Introduction to Neutrino Physics
JINR
The charged lepton at production or detection determines the flavor:
\[ \nu_e,\qquad\nu_\mu,\qquad\nu_\tau. \]
These are three states distinguishable by the weak interaction.
In vacuum, three eigenstates propagate:
\[ H_0|\nu_i\rangle=E_i|\nu_i\rangle, \qquad i=1,2,3. \]
Each acquires a phase \(e^{-i(E_it-p_iL)}\). Of the three phase differences, two are independent.
The three angles describe the relative orientation of the bases; the complex phase appears in the interference of the three mass waves.
\[ U=\begin{pmatrix} U_{e1}&U_{e2}&U_{e3}\\ U_{\mu1}&U_{\mu2}&U_{\mu3}\\ U_{\tau1}&U_{\tau2}&U_{\tau3} \end{pmatrix}, \qquad \boxed{|\nu_\alpha\rangle =\sum_{i=1}^{3}U_{\alpha i}^*|\nu_i\rangle}. \]
Unitarity means
\[ \boxed{UU^\dagger=U^\dagger U= \begin{pmatrix} 1&0&0\\ 0&1&0\\ 0&0&1 \end{pmatrix}}. \]
Rows:
\[ \sum_i|U_{\alpha i}|^2=1, \qquad \sum_iU_{\alpha i}U_{\beta i}^*=0 \quad(\alpha\ne\beta). \]
Columns:
\[ \sum_\alpha|U_{\alpha i}|^2=1, \qquad \sum_\alpha U_{\alpha i}^*U_{\alpha j}=0 \quad(i\ne j). \]
The normalizations give three ones on the diagonal. The six off-diagonal zeros are pairwise conjugate: these are three complex, that is, six real conditions. In total, \(U^\dagger U=I\) amounts to \(3+6=9\) real conditions; for a square matrix, \(UU^\dagger=I\) follows from this and adds no new conditions.
A good agreement of the fit with a unitary matrix tests the model as a whole. Testing unitarity itself requires an analysis in which its constraints are not imposed in advance.
Let \(c_{ij}=\cos\theta_{ij}\), \(s_{ij}=\sin\theta_{ij}\), and \(\delta\equiv\delta_{\rm CP}\). The standard convention has the form
\[ \boxed{U=R_{23}U_{13}(\delta_{\rm CP})R_{12}}, \]
\[ \begin{aligned} R_{23}&=\begin{pmatrix}1&0&0\\0&c_{23}&s_{23}\\0&-s_{23}&c_{23}\end{pmatrix}, &U_{13}&=\begin{pmatrix}c_{13}&0&s_{13}e^{-i\delta}\\0&1&0\\-s_{13}e^{i\delta}&0&c_{13}\end{pmatrix}, &R_{12}&=\begin{pmatrix}c_{12}&s_{12}&0\\-s_{12}&c_{12}&0\\0&0&1\end{pmatrix}. \end{aligned} \]
From right to left: \(R_{12}\) rotates in the \(12\) plane, \(U_{13}\) acts in the \(13\) plane and carries the phase, \(R_{23}\) rotates in the \(23\) plane. Each factor is unitary.
Multiplying the three factors, we obtain
\[ \boxed{ U=\begin{pmatrix} c_{12}c_{13}&s_{12}c_{13}&s_{13}e^{-i\delta}\\ -s_{12}c_{23}-c_{12}s_{23}s_{13}e^{i\delta} &c_{12}c_{23}-s_{12}s_{23}s_{13}e^{i\delta} &s_{23}c_{13}\\ s_{12}s_{23}-c_{12}c_{23}s_{13}e^{i\delta} &-c_{12}s_{23}-s_{12}c_{23}s_{13}e^{i\delta} &c_{23}c_{13} \end{pmatrix}}. \]
The first row and the third column can be read off immediately:
\[ \frac{|U_{e2}|}{|U_{e1}|}=\tan\theta_{12},\qquad |U_{e3}|^2=\sin^2\theta_{13},\qquad \frac{|U_{\mu3}|}{|U_{\tau3}|}=\tan\theta_{23}. \]
The multiplication and additional checks are in the exercises for the lecture.
The example is computed from the NuFIT 6.1 best-fit point (NO, IC24 + SK-atm); the fractions of each column sum to one up to rounding.
A unitary matrix \(U\) of size \(3\times3\) contains three angles and six phases.
\[ \begin{aligned} \mathcal L_{\rm CC} &=-\frac{g}{\sqrt2}\,W^-_\mu \sum_{\alpha,i}\bar\ell_{\alpha L}\gamma^\mu U_{\alpha i}\nu_{iL} +\mathrm{h.c.},\\ \mathcal L_{\rm mass} &=-\sum_\alpha m_\alpha\bar\ell_\alpha\ell_\alpha -\sum_i m_i\bar\nu_i\nu_i. \end{aligned} \]
\[ \ell_\alpha\mapsto e^{i\phi_\alpha}\ell_\alpha, \qquad \nu_i\mapsto e^{i\psi_i}\nu_i. \]
\[ \boxed{U_{\alpha i}'= e^{i(\phi_\alpha-\psi_i)}U_{\alpha i}}. \]
\[ \begin{gathered} \phi_\alpha\mapsto\phi_\alpha+\chi,\quad \psi_i\mapsto\psi_i+\chi:\\ (\phi_\alpha+\chi)-(\psi_i+\chi)=\phi_\alpha-\psi_i. \end{gathered} \]
\[ \phi_e-\psi_3,\ \ \phi_\mu-\psi_3,\ \ \phi_\tau-\psi_3,\ \ \psi_1-\psi_3,\ \ \psi_2-\psi_3. \]
The masses \(m_i\) are chosen real and positive. \(\widetilde U\) denotes the full mixing matrix.
\[ \mathcal L_{\rm mass}^{(M)} =-\frac12\sum_i m_i\,\overline{\nu_{iL}^{\,c}}\nu_{iL} +\mathrm{h.c.} \]
\[ \overline{\nu_{iL}^{\,c}}\nu_{iL} \mapsto e^{2i\psi_i}\overline{\nu_{iL}^{\,c}}\nu_{iL}. \]
For fixed \(m_i\), only \(\psi_i=0,\pi\) are allowed.
\[ \widetilde U'=D_\ell\widetilde U,\qquad D_\ell=\operatorname{diag}(e^{i\phi_e},e^{i\phi_\mu},e^{i\phi_\tau}). \]
\[ \widetilde U_{\alpha i}'=e^{i\phi_\alpha}\widetilde U_{\alpha i} \qquad\text{for all }i. \]
A single \(\phi_\alpha\) multiplies the entire row \(\alpha\) by a common factor. The relative phases of its elements are preserved.
After the phases of the charged leptons are chosen, the full matrix can be written as \(\widetilde U=U(\delta)D_M\). In \(U(\delta)\) there are three angles and one phase \(\delta_{\rm CP}\).
\[ \widetilde U_{\alpha i}=U_{\alpha i}(\delta)e^{i\eta_i}. \]
This is how multiplication from the right by
\[ D_M=\operatorname{diag}(e^{i\eta_1},e^{i\eta_2},e^{i\eta_3}). \]
acts.
\[ D_M=\operatorname{diag} \left(1,e^{i\alpha_{21}/2},e^{i\alpha_{31}/2}\right). \]
\[ \widetilde U_{\beta i}\widetilde U_{\alpha i}^{*} =U_{\beta i}U_{\alpha i}^{*}e^{i\eta_i}e^{-i\eta_i} =U_{\beta i}U_{\alpha i}^{*}. \]
\[ m_{\beta\beta}=\left|\sum_i m_i\widetilde U_{ei}^{2}\right|, \qquad \widetilde U_{ei}^{2}=U_{ei}^{2}e^{2i\eta_i}. \]

1902–1984. The relativistic Dirac equation described a fermion with spin \(1/2\) and led to the prediction of the electron’s antiparticle. In 1933, Dirac shared the Nobel Prize in Physics with Erwin Schrödinger.

1906 — disappeared in 1938. In 1937, Majorana constructed a theory of a neutral fermion that coincides with its own antiparticle. Whether this description applies to the neutrino is for experiment to say.
The source prepares the flavor \(\alpha\):
\[ |\nu_\alpha;0\rangle=\sum_iU_{\alpha i}^*|\nu_i\rangle. \]
Each mass component propagates with its own phase.
For an ultrarelativistic neutrino after a distance \(L\):
\[ |\nu_\alpha;L\rangle =\sum_iU_{\alpha i}^* \exp\!\left(-i\frac{m_i^2L}{2E}\right)|\nu_i\rangle. \]
The phase common to the three components is dropped: it does not enter the probability.
The detector projects the state onto the flavor \(\beta\). The orthogonality of the mass states leaves a single sum:
\[ \boxed{ \mathcal A_{\alpha\to\beta}(L,E) =\sum_{i=1}^{3} U_{\beta i}U_{\alpha i}^* e^{-im_i^2L/(2E)} }. \]
In each term one can see the production, propagation, and detection of a single mass component.
Denote
\[ \Delta_{ij}=\frac{\Delta m_{ij}^2L}{4E}, \qquad \Delta m_{ij}^2=m_i^2-m_j^2. \]
Of the three possible pairs \(21\), \(31\) and \(32\), two are independent:
\[ \boxed{\Delta m_{31}^2=\Delta m_{32}^2+\Delta m_{21}^2}. \]
Put
\[ a_i=U_{\beta i}U_{\alpha i}^*e^{-im_i^2L/(2E)}, \qquad \mathcal A_{\alpha\to\beta}=a_1+a_2+a_3. \]
Then the probability is a sum of three diagonal contributions and the interference of the three pairs:
\[ \boxed{ P_{\alpha\to\beta}=\left|\sum_i a_i\right|^2 =\sum_i|a_i|^2+2\sum_{i>j}\operatorname{Re}(a_i a_j^*) }. \]
For a compact notation we introduce
\[ X_{\alpha\beta}^{ij} =U_{\alpha i}^*U_{\beta i}U_{\alpha j}U_{\beta j}^*. \]
The real part of \(X^{ij}\) gives the familiar oscillation maxima. The imaginary part will be needed when comparing neutrinos and antineutrinos. The full expansion of the sum is exercise 10.3.
For \(\beta=\alpha\) all the products \(X_{\alpha\alpha}^{ij}\) are real:
\[ \boxed{ P_{\alpha\to\alpha} =1-4\sum_{i>j}|U_{\alpha i}|^2|U_{\alpha j}|^2 \sin^2\Delta_{ij} }. \]
For \(\alpha\ne\beta\):
\[ \boxed{ P_{\alpha\to\beta} =-4\sum_{i>j}\operatorname{Re}X_{\alpha\beta}^{ij} \sin^2\Delta_{ij} +2\sum_{i>j}\operatorname{Im}X_{\alpha\beta}^{ij} \sin2\Delta_{ij} }. \]
The sum of the three final probabilities for a fixed initial flavor equals one. The direct derivation and the two-flavor limit are in exercise 10.3.
For antineutrinos the mixing matrix is complex conjugated:
\[ \boxed{\bar U=U^*}. \]
Under this replacement
\[ \operatorname{Re}X^{ij}\longrightarrow\operatorname{Re}X^{ij}, \qquad \operatorname{Im}X^{ij}\longrightarrow-\operatorname{Im}X^{ij}. \]
Consequently, in the appearance channel the difference equals
\[ \boxed{ A_{\alpha\beta}^{\rm CP} =P(\nu_\alpha\to\nu_\beta) -P(\bar\nu_\alpha\to\bar\nu_\beta) =4\sum_{i>j}\operatorname{Im}X_{\alpha\beta}^{ij} \sin2\Delta_{ij} }. \]
For the survival channel in vacuum \(A_{\alpha\alpha}^{\rm CP}=0\).
Open the applet separately (in Russian) · the same program in Python.
The point shows \((P_{\alpha\to e},P_{\alpha\to\mu},P_{\alpha\to\tau})\). The path \(x=L/L_{\rm osc}^{21}\) is extended to three solar periods. The NO and IO buttons set the angles and phase of the best-fit point of the corresponding ordering: NuFIT 6.1, IC24 + SK-atm.
In vacuum one compares transitions at the same \(L\) and \(E\):
\[ \nu_\alpha\to\nu_\beta, \qquad \bar\nu_\alpha\to\bar\nu_\beta. \]
For two flavors the mixing matrix can be made real.
The three-flavor matrix admits a physical complex phase, which can give a nonzero probability difference.
In long-baseline accelerator experiments, Earth’s matter also affects this comparison.
In 1985 Jarlskog proposed, for quarks, a quantity that does not change under redefinition of the field phases:
\[ \boxed{ J_{\rm CP} =\operatorname{Im} \left(U_{e2}^*U_{\mu2}U_{e1}U_{\mu1}^*\right) }. \]
In the standard parametrization
\[ \boxed{ J_{\rm CP} =c_{12}s_{12}c_{23}s_{23}c_{13}^2s_{13}\sin\delta_{\rm CP} }. \]
\(J_{\rm CP}\ne0\) only if all three angles differ from \(0\) and \(90^\circ\), and \(\sin\delta_{\rm CP}\ne0\).
Reminder
Rephasing the fields \(\ell_\alpha\to e^{i\varphi_\alpha}\ell_\alpha\), \(\nu_i\to e^{i\psi_i}\nu_i\) does not change the physics (the “Dirac particle” tab).
\[ Q_{\alpha\beta}^{ij}=U_{\alpha i}U_{\beta j}U_{\alpha j}^*U_{\beta i}^*. \]
Levi-Civita symbol
\(\varepsilon_{e\mu\tau}=\varepsilon_{123}=1\).
Swapping two indices changes the sign; if two indices coincide, \(\varepsilon=0\).
Statement. For three flavors their imaginary parts coincide up to sign:
\[ \boxed{ \operatorname{Im}Q_{\alpha\beta}^{ij} =J_{\rm CP}\sum_{\gamma,k}\varepsilon_{\alpha\beta\gamma}\,\varepsilon_{ijk} }, \qquad J_{\rm CP}=\operatorname{Im}Q_{e\mu}^{12}. \]
What is needed
Orthogonality of rows: \(\sum_iU_{\alpha i}U_{\beta i}^*=0\) for \(\alpha\ne\beta\).
\(\operatorname{Im}|z|^2=0\), \(\operatorname{Im}(w z^*)=-\operatorname{Im}(z w^*)\).
\[ z_2z_3^*=-z_2z_1^*-|z_2|^2 \;\Rightarrow\; \operatorname{Im}(z_2z_3^*)=\operatorname{Im}(z_1z_2^*). \]
\[ \boxed{ S=\frac12\left|z_1\times z_2\right| =\frac12\left|\operatorname{Im}(z_1^*z_2)\right| =\frac12|J_{\rm CP}| }. \]
Reminder
\(X_{\alpha\beta}^{ij}=U_{\alpha i}^*U_{\beta i}U_{\alpha j}U_{\beta j}^*\) enters the probability with \(\sin2\Delta_{ij}\) (slide “Squared Amplitude”).
Jarlskog, 1985
For quarks
\[ \det[H_u,H_d]\propto iJ\,D_uD_d, \]
where \(H=MM^\dagger\), and \(D_q\) is the product of the squared-mass differences. Both the phase and the nondegenerate masses are needed.
\[ J_{\rm CP}=\frac18\sin2\theta_{12}\sin2\theta_{23} \sin2\theta_{13}\cos\theta_{13}\sin\delta_{\rm CP}. \]
\[ |J_{\rm CP}|\le\frac1{6\sqrt3}\approx0.096,\qquad |U_{\alpha i}|^2=\frac13. \]
For the channel \(e\to\mu\) the imaginary parts of the three interference products are expressed through a single \(J_{\rm CP}\). We obtain
\[ \boxed{ A_{e\mu}^{\rm CP} =16J_{\rm CP} \sin\Delta_{21}\sin\Delta_{32}\sin\Delta_{31} }. \]
The derivation of the identity and an estimate of the size of the effect are homework exercise 10.4.
We use three experimental results:
We will need the normalizations of rows and columns, then orthogonality. The connection of the solar result with \(|U_{e2}|^2\) relies on the adiabatic matter effect; its physics will be derived in lecture 13.
The rows correspond to the flavors of production and detection; the columns, to the mass states. We begin with the measurable fractions \(|U_{\alpha i}|^2\).
For now we leave \(|U_{e3}|^2=0\). This reveals the framework of the problem; the reactor result will be included at the end.
For high-energy solar neutrinos \(P_{ee}\simeq1/3\). In the adiabatic approximation and for \(U_{e3}=0\):
\(P_{ee}\simeq |U_{e2}|^2\simeq\frac13.\)
Why the Sun singles out the second mass column will be explained in the lecture on the MSW effect.
Its normalization fills the remaining cell:
\( |U_{e1}|^2+|U_{e2}|^2+|U_{e3}|^2=1 \quad\Longrightarrow\quad |U_{e1}|^2=\frac23. \)
The first row is now equal to \((2/3,\,1/3,\,0)\).
The nearly maximal disappearance \(\nu_\mu\) shows that the muon flavor is distributed roughly equally with respect to the third mode:
\( 4|U_{\mu3}|^2(1-|U_{\mu3}|^2)\simeq1 \quad\Longrightarrow\quad |U_{\mu3}|^2\simeq\frac12. \)
Here we keep the leading atmospheric scale and for now set \(U_{e3}=0\).
The three fractions of a single mass state sum to one:
\( |U_{e3}|^2+|U_{\mu3}|^2+|U_{\tau3}|^2=1 \quad\Longrightarrow\quad |U_{\tau3}|^2=\frac12. \)
In this approximation \(\nu_3\) is equally coupled to \(\nu_\mu\) and \(\nu_\tau\).
From column 3 we already know \(|U_{\mu3}|=|U_{\tau3}|\). Its orthogonality to column 2 gives
\( U_{\mu2}^*U_{\mu3}+U_{\tau2}^*U_{\tau3}=0. \)
Therefore, \(|U_{\mu2}|^2=|U_{\tau2}|^2\). We normalize the second column:
\( \frac13+|U_{\mu2}|^2+|U_{\tau2}|^2=1. \)
\( |U_{\mu2}|^2=|U_{\tau2}|^2=\frac13. \)
We normalize the muon and tau rows:
\( |U_{\mu1}|^2=1-\frac13-\frac12=\frac16, \qquad |U_{\tau1}|^2=\frac16. \)
All rows and columns of the matrix of squares now sum to one.
Each cell on the right so far contains the probability \(|U_{\alpha i}|^2\). We take the square root:
\( |U_{\alpha i}|=\sqrt{|U_{\alpha i}|^2}, \qquad |U_{e1}|=\sqrt{\frac23},\quad |U_{\mu1}|=\sqrt{\frac16}. \)
The matrix of non-negative moduli is not yet \(U\): its columns are not orthogonal. The relative signs are missing.
Denote the columns by \(c_1,c_2,c_3\). For a real representative we choose as positive \(U_{e2},U_{\mu2},U_{\mu3},U_{\tau3}\). From the orthogonality of columns 2 and 3 it follows that
\( c_2\!\cdot c_3= U_{\mu2}U_{\mu3}+U_{\tau2}U_{\tau3}=0. \)
\( U_{\tau2}=-U_{\mu2}=-\sqrt{\frac13}. \)
The first column is so far shown in absolute value: we will find its signs from the next condition.
Choose \(U_{e1}>0\). Orthogonality with the third column gives \(U_{\mu1}=-U_{\tau1}\). With the second:
\( c_1\!\cdot c_2= \sqrt{\frac13} (U_{e1}+U_{\mu1}-U_{\tau1})=0. \)
\( U_{\mu1}=-\sqrt{\frac16},\qquad U_{\tau1}=+\sqrt{\frac16}. \)
We obtained \(U_0^{\mathsf T}U_0=I\): the column norms are equal to one, and the pairwise scalar products are zero.
The signs of this representative depend on the choice of the state phases. For \(U_{e3}=0\) the phase \(\delta_{\rm CP}\) is not observed in oscillations.
A measurement at the near and far detectors gives \(|U_{e3}|^2=\sin^2\theta_{13}\simeq0.0225\). The matrix on the right is an example \(|U|^2\), calculated from the best-fit point of NuFIT 6.1.
Appearance channels and antiparticles provide information about \(\delta_{\rm CP}\). The squared moduli alone do not determine all the complex phases \(U\).
The numbers on the right are calculated in the unitary model. For an independent test of unitarity, this condition is lifted in the data analysis.
| \(\nu_1\) | \(\nu_2\) | \(\nu_3\) | |
|---|---|---|---|
| \(e\) | \(\tfrac23\)\(\sqrt{\tfrac23}\)\(\pm\sqrt{\tfrac23}\)\(+\sqrt{\tfrac23}\)\(0.676\) | \(\tfrac13\)\(\sqrt{\tfrac13}\)\(+\sqrt{\tfrac13}\)\(+\sqrt{\tfrac13}\)\(0.302\) | \(0\)\(0\)\(0\)\(0\)\(0.022\) |
| \(\mu\) | \(\tfrac16\)\(\sqrt{\tfrac16}\)\(\pm\sqrt{\tfrac16}\)\(-\sqrt{\tfrac16}\)\(0.112\) | \(\tfrac13\)\(\sqrt{\tfrac13}\)\(+\sqrt{\tfrac13}\)\(+\sqrt{\tfrac13}\)\(0.428\) | \(\tfrac12\)\(\sqrt{\tfrac12}\)\(+\sqrt{\tfrac12}\)\(+\sqrt{\tfrac12}\)\(0.459\) |
| \(\tau\) | \(\tfrac16\)\(\sqrt{\tfrac16}\)\(\pm\sqrt{\tfrac16}\)\(+\sqrt{\tfrac16}\)\(0.212\) | \(\tfrac13\)\(\sqrt{\tfrac13}\)\(-\sqrt{\tfrac13}\)\(-\sqrt{\tfrac13}\)\(0.270\) | \(\tfrac12\)\(\sqrt{\tfrac12}\)\(+\sqrt{\tfrac12}\)\(+\sqrt{\tfrac12}\)\(0.518\) |
Open the applet separately (in Russian).
At zeroth order we obtain the matrix of squared moduli
\[ \boxed{ |U_0|^2= \begin{pmatrix} 2/3&1/3&0\\ 1/6&1/3&1/2\\ 1/6&1/3&1/2 \end{pmatrix}}. \]
The combined analysis of different sources reconstructed the whole matrix, but its unitarity was an initial condition of the reconstruction. For an independent test, one allows deviations from unitarity and cross-checks different channels.
Normal mass ordering, atmospheric data IC24 and Super-Kamiokande. Best-fit values and \(3\sigma\) intervals:
| Parameter | Best-fit value | \(3\sigma\) interval |
|---|---|---|
| \(\sin^2\theta_{12}\) | \(0.3088\) | \(0.2893\)–\(0.3295\) |
| \(\sin^2\theta_{13}\) | \(0.02248\) | \(0.02064\)–\(0.02418\) |
| \(\sin^2\theta_{23}\) | \(0.470\) | \(0.435\)–\(0.584\) |
| Parameter | Best-fit value | \(3\sigma\) interval |
|---|---|---|
| \(\Delta m_{21}^2\) | \(7.537\cdot10^{-5}\ \mathrm{eV}^2\) | \((7.236\text{–}7.823)\cdot10^{-5}\ \mathrm{eV}^2\) |
| \(\Delta m_{31}^2\) (NO) | \(+2.511\cdot10^{-3}\ \mathrm{eV}^2\) | \((2.450\text{–}2.576)\cdot10^{-3}\ \mathrm{eV}^2\) |
| \(\delta_{\rm CP}\) (NO) | \(212^\circ\) | \(125^\circ\)–\(365^\circ\) |
The interval for \(\delta_{\rm CP}\) allows \(180^\circ\) and \(360^\circ\equiv0^\circ\): CP-conserving values remain possible. Separate intervals are given for the inverted mass ordering.
\(3\sigma\) ranges for \(|U_{\alpha i}|\) when the atmospheric data IC24 and Super-Kamiokande are included:
| Flavor | \(\nu_1\) | \(\nu_2\) | \(\nu_3\) |
|---|---|---|---|
| \(e\) | \(0.810\)–\(0.834\) | \(0.532\)–\(0.568\) | \(0.144\)–\(0.156\) |
| \(\mu\) | \(0.259\)–\(0.498\) | \(0.514\)–\(0.678\) | \(0.652\)–\(0.756\) |
| \(\tau\) | \(0.280\)–\(0.512\) | \(0.488\)–\(0.659\) | \(0.637\)–\(0.743\) |
The intervals of different entries are correlated: their extreme values cannot be substituted simultaneously into a single matrix. The table was obtained within the unitary three-neutrino model.


The \(\theta_{23}\) profile allows solutions on both sides of \(45^\circ\). When comparing NO and IO, watch the notation \(\Delta m_{3\ell}^2\): for NO it is \(\Delta m_{31}^2\), for IO it is \(\Delta m_{32}^2\).
Red: NO; blue: IO. Solid curves: without tabulated SK-atm; dashed: with them.

\(\theta_{13}\) has a narrow minimum. The profile of the phase is much wider, and its shape changes noticeably depending on the choice of the atmospheric data set.
Red: NO; blue: IO. Solid curves: without tabulated SK-atm; dashed: with them. Source of the plot.

\[ U_{e1}U_{\mu1}^*+U_{e2}U_{\mu2}^*+U_{e3}U_{\mu3}^*=0. \]
Three complex terms close a triangle. In the NuFIT figure, the closure is imposed in advance, and the triangle shapes allowed in the unitary model are shown. For a direct test, the closure is left free.
The next lecture will begin with a question: how does matter change the phases of the neutrinos passing through it?
Exercises for Lecture 10 · Flavor triangle (in Russian) · Assemble the matrix (in Russian).
