Advances in High Energy Physics

Advances in High Energy Physics / 2020 / Article

Research Article | Open Access

Volume 2020 |Article ID 2491897 | https://doi.org/10.1155/2020/2491897

T. K. Kuo, S. H. Chiu, "Flavor Mixing and the Permutation Symmetry among Generations", Advances in High Energy Physics, vol. 2020, Article ID 2491897, 8 pages, 2020. https://doi.org/10.1155/2020/2491897

Flavor Mixing and the Permutation Symmetry among Generations

Academic Editor: Ricardo G Felipe
Received30 Sep 2019
Revised27 Nov 2019
Accepted29 Nov 2019
Published07 Jan 2020

Abstract

In the standard model, the permutation symmetry among the three generations of fundamental fermions is usually regarded to be broken by the Higgs couplings. It is found that the symmetry is restored if we include the mass matrix parameters as physical variables which transform appropriately under the symmetry operation. Known relations between these variables, such as the renormalization group equations, as well as formulas for neutrino oscillations (in vacuum and in matter), are shown to be covariant tensor equations under the permutation symmetry group.

1. Introduction

One of the long-standing puzzles in the standard model (SM) is the existence of three generations of fermions which behave identically under the gauge interactions. The resulting exchange symmetry will be dubbed as the g-permutation symmetry in this paper. This symmetry is commonly regarded as broken by the Higgs coupling through its vacuum expectation value (VEV), resulting in four mass matrices and a plethora of physical parameters, viz., the fermion masses and the mixing matrices for quarks () and for neutrinos (). If these parameters are considered as fixed entities, then they would seem to be a collection of arbitrary numbers, which do not transform under the symmetry operation, and the g-permutation would just be broken. However, there are at least three classes of physical phenomena which suggest an alternative interpretation. (1) Neutrino oscillation in vacuum: here, as a neutrino beam travels, the mixing parameters evolve along and are not static. (2) Neutrino oscillation in matter (see, e.g., [13]): when neutrinos propagate in a medium, an induced mass is obtained which changes the mixing pattern. (3) The renormalization group equations (RGE) for quarks (see, e.g., [48]) and for neutrinos (see, e.g., [9, 10]): a change in energy scales entails a new set of parameters and are governed by the RGE. For cases (2) and (3), one could say that the physical “vacuum” itself is evolving. In all of these examples, conceptually, it is more natural to regard the mass matrix parameters as changeable physical variables. And, when one considers g-permutation, these variables should also transform under the symmetry operations. Once we do that, it becomes clear that they have natural assignments as tensors under , the permutation group of three objects. With this interpretation, one can show that the g-permutation symmetry, now operating on both the fundamental fermions and the mass matrix parameters, is restored. In this connection, it should be noted that, in SM, the mass parameters are, apart from a common Higgs VEV, identified with the “coupling constants” of the Higgs to the fermions. The permutation operation, , is not unlike the charge conjugation transformation, . Thus, it is reasonable to include masses in a permutation operation.

In the literature, there are numerous relations amongst the mass matrix parameters associated with neutrino oscillations and RGE of quarks and neutrinos (see, e.g., [8, 10, 11], and the references therein). These are obtained by direct and explicit calculations. When written in appropriate variables, hints of a permutation symmetry seem ubiquitous. In this paper, we present a general analysis of these equations. It is found that the SM has a g-permutation symmetry group (or ), where the factors denote permutations in sectors of the - and -type quarks, the charged leptons and the neutrinos, respectively. Also, the relations mentioned above are all covariant tensor equations under , just like the tensor equations in theories with rotational symmetry. It should be emphasized that, to establish a symmetry for a given Lagrangian, it is necessary to assign appropriate transformation properties to the variables contain therein. The symmetry would be broken if one assigns the mass matrix variables as singlets under its operation.

Our considerations are similar to those of another example of symmetry restoration in a familiar setting. Consider the case of an atom in an external -field. The interaction term is proportional to . If we treat as a fixed external field, then this term breaks the rotational symmetry. On the other hand, we can include as a dynamical variable in the atomic system, transforming as a vector, then rotational symmetry is restored. The transformation of the mass matrix parameters under g-permutation is analogous to the rotation of the -field.

We add that the Particle Data Group (PDG) parametrization [12] is ill-equipped to exploit the g-permutation symmetry. Besides being rephasing dependent, the PDG variables ’s, despite their appearances, have very complicated behaviour under g-permutation, making it difficult to uncover possible symmetries in an equation.

2. Tensor Analysis of

We turn now to an analysis of the representation of the g-permutation group, which is based on . The elements of operate on three objects, say , . For our purposes, it suffices to concentrate on the exchange operators:

To borrow the terminology of , we will call a P-vector or . The three-dimensional representation of , however, is reducible (). Nevertheless, it is convenient to use the reducible 3 and develop a tensor analysis for , similar to that for . This is useful because, as it turns out, the physical variables behave like P-tensors under permutations, and relations between them are covariant P-tensor equations.

To begin, we note that, different from the linear algebra of , simple functions of behave like under permutations and are also P-vectors, e.g.,

Next, out of two P-vectors, and , we can construct rank-two P-tensors such as or , where is some regular function. The simplest of these tensors are or . Thus, the product can be decomposed into three P-vectors: (1) diagonal: (no sum), (2) symmetrical: , and (3) antisymmetrical: . Their transformation properties may be further elucidated by the use of invariant tensors in . In addition to the familiar tensors and , in there is a third, which is defined as

This may be dubbed as the “symmetrical Levi-Civita symbol.” Using these, we have the following:

is a pseudo-P-vector since under the exchange operator,

Thus, the rank-two P-tensor is decomposed into three 3’s under , two of them are P-vectors, while the third is a pseudo-P-vector.

Other useful constructions are

In addition, for odd or even functions of , e.g.,

In summary, the tensor analysis of has a lot in common with that of , though with two important differences: (1) the existence of the symmetric Levi-Civita symbol ; (2) the linear tensor algebra is generalized to include functions of tensors for . Once these two differences are properly managed, the implementation of the symmetry amounts to demanding that all relations are covariant tensor equations, just like the familiar equations which are covariant under rotation.

3. The Broken g-Permutation Symmetry and Its Restoration

We will now turn to the g-permutation symmetry in the SM. To accommodate neutrino oscillations which are central to the consideration in this paper, the SM will be augmented by the inclusion of Dirac neutrino mass term. This minimal extension of the SM brings the leptonic sector on a par with the quark sector and will facilitate the ensuing discussions. The interesting possibility of neutrinos being Majorana particles will not be dealt with here but could hopefully be the topic of a future investigation.

In order not to clutter our notations, we will first concentrate our discussion to the leptonic sector of the SM. The parallel case of the quark sector will be brought in when appropriate. Also, to study the effect of g-permutation, one need only to focus on the part of the SM Lagrangian which contains the fermion-Higgs interaction, after it has acquired its VEV. The result, after diagonalization of the mass matrix, can be represented by the following terms in the Lagrangian (see, e.g., Ref. [13]), schematically,

Here, to highlight the part of the lepton-Higgs which is relevant for our discussion, we omit the gauge coupling constants and proper Dirac matrices in . Also, , refers to , and are their masses, refers to the -boson, denotes the Higgs field and is its VEV, and is an element of the PMNS matrix.

We may now study the action of g-permutation on . If the permutation only acts on the fermions (with , ), then clearly is not invariant and the g-permutation symmetry is broken. However, we may include as dynamical variables which also transform under the action of and . The structure of suggests that they transform like P-tensor. So now we have

With these assignments and referring to the tensor analysis in Section 2, it is evident that is invariant:

The symmetry group here is . Exactly the same argument can be given for the quark sector, with the replacement of by and by . We conclude that the SM has a g-permutation symmetry group, given by that operate not only on the fundamental fermions but also on the masses and mixing parameters, which transform like P-vectors, as indicated by the indices they carry. A more concrete interpretation of Equation (12) is to regard as an effective Lagrangian. It is used as a starting point for calculations in flavor physics. The results thus obtained are expressed in terms of the physical parameters contained in . Equation (12) then implies that these results must exhibit the symmetry. Some examples are cited in Section 5.

The existence of the symmetry group can also be established from another approach. The diagonalization of the Yukawa coupling , and the absorption of into the wave functions yield the Lagrangian in the mass eigenstate basis. This procedure also constrains additional transformations on , so that the global symmetry of the gauge interaction Lagrangian is broken down to , as stated in the literature. However, the solution to the diagonalization of a matrix has a six -fold symmetry, where is a permutation matrix, e.g.,

The replacement of by corresponds to an operation of , which survives the diagonalization process, and is a symmetry of the Lagrangian. Thus, the SM (with Dirac neutrinos) is found to have the global symmetry group . The action of is given by Equation (11).

We now pause to consider the effect of rephasing invariance, which was glossed over earlier. With rephasing, the transformation of can acquire a phase:

This means that only rephasing invariant combinations of a set of ’s can have definite transformation laws under exchange. Two well-known combinations are and the Jarlskog invariant [14], defined by

Thus, for physical variables, the transformation laws under exchange are (for the lepton sector)

Note that, in the terminology of Section 2, is a pseudo-P-scalar. Also, for the quark sector, the corresponding invariant, , is also a pseudo-P-scalar:

While the transformation of is not surprising, under any exchange is a remarkable property.

Another interesting aspect of rephasing invariance is that one can take out an overall phase from and demand, without loss of generality, that , while restricting further rephasing by , where is a diagonal phase matrix [15]. Under this condition, there are rephasing invariants: where , . This yields an alternative definition for :

Since changes sign under both and the exchange of rows or columns, to keep under the exchange operation, we have now

Note that for , the invariants and are unaffected. The variables [15], which was defined in terms of , now have the transformation laws: where is a permutation of . This implies, in particular, that and . With , we have , consistent with .

In summary, the SM has the symmetry group when the physical mass matrix parameters behave as tensors. This set includes the fermion masses, the mixing matrices and , and two signs for the Jarlskog invariants, , in the quark and lepton sectors, respectively. The transformation laws are given in Equations (11), (18), and (22).

4. Composite Tensors

To apply the g-permutation symmetry to physical processes, it turns out that, besides the basic tensors, certain combinations make frequent appearances. We now present a brief discussion of their properties. (a)For the masses (and similarly for ), we have a scalar, , and an antisymmetric tensor , which becomes a pseudo-P-vector: This combination will appear repeatedly in applications(b)Out of two ’s, we have (i), or , which transforms as a 3 in and a in (ii). Here, is an element of the cofactor matrix of , as defined before [15]. Sums of its rows and columns are given by . It transforms as the product of pseudo-P-vectors , or in the quark sector. For specific forms of the matrix, with (a) and (b) (maximal mixing, , for all and ), we have (a) and (b) . These properties will be useful later(iii). This combination was also used before [8, 10, 11]. It played an essential role in many of the formulas in neutrino oscillation and in RGE. The transformation properties of are exactly like . What sets them apart is its structure for specific forms of the matrix. Of particular interests are: (i) if , then , , , and (ii) if , then except possibly for , all other . (iii) If , for maximal mixing, then . If , then . To prove (i), note that implies . One can then use the alternative definition to deduce . As for (ii), if , then , , . Using (i), (ii) follows(iv), or . This is yet another composite which transforms like . It is, however, not independent because of the relation: Nevertheless, it is sometimes used for simplicity(c)We can also construct Under or , , so that is a pseudo-P-scalar. So far, no practical use has been found for , nor for other higher rank tensors out of the basic ones

5. Applications

We may now turn to detailed analyses of neutrino oscillations and RGE, in which one can arrange to vary certain parameters to induce changes to all the parameters as a set. The resulting equations will now be written in the tensor notation. This new look offers fresh insights into their structure, making them more understandable. In the following, we will study these issues case by case.

5.1. Neutrino Oscillation in Vacuum

When a neutrino beam travels down a path, the neutrino mass eigenstates pick up a phase, , , which then causes change of the mixing matrix. This effect depends only on the phase difference, . In the tensor terminology, neutrino oscillation is driven by the pseudo-P-vector

The probability is well known, and, in a notation that is adoptable for our use, given by Equations (58) and (59) of Ref. [11],

To transcribe these equations, we start with , . In tensor notation it reads

Thus, first of all, is a P-scalar under , which is reasonable. This is achieved by combining with and with (also ). Note also that if , and is the unique matrix (not or ) which also vanishes if . The formula for shows that it consists of a symmetric part, , and an antisymmetric part, . The antisymmetric part is CP and T violating. With being a pseudo-P-scalar, we can apply repeatedly and obtain which is a well-known result. It should also be noted that, in the quark sector, the CP-measure, , is a P-scalar under , again a reasonable requirement for general CP violations.

Finally, the probability can be obtained by unitarity, , with use of the relation in Equation (25).

5.2. Neutrino Oscillation in Matter

When neutrinos propagate in a medium rich in electrons, the effective Hamiltonian acquires an induced mass . We may regard this as the first component of a P-vector, , which also covers the possibility of “gedanken media” that are rich in and/or in . The addition of generates changes in the physical variables. These were expressed [11] as differential equations given by, with and ,

In tensor notation, these equations read

Here, , . For normal medium, we will take . In this case, Equation (35) does not cover , which can be obtained by

We can now discuss the salient features of these equations. To begin with, it is clear that they are covariant tensor (including P-parity) equations under . It is noteworthy that these equations utilize the tensors , , and (but not or ), all of which have similar transformation properties. It turns out that there are consistency conditions which dictate where they belong. For Equation (34), in the special case , it is known that , thus ruling out the use of , since for . For Equation (35), we note that since , it is necessary that at the boundary or . From the properties listed in Section 2, we find that if or , for , . These conditions are exactly met owing to the factor , so that from Equation (35), if or . Finally, for Equation (36), there are also two consistency checks. First, is known to have a maximum at , with . Also, and belong to two separate regimes reachable by discrete transformations, but not by infinitesimal increments. It follows that we must demand that for or . This also means that if any or , since these last conditions imply . To satisfy the requirement at , is a possible (with wrong parity?) candidate in Equation (36). But the second condition, that if any or , cannot be fulfilled by any tensor. Equation (36) solves this problem (and the P-parity problem) by using so that , and if . It is remarkable how the symmetry argument and the direct calculations reinforce each other in confirming these equations.

5.3. RGE for Quarks and Neutrinos

In this section, we will deal exclusively with the RGE for quarks. The RGE for Dirac neutrinos are almost identical (see Equations (26) and (32) in Ref. [10]) but are simpler since terms proportional to neutrino masses can be dropped. It is thus sufficient to consider quarks only.

One loop RGE for quark mass matrices has been studied for a long time. When written in the matrix form, they are given by [46]

Here, (), () is the Yukawa coupling matrix for the -type (-type) quarks; , , is the energy scale, and is the boson mass. The model dependence of the RGE is contained in the constants ().

Although the RGE for the mass matrices are simple, they are not directly useful since the matrices contain a large number of unphysical degrees of freedom. One needs to extract the RGE for the physical parameters. This was carried out, but usually in variables which mask the underlying symmetry. The easiest for our adaptation are the equations obtained in Ref. [7, 8]. These equations describe the variations of the mass ratios, the mixing parameters, and .

We now write down the tensor form of these equations and then justify them by comparing with the established ones which were obtained by direct and explicit calculations. In the following, as before, the indices and refer to and , respectively. We define the mass ratios,

Also, the mass differences,

Finally, the combinations,

Note that they transform as tensors according to the indices they carry, including pseudo-P-tensors which are identified with a “” symbol.

With these, we can write down the following RGE in tensor form

These equations are just Equations (3.17) and (3.18) in Ref. [7] and Equations (28) and (29) in Ref. [8], although the indices and were not distinguished nor were the tensors clearly identified. Also, , , since masses are used directly here.

The first thing that catches the eye in these equations is that they are manifestly covariant tensor equations under . Let us now concentrate on the -dependent part of them. The resemblance to Equations (34), (35), and (36) is striking, although there are also differences. For Equations (43), (44), (45), and (46), there are two “source” terms, and , which generate the changes. Their effects on and are combined in , and thus in and . Also, the simple pole terms in Equations (35) and (36) are replaced by and , reflecting the nature of the new situation, while keeping the singular behaviour if . In addition, for neutrino oscillations, while and for RGE. This results in replacing (in Equation (35)) by (in Equation (45)), while keeping intact so that if or . As for , P-parity calls for switching to , and all consistency requirements are met. Now a comment on terms that depend on or in Equations (38) and (39). These terms do not contribute to changes in mixing, since the diagonalization of is the same as that of a polynomial in . This is also why only mass differences, and , appear in these equations. A common mass in or , according to Equations (38) and (39), can always be absorbed in and , respectively.

Just as for neutrino oscillations, it is impressive to see how the results of direct calculations fit into the framework of permutation symmetry. Conversely, except for some overall constants, and barring the use of higher-rank tensors (e.g., ), one could almost write down these equations without any detailed computations.

Another consequence of permutation symmetry is that tensors are the entities being measured, e.g., neutrino oscillations determine the tensors . They, in turn, are simple functions of . It is therefore useful to analyze data directly in terms of , thereby avoiding the possible loss of information in translation. Some of the issues were also discussed elsewhere [11].

6. Conclusion

The SM is notorious for having a multitude of parameters. They originate from the breaking of the g-permutation symmetry by the Higgs interaction. In this paper, we suggest that, instead of regarding them as fixed numbers, these parameters can be included as physical variables which also transform under the actions of the g-permutation operation. By assigning them as appropriate tensors, the symmetry is shown to be restored. Indeed, using this procedure, the SM (with inclusion of Dirac neutrino mass terms) is found to have the discrete symmetry, .

We apply the symmetry to physical processes, including neutrino oscillations and RGE, for which there are established relations between the parameters due to a change in certain variables. These relations are the results of direct calculations. When we rewrite them in terms of tensors, it is revealed that they are indeed covariant tensor equations under . The tensor notation helps to make them very compact and simple in form. In addition, one gains insights that could otherwise be obscured by a different notation. It is hoped that there will be further developments and applications of the symmetry principle in other areas of flavor physics.

Data Availability

No data were used to support dis study.

Conflicts of Interest

The authors declare that they have no conflicts of interest.

Acknowledgments

SHC is supported by the Ministry of Science and Technology of Taiwan, Grant No.: MOST 107-2119-M-182-002.

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Copyright © 2020 T. K. Kuo and S. H. Chiu. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. The publication of this article was funded by SCOAP3.


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