Cabibbo–Kobayashi–Maskawa matrix

In the Standard Model of particle physics, the Cabibbo–Kobayashi–Maskawa matrix (CKM matrix, quark mixing matrix, sometimes also called KM matrix) is a unitary matrix which contains information on the strength of flavour-changing weak decays. Technically, it specifies the mismatch of quantum states of quarks when they propagate freely and when they take part in the weak interactions. It is important in the understanding of CP violation. A precise mathematical definition of this matrix is given in the article on the formulation of the standard model. This matrix was introduced for three generations of quarks by Makoto Kobayashi and Toshihide Maskawa, adding one generation to the matrix previously introduced by Nicola Cabibbo. This matrix is also an extension of the GIM mechanism, which only includes two of the three current families of quarks.

The matrix

A pictorial representation of the six quarks' decay modes, with mass increasing from left to right.

In 1963, Nicola Cabibbo introduced the Cabibbo angle (θ_c) to preserve the universality of the weak interaction,, with crucial reliance on prior work by Gell-Mann and Lévy.

In light of current knowledge (quarks were not yet theorized), the Cabibbo angle is related to the relative probability that down and strange quarks decay into up quarks (|Vud|2 and |Vus|2 respectively). In particle physics parlance, the object that couples to the up quark via charged-current weak interaction is a superposition of down-type quarks, here denoted by d′. Mathematically this is:

$|d^{\prime }\rangle =V_{ud}|d\rangle +V_{us}|s\rangle ,$

or using the Cabbibo angle:

$|d^{\prime }\rangle =\cos \theta _{\mathrm {c} }|d\rangle +\sin \theta _{\mathrm {c} }|s\rangle .$

Using the currently accepted values for |V_ud| and |V_us| (see below), the Cabbibo angle can be calculated using

$\tan \theta _{\mathrm {c} }={\frac {|V_{us}|}{|V_{ud}|}}={\frac {0.2257}{0.97419}}\rightarrow \theta _{\mathrm {c} }=~13.04^{\circ }.$

If this were a valid treatment, the probabilities |V_ud|² and |V_us|² should add up to 1, but instead add up to 0.99999, indicative of the missing top quark (the missing term is |V_ut|² = 0.00001). However, determining |V_ud|² and |V_us|² with a high-enough precision to predict the existence of the t quark was not possible at the time.

When the charm quark was discovered in 1974, it was noticed that the down and strange quark could decay into either the up or charm quark, leading to two sets of equations:

The Cabibbo angle represents the rotation of the mass eigenstate vector space formed by the mass eigenstates $\scriptstyle {|d\rangle ,\ |s\rangle }$ into the weak eigenstate vector space formed by the weak eigenstates $\scriptstyle {|d^{\prime }\rangle ,\ |s^{\prime }\rangle }$. θ_C = 13.04°.

$|d^{\prime }\rangle =V_{ud}|d\rangle +V_{us}|s\rangle ;$

$|s^{\prime }\rangle =V_{cd}|d\rangle +V_{cs}|s\rangle ,$

or using the Cabibbo angle:

$|d^{\prime }\rangle =\cos {\theta _{\mathrm {c} }}|d\rangle +\sin {\theta _{\mathrm {c} }}|s\rangle ;$

$|s^{\prime }\rangle =-\sin {\theta _{\mathrm {c} }}|d\rangle +\cos {\theta _{\mathrm {c} }}|s\rangle .$

This can also be written in matrix notation as:

${\begin{bmatrix}\left|d^{\prime }\right\rangle \\\left|s^{\prime }\right\rangle \end{bmatrix}}={\begin{bmatrix}V_{ud}&V_{us}\\V_{cd}&V_{cs}\\\end{bmatrix}}{\begin{bmatrix}\left|d\right\rangle \\\left|s\right\rangle \end{bmatrix}},$

or using the Cabibbo angle

${\begin{bmatrix}\left|d^{\prime }\right\rangle \\\left|s^{\prime }\right\rangle \end{bmatrix}}={\begin{bmatrix}\cos {\theta _{\mathrm {c} }}&\sin {\theta _{\mathrm {c} }}\\-\sin {\theta _{\mathrm {c} }}&\cos {\theta _{\mathrm {c} }}\\\end{bmatrix}}{\begin{bmatrix}\left|d\right\rangle \\\left|s\right\rangle \end{bmatrix}},$

where the various |V_ij|² represent the probability that the quark of i flavor decays into a quark of j flavor. This 2 × 2 rotation matrix is called the Cabibbo matrix. Observing that CP-violation could not be explained in a four-quark model, Kobayashi and Maskawa generalized the Cabbibo matrix into the Cabibbo–Kobayashi–Maskawa matrix (or CKM matrix) to keep track of the weak decays of three generations of quarks:

${\begin{bmatrix}\left|d^{\prime }\right\rangle \\\left|s^{\prime }\right\rangle \\\left|b^{\prime }\right\rangle \end{bmatrix}}={\begin{bmatrix}V_{ud}&V_{us}&V_{ub}\\V_{cd}&V_{cs}&V_{cb}\\V_{td}&V_{ts}&V_{tb}\end{bmatrix}}{\begin{bmatrix}\left|d\right\rangle \\\left|s\right\rangle \\\left|b\right\rangle \end{bmatrix}}.$

On the left is the weak interaction doublet partners of up-type quarks, and on the right is the CKM matrix along with a vector of mass eigenstates of down-type quarks. The CKM matrix describes the probability of a transition from one quark i to another quark j. These transitions are proportional to |V_ij|².

Currently, the best determination of the magnitudes of the CKM matrix elements is:

${\begin{bmatrix}|V_{ud}|&|V_{us}|&|V_{ub}|\\|V_{cd}|&|V_{cs}|&|V_{cb}|\\|V_{td}|&|V_{ts}|&|V_{tb}|\end{bmatrix}}={\begin{bmatrix}0.97428\pm 0.00015&0.2253\pm 0.0007&0.00347_{-0.00012}^{+0.00016}\\0.2252\pm 0.0007&0.97345_{-0.00016}^{+0.00015}&0.0410_{-0.0007}^{+0.0011}\\0.00862_{-0.00020}^{+0.00026}&0.0403_{-0.0007}^{+0.0011}&0.999152_{-0.000045}^{+0.000030}\end{bmatrix}}.$

Note that the choice of usage of down-type quarks in the definition is purely arbitrary and does not represent some sort of deep physical asymmetry between up-type and down-type quarks. We could just as easily define the matrix the other way around, describing weak interaction partners of mass eigenstates of down-type quarks, u′, c′ and t′, in terms of u, c, and t. Since the CKM matrix is unitary (and therefore its inverse is the same as its conjugate transpose), we would obtain essentially the same matrix.

Counting

To proceed further, it is necessary to count the number of parameters in this matrix, V which appear in experiments, and therefore are physically important. If there are N generations of quarks (2N flavours) then

• An N × N unitary matrix (that is, a matrix V such that VV^† = I, where V^† is the conjugate transpose of V and I is the identity matrix) requires N² real parameters to be specified.
• 2N − 1 of these parameters are not physically significant, because one phase can be absorbed into each quark field (both of the mass eigenstates, and of the weak eigenstates), but an overall common phase is unobservable. Hence, the total number of free variables independent of the choice of the phases of basis vectors is N² − (2N − 1) = (N − 1)².
  • Of these, N(N − 1)/2 are rotation angles called quark mixing angles.
  • The remaining (N − 1)(N − 2)/2 are complex phases, which cause CP violation.

For the case N = 2, there is only one parameter which is a mixing angle between two generations of quarks. Historically, this was the first version of CKM matrix when only two generations were known. It is called the Cabibbo angle after its inventor Nicola Cabibbo.

For the Standard Model case (N = 3), there are three mixing angles and one CP-violating complex phase.

Observations and predictions

Cabibbo's idea originated from a need to explain two observed phenomena:

1. the transitions u ↔ d, e ↔ ν_e, and μ ↔ ν_μ had similar amplitudes.
2. the transitions with change in strangeness ΔS = 1 had amplitudes equal to 1/4 of those with ΔS = 0.

Cabibbo's solution consisted of postulating weak universality to resolve the first issue, along with a mixing angle θ_c, now called the Cabibbo angle, between the d and s quarks to resolve the second.

For two generations of quarks, there are no CP violating phases, as shown by the counting of the previous section. Since CP violations were seen in neutral kaon decays already in 1964, the emergence of the Standard Model soon after was a clear signal of the existence of a third generation of quarks, as pointed out in 1973 by Kobayashi and Maskawa. The discovery of the bottom quark at Fermilab (by Leon Lederman's group) in 1976 therefore immediately started off the search for the missing third-generation quark, the top quark.

Weak universality

The constraints of unitarity of the CKM-matrix on the diagonal terms can be written as

$\sum _{k}|V_{ik}|^{2}=1$

for all generations i. This implies that the sum of all couplings of any of the up-type quarks to all the down-type quarks is the same for all generations. This relation is called weak universality after Nicola Cabibbo, who first pointed it out in 1967. Theoretically it is a consequence of the fact that all SU(2) doublets couple with the same strength to the vector bosons of weak interactions. It has been subjected to continuing experimental tests.

The unitarity triangles

The remaining constraints of unitarity of the CKM-matrix can be written in the form

$\sum _{k}V_{ik}V_{jk}^{*}=0.$

For any fixed and different i and j, this is a constraint on three complex numbers, one for each k, which says that these numbers form the sides of a triangle in the complex plane. There are six choices of i and j (three independent), and hence six such triangles, each of which is called an unitary triangle. Their shapes can be very different, but they all have the same area, which can be related to the CP violating phase. The area vanishes for the specific parameters in the Standard Model for which there would be no CP violation. The orientation of the triangles depend on the phases of the quark fields.

Since the three sides of the triangles are open to direct experiment, as are the three angles, a class of tests of the Standard Model is to check that the triangle closes. This is the purpose of a modern series of experiments under way at the Japanese BELLE and the Californian BaBar experiments, as well as at LHCb in CERN, Switzerland.

Parameterizations

Four independent parameters are required to fully define the CKM matrix. Many parameterizations have been proposed, and three of the most common ones are shown below.

KM parameters

The original parameterization of Kobayashi and Maskawa used three angles (θ₁, θ₂, θ₃) and a CP-violating phase (δ). Cosines and sines of the angles are denoted c_i and s_i, respectively. θ₁ is the Cabibbo angle.

${\begin{bmatrix}c_{1}&-s_{1}c_{3}&-s_{1}s_{3}\\s_{1}c_{2}&c_{1}c_{2}c_{3}-s_{2}s_{3}e^{i\delta }&c_{1}c_{2}s_{3}+s_{2}c_{3}e^{i\delta }\\s_{1}s_{2}&c_{1}s_{2}c_{3}+c_{2}s_{3}e^{i\delta }&c_{1}s_{2}s_{3}-c_{2}c_{3}e^{i\delta }\end{bmatrix}}.$

"Standard" parameters

A "standard" parameterization of the CKM matrix uses three Euler angles (θ₁₂, θ₂₃, θ₁₃) and one CP-violating phase (δ₁₃). Couplings between quark generation i and j vanish if θ_ij = 0. Cosines and sines of the angles are denoted c_ij and s_ij, respectively. θ₁₂ is the Cabibbo angle.

${\begin{bmatrix}c_{12}c_{13}&s_{12}c_{13}&s_{13}e^{-i\delta _{13}}\\-s_{12}c_{23}-c_{12}s_{23}s_{13}e^{i\delta _{13}}&c_{12}c_{23}-s_{12}s_{23}s_{13}e^{i\delta _{13}}&s_{23}c_{13}\\s_{12}s_{23}-c_{12}c_{23}s_{13}e^{i\delta _{13}}&-c_{12}s_{23}-s_{12}c_{23}s_{13}e^{i\delta _{13}}&c_{23}c_{13}\end{bmatrix}}.$

The currently best known values for the standard parameters are:

θ₁₂ = 13.04±0.05°, θ₁₃ = 0.201±0.011°, θ₂₃ = 2.38±0.06°, and δ₁₃ = 1.20±0.08.

Wolfenstein parameters

A third parameterization of the CKM matrix was introduced by Lincoln Wolfenstein with the four parameters λ, A, ρ, and η. The four Wolfenstein parameters have the property that all are of order 1 and are related to the "standard" parameterization:

λ = s₁₂

Aλ² = s₂₃

Aλ³(ρ − iη) = s₁₃e^−iδ

The Wolfenstein parameterization of the CKM matrix, to order λ³, is

${\begin{bmatrix}1-\lambda ^{2}/2&\lambda &A\lambda ^{3}(\rho -i\eta )\\-\lambda &1-\lambda ^{2}/2&A\lambda ^{2}\\A\lambda ^{3}(1-\rho -i\eta )&-A\lambda ^{2}&1\end{bmatrix}}.$

The CP violation can be determined by measuring ρ − iη.

Using the values of the previous section for the CKM matrix, the best determination of the Wolfenstein parameters is:

λ = 0.2257+0.0009
−0.0010, A = 0.814+0.021
−0.022, ρ = 0.135+0.031
−0.016, and η = 0.349+0.015
−0.017.

Nobel Prize

In 2008, Kobayashi and Maskawa shared one half of the Nobel Prize in Physics "for the discovery of the origin of the broken symmetry which predicts the existence of at least three families of quarks in nature". Some physicists were reported to harbor bitter feelings about the fact that the Nobel Prize committee failed to reward the work of Cabibbo, on which the work of the other two was based. Asked for a reaction on the prize, Cabibbo preferred to give no comment.

See also

• Formulation of the Standard Model and CP violations.
• Quantum chromodynamics, flavour and strong CP problem.
• Pontecorvo–Maki–Nakagawa–Sakata matrix, the equivalent mixing matrix for neutrinos.

Further reading

• D.J Griffiths (2008). Introduction to Elementary Particles (2nd ed.). John Wiley & Sons. ISBN 978-3-527-40601-2.
• B. Povh; et al. (1995). Particles and Nuclei: An Introduction to the Physical Concepts. Springer. ISBN 3-540-20168-8. {{cite book}}: Explicit use of et al. in: |author= (help)
• I.I. Bigi, A.I. Sanda (2000). CP violation. Cambridge University Press. ISBN 0-521-44349-0.
• Particle Data Group: the CKM matrix
• Particle Data Group: CP violation in meson decays
• The Babar experiment at SLAC and the BELLE experiment at KEK Japan