1. Introduction
1.1. Koide’s Mass Formula
Let the masses of the charged leptons , , and be denoted by , , and , respectively.
In 1982, Yoshio Koide proposed a mass formula inspired by the work of Harari, Haut, and Weyers [
1], which relates the masses of the three generations of charged leptons [
2,
3]:
This empirical formula remarkably reproduces the observed mass hierarchy of the electron, muon, and tauon with surprising precision.
1.2. Extension by Carl A. Brannen
In 2006, Carl A. Brannen proposed an extension of the Koide mass formula in his paper [
4].
We now denote the masses of , , and as , , and , respectively.
According to Brannen, the square root of each mass can be parameterized as:
Note that the inside the cosine is , not .
1.3. Generalization of the Formula
Since
we use this as a normalization factor.
Following Brannen’s approach, in which the parameters (theta angle) and are introduced to generalize the mass formula, we adopt the notation in place of throughout this work to improve readability.
In this framework, the parameter
is defined as follows:
The two forms are shown below.
Here, for charged leptons, Brannen sets:
1.4. Down-Type Quarks
We obtain the masses of the down-type quarks from the 2024 edition of the Particle Data Group (PDG) [
5]. In what follows, all experimental values are taken from that edition. Although the energy scales for
,
are given at
and for
at
, we use the following representative values.
Let
,
, and
denote the masses of the
,
, and
quarks, respectively:
From these values, we find:
Based on this observation, we hypothesize that the down-type quark mass formula takes the form:
Next, upon substituting
into the above hypothetical mass formula, we obtain:
These values are in good agreement with the experimental measurements.
Taking yields .
1.5. Proposed Mass Formula for Down-Type Quarks
We obtain the following two forms.
With this formulation, the resulting masses are:
1.6. The Cabibbo–Kobayashi–Maskawa Matrix
We now employ
and
newly introduced in this work, to explore its potential role in describing the rotational structure of the Cabibbo–Kobayashi–Maskawa (CKM) matrix [
6,
7].
2. Method
2.1. Construction of the CKM Matrix
First, we denote the mass eigenstates of the down-type quarks by and the flavor eigenstates by .
Similarly, we denote the mass eigenstates of the up-type quarks by and the flavor eigenstates by .
The relationship between flavor and mass eigenstates is given by:
These states are connected through the charged-current interaction mediated by the
-boson:
Hence, at first glance, the CKM matrix can be expressed as:
However, in vacuum, the Pontecorvo–Maki–Nakagawa–Sakata (PMNS) matrix [
8] is expected to be expressible as:
where
is the Tribimaximal mixing matrix [
9],
, and
[
10].
It is therefore predicted that, by the same reasoning and considering the direction of the
-boson interaction (see
Figure 1), the inverse CKM matrix takes the form:
where
is the 3–1 angle of the CKM matrix and
is the complex phase in that rotation.
Hence, the CKM matrix can be equivalently expressed as:
2.2. The 1–2 Rotation
We now turn to the 1–2 rotation, commonly referred to as the Cabibbo rotation and parameterized by the Cabibbo angle
[
6,
11].
The experimentally determined value is given in the PDG:
Next, we introduce a "half-Cabibbo" angle
by defining:
We note explicitly that need not equal .
Denoting the down-type and up-type 1–2 rotation angles by and , respectively.
Then the individual rotation matrices are:
Note that can in principle be either .
It follows that the combined rotation takes the form:
The magnitudes of the and entries are in good agreement with the experimental values of and in the CKM matrix.
2.3. The 2–3 Rotation
In the 2–3 rotation, we denote the down-type quark rotation by and the up-type quark rotation by .
The individual rotation matrices are:
For the complex phases, we set:
Numerically, the matrix can be expressed approximately as:
The magnitudes of the and entries are in good agreement with the experimental values of and in the CKM matrix.
2.4. Combining the Matrices
We define the following matrices:
3. Result
The result is obtained as follows:
The absolute values of each element are:
4. Discussion
The absolute values of each element obtained in
Section 3, with the exception of the
and
entries, are close to the experimentally determined values.
The only remaining free parameters are those of the 3–1 rotation, because the up-type quark mass formula remains unspecified. Hence the parameters
and
cannot be determined in advance. To resolve these, we have performed a two-dimensional grid search over
and
, selecting the values that minimize the deviation of
and
from their experimental counterparts. The optimal parameters are found to be:
At these values the CKM matrix takes the form:
The absolute values of each element are:
These values are in excellent agreement with the PDG 2024 global-fit values, with all deviations within 0.7 standard deviations ().
Moreover, the three interior angles of the corresponding unitarity triangle are found to be:
Hence, we have
which is in excellent agreement with the experimental value
Finally, we calculate the Jarlskog invariant [
12]
which is in excellent agreement with the experimental value
All parameters are in excellent agreement with the experimental values, but and cannot be uniquely determined because a corresponding mass formula for up-type quarks remains undetermined. We anticipate that future investigations will shed light on this issue.
5. Conclusion
By postulating a mass formula for down-type quarks—which yields the values:
—and by introducing a "half-Cabibbo" angle:
we have been able to construct a matrix that closely approximates the CKM matrix except for the 3–1 rotation. However, since no analogous mass formula for up-type quarks has yet been deduced, the 3–1 rotation matrix remains undetermined, and only a rough estimate of its value could be obtained. It is anticipated that, with the successful conjecture of an up-type quark mass formula in future work, a more accurate reconstruction of the CKM matrix will become possible.
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