Questions: Neutrino Masses and Oscillations

3 questions to test your understanding

Score: 0 / 3
Question 1 Multiple Choice

A muon neutrino produced in the atmosphere with energy E = 1 GeV travels a distance L through the Earth. The probability of it being detected as a muon neutrino is approximately P(nu_mu -> nu_mu) = 1 - sin^2(2*theta_23) * sin^2(1.27 * Delta m^2_{32} * L/E), where Delta m^2 is in eV^2, L in km, and E in GeV. What physical effect causes this disappearance?

AThe neutrino decays into lighter particles during propagation
BThe neutrino flavor state nu_mu is a superposition of mass eigenstates nu_2 and nu_3, which propagate with slightly different phases (because they have different masses); after traveling distance L, the phase difference causes the flavor composition to change — the muon neutrino has partially transformed into a tau neutrino
CThe neutrino interacts with matter in the Earth and changes flavor
DThe neutrino loses energy and falls below the detection threshold
Question 2 Short Answer

Neutrino oscillation experiments measure mass-squared differences (Delta m^2_{21} ~ 7.5 x 10^{-5} eV^2 and |Delta m^2_{32}| ~ 2.5 x 10^{-3} eV^2) but not the absolute mass scale. Why can't oscillation experiments determine the individual neutrino masses?

Think about your answer, then reveal below.
Question 3 True / False

The solar neutrino problem -- a deficit of electron neutrinos from the Sun compared to theoretical predictions -- was resolved by the SNO experiment in 2001. SNO detected all three neutrino flavors and found that the total neutrino flux agreed with the solar model prediction.

TTrue
FFalse