research29 min studyLesson 637 in Physics

Matter-enhanced neutrino oscillations

Diagonalize a two-flavor matter Hamiltonian, track neutrino-antineutrino signs, and distinguish resonance from adiabatic conversion.

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What you’ll understand

  • Derive the effective mixing and positive eigenvalue gap in constant density.
  • Apply the signed resonance condition to neutrinos and antineutrinos.
  • Separate constant-density interference from varying-density adiabatic evolution.

Ordinary matter treats electron neutrinos differently from the other active flavors because electrons support an additional charged-current forward-scattering amplitude. Coherent scattering changes the propagation Hamiltonian without requiring an observed collision or absorption. The resulting effective mixing can differ greatly from its vacuum value. We will first use an ideal constant-density two-flavor medium, where exact diagonalization is elementary, and then identify the additional assumptions needed to describe a neutrino crossing a changing density profile.

A flavor-dependent potential changes relative phases

Use the flavor basis electron and x, where x is an active muon-tau combination with no charged-current interaction on ambient electrons. Assume electrically neutral, unpolarized ordinary matter with negligible muon or tau populations and negligible incoherent attenuation. The electron potential for neutrinos is V=2GFneV=\sqrt2G_Fn_e, with electron number density n e. In natural units V has energy units. Density expressed in inverse cubic metres must be converted consistently before multiplication by a Fermi constant quoted in inverse energy squared.

A common neutral-current potential is proportional to the identity in this active two-flavor space and can be subtracted without affecting transition probabilities. After also subtracting the vacuum trace, add the remaining potential only to the electron diagonal entry. For antineutrinos reverse V and complex conjugate the vacuum mixing matrix; the latter has no effect in our real two-flavor limit. Matter itself is not CP symmetric, so unequal neutrino and antineutrino transition probabilities in this environment do not by themselves establish an intrinsic CP-violating phase.

H=Δm24E(−cos⁡2θsin⁡2θsin⁡2θcos⁡2θ)+(V000),V=2GFne,a=2EVΔm2H=\frac{\Delta m^2}{4E}\begin{pmatrix}-\cos2\theta&\sin2\theta\\\sin2\theta&\cos2\theta\end{pmatrix}+\begin{pmatrix}V&0\\0&0\end{pmatrix},\qquad V=\sqrt2G_Fn_e,\qquad a=\frac{2EV}{\Delta m^2}
The signed splitting is delta m squared = m2 squared minus m1 squared, and a is dimensionless. The Hamiltonian is written in natural units; its identity part can be removed. For antineutrinos use V to minus V.↔ Scroll wide equations horizontally.

Diagonalization separates mixing from wavelength

The difference of the two diagonal entries competes with the off-diagonal mixing term. Define D=(cos⁡2θ−a)2+sin⁡2(2θ)D=\sqrt{(\cos2\theta-a)^2+\sin^2(2\theta)}. Then the effective mixing prefactor is the vacuum sine squared divided by D squared, while the positive mass-squared-equivalent gap is the absolute vacuum splitting times D. These are two separate changes. A large mixing prefactor does not guarantee large conversion at a specified baseline because the propagation phase can still land near an integer multiple of pi.

For nonzero vacuum mixing, resonance occurs at a=cos⁡2θa=\cos2\theta, where the effective angle is maximal. The condition requires the sign of the potential to match the signed vacuum splitting times the cosine. Reversing the mass ordering or switching to antineutrinos can therefore remove the resonance in the same medium. At resonance the gap remains nonzero when the vacuum off-diagonal term is nonzero: this is an avoided crossing, not an exact degeneracy. With zero vacuum mixing, a formal diagonal crossing does not produce conversion by itself.

D=(cos⁡2θ−a)2+sin⁡2(2θ),sin⁡2(2θm)=sin⁡2(2θ)D2,Δmm2=∣Δm2∣D,Pe→x=sin⁡2(2θm)sin⁡2Δmm2L4ED=\sqrt{(\cos2\theta-a)^2+\sin^2(2\theta)},\qquad \sin^2(2\theta_m)=\frac{\sin^2(2\theta)}{D^2},\qquad \Delta m_m^2=|\Delta m^2|D,\qquad P_{e\to x}=\sin^2(2\theta_m)\sin^2\frac{\Delta m_m^2L}{4E}
This exact two-state constant-density formula assumes coherent ultrarelativistic propagation and nonzero D. The defined matter gap is positive even if the vacuum splitting is negative. Restore the same practical phase-unit conversion as in vacuum.↔ Scroll wide equations horizontally.

A changing medium needs an evolution criterion

When density varies along the path, the instantaneous matter angle and eigenvalue gap vary too. Following an instantaneous eigenstate requires the basis to change slowly compared with the local eigenfrequency separation. This adiabatic condition is additional information, not a consequence of crossing the resonance density. Rapid changes can cause transitions between matter eigenstates. A solar-neutrino prediction also combines the production region, full density profile, mixing channels, and possible phase averaging before detection. Substituting a single average density into the constant-density formula need not reproduce that physics.

The signed two-state calculation explains how a known matter potential can introduce ordering sensitivity absent from the elementary vacuum probability. A real three-flavor fit includes multiple splittings, the CP phase, realistic density uncertainty, energy spectra, and experimental response. It must not identify every matter-induced difference with fundamental CP violation or infer an ordering from one enhancement without fixing channel and sign conventions. The useful sequence is to specify the potential, diagonalize or evolve the Hamiltonian, compute phases, and only then average over the measured ensemble.

Maximal effective mixing at a tuned density

Take positive Δm2\Delta m^2, vacuum angle θ=30∘\theta=30^\circ, and constant-density parameter a = 1/2. Choose a baseline whose vacuum phase is Δm2L/(4E)=π/3\Delta m^2L/(4E)=\pi/\sqrt3. Find the effective mixing prefactor, matter gap, and transition probability.

  1. The vacuum cosine is cos⁡60∘=1/2\cos60^\circ=1/2, exactly equal to a. The resonance condition holds and the denominator becomes D2=sin⁡260∘=3/4D^2=\sin^260^\circ=3/4.

  2. The effective mixing prefactor is one, while D=3/2D=\sqrt3/2. Thus the positive matter gap is Δmm2=(3/2)Δm2\Delta m_m^2=(\sqrt3/2)\Delta m^2, smaller than the vacuum gap.

  3. The matter phase is D times the given vacuum phase, namely pi over two. Its sine squared is one, so the transition probability is one in this ideal coherent constant-density model.

The result

The effective mixing is maximal, the matter gap is √3/2 times the positive vacuum splitting, and the chosen baseline gives complete two-flavor conversion.

Explore the model

Interactive lab

Interactive lab · quantum

Changing a basis projection changes its weights

Reset and set BOTH Mixing angle θ = 60° and Relative phase φ = 0°; predict P(1) = 0.25. For a fresh comparison, Reset and set θ = 90° and φ = 0°; predict equal basis probabilities. Inspect the probabilities at time zero.

Changing a basis projection changes its weightsA normalized two-level pure state, not an interacting field simulation. Playback adds one radian per second to the relative phase; basis probabilities stay fixed. Current readings: Probability |0⟩: 71.1%; Probability |1⟩: 28.9%; Bloch (x, y, z): 0.78, 0.45, 0.42. All parameters are adjustable with the labeled controls below.xyz|0⟩|1⟩Basis probabilitiesP(0)71.1%P(1)28.9%
Bloch vector / P(0)P(1)Phase latitude
Probability |0⟩
71.1%
Probability |1⟩
28.9%
Bloch (x, y, z)
0.78, 0.45, 0.42
t = 0 s

A normalized two-level pure state, not an interacting field simulation. Playback adds one radian per second to the relative phase; basis probabilities stay fixed. Parameter changes pause playback and recompute the model at the current elapsed time. Reset restores both parameters and returns time to zero. Playback starts paused. Adjust either parameter, then choose Play or Step.

Look forThe lab's state angle enters through θ/2. It illustrates changed two-component projections, but has no density, matter Hamiltonian, resonance condition, or adiabatic propagation control.

Check your understanding

What additional statement is needed before using a resonance crossing to infer adiabatic conversion through varying density?

Try it yourself

Let sin⁡2θ=3/5\sin2\theta=3/5, cos⁡2θ=4/5\cos2\theta=4/5, and positive vacuum splitting. In one medium a = 8/5 for neutrinos. Compute the neutrino and antineutrino effective mixing prefactors, without predicting a baseline-dependent probability.

Take a moment to make a prediction or work it out on paper. Open a hint when you need one.

Give me a hint

For antineutrinos reverse a. The off-diagonal sine is unchanged in this real two-state model.

Compare with the solution

For neutrinos the denominator is (4/5−8/5)2+(3/5)2=1(4/5-8/5)^2+(3/5)^2=1, giving prefactor 9/259/25. For antineutrinos a becomes minus eight fifths, so the denominator is (12/5)2+(3/5)2=153/25(12/5)^2+(3/5)^2=153/25. The prefactor is therefore 9/153=1/179/153=1/17. These unequal prefactors are a matter effect even without an intrinsic CP phase. An actual transition probability still needs the appropriate matter gap, baseline, and energy through its sine-squared phase.

Take it with you

  • Coherent forward scattering adds a signed flavor potential without implying absorption.
  • Matter changes both effective mixing and oscillation wavelength.
  • Resonance, adiabatic following, ordering sensitivity, and intrinsic CP violation are different statements.

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