symmetric models
In this section, we discuss the flavor model of quark and lepton mass matrices. There is a difference between the modular symmetry and the usual flavor symmetry. Coupling constants such as Yukawa couplings also transform non-trivially under the modular symmetry and are written as functions of the modulus called modular forms, which are holomorphic functions of the modulus . On the other hand, coupling constants are invariant under the traditional flavor symmetries.
The flavor model of lepton mass matrices have been proposed based on the finite modular group [57]. This approach based on modular invariance opened up a new promising direction in the studies of the flavor physics and correspondingly in flavor model building.
3.1 Modular invariance and neutrino mixing
We present a phenomenological discussion of the modular invariant lepton mass matrix by using the finite modular group , where a simple model was proposed by Feruglio [57]. We have shown that it can predict a clear correlation between the neutrino mixing angle and the CP violating Dirac phase [97].
The mass matrices of neutrinos and charged leptons are essentially given by fixing the expectation value of the modulus , which is the only source of the breaking of the modular invariance. Since there are freedoms for the assignment of irreducible representations and modular weights to leptons, suppose that three left-handed lepton doublets are of a triplet of the group. The three right-handed neutrinos are also of a triplet of . On the other hand, the Higgs doublets are supposed to be a trivial singlet of for simplicity (In the next section, we modify this assumption.). We also assign three right-handed charged leptons for three different singlets of , , respectively. Therefore, there are three independent couplings in the superpotential of the charged lepton sector. Those coupling constants can be adjusted to the observed charged lepton masses.
The assignments of representations and modular weights to the MSSM fields as well as right-handed neutrino superfields are presented in Table 1.
SU(2) | ||||||
---|---|---|---|---|---|---|
1, 1”, 1’ | ||||||
0 | 0 |
In terms of modular forms of triplet, in Eq.(A) of Appendix A, the modular invariant Yukawa coupling and Majorana mass terms of the leptons are given by the following superpotentials:
(39) | |||||
(40) | |||||
(41) |
where the sums of the modular weights vanish. The parameters , , , (), and are constant coefficients.
VEVs of the neutral component of and are written as and , respectively. Then, the mass matrix of charged leptons is given by the superpotential Eq. (39) as follows:
(42) |
The coefficients , , and are taken to be real positive by rephasing right-handed charged lepton fields without loss of generality.
Since the tensor product of is decomposed into the symmetric triplet and the antisymmetric triplet as seen in Appendix B, the superpotential of the Dirac neutrino mass in Eq. (40) is expressed by introducing additional two parameters and as:
(43) |
The Dirac neutrino mass matrix is given as
(44) |
On the other hand, since the Majorana neutrino mass terms are symmetric, the superpotential in Eq. (41) is expressed simply as
(45) |
Then, the modular invariant right-handed Majorana neutrino mass matrix is given as
(46) |
Finally, the effective neutrino mass matrix is obtained by the type I seesaw as follows:
(47) |
When is fixed, the modular invariance is broken, and then the lepton mass matrices give the mass eigenvalues and flavor mixing numerically. In order to determine the value of , we use the result of NuFIT 5.1 [98]. By inputting the data of , , and three mixing angles , , and with error-bar, we can severely constraint values of the modulus and the other parameters, and then we can predict the CP violating Dirac phases . We consider both the normal hierarchy (NH) of neutrino masses and the inverted hierarchy (IH) of neutrino masses , where , , and denote three light neutrino masses. Since the sum of three neutrino masses is constrained by the recent cosmological data [99, 100, 101], we exclude the predictions with meV even if mixing angles are consistent with observed one.
The coefficients and in the charged lepton mass matrix are given only in terms of by the input of the observed values and . As the input charged lepton masses, we take Yukawa couplings of charged leptons at the GUT scale GeV, where is taken as a bench mark [102, 103]:
(48) |
Lepton masses are given by with GeV.
Then, we have two free complex parameters, and the modulus apart from the overall factors in the neutrino sector. The value of is scanned in the fundamental domain of .
![]() ![]() |
In Fig.5, we show allowed regions in the - plain for NH of neutrino masses. Those are given in the sum of neutrino masses – meV and – meV. The and regions are presented by black and grey points, respectively. If the cosmological observation confirms meV, the region of is severely restricted in this model.
We present the prediction of the Dirac CP violating phase versus for NH of neutrino masses in Fig.5. The predicted regions correspond to regions of in Fig.5. It is emphasized that the predicted is larger than , and – in the region of meV. Since the correlation of and is clear, this prediction is testable in the future experiments of neutrinos. On the other hand, predicted and cover observed full region with error-bar, and there are no correlations with .
The prediction of the effective mass , which is the measure of the neutrinoless double beta decay, is around – meV and – meV. We present a sample set of parameters and outputs for NH in Table 2.
meV | |
meV | |
We have also scanned the parameter space for the case of IH of neutrino masses. We have found parameter sets which fit the data of and reproduce the observed three mixing angles , , and . However, the predicted is around meV, which may be excluded.
It is helpful to comment on the effects of the supersymmetry breaking and the radiative corrections because we have discussed our model in the limit of exact supersymmetry. The supersymmetry breaking effect can be neglected if the separation between the supersymmetry breaking scale and the supersymmetry breaking mediator scale is sufficiently large. In our numerical results, the corrections by the renormalization are very small as far as we take the relatively small value of .
3.2 Other modular invariant flavor models
In addition of this flavor model, other viable models have been also presented for [104, 105, 106, 107], [108, 109, 110, 111] and for [112, 113]. The double covering groups, [114], [115, 116] and [117, 118] have also discussed in the modular symmetry. Subsequently these groups have been used for flavor model building [119, 120, 121, 122]. Furthermore, modular forms for and have been constructed[46], and the level finite modular group as well as the level 6 group has been examined for the lepton mixing[123, 124].
On the other hand, the quark mass matrix has been also studied in the flavor symmetries[125, 126]. Hence, the unification of quarks and leptons has been applied in the framework of the SU or SO GUT [127, 112, 128, 129, 130, 131, 132, 133].
There are also another important physics, the baryon asymmetry in the universe, which is discussed with the modular symmetry. Indeed, the modular flavor symmetry has been examined in the leptogenesis[134, 135, 136].
The modular symmetry keeps a residual symmetry at the fixed points even if the modular symmetry is broken. The symmetry generated by remains at , while the symmetry generated by remains at , and it corresponds to the symmetry in and the symmetry in . Furthermore, the symmetry in remains in the limit . That gives interesting lepton mass matrices for the flavor mixing [137, 138]. In the modular invariant flavor model of , the hierarchical structure of lepton and quark flavors has been examined at nearby fixed points [139]. It is also remarked that the hierarchical structure of quark and lepton mass matrices could be derived without fine-tuning of parameters at the nearby fixed points of the modular symmetry [140]. (See also Refs.[141, 142].) For example, the modular forms and among the triplet of weight 2 vanish in the limit . When is large, but finite, the triplet modular forms of weight 2 behave
(49) |
where . In general, the modular form of behaves as
(50) |
when is large, where denotes charges. These can lead to hierarchical structures in Yukawa matrices. Similarly, certain modular forms vanish at the fixed point . Around this fixed, it is convenient to define the following parameter[140]:
(51) |
By use of this parameter, generic modular form can be approximated as
(52) |
around the fixed point , where depends on charges. We have a similar behavior around the fixed pint .
These behaviors around the fixed points allow to construct models in which the fermion mass hierarchies follow solely from the properties of the modular forms. For example, one can derive mass matrices such as and depending on charges of matter fields. Indeed, viable lepton and quark mass matrices are obtained without fine-tuning of parameters [140, 143, 144, 145, 146, 147, 148, 149].
Further phenomenology has been developed in many works [150, 151, 152, 153, 154, 155, 156, 157, 158, 159, 160, 161, 175, 162, 164, 165, 163, 166, 167, 168, 169, 170, 171, 172, 173, 174, 176, 177, 178, 179, 180, 181, 182, 183, 184, 185, 186, 187, 188, 189, 190, 191, 192, 193, 194, 195, 196, 197, 198, 199, 200, 204, 206, 201, 202, 203, 205, 207, 208, 209], while theoretical investigations have been also proceeded [210, 211, 218, 215, 216, 217, 219, 212, 213, 214, 220, 221, 222, 223, 224, 225, 226, 227].
4 Texture zeros in modular symmetry
Texture zeros of the fermion mass matrix provide an attractive approach to understand the flavor mixing. Those can be related with some flavor symmetries. Indeed, zeros of the mass matrix are discussed in the modular symmetry of flavors [162, 163, 121].
The flavor structure has been investigated in magnetized orbifold models with multi-Higgs modes[228, 229, 230], which are interesting compactification from higher dimensional theory such as superstring theory. They lead to a four-dimensional chiral theory, which has the modular symmetry [45, 46, 47, 48, 49, 50, 51]. In these models, quark and lepton masses and their mixing angles were discussed [231, 233, 232, 214, 234, 235, 236]. These magnetized orbifold models lead to multi-Higgs modes, while generic string compactification also leads more than one candidates for Higgs fields.
In this section, we show that texture zeros are generally realized at the fixed points in the modular flavor models with multi-Higgs [237].
4.1 Quark mass matrices with mluti-Higgs
4.1.1 Three pairs of Higgs fields
We present a simple model of quark mass matrices in the level modular flavor symmetry with the multi-Higgs at , which is referred to as Model 1. We assign the representation and the weights for the relevant chiral superfields as
-
•
quark doublet : triplet with weight 2
-
•
up-type quark singlets : singlets with weight 0
-
•
down-type quark singlets : singlets with weight 0
-
•
up and down sector Higgs fields : singlets with weight 0
which are summarized in Table 3.
2 | 1 | 1 | 2 | 2 | |
3 | |||||
2 | 0 | 0 | 0 | 0 |
Then, the superpotential terms of the up-type quark masses and down-type quark masses are written by
(53) | ||||
(54) |
where the decompositions of the tensor products are
(55) | |||
(56) | |||
(57) |
The superpotential terms are rewritten as:
(58) | ||||
(59) |
Finally, the quark mass matrices are given as:
(60) | ||||
(61) |
where the chiralities of the mass matrix, and are defined as . At the fixed point , modular forms are given as
(62) |
4.1.2 -eigenstate base at
Let us discuss the mass matrices at in the -eigenstates. The -transformation of the triplet of the left-handed quarks is
(63) |
where representations of and are given explicitly for the triplet in Appendix A. The -eigenstate is obtained by using the unitary matrix as follows:
(64) | |||
(65) |
The -eigenstates are .
On the other hand, right-handed quarks, which are singlets , are the eigenstates of ; that is, the -transformation is
(66) |
Higgs fields are also the -eigenstates since they are singlets . Therefore, -transformation of them is
(67) |
In the -eigenstates, the quark mass matrices are transformed by Eq. (64). It is given as:
(68) | |||
(69) |
where . Thus, some zeros appear for quark mass matrices.
Now, we impose , we obtain the nearest neighbor interaction (NNI) form,444The NNI form of three families has vanishing entries of (1,1), (2,2), (1,3), (3,1), but is not necessary to be Hermitian. which is considered as a general form of both up- and down-types quark mass matrices because this form is achieved by the transformation that leaves the left- handed gauge interaction invariant [6]. The NNI form is a desirable base to derive the Fritzsch-type quark mass matrix while the NNI form is a general form of quark mass matrices.
Therefore, the quark masses and the CKM matrix are reproduced taking relevant values of parameters. It is noticed that the flavor mixing is not realized in the case of one Higgs doublets for up- and down-type quark sectors. Thus, the NNI forms at are simply obtained unless the VEVs of two-Higgs vanish.
The CP symmetry is not violated at in modular flavor symmetric models with a pair of Higgs fields because of the symmetry [79]. However, the models with multi-Higgs fields can break the CP symmetry at the fixed point even if all of the Higgs VEVs are real [80]. Thus, the CP phase appears in our models, in general. Our models are interesting from the viewpoint of the CP violation, too.
The non-vanishing VEVs of both Higgs fields and are important to realize the NNI forms. We expect the scenario that these Higgs fields have a -matrix to mix them,
(70) |
Then, a light linear combination develops its VEV, which includes and . However, the above assignment of representations for the Higgs fields allows the -term of only , and the others vanish. That is, the mixing does not occur. When we assume the singlet with the representation develops its VEV, the and elements appear as like the next-to-minimal supersymmetric standard model.
It is noted that the alternative assignment of weights for the Higgs and the left-handed quarks also gives desirable term [237].
4.1.3 Three pairs of Higgs fields
We also study three pairs of Higgs fields with the representations. We add another pair of Higgs fields with the representation of the modular weight . Then, we easily obtain the mass matrices as follows:
(71) | |||
(72) |
This model can lead to a quite generic mass matrix. For example, by setting some of to be zero, we can drive some of texture zero structures including the NNI form. In addition, we can assume or to reduce the number of free parameters and realize a certain form of mass matrices. Thus, the different assignment of the singlets for Higgs leads to different texture zeros.
4.2 Extensions of models
In this section, the quark mass matrices are discussed in the specific modular symmetry of in order to show the derivation of NNI forms clearly.
It is noted that one can obtain flavor models leading to the NNI forms in the and modular flavor symmetries. Such texture zero structure originates from the charge of the residual symmetry of . The NNI form can be realized at the fixed point in and modular flavor models with two pairs of Higgs fields, when we assign properly modular weights to Yukawa couplings and and representations to three generations of quarks. It is found that four pairs of Higgs fields to realize the NNI form in modular flavor models. Thus, the modular flavor models with multi-Higgs fields at the fixed point leads to successful quark mass matrices [237].
Texture zeros have been studied phenomenologically in the lepton sector [238, 239, 240, 241, 242, 243]. We can extend our formula of the quark mass matrices to the lepton sector. Extension to the charged lepton mass matrix is straightforward, and we obtain the same results. On the other hand, there is some freedoms for the neutrino mass matrix, depending on the mechanism of producing tiny masses, for example, seesaw mechanism.
5 CP Symmetry
In this section, we study CP violation in modular symmetric flavor models.
The 4D CP symmetry can be embedded into a proper Lorentz transformation in a higher dimensional theory. Here, we concentrate on 6D theory, that is, extra two dimensions in addition to our 4D space-time. is one of examples of two-dimensional compact space. We denote the coordinate on extra dimension, e.g. , by . Then, we consider the following transformation
(73) |
at the same time as the 4D CP transformation. Such a combination is included in a 6D proper Lorentz symmetry. Because of the above coordinate transformation, the modulus on transforms
(74) |
under the CP symmetry [73, 74]. Note that the upper half plane of maps onto itself by this transformation. Another transformation such as can also correspond to a 6D proper Lorentz symmetry, but such a transformation maps the upper half plane onto the lower half plane. Thus, we do not use such a transformation.
Obviously, we find that the line is CP invariant. Other values are also CP invariant up to the modular symmetry. For example, transforms
(75) |
under the CP transformation Eq. (74). However, these values are related with each other by the -transformation. Thus, the fixed point is also CP invariant point. Similarly, the line is CP invariant.
The typical Kähler potential of the modulus field is written by
(76) |
The Kähler potential is invariant under the transformation, . In addition, the superpotential is invariant if it transforms
(77) |
under the CP symmetry with including the CP transformation of chiral matter fields.
We study the CP violation through the modulus stabilization. One of the moduli stabilization scenarios is due to the three-form fluxes [244]. Indeed, the moduli stabilization due to the three-from fluxes was studied in modular flavor models in Ref. [212]. Its result shows that the fixed point is favored statistically with highest probability. The above discussions implies that the CP violation does not occur at this fixed point. In Ref. [213] the moduli stabilization was studied by one-loop induced Fayet-Illiopoulos terms, and the modulus is stabilized at the same fixed point555See also for recent studies on moduli stabilization in modular flavor models Refs. [196, 245].. In addition, we study another mechanism of the moduli stabilization by assuming non-perturbative effects. We start with the superpotential with the modular flavor symmetry. Then, we assume the condensation . The superpotential is trivial singlet. We assume the following superpotential:
(78) |
where corresponds to and must have a proper modular weight. The minimum of the supergravity scalar potential with the above superpotential is obtained as , where is odd integer[79]. The above discussion implies that the CP violation does not occur at this point. On the other hand, we assume the following superpotential:
(79) |
where must have a proper modular weight. The minimum of the supergravity scalar potential with the above superpotential is obtained as , where is integer[79]. Obviously, this is CP invariant point. Similarly, we can study other modular flavor models such as and modular symmetries, and the potential minimum corresponds to either or (mod 1) [79]. In both cases, CP violation does not occur.
We examine explicitly mass matrices at and in order to understand that the CP symmetry is not violated at these lines. We study the flavor model with the modular flavor symmetry. We use the basis that is diagonal and satisfies . Then, the chiral fields such as left-handed quarks , up-sector and down-sector right-handed quarks , , and the Higgs field as well as lepton fields transform
(80) |
under the -transformation, where is integer. That is the rotation. Here, we assume one pair of Higgs fields and , which are trivial singlets under the modular symmetry. Then, the quark Yukawa terms in the superpotential can be written by
(81) |
We replace the Higgs fields by their VEVs so as to obtain the mass terms,
(82) |
Note that the Yukawa couplings are modular forms. Then, the above mass matrices can also be written by modular forms after replacing the Higgs fields by their VEVs. Since these mass terms must be invariant under the -transformation, the mass matrix must transform as
(83) |
That implies that the mass matrices can be written by
(84) |
in terms of , where include series of integer powers of as
(85) |
It is obvious that all of the entries in are real when . CP is not violated. On the other hand, it seems that the mass matrix has phases for other values of . For example, when , the phase structure of the mass matrix can be written by
(86) |
where , , and they are real. However, such phases can be canceled by rephasing
(87) |
and there is no physical CP phase for . That is the rotation. Note that can have a physical CP phase, which can not be canceled, except . Similarly, we can discuss the lepton sector, and the CP phase does not appear when .
The fixed point is statistically favored with highest probability, and phenomenological interesting because there remains symmetry. However, the CP violation does not occur in modular flavor models with one pair of Higgs fields. That suggests extension to models with multi-Higgs fields. Indeed many string compactifications lead more than one candidates of Higgs fields, which have the same quantum numbers of and can couple with quarks and leptons. We extend the above discussion to modular flavor models with multi-Higgs fields . The quark Yukawa terms in the superpotential can be written by
(88) |
Since these terms are invariant under the -transformation, Yukawa couplings must transform as
(89) |
under the -transformation, where
(90) |
That implies that the modular forms of Yukawa couplings can be written by
(91) |
where the functions and are series of positive integer powers of .
We denote Higgs VEVs by
(92) |
where or is not integer for a generic VEV. Then, the mass matrices can be written by
(93) |
When , all of the Yukawa coupligs are real. In this case, the non-trivial CP phase appears only if the VEVs have phases different relatively from each other. When , e.g. , the Yukawa coupligs have different phases. Thus, the non-trivial CP phase appears for generic values of VEVs. However, if they satisfy
(94) |
for all of allowed Yukawa couplings with fixed, one can cancel phases of mass matrix elements up to an overall phase by rotation. We can compare this condition with the relations Eq. (90), where the factor originates from . Thus, the -symmetry determines the VEV direction , where the CP symmetry remains. CP violation was also studied in an explicit magnetized orbifold model [80].
6 SMEFT
So far, we have studied renormalizable coupligs such as Yukawa couplings. Since the SM is effective theory of underlying theory, it may include higher dimensional operators and they may lead to flavor and CP violating processes. Here, we study higher dimensional operators.
The SM with renormalizable couplings has the flavor symmetry in the limit that all of the Yukawa couplings vanish, where the symmetry is explicitly written by and they correspond to the symmetries of three generations of left-handed quarks, up-sector and down-sector right-handed quarks, left-handed leptons, and right-handed charged leptons. Even for non-vanishing Yukawa couplings, the SM can have the flavor symmetry by assuming that Yukawa couplings are spurion fields, which transform non-trivially under the flavor symmetry. That is, the up-sector and down-sector Yukawa couplings transform as and under the symmetry while the lepton Yukawa couplings transform as . We require that higher dimensional operators also satisfy the flavor symmetry. Then coefficients of higher dimensional operators can be written in terms of Yukawa couplings, which are spurion fields. That is the MFV scenario [31, 32].
We can compute -point couplings within the framework of superstring theory. For example, -point couplings were calculated in intersecting D-brane models [246, 247, 248], magnetized D-brane models[249, 250], and heterotic orbifold models [251, 252, 253, 254, 255, 256]. These computations are carried out by two-dimensional conformal field theory (CFT) and integral of products of wave functions in compact space.
Massless modes in string theory correspond to vertex operators in CFT, where denotes the complex coordinate on the world-sheet. These vertex operators satisfy the operator product expansion,
(95) |
where denote the conformal dimensions of vertex operators . The coefficients provide us with 3-point couplings among massless modes corresponding vertex operators, , , in low-energy effective field theory. Furthermore, 4-point couplings can be written by products of 3-point couplings,
(96) |
Similarly, generic -point couplings can be written by products of 3-point couplings. That implies that when the 3-point couplings have the modular symmetry, 4-point couplings and higher order couplings are also controlled by the modular symmetry. Indeed, these couplings can be written by modular forms, which depend on the moduli fields. In this sense, these couplings are spurion fields. Thus, this theory can provide us with the stringy origin of minimal flavor violation, where the flavor symmetry is the modular symmetry instead of .
Similarly, various classes of 4D low-energy effective field theory derived string theory satisfy the requirement of minimal flavor violation hypothesis at the compactification scale. However, several physical stages may occur between the compactification scale and low energy scale, (i) some modes gain masses and (ii) some scalar fields develop their VEVs. At the stage (i), we just integrate out massive modes. Effective field theory after such an integration also satisfies the above structure. At the stage (ii), new operators appear. For example, suppose that we have the coupling, and develops its VEV. Then, the new operator appears, where . Both and are spurion fields, and the transformation behavior of is the same as . Thus, the minimal flavor violation structure with the modular symmetry is not violated.
One of non-trivial symmetry breaking is the supersymmetry breaking. The supersymmetry breaking can occur by non-vanishing F-terms. If all of the F-terms are trivial singlets under the modular symmetry, obviously all of the soft terms are modular invariant. The supersymmetry breaking due to modulus F-term is non-trivial from the viewpoint of the modular symmetry. Detailed study was done in Ref. [88]. It was found that all of the soft terms except the B-term are modular invariant. If the generation mechanism of the -term is modular invariant, the B-term is also modular invariant.
If the above scenario holds true, the low-energy effective field theory around the weak scale has the minimal flavor violation structure with the modular symmetry. That is, the SMEFT can have the modular symmetry. For example, there appear the four-fermi operators and dipole operators,
(97) |
where denotes a generic combination of gamma matrices. These operators must be modular invariant and their coefficients and are modular forms. Furthermore, the coefficients can be written by productions of 3-point couplings as Eq. (96), where the mode may correspond to known modes like the Higgs field or unknown modes. The cut-off scale depends on the scenario with the stages (i) and (ii), that is, mass scales and symmetry breaking scales including the supersymmetry breaking scale. Phenomenological implications of modular symmetric SMEFT were studied, e.g. flavor violations and lepton processes [81, 82, 83].
7 Conclusion
We have reviewed on modular flavor symmetric models from several viewpoints, realization of fermion mass matrices, the texture structure, the CP violation and higher dimensional operators in SMEFT. Indeed many works have been done recently, in particular in realization of quark and lepton masses and mixing angles as well as the CP violation. In addition, the modular flavor symmetry have been used for dark matter, inflation models, and leptogenesis in bottom-up approach. The modular flavor symmetry may originate from compactification of higher dimensional theory such as superstring theory. Also the modular flavor symmetry have been studied in top-down approach. Thus, the modular flavor symmetry can become a bridge to connect the low-energy physics and high-energy physic such as superstring theory and would provide us with a missing piece to solve the flavor puzzle in particle physics.
Acknowledgement
The authors would like to thank Y. Abe, T. Higaki, K. Ishiguro, J. Kawamura, S. Kikuchi, S. Nagamoto, K. Nasu, T. Nomura, H. Okada, N. Omoto, Y. Orisaka, H. Otsuka, S.T. Petcov, Y. Shimizu, T. Shimomura, S. Takada, K. Takagi, S. Tamba, K. Tanaka, T.H. Tatsuishi, H. Uchida, S. Uemura, K. Yamamoto, T. Yoshida for useful discussions.
Appendix
Appendix A Modular forms of
The modular forms of weight transforming as a triplet of can be written in terms of and its derivative [57]:
(98) | |||||
which satisfy also the constraint [57]:
(99) |
They have the following -expansions:
(100) |
where
(101) |
For weigh 6, there are seven modular forms as:
For weigh 8, there are nine modular forms as:
For weigh 10, there are eleven modular forms as:
(102) |
At the fixed point , they are given as:
Appendix B Tensor product of group
References
- [1] S. Weinberg, Trans. New York Acad. Sci. 38 (1977), 185-201.
- [2] H. Fritzsch, Phys. Lett. B 70 (1977), 436-440.
- [3] H. Fritzsch, Phys. Lett. B 73 (1978), 317-322.
- [4] H. Fritzsch, Nucl. Phys. B 155 (1979), 189-207.
- [5] H. Georgi and C. Jarlskog, Phys. Lett. B 86 (1979), 297-300.
- [6] G. C. Branco, L. Lavoura and F. Mota, Phys. Rev. D 39 (1989), 3443.
- [7] S. Dimopoulos, L. J. Hall and S. Raby, Phys. Rev. D 45 (1992), 4192-4200.
- [8] P. Ramond, R. G. Roberts and G. G. Ross, Nucl. Phys. B 406 (1993), 19-42. [arXiv:hep-ph/9303320 [hep-ph]].
- [9] P. H. Frampton, S. L. Glashow and D. Marfatia, Phys. Lett. B 536 (2002), 79-82 [arXiv:hep-ph/0201008 [hep-ph]].
- [10] C. D. Froggatt and H. B. Nielsen, Nucl. Phys. B 147 (1979), 277-298
- [11] S. Pakvasa and H. Sugawara, Phys. Lett. 73B (1978) 61.
- [12] F. Wilczek and A. Zee, Phys. Lett. 70B (1977) 418 Erratum: [Phys. Lett. 72B (1978) 504].
- [13] M. Fukugita, M. Tanimoto and T. Yanagida, Phys. Rev. D 57 (1998) 4429 [hep-ph/9709388].
- [14] Y. Fukuda et al. [Super-Kamiokande Collaboration], Phys. Rev. Lett. 81 (1998) 1562 [hep-ex/9807003].
- [15] G. Altarelli and F. Feruglio, Rev. Mod. Phys. 82 (2010) 2701 [arXiv:1002.0211 [hep-ph]].
- [16] H. Ishimori, T. Kobayashi, H. Ohki, Y. Shimizu, H. Okada and M. Tanimoto, Prog. Theor. Phys. Suppl. 183 (2010) 1 [arXiv:1003.3552 [hep-th]].
- [17] H. Ishimori, T. Kobayashi, H. Ohki, H. Okada, Y. Shimizu and M. Tanimoto, Lect. Notes Phys. 858 (2012) 1, Springer.
- [18] T. Kobayashi, H. Ohki, H. Okada, Y. Shimizu and M. Tanimoto, Lect. Notes Phys. 995 (2022) 1, Springer doi:10.1007/978-3-662-64679-3.
- [19] D. Hernandez and A. Y. Smirnov, Phys. Rev. D 86 (2012) 053014 [arXiv:1204.0445 [hep-ph]].
- [20] S. F. King and C. Luhn, Rept. Prog. Phys. 76 (2013) 056201 [arXiv:1301.1340 [hep-ph]].
- [21] S. F. King, A. Merle, S. Morisi, Y. Shimizu and M. Tanimoto, New J. Phys. 16, 045018 (2014) [arXiv:1402.4271 [hep-ph]].
- [22] M. Tanimoto, AIP Conf. Proc. 1666 (2015) 120002.
- [23] S. F. King, Prog. Part. Nucl. Phys. 94 (2017) 217 [arXiv:1701.04413 [hep-ph]].
- [24] S. T. Petcov, Eur. Phys. J. C 78 (2018) no.9, 709 [arXiv:1711.10806 [hep-ph]].
- [25] F. Feruglio and A. Romanino, arXiv:1912.06028 [hep-ph].
- [26] W. Buchmuller and D. Wyler, Nucl. Phys. B 268 (1986), 621-653.
- [27] B. Grzadkowski, M. Iskrzynski, M. Misiak and J. Rosiek, JHEP 10 (2010), 085 [arXiv:1008.4884 [hep-ph]].
- [28] R. Alonso, E. E. Jenkins, A. V. Manohar and M. Trott, JHEP 04 (2014), 159 [arXiv:1312.2014 [hep-ph]].
- [29] D. A. Faroughy, G. Isidori, F. Wilsch and K. Yamamoto, JHEP 08 (2020), 166 [arXiv:2005.05366 [hep-ph]].
- [30] J. M. Gerard, Z. Phys. C 18 (1983), 145.
- [31] R. S. Chivukula and H. Georgi, Phys. Lett. B 188 (1987), 99-104.
- [32] G. D’Ambrosio, G. F. Giudice, G. Isidori and A. Strumia, Nucl. Phys. B 645 (2002), 155-187 [arXiv:hep-ph/0207036 [hep-ph]].
- [33] R. Barbieri, G. Isidori, J. Jones-Perez, P. Lodone and D. M. Straub, Eur. Phys. J. C 71 (2011), 1725 [arXiv:1105.2296 [hep-ph]].
- [34] R. Barbieri, D. Buttazzo, F. Sala and D. M. Straub, JHEP 07 (2012), 181 [arXiv:1203.4218 [hep-ph]].
- [35] G. Blankenburg, G. Isidori and J. Jones-Perez, Eur. Phys. J. C 72 (2012), 2126 [arXiv:1204.0688 [hep-ph]].
- [36] T. Kobayashi, S. Raby and R. J. Zhang, Nucl. Phys. B 704, 3-55 (2005) [arXiv:hep-ph/0409098 [hep-ph]].
- [37] T. Kobayashi, H. P. Nilles, F. Ploger, S. Raby and M. Ratz, Nucl. Phys. B 768, 135-156 (2007) [arXiv:hep-ph/0611020 [hep-ph]].
- [38] P. Ko, T. Kobayashi, J. h. Park and S. Raby, Phys. Rev. D 76, 035005 (2007) [erratum: Phys. Rev. D 76, 059901 (2007)] [arXiv:0704.2807 [hep-ph]].
- [39] H. Abe, K. S. Choi, T. Kobayashi and H. Ohki, Nucl. Phys. B 820, 317-333 (2009) [arXiv:0904.2631 [hep-ph]].
- [40] F. Beye, T. Kobayashi and S. Kuwakino, Phys. Lett. B 736, 433-437 (2014) [arXiv:1406.4660 [hep-th]].
- [41] S. Ferrara, D. Lust and S. Theisen, Phys. Lett. B 233 (1989), 147-152.
- [42] W. Lerche, D. Lust and N. P. Warner, Phys. Lett. B 231 (1989), 417-424.
- [43] J. Lauer, J. Mas and H. P. Nilles, Phys. Lett. B 226, 251-256 (1989) doi:10.1016/0370-2693(89)91190-8.
- [44] J. Lauer, J. Mas and H. P. Nilles, Nucl. Phys. B 351, 353 (1991).
- [45] T. Kobayashi, S. Nagamoto, S. Takada, S. Tamba and T. H. Tatsuishi, Phys. Rev. D 97, no. 11, 116002 (2018) [arXiv:1804.06644 [hep-th]].
- [46] T. Kobayashi and S. Tamba, Phys. Rev. D 99, no.4, 046001 (2019) [arXiv:1811.11384 [hep-th]].
- [47] H. Ohki, S. Uemura and R. Watanabe, Phys. Rev. D 102, no.8, 085008 (2020) [arXiv:2003.04174 [hep-th]].
- [48] S. Kikuchi, T. Kobayashi, S. Takada, T. H. Tatsuishi and H. Uchida, Phys. Rev. D 102, no.10, 105010 (2020) [arXiv:2005.12642 [hep-th]].
- [49] S. Kikuchi, T. Kobayashi, H. Otsuka, S. Takada and H. Uchida, JHEP 11, 101 (2020) [arXiv:2007.06188 [hep-th]].
- [50] S. Kikuchi, T. Kobayashi and H. Uchida, Phys. Rev. D 104, no.6, 065008 (2021) [arXiv:2101.00826 [hep-th]].
- [51] Y. Almumin, M. C. Chen, V. Knapp-Perez, S. Ramos-Sanchez, M. Ratz and S. Shukla, JHEP 05 (2021), 078 [arXiv:2102.11286 [hep-th]].
- [52] A. Strominger, Commun. Math. Phys. 133 (1990), 163-180.
- [53] P. Candelas and X. de la Ossa, Nucl. Phys. B 355 (1991), 455-481.
- [54] K. Ishiguro, T. Kobayashi and H. Otsuka, Nucl. Phys. B 973, 115598 (2021) [arXiv:2010.10782 [hep-th]].
- [55] K. Ishiguro, T. Kobayashi and H. Otsuka, JHEP 01, 020 (2022) [arXiv:2107.00487 [hep-th]].
- [56] R. de Adelhart Toorop, F. Feruglio and C. Hagedorn, Nucl. Phys. B 858, 437 (2012) [arXiv:1112.1340 [hep-ph]].
- [57] F. Feruglio, in From My Vast Repertoire …: Guido Altarelli’s Legacy, A. Levy, S. Forte, Stefano, and G. Ridolfi, eds., pp.227–266, 2019, arXiv:1706.08749 [hep-ph].
- [58] T. Kobayashi, K. Tanaka and T. H. Tatsuishi, Phys. Rev. D 98 (2018) no.1, 016004 [arXiv:1803.10391 [hep-ph]].
- [59] J. T. Penedo and S. T. Petcov, Nucl. Phys. B 939 (2019) 292 [arXiv:1806.11040 [hep-ph]].
- [60] P. P. Novichkov, J. T. Penedo, S. T. Petcov and A. V. Titov, JHEP 1904, 174 (2019) [arXiv:1812.02158 [hep-ph]].
- [61] G. J. Ding, S. F. King and X. G. Liu, Phys. Rev. D 100 (2019) no.11, 115005 [arXiv:1903.12588 [hep-ph]].
- [62] M. B. Green, J. H. Schwarz and E. Witten, Cambridge, Uk: Univ. Pr. ( 1987) 596 P. ( Cambridge Monographs On Mathematical Physics)
- [63] A. Strominger and E. Witten, Commun. Math. Phys. 101, 341 (1985).
- [64] M. Dine, R. G. Leigh and D. A. MacIntire, Phys. Rev. Lett. 69, 2030 (1992) [hep-th/9205011].
- [65] K. w. Choi, D. B. Kaplan and A. E. Nelson, Nucl. Phys. B 391, 515 (1993) [hep-ph/9205202].
- [66] C. S. Lim, Phys. Lett. B 256, 233 (1991).
- [67] T. Kobayashi and C. S. Lim, Phys. Lett. B 343, 122 (1995) [hep-th/9410023].
- [68] B. S. Acharya, D. Bailin, A. Love, W. A. Sabra and S. Thomas, Phys. Lett. B 357, 387 (1995) Erratum: [Phys. Lett. B 407, 451 (1997)] [hep-th/9506143].
- [69] T. Dent, Phys. Rev. D 64, 056005 (2001) [hep-ph/0105285].
- [70] S. Khalil, O. Lebedev and S. Morris, Phys. Rev. D 65, 115014 (2002) [hep-th/0110063].
- [71] J. Giedt, Mod. Phys. Lett. A 17, 1465 (2002) [hep-ph/0204017].
- [72] T. Kobayashi and H. Otsuka, Phys. Rev. D 102, no.2, 026004 (2020) [arXiv:2004.04518 [hep-th]].
- [73] A. Baur, H. P. Nilles, A. Trautner and P. K. S. Vaudrevange, Phys. Lett. B 795, 7 (2019) [arXiv:1901.03251 [hep-th]];
- [74] P. P. Novichkov, J. T. Penedo, S. T. Petcov and A. V. Titov, JHEP 1907, 165 (2019) [arXiv:1905.11970 [hep-ph]].
- [75] A. Baur, H. P. Nilles, A. Trautner and P. K. S. Vaudrevange, Nucl. Phys. B 947 (2019), 114737 [arXiv:1908.00805 [hep-th]].
- [76] A. Baur, M. Kade, H. P. Nilles, S. Ramos-Sanchez and P. K. S. Vaudrevange, JHEP 02 (2021), 018 [arXiv:2008.07534 [hep-th]].
- [77] H. P. Nilles, S. Ramos–Sánchez and P. K. S. Vaudrevange, Nucl. Phys. B 966 (2021), 115367 [arXiv:2010.13798 [hep-th]].
- [78] K. Bönisch, M. Elmi, A. K. Kashani-Poor and A. Klemm, [arXiv:2204.06506 [hep-th]].
- [79] T. Kobayashi, Y. Shimizu, K. Takagi, M. Tanimoto, T. H. Tatsuishi and H. Uchida, Phys. Rev. D 101, no.5, 055046 (2020) [arXiv:1910.11553 [hep-ph]].
- [80] S. Kikuchi, T. Kobayashi, M. Tanimoto and H. Uchida, PTEP 2022, no.11, 113B07 (2022) [arXiv:2206.08538 [hep-ph]].
- [81] T. Kobayashi and H. Otsuka, Eur. Phys. J. C 82, no.1, 25 (2022) [arXiv:2108.02700 [hep-ph]].
- [82] T. Kobayashi, H. Otsuka, M. Tanimoto and K. Yamamoto, Phys. Rev. D 105, no.5, 055022 (2022) [arXiv:2112.00493 [hep-ph]].
- [83] T. Kobayashi, H. Otsuka, M. Tanimoto and K. Yamamoto, JHEP 08, 013 (2022) [arXiv:2204.12325 [hep-ph]].
- [84] T. Nomura and H. Okada, Phys. Lett. B 797, 134799 (2019) [arXiv:1904.03937 [hep-ph]].
- [85] T. Kobayashi, H. Okada and Y. Orikasa, Phys. Dark Univ. 37, 101080 (2022) [arXiv:2111.05674 [hep-ph]].
- [86] T. Kobayashi, T. Shimomura and M. Tanimoto, Phys. Lett. B 819, 136452 (2021) [arXiv:2102.10425 [hep-ph]].
- [87] M. Tanimoto and K. Yamamoto, JHEP 10, 183 (2021) [arXiv:2106.10919 [hep-ph]].
- [88] S. Kikuchi, T. Kobayashi, K. Nasu, H. Otsuka, S. Takada and H. Uchida, PTEP 2022, no.12, 123B02 (2022) [arXiv:2203.14667 [hep-ph]].
- [89] T. Kobayashi, S. Nishimura, H. Otsuka, M. Tanimoto and K. Yamamoto, [arXiv:2207.14014 [hep-ph]].
- [90] F. Feruglio, A. Strumia and A. Titov, [arXiv:2305.08908 [hep-ph]].
- [91] R. C. Gunning, Lectures on Modular Forms (Princeton University Press, Princeton, NJ, 1962).
- [92] B. Schoeneberg, Elliptic Modular Functions (Springer-Verlag, 1974).
- [93] N. Koblitz, Introduction to Elliptic Curves and Modular Forms (Springer-Verlag, 1984).
- [94] J.H. Bruinier, G.V.D. Geer, G. Harder, and D. Zagier, The 1-2-3 of Modular Forms (Springer, 2008).
- [95] S. Ferrara, D. Lust, A. D. Shapere and S. Theisen, Phys. Lett. B 225, 363 (1989).
- [96] M. Chen, S. Ramos-Sánchez and M. Ratz, Phys. Lett. B 801 (2020), 135153 [arXiv:1909.06910 [hep-ph]].
- [97] T. Kobayashi, N. Omoto, Y. Shimizu, K. Takagi, M. Tanimoto and T. H. Tatsuishi, JHEP 11 (2018), 196 [arXiv:1808.03012 [hep-ph]].
- [98] I. Esteban, M. C. Gonzalez-Garcia, M. Maltoni, T. Schwetz and A. Zhou, JHEP 09 (2020), 178 [arXiv:2007.14792 [hep-ph]].
- [99] S. Vagnozzi, E. Giusarma, O. Mena, K. Freese, M. Gerbino, S. Ho and M. Lattanzi, Phys. Rev. D 96 (2017) no.12, 123503 [arXiv:1701.08172 [astro-ph.CO]].
- [100] N. Aghanim et al. [Planck], Astron. Astrophys. 641 (2020), A6 [arXiv:1807.06209 [astro-ph.CO]].
- [101] R. L. Workman et al. [Particle Data Group], PTEP 2022 (2022), 083C01.
- [102] S. Antusch and V. Maurer, JHEP 1311 (2013) 115 [arXiv:1306.6879 [hep-ph]].
- [103] F. Björkeroth, F. J. de Anda, I. de Medeiros Varzielas and S. F. King, JHEP 1506 (2015) 141 [arXiv:1503.03306 [hep-ph]].
- [104] J. C. Criado and F. Feruglio, SciPost Phys. 5 (2018) no.5, 042 [arXiv:1807.01125 [hep-ph]].
- [105] G. J. Ding, S. F. King and X. G. Liu, JHEP 1909 (2019) 074 [arXiv:1907.11714 [hep-ph]].
- [106] H. Okada and M. Tanimoto, JHEP 03 (2021), 010 [arXiv:2012.01688 [hep-ph]].
- [107] C. Y. Yao, J. N. Lu and G. J. Ding, JHEP 05 (2021), 102 [arXiv:2012.13390 [hep-ph]].
- [108] P. P. Novichkov, J. T. Penedo, S. T. Petcov and A. V. Titov, JHEP 1904 (2019) 005 [arXiv:1811.04933 [hep-ph]].
- [109] T. Kobayashi, Y. Shimizu, K. Takagi, M. Tanimoto and T. H. Tatsuishi, JHEP 02 (2020), 097 [arXiv:1907.09141 [hep-ph]].
- [110] X. Wang and S. Zhou, JHEP 05 (2020), 017 [arXiv:1910.09473 [hep-ph]].
- [111] J. Gehrlein and M. Spinrath, JHEP 03 (2021), 177 [arXiv:2012.04131 [hep-ph]].
- [112] T. Kobayashi, Y. Shimizu, K. Takagi, M. Tanimoto and T. H. Tatsuishi, PTEP 2020, no.5, 053B05 (2020) [arXiv:1906.10341 [hep-ph]].
- [113] D. Meloni and M. Parriciatu, [arXiv:2306.09028 [hep-ph]].
- [114] X. G. Liu and G. J. Ding, JHEP 1908 (2019) 134 [arXiv:1907.01488 [hep-ph]].
- [115] P. P. Novichkov, J. T. Penedo and S. T. Petcov, Nucl. Phys. B 963 (2021), 115301 [arXiv:2006.03058 [hep-ph]].
- [116] X. G. Liu, C. Y. Yao and G. J. Ding, Phys. Rev. D 103 (2021) no.5, 056013 [arXiv:2006.10722 [hep-ph]].
- [117] X. Wang, B. Yu and S. Zhou, Phys. Rev. D 103 (2021) no.7, 076005 [arXiv:2010.10159 [hep-ph]].
- [118] C. Y. Yao, X. G. Liu and G. J. Ding, [arXiv:2011.03501 [hep-ph]].
- [119] H. Okada and Y. Orikasa, Chin. Phys. C 46 (2022) no.12, 123108 [arXiv:2206.12629 [hep-ph]].
- [120] G. J. Ding, X. G. Liu and C. Y. Yao, [arXiv:2211.04546 [hep-ph]].
- [121] G. J. Ding, F. R. Joaquim and J. N. Lu, [arXiv:2211.08136 [hep-ph]].
- [122] P. Beneš, H. Okada and Y. Orikasa, [arXiv:2212.07245 [hep-ph]].
- [123] G. J. Ding, S. F. King, C. C. Li and Y. L. Zhou, JHEP 08 (2020), 164 [arXiv:2004.12662 [hep-ph]].
- [124] C. C. Li, X. G. Liu and G. J. Ding, JHEP 10 (2021), 238 [arXiv:2108.02181 [hep-ph]].
- [125] H. Okada and M. Tanimoto, Phys. Lett. B 791 (2019) 54 [arXiv:1812.09677 [hep-ph]].
- [126] H. Okada and M. Tanimoto, Eur. Phys. J. C 81 (2021) no.1, 52 [arXiv:1905.13421 [hep-ph]].
- [127] F. J. de Anda, S. F. King and E. Perdomo, Phys. Rev. D 101 (2020) no.1, 015028 [arXiv:1812.05620 [hep-ph]].
- [128] S. F. King and Y. L. Zhou, JHEP 04 (2021), 291 [arXiv:2103.02633 [hep-ph]].
- [129] P. Chen, G. J. Ding and S. F. King, JHEP 04 (2021), 239 [arXiv:2101.12724 [hep-ph]].
- [130] X. Du and F. Wang, JHEP 02, 221 (2021) [arXiv:2012.01397 [hep-ph]].
- [131] G. J. Ding, S. F. King and C. Y. Yao, [arXiv:2103.16311 [hep-ph]].
- [132] G. J. Ding, S. F. King and J. N. Lu, JHEP 11 (2021), 007 [arXiv:2108.09655 [hep-ph]].
- [133] G. J. Ding, S. F. King, J. N. Lu and B. Y. Qu, JHEP 10 (2022), 071 [arXiv:2206.14675 [hep-ph]].
- [134] T. Asaka, Y. Heo, T. H. Tatsuishi and T. Yoshida, JHEP 2001 (2020) 144 [arXiv:1909.06520 [hep-ph]].
- [135] H. Okada, Y. Shimizu, M. Tanimoto and T. Yoshida, JHEP 07 (2021), 184 [arXiv:2105.14292 [hep-ph]].
- [136] B. Y. Qu, X. G. Liu, P. T. Chen and G. J. Ding, Phys. Rev. D 104 (2021) no.7, 076001 [arXiv:2106.11659 [hep-ph]].
- [137] P. P. Novichkov, S. T. Petcov and M. Tanimoto, Phys. Lett. B 793 (2019) 247 [arXiv:1812.11289 [hep-ph]].
- [138] G. J. Ding, S. F. King, X. G. Liu and J. N. Lu, JHEP 1912 (2019) 030 [arXiv:1910.03460 [hep-ph]].
- [139] H. Okada and M. Tanimoto, Phys. Rev. D 103 (2021) no.1, 015005 [arXiv:2009.14242 [hep-ph]].
- [140] P. P. Novichkov, J. T. Penedo and S. T. Petcov, JHEP 04, 206 (2021) [arXiv:2102.07488 [hep-ph]].
- [141] F. Feruglio, V. Gherardi, A. Romanino and A. Titov, JHEP 05 (2021), 242 [arXiv:2101.08718 [hep-ph]].
- [142] F. Feruglio, Phys. Rev. Lett. 130 (2023) no.10, 101801 doi:10.1103/PhysRevLett. 130.101801.
- [143] S. T. Petcov and M. Tanimoto, [arXiv:2212.13336 [hep-ph]].
- [144] S. T. Petcov and M. Tanimoto, [arXiv:2306.05730 [hep-ph]].
- [145] S. Kikuchi, T. Kobayashi, K. Nasu, S. Takada and H. Uchida, Phys. Rev. D 107, no.5, 055014 (2023) [arXiv:2301.03737 [hep-ph]].
- [146] Y. Abe, T. Higaki, J. Kawamurab and T. Kobayashi, [arXiv:2301.07439 [hep-ph]].
- [147] S. Kikuchi, T. Kobayashi, K. Nasu, S. Takada and H. Uchida, [arXiv:2302.03326 [hep-ph]].
- [148] Y. Abe, T. Higaki, J. Kawamura and T. Kobayashi, [arXiv:2302.11183 [hep-ph]].
- [149] Y. Abe, T. Higaki, J. Kawamura and T. Kobayashi, [arXiv:2307.01419 [hep-ph]].
- [150] T. Kobayashi, Y. Shimizu, K. Takagi, M. Tanimoto, T. H. Tatsuishi and H. Uchida, Phys. Lett. B 794 (2019) 114 [arXiv:1812.11072 [hep-ph]].
- [151] T. Kobayashi, Y. Shimizu, K. Takagi, M. Tanimoto and T. H. Tatsuishi, Phys. Rev. D 100 (2019) no.11, 115045 [erratum: Phys. Rev. D 101 (2020) no.3, 039904] [arXiv:1909.05139 [hep-ph]].
- [152] T. Asaka, Y. Heo and T. Yoshida, Phys. Lett. B 811 (2020), 135956 [arXiv:2009.12120 [hep-ph]].
- [153] M. K. Behera, S. Mishra, S. Singirala and R. Mohanta, Phys. Dark Univ. 36 (2022), 101027 [arXiv:2007.00545 [hep-ph]].
- [154] S. Mishra, [arXiv:2008.02095 [hep-ph]].
- [155] H. Okada and Y. Orikasa, Phys. Rev. D 100, no.11, 115037 (2019) [arXiv:1907.04716 [hep-ph]].
- [156] Y. Kariyazono, T. Kobayashi, S. Takada, S. Tamba and H. Uchida, Phys. Rev. D 100, no.4, 045014 (2019) [arXiv:1904.07546 [hep-th]].
- [157] T. Nomura and H. Okada, Nucl. Phys. B 966 (2021), 115372 [arXiv:1906.03927 [hep-ph]].
- [158] H. Okada and Y. Orikasa, arXiv:1908.08409 [hep-ph].
- [159] T. Nomura, H. Okada and O. Popov, Phys. Lett. B 803 (2020) 135294 [arXiv:1908.07457 [hep-ph]].
- [160] J. C. Criado, F. Feruglio and S. J. D. King, JHEP 2002 (2020) 001 [arXiv:1908.11867 [hep-ph]].
- [161] S. F. King and Y. L. Zhou, Phys. Rev. D 101 (2020) no.1, 015001 [arXiv:1908.02770 [hep-ph]].
- [162] D. Zhang, Nucl. Phys. B 952 (2020) 114935 [arXiv:1910.07869 [hep-ph]].
- [163] J. N. Lu, X. G. Liu and G. J. Ding, Phys. Rev. D 101 (2020) no.11, 115020 [arXiv:1912.07573 [hep-ph]].
- [164] T. Nomura, H. Okada and S. Patra, Nucl. Phys. B 967 (2021), 115395 [arXiv:1912.00379 [hep-ph]].
- [165] T. Kobayashi, T. Nomura and T. Shimomura, Phys. Rev. D 102 (2020) no.3, 035019 [arXiv:1912.00637 [hep-ph]].
- [166] X. Wang, Nucl. Phys. B 957 (2020), 115105 [arXiv:1912.13284 [hep-ph]].
- [167] S. J. D. King and S. F. King, JHEP 09 (2020), 043 [arXiv:2002.00969 [hep-ph]].
- [168] M. Abbas, Phys. Rev. D 103 (2021) no.5, 056016 [arXiv:2002.01929 [hep-ph]].
- [169] H. Okada and Y. Shoji, Phys. Dark Univ. 31 (2021), 100742 [arXiv:2003.11396 [hep-ph]].
- [170] H. Okada and Y. Shoji, Nucl. Phys. B 961 (2020), 115216 [arXiv:2003.13219 [hep-ph]].
- [171] G. J. Ding and F. Feruglio, JHEP 06 (2020), 134 [arXiv:2003.13448 [hep-ph]].
- [172] T. Nomura and H. Okada, JCAP 09 (2022), 049 doi:10.1088/1475-7516/2022/09/049 [arXiv:2007.04801 [hep-ph]].
- [173] T. Nomura and H. Okada, arXiv:2007.15459 [hep-ph].
- [174] H. Okada and M. Tanimoto, Phys. Dark Univ. 40 (2023), 101204 [arXiv:2005.00775 [hep-ph]].
- [175] I. de Medeiros Varzielas, M. Levy and Y. L. Zhou, JHEP 11 (2020), 085 [arXiv:2008.05329 [hep-ph]].
- [176] K. I. Nagao and H. Okada, JCAP 05 (2021), 063 [arXiv:2008.13686 [hep-ph]].
- [177] K. I. Nagao and H. Okada, Nucl. Phys. B 980 (2022), 115841 [arXiv:2010.03348 [hep-ph]].
- [178] M. Abbas, Phys. Atom. Nucl. 83 (2020) no.5, 764-769.
- [179] H. Kuranaga, H. Ohki and S. Uemura, JHEP 07 (2021), 068 [arXiv:2105.06237 [hep-ph]].
- [180] H. Okada and Y. h. Qi, [arXiv:2109.13779 [hep-ph]].
- [181] A. Dasgupta, T. Nomura, H. Okada, O. Popov and M. Tanimoto, [arXiv:2111.06898 [hep-ph]].
- [182] T. Nomura and H. Okada, Chin. Phys. C 46 (2022) no.5, 053101 [arXiv:2109.04157 [hep-ph]].
- [183] K. I. Nagao and H. Okada, Phys. Dark Univ. 36 (2022), 101039 [arXiv:2108.09984 [hep-ph]].
- [184] T. Nomura, H. Okada and Y. Orikasa, Eur. Phys. J. C 81 (2021) no.10, 947 [arXiv:2106.12375 [hep-ph]].
- [185] T. Nomura and H. Okada, Phys. Rev. D 105 (2022) no.7, 075010 [arXiv:2106.10451 [hep-ph]].
- [186] X. Zhang and S. Zhou, JCAP 09 (2021), 043 [arXiv:2106.03433 [hep-ph]].
- [187] X. Wang and S. Zhou, JHEP 07 (2021), 093 [arXiv:2102.04358 [hep-ph]].
- [188] X. Wang, Nucl. Phys. B 962 (2021), 115247 [arXiv:2007.05913 [hep-ph]].
- [189] P. Ko, T. Nomura and H. Okada, JHEP 05 (2022), 098 [arXiv:2110.10513 [hep-ph]].
- [190] T. Nomura, H. Okada and Y. h. Qi, [arXiv:2111.10944 [hep-ph]].
- [191] T. Nomura and H. Okada, [arXiv:2201.10244 [hep-ph]].
- [192] H. Otsuka and H. Okada, [arXiv:2202.10089 [hep-ph]].
- [193] G. J. Ding, F. Feruglio and X. G. Liu, SciPost Phys. 10 (2021) no.6, 133 [arXiv:2102.06716 [hep-ph]].
- [194] G. Charalampous, S. F. King, G. K. Leontaris and Y. L. Zhou, Phys. Rev. D 104 (2021) no.11, 115015 [arXiv:2109.11379 [hep-ph]].
- [195] X. G. Liu and G. J. Ding, JHEP 03 (2022), 123 [arXiv:2112.14761 [hep-ph]].
- [196] P. P. Novichkov, J. T. Penedo and S. T. Petcov, JHEP 03 (2022), 149 [arXiv:2201.02020 [hep-ph]].
- [197] S. Kikuchi, T. Kobayashi, H. Otsuka, M. Tanimoto, H. Uchida and K. Yamamoto, Phys. Rev. D 106 (2022) no.3, 035001 [arXiv:2201.04505 [hep-ph]].
- [198] M. K. Behera, S. Singirala, S. Mishra and R. Mohanta, J. Phys. G 49 (2022) no.3, 035002 [arXiv:2009.01806 [hep-ph]].
- [199] Y. H. Ahn, S. K. Kang, R. Ramos and M. Tanimoto, Phys. Rev. D 106 (2022) no.9, 095002 [arXiv:2205.02796 [hep-ph]].
- [200] Y. Gunji, K. Ishiwata and T. Yoshida, JHEP 11 (2022), 002 [arXiv:2208.10086 [hep-ph]].
- [201] J. Kim and H. Okada, [arXiv:2302.09747 [hep-ph]].
- [202] T. Nomura, H. Okada and Y. Shoji, PTEP 2023 (2023) no.2, 023B04.
- [203] D. W. Kang, J. Kim, T. Nomura and H. Okada, JHEP 07 (2022), 050 [arXiv:2205.08269 [hep-ph]].
- [204] Y. Abe, T. Higaki, F. Kaneko, T. Kobayashi and H. Otsuka, [arXiv:2303.02947 [hep-ph]].
- [205] I. de Medeiros Varzielas, S. F. King and M. Levy, JHEP 02 (2023), 143 [arXiv:2211.00654 [hep-ph]].
- [206] G. J. Ding, S. F. King, C. C. Li, X. G. Liu and J. N. Lu, [arXiv:2303.02071 [hep-ph]].
- [207] F. J. de Anda and S. F. King, [arXiv:2304.05958 [hep-ph]].
- [208] T. Nomura and H. Okada, [arXiv:2304.13361 [hep-ph]].
- [209] Y. H. Ahn and S. K. Kang, [arXiv:2306.14467 [hep-ph]].
- [210] T. Kobayashi, S. Nagamoto and S. Uemura, PTEP 2017, no.2, 023B02 (2017) [arXiv:1608.06129 [hep-th]].
- [211] I. de Medeiros Varzielas, S. F. King and Y. L. Zhou, Phys. Rev. D 101 (2020) no.5, 055033 [arXiv:1906.02208 [hep-ph]].
- [212] K. Ishiguro, T. Kobayashi and H. Otsuka, JHEP 03, 161 (2021) [arXiv:2011.09154 [hep-ph]].
- [213] H. Abe, T. Kobayashi, S. Uemura and J. Yamamoto, Phys. Rev. D 102, no.4, 045005 (2020) [arXiv:2003.03512 [hep-th]].
- [214] S. Kikuchi, T. Kobayashi, Y. Ogawa and H. Uchida, PTEP 2022, no.3, 033B10 (2022) [arXiv:2112.01680 [hep-ph]].
- [215] H. P. Nilles, S. Ramos-Śanchez and P. K. S. Vaudrevange, JHEP 02 (2020), 045 [arXiv:2001.01736 [hep-ph]].
- [216] H. P. Nilles, S. Ramos-Sánchez and P. K. S. Vaudrevange, Nucl. Phys. B 957 (2020), 115098 [arXiv:2004.05200 [hep-ph]].
- [217] H. P. Nilles, S. Ramos–Sánchez and P. K. S. Vaudrevange, Phys. Lett. B 808 (2020), 135615 [arXiv:2006.03059 [hep-th]].
- [218] A. Baur, M. Kade, H. P. Nilles, S. Ramos-Sanchez and P. K. S. Vaudrevange, Phys. Lett. B 816 (2021), 136176 [arXiv:2012.09586 [hep-th]].
- [219] G. J. Ding, F. Feruglio and X. G. Liu, JHEP 01 (2021), 037 [arXiv:2010.07952 [hep-th]].
- [220] A. Baur, M. Kade, H. P. Nilles, S. Ramos-Sanchez and P. K. S. Vaudrevange, JHEP 06 (2021), 110 [arXiv:2104.03981 [hep-th]].
- [221] H. P. Nilles, S. Ramos-Sanchez and P. K. S. Vaudrevange, [arXiv:2105.02984 [hep-th]].
- [222] H. P. Nilles, S. Ramos-Sanchez, A. Trautner and P. K. S. Vaudrevange, Nucl. Phys. B 971 (2021), 115534 [arXiv:2105.08078 [hep-th]].
- [223] A. Baur, H. P. Nilles, S. Ramos-Sanchez, A. Trautner and P. K. S. Vaudrevange, Phys. Rev. D 105 (2022) no.5, 055018 [arXiv:2112.06940 [hep-th]].
- [224] A. Baur, H. P. Nilles, S. Ramos-Sanchez, A. Trautner and P. K. S. Vaudrevange, JHEP 09 (2022), 224 [arXiv:2207.10677 [hep-ph]].
- [225] S. Kikuchi, T. Kobayashi, K. Nasu, H. Otsuka, S. Takada and H. Uchida, JHEP 04, 003 (2023) [arXiv:2301.10356 [hep-th]].
- [226] F. Feruglio, JHEP 03 (2023), 236 [arXiv:2302.11580 [hep-ph]].
- [227] V. Knapp-Perez, X. G. Liu, H. P. Nilles, S. Ramos-Sanchez and M. Ratz, [arXiv:2304.14437 [hep-th]].
- [228] H. Abe, T. Kobayashi and H. Ohki, JHEP 09 (2008), 043 [arXiv:0806.4748 [hep-th]].
- [229] T. H. Abe, Y. Fujimoto, T. Kobayashi, T. Miura, K. Nishiwaki and M. Sakamoto, JHEP 1401, 065 (2014) [arXiv:1309.4925 [hep-th]].
- [230] H. Abe, T. Kobayashi, K. Sumita and S. Uemura, Phys. Rev. D 96, no.2, 026019 (2017) [arXiv:1703.03402 [hep-th]].
- [231] H. Abe, T. Kobayashi, H. Ohki, A. Oikawa and K. Sumita, Nucl. Phys. B 870, 30-54 (2013) [arXiv:1211.4317 [hep-ph]].
- [232] H. Abe, T. Kobayashi, K. Sumita and Y. Tatsuta, Phys. Rev. D 90, no.10, 105006 (2014) [arXiv:1405.5012 [hep-ph]].
- [233] Y. Fujimoto, T. Kobayashi, K. Nishiwaki, M. Sakamoto and Y. Tatsuta, Phys. Rev. D 94, no.3, 035031 (2016) [arXiv:1605.00140 [hep-ph]].
- [234] W. Buchmuller and J. Schweizer, Phys. Rev. D 95, no.7, 075024 (2017) [arXiv:1701.06935 [hep-ph]].
- [235] W. Buchmuller and K. M. Patel, Phys. Rev. D 97, no.7, 075019 (2018) [arXiv:1712.06862 [hep-ph]].
- [236] K. Hoshiya, S. Kikuchi, T. Kobayashi and H. Uchida, Phys. Rev. D 106 (2022) no.11, 115003 [arXiv:2209.07249 [hep-ph]].
- [237] S. Kikuchi, T. Kobayashi, M. Tanimoto and H. Uchida, [arXiv:2207.04609 [hep-ph]].
- [238] M. Fukugita, M. Tanimoto and T. Yanagida, Phys. Lett. B 562 (2003), 273-278 doi:10.1016/S0370-2693(03)00568-9 [arXiv:hep-ph/0303177 [hep-ph]].
- [239] Z. z. Xing and S. Zhou, Phys. Lett. B 593 (2004), 156-164 [arXiv:hep-ph/0403261 [hep-ph]].
- [240] M. Obara and Z. z. Xing, Phys. Lett. B 644 (2007), 136-146 doi:10.1016/j.physletb. 2006.11.010 [arXiv:hep-ph/0608280 [hep-ph]].
- [241] M. Fukugita, Y. Shimizu, M. Tanimoto and T. T. Yanagida, Phys. Lett. B 716 (2012), 294-297 doi:10.1016/j.physletb.2012.06.049 [arXiv:1204.2389 [hep-ph]].
- [242] M. Fukugita, Y. Kaneta, Y. Shimizu, M. Tanimoto and T. T. Yanagida, Phys. Lett. B 764 (2017), 163-166 doi:10.1016/j.physletb.2016.11.024 [arXiv:1609.01864 [hep-ph]].
- [243] H. Fritzsch and S. Zhou, Phys. Lett. B 718 (2013), 1457-1464 [arXiv:1212.0411 [hep-ph]].
- [244] S. Gukov, C. Vafa and E. Witten, Nucl. Phys. B 584, 69-108 (2000) [erratum: Nucl. Phys. B 608, 477-478 (2001)] [arXiv:hep-th/9906070 [hep-th]].
- [245] K. Ishiguro, H. Okada and H. Otsuka, JHEP 09 (2022), 072 [arXiv:2206.04313 [hep-ph]].
- [246] M. Cvetic and I. Papadimitriou, Phys. Rev. D 68, 046001 (2003) [erratum: Phys. Rev. D 70, 029903 (2004)] [arXiv:hep-th/0303083 [hep-th]].
- [247] S. A. Abel and A. W. Owen, Nucl. Phys. B 663, 197-214 (2003) [arXiv:hep-th/0303124 [hep-th]].
- [248] S. A. Abel and A. W. Owen, Nucl. Phys. B 682, 183-216 (2004) [arXiv:hep-th/0310257 [hep-th]].
- [249] D. Cremades, L. E. Ibanez and F. Marchesano, JHEP 05 (2004), 079 [arXiv:hep-th/0404229 [hep-th]].
- [250] H. Abe, K. S. Choi, T. Kobayashi and H. Ohki, JHEP 06, 080 (2009) [arXiv:0903.3800 [hep-th]].
- [251] S. Hamidi and C. Vafa, Nucl. Phys. B 279, 465-513 (1987).
- [252] L. J. Dixon, D. Friedan, E. J. Martinec and S. H. Shenker, Nucl. Phys. B 282, 13-73 (1987).
- [253] J. J. Atick, L. J. Dixon, P. A. Griffin and D. Nemeschansky, Nucl. Phys. B 298, 1-35 (1988).
- [254] T. T. Burwick, R. K. Kaiser and H. F. Muller, Nucl. Phys. B 355, 689-711 (1991).
- [255] S. Stieberger, D. Jungnickel, J. Lauer and M. Spalinski, Mod. Phys. Lett. A 7, 3059-3070 (1992) [arXiv:hep-th/9204037 [hep-th]].
- [256] K. S. Choi and T. Kobayashi, Nucl. Phys. B 797, 295-321 (2008) [arXiv:0711.4894 [hep-th]].