Neutrino Oscillations in Vacuum and Matter

Fall School on Interdisciplinary Neutrino Science · Zhuhai, 12 November 2026

Dmitry V. Naumov

Joint Institute for Nuclear Research, Dubna

Vacuum

The problem

Two flavors, \(\sin^2\theta=\sin^2\theta_{12}=0.3088\) (NuFIT 6.1); \(L_{\rm osc}=4\pi E/\Delta m^2\). Each event is drawn at random with \(P(\nu_e\to\nu_\mu)\).

Neutrino = Quantum Chameleon

What is the mass of the electron neutrino?

A. Zero, as in the Standard Model

B. It depends on its mood: it is a chameleon

C. It has no mass of its own: it is a mix of \(\nu_1\), \(\nu_2\), \(\nu_3\)

What is the mass of the electron neutrino?

A. Zero, as in the Standard Model

B. It depends on its mood: it is a chameleon

C. It has no mass of its own: it is a mix of \(\nu_1\), \(\nu_2\), \(\nu_3\)

Each of \(\nu_1\), \(\nu_2\), \(\nu_3\) has its own mass. \(\nu_e\) is their mix, so it has none of its own.

Surprise: \(\nu_e\), \(\nu_\mu\), \(\nu_\tau\) have no mass

  • In QFT a fundamental particle is a quantum wave: an excitation of a quantum field with a mass, \(E_i=\sqrt{p^2+m_i^2}\).
  • There are no \(\nu_e\), \(\nu_\mu\), \(\nu_\tau\) fields with a mass. The massive fields are \(\nu_1\), \(\nu_2\), \(\nu_3\).
  • \(\nu_e\), \(\nu_\mu\), \(\nu_\tau\) are the combinations that the weak interaction creates and absorbs. For two of them:

\[ \boxed{ \begin{aligned} |\nu_e\rangle&=\cos\theta\,|\nu_1\rangle+\sin\theta\,|\nu_2\rangle\\ |\nu_\mu\rangle&=-\sin\theta\,|\nu_1\rangle+\cos\theta\,|\nu_2\rangle \end{aligned}} \]

  • One state space, two pairs of axes, turned by the mixing angle \(\theta\). For \(\nu_e\) and the slow clock below: \(\theta_{12}\approx34^\circ\).

Flavor axes nu_e and nu_x, the projections psi_e and psi_x of a state, and the mass axes nu_1 and nu_2 turned by the angle theta.

Here \(\nu_x=\nu_\mu\).

Two waves: in phase and out of phase

Move the detector. \(\nu_1\) and \(\nu_2\) leave the source in phase: \(\nu_e\). In antiphase the detector finds \(\nu_\mu\); in phase again, \(\nu_e\). A real geoneutrino makes about \(2\times10^{17}\) waves over \(L_{\rm osc}\approx100\) km.

The formula

Natural units

\(\hbar=c=1\)

\(E,\ p,\ m\) in eV

\(L,\ t\) in eV\(^{-1}\)

\(\hbar c=1.973\times10^{-7}\) eV m

\(\hbar=6.582\times10^{-16}\) eV s

CODATA 2022

\[ \boxed{ P(\nu_e\to\nu_\mu)=\sin^2 2\theta\;\sin^2\!\left(\frac{\Delta m^2L}{4E}\right) =\sin^2 2\theta\;\sin^2\!\left(1.267\,\frac{\Delta m^2[\mathrm{eV^2}]\;L[\mathrm{km}]}{E[\mathrm{GeV}]}\right)}, \qquad P(\nu_e\to\nu_e)=1-P(\nu_e\to\nu_\mu). \]

  • The angle sets the depth: \(P_{\max}=\sin^22\theta\).
  • \(\Delta m^2L/E\) sets where the maxima are. The oscillation length

\[ L_{\rm osc}=\frac{4\pi E}{\Delta m^2}=2.48\ \mathrm{km}\;\frac{E[\mathrm{GeV}]}{\Delta m^2[\mathrm{eV^2}]}. \]

The first maximum of the transition is at \(L=L_{\rm osc}/2\).

Let \(\varphi_i\) be the phase that mass component \(i\) accumulates between the source and the detector:

\[ |\nu_e;L\rangle=\cos\theta\,e^{-i\varphi_1}|\nu_1\rangle+\sin\theta\,e^{-i\varphi_2}|\nu_2\rangle . \]

A single mass state would carry only an overall phase, invisible in any probability. Here there are two waves: after the common factor is taken out, the difference \(\Delta\varphi=\varphi_2-\varphi_1\) remains.

The detector looks for \(|\nu_\mu\rangle=-\sin\theta\,|\nu_1\rangle+\cos\theta\,|\nu_2\rangle\). The mass states are orthonormal, \(\langle\nu_i|\nu_j\rangle=\delta_{ij}\), and two terms survive:

\[ \mathcal A_{e\to\mu}=\langle\nu_\mu|\nu_e;L\rangle =\sin\theta\cos\theta\left(e^{-i\varphi_2}-e^{-i\varphi_1}\right). \]

At \(L=0\) the phases are equal and the two terms cancel: the source prepared a pure \(\nu_e\).

\[ \left|e^{-i\varphi_2}-e^{-i\varphi_1}\right|^2=4\sin^2\frac{\Delta\varphi}{2}, \qquad 4\sin^2\theta\cos^2\theta=\sin^22\theta, \qquad P(\nu_e\to\nu_\mu)=\sin^22\theta\,\sin^2\frac{\Delta\varphi}{2}. \]

For a plane wave \(\varphi_i=E_it-p_iL\). With \(t\simeq L\) (\(\hbar=c=1\)) and \(E_i^2-p_i^2=m_i^2\):

\[ \varphi_i\simeq(E_i-p_i)L=\frac{m_i^2L}{E_i+p_i}\simeq\frac{m_i^2L}{2E}, \qquad \Delta\varphi\simeq\frac{\Delta m^2L}{2E}. \]

Geoneutrino Example

The Earth cut through the detector: the thin crust and the mantle hold uranium and thorium, the core none; one source at distance L from the detector and the sphere of radius L around it.

One source at distance \(L\): \(P_{ee}(L)\). All sources of the Earth closer than \(L\): \(\bar P_{ee}(L)=\int_0^L w(x)\,P_{ee}(x)\,dx\Big/\!\int_0^L w(x)\,dx\).

neutrino energy
Losc, slow clock Δm²21 Losc, fast clock Δm²31 signal from closer than Losc half of the signal from beyond crust : mantle without oscillations detected as ν̄e the whole Earth

A volume \(dV\) emitting \(n\) antineutrinos per cm³ per s gives the flux \(n\,dV/4\pi x^2\); around the detector \(dV=x^2dx\,d\Omega\), so \(d\Phi=\frac{n}{4\pi}\,dx\,d\Omega\). Only the solid angle inside a shell \(a<r<b\) is left; \(\beta\) is the angle from the vertical, \(r^2=R^2+x^2-2Rx\cos\beta\):

\[ \frac{d\Phi}{dx}=\frac{n}{2}\,\bigl[\cos\beta(a)-\cos\beta(b)\bigr], \qquad \cos\beta(r)=\frac{R^2+x^2-r^2}{2Rx}\ \ \text{clipped to}\ [-1,1]. \]

  • Crust: \(d\Phi/dx\approx n/2\) for \(x<H=35\) km, \(\approx nH/2x\) beyond. A uniform ball: \(\Phi=\frac{nR}{2}\).
  • Each shell emits \(n=\rho\,(\ell_{\rm U}c_{\rm U}+\ell_{\rm Th}c_{\rm Th})\), \(\ell_{\rm U}=7.46\times10^7\), \(\ell_{\rm Th}=1.62\times10^7\) ν̄ per kg per s. Crust: 2.7 g/cm³, U 1.3 ppm, Th 5.6 ppm; mantle: U 12 ppb, Th 48 ppb; core: none.

The detector does not know where a neutrino came from; it counts all of them:

\[ S(L)=\sum_{\rm shells}\int_0^L \frac{d\Phi}{dx}\,P_{ee}(x)\,dx, \qquad w(x)=\frac{1}{S_0}\sum_{\rm shells}\frac{d\Phi}{dx}, \qquad S_0:\ \text{the whole Earth without oscillations.} \]

Continental crust 35 km (Rudnick & Gao 2003); mantle: bulk silicate Earth (McDonough & Sun 1995) minus the crust; TNU after Fiorentini et al. 2007. Spectrum: U and Th chains (S. Enomoto) times the IBD cross section (Vogel & Beacom 1999), U : Th = 30.3 : 9.0 TNU. Oscillations: NuFIT 6.1, normal ordering. Earth picture: radii to scale, interior colors schematic; surface: NASA Blue Marble.

Atmospheric Neutrino Example

The Earth cut through the detector; the path of an atmospheric neutrino at the chosen zenith angle is drawn over it.

A \(\nu_\mu\) born in the atmosphere at height \(h\approx15\) km; the zenith angle fixes the path: \(L=15\) km from above, \(437\) km from the horizon, \(12\,757\) km from below.

neutrino energy
direction
distance L Losc, fast clock Δm²31 Losc, slow clock Δm²21 νμ → νμ νμ → ντ νμ → νe

The path from the birth point at height \(h\) to a detector on the surface, \(R=6371\) km:

\[ L(\theta_z)=\sqrt{(R+h)^2-R^2\sin^2\theta_z}-R\cos\theta_z , \qquad h\approx15\ \text{km}. \]

Three flavors in vacuum, one energy and one direction:

\[ P(\nu_\mu\to\nu_\beta)=\Bigl|\sum_{i=1}^{3}U_{\beta i}\,U^*_{\mu i}\,e^{-i m_i^2L/2E}\Bigr|^2 . \]

  • No averaging over \(L\) or \(E\): atmospheric detectors reconstruct the energy and the direction of each event.
  • No matter yet: the Earth’s electrons change these curves at a few GeV (slide “Matter turns the axes”, tab Picture).

\(h\approx15\) km: the most probable production height of vertical neutrinos from pion decay (Gaisser & Stanev, Phys. Rev. D 57, 1977 (1998)). NuFIT 6.1 best fit (IC24 + SK-atm), normal ordering: \(\sin^2\theta_{12}=0.3088\), \(\sin^2\theta_{13}=0.02248\), \(\sin^2\theta_{23}=0.470\), \(\delta=212^\circ\), \(\Delta m^2_{21}=7.537\times10^{-5}\) eV², \(\Delta m^2_{31}=2.511\times10^{-3}\) eV². Earth picture: radii to scale (PREM), interior colors schematic; surface: NASA Blue Marble.

Vacuum = Birefringent Crystal

A calcite crystal on graph paper: every blue line seen through the crystal appears twice.

Calcite on graph paper: every line is seen twice. Photo: APN MJM, Wikimedia Commons, CC BY-SA 3.0.

Light in a birefringent plate

In. The polarizer passes light polarized along \(H\).

Crystal, thickness \(L\), axes at the angle \(\theta\) to \(H\): two waves, \(\cos\theta\) along the fast axis, \(\sin\theta\) along the slow one.

Out. The slow wave lags by \(\Delta\varphi=2\pi\,(n_o-n_e)\,L/\lambda\): the polarization is elliptical.

Filter \(V\). The detector sees \(I_V/I_0=\sin^22\theta\,\sin^2(\Delta\varphi/2)\).

Calcite at 589 nm: \(n_o=1.658\), \(n_e=1.486\) (G. Ghosh, Opt. Commun. 163, 95 (1999)); a full-wave plate is \(\lambda/(n_o-n_e)=3.42\ \mu\)m thick. The drawing is schematic: wavelength and thickness not to scale.

\(I_V/I_0\)\(I_H/I_0\)
crystal: calcite, \(\lambda=589\) nm
\(n_o,\ n_e\)1.658, 1.486 \(L/\lambda\) \(\Delta\varphi=2\pi\,(n_o-n_e)\,L/\lambda\) output polarization axis ratio \(b/a\) \(I_H/I_0\) \(I_V/I_0=\sin^2 2\theta\,\sin^2\frac{\Delta\varphi}{2}\)

The vacuum is a birefringent crystal for neutrinos

In the mass basis the vacuum is diagonal: one refractive index per mass state,

\[ n=\begin{pmatrix}n_1&0&0\\0&n_2&0\\0&0&n_3\end{pmatrix}, \qquad n_i\simeq1-\frac{m_i^2}{2E^2}, \qquad E\,(n_i-n_j)\,L=\frac{\Delta m^2_{ji}\,L}{2E}. \]

Light in calcite Neutrinos in vacuum
two axes, \(o\) and \(e\) three axes, \(\nu_1,\nu_2,\nu_3\)
angle \(\theta\) of the axes to \(H\) mixing angles \(\theta_{12},\theta_{13},\theta_{23}\)
polarizer \(H\), analyzer \(V\) \(\nu_e\) at the source, \(\nu_\mu\) at the detector
\(\Delta\varphi=2\pi\,(n_o-n_e)\,L/\lambda\) \(\Delta\varphi_{ji}=\Delta m^2_{ji}\,L/2E\)

Three neutrinos, three axes: even empty space is a crystal for them.

Matter

Everything is tiny

\(\Delta n\) a full turn of the phase
light, 589 nm calcite: \(n_o-n_e\) \(0.17\) \(3.4\ \mu\mathrm{m}\)
\(\nu\), 10 MeV vacuum: \(n_1-n_2\) \(3.8\times10^{-19}\) \(329\ \mathrm{km}\)
\(\nu\), 10 MeV solar center: \(n_{\nu_\mu}-n_{\nu_e}\) \(7.9\times10^{-19}\) \(158\ \mathrm{km}\)

\(5\times10^{17}\) times weaker than calcite. The flavor still turns: the paths are hundreds of kilometers.

\(\Delta n=\Delta m^2_{21}/2E^2\) and \(V/E\) with \(V=\sqrt2\,G_Fn_e\), \(n_e/N_A=102.9\ \mathrm{cm^{-3}}\) at the solar center (BS05(OP)); a full turn: \(E\,\Delta n\,L=2\pi\).

A \(\nu_e\) crosses the Sun. Its phase velocity is…

A. Above \(c\)

B. Below \(c\), as for light in glass

C. Whatever the solar weather allows today

A \(\nu_e\) crosses the Sun. Its phase velocity is…

A. Above \(c\)

B. Below \(c\), as for light in glass

C. Whatever the solar weather allows today

\(n_{\nu_e}-1=-V/E<0\): the phase runs faster than light. The group velocity, which carries the signal, stays below \(c\). Einstein is safe.

Only \(\nu_e\) feels the electrons

Charged-current forward scattering of an electron neutrino on an electron through W exchange, in the flavor basis.

\[ \boxed{\,n_{\nu_e}-1=-\frac{V}{E}<0\,}, \qquad V=\sqrt2\,G_F\,n_e . \]

  • Only \(\nu_e\) exchanges a \(W\) with the electrons; the \(Z\) part is the same for all flavors.
  • \(V>0\) is a repulsion: \(p=E-V\). The wavelength grows, the phase velocity exceeds \(c\), as for X-rays on free electrons.
  • The group velocity stays below \(c\): \(E=\sqrt{p^2+m^2}+V\) gives \(v_g=dE/dp=p/\sqrt{p^2+m^2}<1\).
  • \(\bar\nu_e\): \(V<0\), \(n>1\).

\[ n-1=-\frac{V}{E}\begin{pmatrix}1&0\\0&0\end{pmatrix}: \ \text{the axes } \nu_e,\nu_\mu \text{ stay.} \]

The same diagram in the mass basis: an incoming nu_i and an outgoing nu_j, with the factors U_ei and the complex conjugate of U_ej at the vertices.

The same scattering, written for \(\nu_1,\nu_2\) (\(U_{e1}=\cos\theta\), \(U_{e2}=\sin\theta\)):

\[ n-1=-\frac{V}{E}\begin{pmatrix}\cos^2\theta&\sin\theta\cos\theta\\\sin\theta\cos\theta&\sin^2\theta\end{pmatrix}. \]

  • One scattering turns \(\nu_1\) into \(\nu_2\): the amplitude is \(\propto U_{e1}U_{e2}^*=\sin\theta\cos\theta\neq0\).
  • Add the vacuum, \(\mathrm{diag}(n_1,n_2)\): the sum is not diagonal.

The crystal turns its axes, \(\nu_{1,2}\to\nu_{1m,2m}\), and its indices change, \(n_{1,2}\to n_{1m,2m}\).

A plane wave \(e^{ikz}\) crosses a slab \(dz\) with \(N\) scatterers per volume, each scattering \(f(\theta)\,e^{ikr}/r\). The first Fresnel zones add up to

\[ e^{ikz}\Bigl[1+\frac{2\pi i}{k}\,N f(0)\,dz\Bigr]=e^{inkz} \quad\Rightarrow\quad n-1=\frac{2\pi N f(0)}{k^2}. \]

Only the forward amplitude \(f(0)\) enters.

\(W\) exchange at \(q^2\ll M_W^2\), after the Fierz rearrangement (coefficient \(+1\) for anticommuting fields):

\[ \mathcal L=-\frac{G_F}{\sqrt2}\,[\bar\nu_e\gamma^\mu(1-\gamma_5)\nu_e]\,[\bar e\gamma_\mu(1-\gamma_5)e]. \]

Forward, left-handed \(\nu_e\), unpolarized \(e^-\) at rest: \(\bar u_\nu\gamma^\mu(1-\gamma_5)u_\nu=4p^\mu\), \(\langle\bar u_e\gamma_\mu(1-\gamma_5)u_e\rangle=2k_\mu\):

\[ \mathcal M_{\rm fwd}=-4\sqrt2\,G_F\,E\,m_e, \qquad f(0)=\frac{\mathcal M_{\rm fwd}}{8\pi m_e}=-\frac{G_F E}{\sqrt2\,\pi}<0 . \]

Born: \(f=-\dfrac{E}{2\pi}\displaystyle\int U\,d^3r\), so \(U=\sqrt2\,G_F\,\delta^3(\mathbf r)\). A vector exchange between like charges: repulsion; \(\bar\nu_e\): \(V\to-V\).

\[ V=N_e\!\int U\,d^3r=-\frac{2\pi N_e f(0)}{E}=\sqrt2\,G_F N_e>0, \qquad n-1=-\frac{\sqrt2\,G_F N_e\,E}{p^2}\simeq-\frac{V}{E}<0 . \]

The role of \(\omega_0\). Light on an oscillator: \(f(0)=r_e\,\omega^2/(\omega_0^2-\omega^2)\); a free electron, \(\omega_0=0\): \(f(0)=-r_e\), \(n<1\) (X-rays). Here the pole is the \(W\): for \(\nu_e e^-\) it sits in the \(u\) channel and is never reached, \(n<1\) at all energies; for \(\bar\nu_e e^-\) it is in the \(s\) channel, at \(E=M_W^2/2m_e\approx6.3\) PeV (Glashow): below it \(n>1\).

R. D. Peccei, hep-ph/9906509, Eqs. (91)–(92); E. Kh. Akhmedov, hep-ph/0001264, Eqs. (84)–(88); L. Wolfenstein, Phys. Rev. D 17, 2369 (1978). \(Z\) exchange is common to all flavors and drops out.

Matter against vacuum: one ratio

\[ \boxed{A=\frac{V}{\Delta m^2/2E}=\frac{2EV}{\Delta m^2}}, \qquad V=\sqrt2\,G_Fn_e=7.63\times10^{-14}\ \mathrm{eV}\cdot\frac{Y_e\rho}{\mathrm{g\,cm^{-3}}}, \qquad \bar\nu:\ A<0 . \]

\(E\) \(\Delta m^2\) \(Y_e\rho\), g/cm³ \(A\)
solar center, \(\nu_e\) 10 MeV \(\Delta m^2_{21}\) 103 \(2.08\)
mantle, geo-\(\bar\nu_e\) 3 MeV \(\Delta m^2_{21}\) 2.2 \(-0.013\)
mantle, atmospheric \(\nu\) 6 GeV \(\Delta m^2_{31}\) 2.2 \(0.80\)

The Sun: matter wins. Geoneutrinos: vacuum wins, 75 times. GeV neutrinos in the Earth: a draw.

Matter turns the axes of the crystal

After a length \(L\) each state collects the phase \(E\,(1-n)\,L\). In the basis \(\nu_1,\nu_2\):

\[ E\,(1-n)\,L=\underbrace{\varphi_0\,\mathbf{1}}_{\text{same for all}} +\underbrace{\frac{L}{2E}\begin{pmatrix}0&0\\0&\Delta m^2\end{pmatrix}}_{\text{vacuum}} +\underbrace{V L\begin{pmatrix}\cos^2\theta&\sin\theta\cos\theta\\\sin\theta\cos\theta&\sin^2\theta\end{pmatrix}}_{\text{matter}} \]

\(\varphi_0\) is not seen. Take out \(\dfrac{\Delta m^2L}{2E}=2\pi\dfrac{L}{L_{\rm osc}}\):

\[ E\,(1-n)\,L=\varphi_0\,\mathbf{1}+2\pi\,\frac{L}{L_{\rm osc}}\, \boxed{\begin{pmatrix}0&0\\0&1\end{pmatrix}+A\begin{pmatrix}\cos^2\theta&\sin\theta\cos\theta\\\sin\theta\cos\theta&\sin^2\theta\end{pmatrix}}, \qquad A=\frac{2EV}{\Delta m^2}. \]

The box is a matrix of numbers: the crystal.

In its own axes \(\nu_{1m},\nu_{2m}\) the crystal is diagonal: each axis keeps its own phase, nothing mixes.

\[ \psi_{km}(L)=e^{-2\pi i\,\lambda_k L/L_{\rm osc}}\,\psi_{km}(0), \qquad \lambda_{1,2}=\tfrac12\bigl(1+A\mp R\bigr), \qquad R=\sqrt{(\cos2\theta-A)^2+\sin^22\theta}. \]

\[ \nu_e=\cos\theta_m\,\nu_{1m}+\sin\theta_m\,\nu_{2m}, \qquad \sin2\theta_m=\frac{\sin2\theta}{R}, \qquad \cos2\theta_m=\frac{\cos2\theta-A}{R}. \]

The phase between the axes grows as \(2\pi R\,L/L_{\rm osc}\). In vacuum, \(A=0\): \(R=1\), \(\theta_m=\theta\).

\(P(\nu_e\to\nu_\mu)\), this medium vacuum
\(L/L_{\rm osc}\), \(L_{\rm osc}=4\pi E/\Delta m^2\)
matter
length
angle of \(\nu_e\) to \(\nu_{1m}\): \(\theta_m\) depth \(\sin^2 2\theta_m\) \(L^m_{\rm osc}/L_{\rm osc}=1/R\) \(P(\nu_e\to\nu_\mu)\) \(P(\nu_e\to\nu_e)\)
\(P=\sin^2 2\theta_m\,\sin^2\dfrac{\Delta m^2_m L}{4E}\)

\[ \boxed{P(\nu_e\to\nu_\mu)=\sin^22\theta_m\,\sin^2\!\left(\frac{\Delta m^2_m\,L}{4E}\right)} \]

\[ \sin^22\theta_m=\frac{\sin^22\theta}{(\cos2\theta-A)^2+\sin^22\theta}, \qquad \Delta m^2_m=\Delta m^2\sqrt{(\cos2\theta-A)^2+\sin^22\theta}. \]

The vacuum formula with \(\theta\to\theta_m\) and \(\Delta m^2\to\Delta m^2_m\).

  • \(A=0\): the vacuum.
  • Resonance at \(A=\cos2\theta\): \(\sin^22\theta_m=1\) for any vacuum angle (Mikheyev, Smirnov, Wolfenstein).
  • \(A\gg1\): \(\theta_m\to90^\circ\), \(\nu_e\) is itself an axis of the crystal, the flavor freezes.
  • \(A<0\) (antineutrinos for \(\Delta m^2>0\)): no resonance. Matter tells \(\nu\) from \(\bar\nu\), and the sign of \(\Delta m^2\).

Left: effective mixing in matter against A for the two vacuum angles; both reach unit height at the resonance, A = cos 2 theta. Right: effective theta13 mixing in the Earth against energy: neutrinos resonate near 7 GeV in the mantle and 3 GeV in the core; antineutrinos are suppressed.

The Sun

What leaves the Sun when a 10 MeV \(\nu_e\) is born at its center?

A. A \(\nu_e\), of course

B. Almost only \(\nu_2\)

C. Nothing: the Sun keeps it as a souvenir

What leaves the Sun when a 10 MeV \(\nu_e\) is born at its center?

A. A \(\nu_e\), of course

B. Almost only \(\nu_2\)

C. Nothing: the Sun keeps it as a souvenir

About 94 % \(\nu_2\), a mass state: it no longer oscillates on the way to the Earth. Two flavors, adiabatic; see the next slide.

Solar Neutrinos

Solar electron-neutrino survival probability against energy from 0.1 to 20 MeV: the three-flavor adiabatic MSW curve falls from the vacuum average 0.55 at low energy to 0.30 above 10 MeV; Borexino points for pp, 7Be, pep and 8B neutrinos follow it.

Curve: three flavors, adiabatic MSW, NuFIT 6.1, BS05(OP) density where \(^8\)B neutrinos are made. Points: Borexino with high-metallicity solar fluxes, Nature 562, 505 (2018); values as quoted in arXiv:2105.13858.

Lepton Mixing

Unitarity

Three flavors, three masses: \(\nu_\alpha=\sum_{i=1}^{3}U_{\alpha i}\,\nu_i\), \(\alpha=e,\mu,\tau\). Both sets are orthonormal bases of one space, so \(U\) is unitary:

\[ UU^\dagger=U^\dagger U=\mathbf 1:\qquad \underbrace{\sum_{i}|U_{\alpha i}|^2=1}_{\text{rows}},\qquad \underbrace{\sum_{\alpha}|U_{\alpha i}|^2=1}_{\text{columns}},\qquad \underbrace{\sum_{\alpha}U_{\alpha i}U^*_{\alpha j}=0,\ i\ne j}_{\text{orthogonal columns}} . \]

\(|U_{\alpha i}|^2\) is the share of \(\nu_i\) in \(\nu_\alpha\). Two measurements, to leading order:

\[ \text{solar }{}^8\text{B}:\ P_{ee}\simeq|U_{e2}|^2\simeq\tfrac13, \qquad \text{atmospheric}:\ 4|U_{\mu3}|^2\bigl(1-|U_{\mu3}|^2\bigr)\simeq1, \qquad |U_{e3}|^2\simeq0 . \]

Nine shares \(|U_{\alpha i}|^2\): two measurements, \(|U_{e3}|^2\simeq0\) and unitarity fix them all.

The mixing matrix from data

Step 0 of 10

We start with an empty matrix

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.

\(\bigl|U_{\alpha i}\bigr|^2\)
\(\nu_1\) \(\nu_2\) \(\nu_3\)
\(e\) \(\tfrac23\)\(\sqrt{\tfrac23}\)\(\pm\sqrt{\tfrac23}\)\(+\sqrt{\tfrac23}\)\(0.676\) \(\tfrac13\)\(\sqrt{\tfrac13}\)\(+\sqrt{\tfrac13}\)\(+\sqrt{\tfrac13}\)\(0.302\) \(0\)\(0\)\(0\)\(0\)\(0.022\)
\(\mu\) \(\tfrac16\)\(\sqrt{\tfrac16}\)\(\pm\sqrt{\tfrac16}\)\(-\sqrt{\tfrac16}\)\(0.112\) \(\tfrac13\)\(\sqrt{\tfrac13}\)\(+\sqrt{\tfrac13}\)\(+\sqrt{\tfrac13}\)\(0.428\) \(\tfrac12\)\(\sqrt{\tfrac12}\)\(+\sqrt{\tfrac12}\)\(+\sqrt{\tfrac12}\)\(0.459\)
\(\tau\) \(\tfrac16\)\(\sqrt{\tfrac16}\)\(\pm\sqrt{\tfrac16}\)\(+\sqrt{\tfrac16}\)\(0.212\) \(\tfrac13\)\(\sqrt{\tfrac13}\)\(-\sqrt{\tfrac13}\)\(-\sqrt{\tfrac13}\)\(0.270\) \(\tfrac12\)\(\sqrt{\tfrac12}\)\(+\sqrt{\tfrac12}\)\(+\sqrt{\tfrac12}\)\(0.518\)
The first ten steps: \(U_{e3}=0\). The last step: NuFIT 6.1, NO, IC24 + SK-atm (2025).

What is measured, what is open

NuFIT 6.1 JUNO, 59.1 d JUNO, 207.2 d
\(\sin^2\theta_{12}\) 0.3088 \(0.3092\pm0.0087\) \(0.3036\pm0.0064\)
\(\Delta m^2_{21}/10^{-5}\,\mathrm{eV^2}\) 7.537 \(7.50\pm0.12\) \(7.388\pm0.078\)
\(\sin^2\theta_{13}\) 0.02248
\(\sin^2\theta_{23}\) 0.470
\(\Delta m^2_{31}/10^{-3}\,\mathrm{eV^2}\) \(+2.511\) \(+2.509^{+0.027}_{-0.025}\)
\(\delta_{CP}\) \(212^\circ\)

Open

  • The ordering: is \(\nu_3\) the heaviest? Normal ordering is preferred at about 2–3σ; JUNO alone, with long-baseline \(\Delta m^2_{31}\), at ≥ 2.1σ.
  • CP violation: is \(\delta_{CP}\) different from 0 and \(180^\circ\)?
  • The octant: is \(\theta_{23}\) above or below \(45^\circ\)?
  • The masses themselves: oscillations see only differences.

NuFIT 6.1, best fit, normal ordering, IC24 with SK atmospheric data (www.nu-fit.org). JUNO: arXiv:2511.14593 (59.1 days), arXiv:2609.37895 (207.2 days, normal ordering).

Summary

  1. There are no \(\nu_e\), \(\nu_\mu\), \(\nu_\tau\) fields with a mass: each is a superposition of the massive \(\nu_1\), \(\nu_2\), \(\nu_3\). Two waves beat: \(P=\sin^22\theta\,\sin^2(\Delta m^2L/4E)\).
  2. Far from the source the beat averages out. Geoneutrinos arrive as a mixture of \(\nu_1,\nu_2,\nu_3\): \(\langle P_{ee}\rangle=0.68\cdot0.68+0.30\cdot0.30+0.02\cdot0.02=0.55\).
  3. For neutrinos the vacuum is a birefringent crystal, diagonal in \(\nu_1,\nu_2\). Matter acts only on \(\nu_e\): the crystal turns and its indices change. The same formula with \(\theta_m\) and \(\Delta m^2_m\); resonance at \(A=\cos2\theta\).
  4. The Sun: at low energy the vacuum average, \(P_{ee}\approx0.55\); for \(^8\)B the axes turn slowly and \(\nu_2\) leaves the Sun, \(P_{ee}\approx0.30\). The Earth changes geoneutrinos by less than 1 %, and GeV neutrinos strongly: tomography (S. Petcov, next lectures).

The Textbook

Front cover of Quantum Field Theory for Experimentalists and Beyond by Dmitry Naumov, volume 1.

Quantum Field Theory for Experimentalists and Beyond

A practical course with examples, problems, and solutions: from the foundations to renormalization, anomalies and functional integrals, always tied to experiment.

  • In English: three volumes, electronic edition, November 2026.
  • In Russian: two volumes, IKI, 2026.

Appendix

Matter: eigenvalues and angle

At fixed energy, in the mass basis, with \(\Delta=\Delta m^2/2E\) (terms common to both states dropped):

\[ i\frac{d}{dx}\binom{\psi_1}{\psi_2}= \left[ \begin{pmatrix}0&0\\0&\Delta\end{pmatrix} +V\begin{pmatrix}\cos^2\theta&\sin\theta\cos\theta\\\sin\theta\cos\theta&\sin^2\theta\end{pmatrix} \right] \binom{\psi_1}{\psi_2}. \]

The first matrix is the vacuum, diagonal. The second is \(V\) times the projector on \(\nu_e=\cos\theta\,\nu_1+\sin\theta\,\nu_2\): \(\nu_1\) and \(\nu_2\) are no longer eigenstates. In units of \(\Delta\) this is the matrix \(\mathrm{diag}(0,1)+A\,P_e\) of the slide “Matter turns the axes”.

In units of \(\Delta\) the matrix is \(M=\begin{pmatrix}A\cos^2\theta&A\sin\theta\cos\theta\\A\sin\theta\cos\theta&1+A\sin^2\theta\end{pmatrix}\), with \(\operatorname{tr}M=1+A\) and \(\det M=A\cos^2\theta\). Then \(\det(M-\lambda)=0\) gives

\[ \lambda_{1,2}=\frac{1+A\mp\sqrt{(1+A)^2-4A\cos^2\theta}}{2}=\frac{1+A\mp R}{2}, \qquad (1+A)^2-4A\cos^2\theta=(\cos2\theta-A)^2+\sin^22\theta=R^2 . \]

The phase difference is \((\lambda_2-\lambda_1)\Delta L=R\,\Delta m^2L/2E\): hence \(\Delta m^2_m=R\,\Delta m^2\). Its smallest value, \(R=\sin2\theta\), is at \(A=\cos2\theta\): the levels would cross there; mixing keeps them apart.

Rotate to the flavor basis, \(\nu_e=\cos\theta\,\nu_1+\sin\theta\,\nu_2\):

\[ M_{\rm flavor}=\frac{1+A}{2}\,\mathbf 1+\frac12\begin{pmatrix}A-\cos2\theta&\sin2\theta\\\sin2\theta&\cos2\theta-A\end{pmatrix} =\frac{1+A}{2}\,\mathbf 1+\frac R2\begin{pmatrix}-\cos2\theta_m&\sin2\theta_m\\\sin2\theta_m&\cos2\theta_m\end{pmatrix}, \]

\[ \sin2\theta_m=\frac{\sin2\theta}{R},\qquad \cos2\theta_m=\frac{\cos2\theta-A}{R}. \]

The same form as the vacuum (\(A=0\), \(R=1\)) with \(\theta\to\theta_m\): the eigenvectors are \(\nu_{1m}=\cos\theta_m\,\nu_e-\sin\theta_m\,\nu_\mu\), \(\nu_{2m}=\sin\theta_m\,\nu_e+\cos\theta_m\,\nu_\mu\), and the vacuum derivation of \(P\) repeats with \(\theta\to\theta_m\), \(\Delta m^2\to R\,\Delta m^2\).

Follow the twist

max η—
min Δm/Δ—
P2m(exit)—
P2(exit)—
Pe(exit)—
one wave, three decompositions
exact state at the avoided crossing

“Adiabatic”: the state follows the upper branch and leaves as the other flavor. “Fast”: it jumps across the gap. “Small θ”: the gap is narrow and following is harder.

Decoherence: why the phase is lost

  • \(\nu_1\) and \(\nu_2\) of one energy travel with different group velocities, \(v_i\simeq1-\dfrac{m_i^2}{2E^2}\).
  • A wave packet of length \(\sigma_x\): the two packets separate after \[ L_{\rm coh}\sim\sigma_x\,\frac{2E^2}{\Delta m^2}\qquad(\Delta v\,L=\sigma_x). \]
  • Beyond \(L_{\rm coh}\) the detector meets \(\nu_1\) and \(\nu_2\) apart: probabilities add, not amplitudes, \[ P_{ee}=\sum_i|U_{ei}|^4 . \]
  • The same result comes earlier from averaging: a source region or an energy spread much wider than one \(L_{\rm osc}\) washes out \(\sin^2(\Delta m^2L/4E)\to\tfrac12\). Geoneutrinos: sources all over the Earth, \(L_{\rm osc}\approx100\) km. The Sun: neutrinos are made over \(10^4\)–\(10^5\) km, \(L_{\rm osc}\lesssim300\) km.

The same physics with two pendulums

1: m₁ 2: m₂ exact two-level amplitude start: pendulum 1 xᵢ = √mᵢ φᵢ θ = 45.0° sin²2θ = 1.000 actual motion = Re aᵢ/√mᵢ 1 0 P₁ P₂ 0 1 2 Δωt / π
1.00
0.15
14°
0°
×1.0
0.00
θ45.0° ω₊ / ω₀1.000 ω₋ / ω₀1.140 Pmax1.000
P₁
1.000
P₂
0.000

P₁ + P₂ = 1 exactly, no averaging

Push one pendulum: the swing moves to the other one and back. Each normal mode keeps its own frequency; the energy transfer is their beat, \(P_{1\to2}(t)=\sin^22\theta\,\sin^2[(\omega_--\omega_+)t/2]\).

Explore three-flavor probabilities