Research pillar · Informs Φ(E,θ,t), σ(E)

Neutrino Physics

Oscillation, solar and atmospheric measurements, and coherent scattering established neutrinos as real, massive and abundant. This pillar underwrites the flux density Φ(E,θ,t) and the coupling cross-section σ(E).

Deep-dive papers

Supporting literature

  • Freedman, D. Z. (1974). Coherent effects of a weak neutral current. Physical Review D 9, 1389. doi:10.1103/PhysRevD.9.1389 ↗ First prediction of coherent elastic neutrino–nucleus scattering (CEνNS).
  • COHERENT Collaboration (Akimov, D. et al.) (2017). Observation of coherent elastic neutrino–nucleus scattering. Science 357, 1123–1126. doi:10.1126/science.aao0990 ↗ First experimental confirmation of CEνNS, above six sigma.
  • COHERENT Collaboration (Akimov, D. et al.) (2021). First measurement of coherent elastic neutrino–nucleus scattering on argon. Physical Review Letters 126, 012002. doi:10.1103/PhysRevLett.126.012002 ↗ Independent confirmation of CEνNS on a second target nucleus.
  • Super-Kamiokande Collaboration (Fukuda, Y. et al.) (1998). Evidence for oscillation of atmospheric neutrinos. Physical Review Letters 81, 1562–1567. doi:10.1103/PhysRevLett.81.1562 ↗ First compelling evidence that neutrinos oscillate and therefore have mass.
  • SNO Collaboration (Ahmad, Q. R. et al.) (2002). Direct evidence for neutrino flavor transformation from neutral-current interactions. Physical Review Letters 89, 011301. doi:10.1103/PhysRevLett.89.011301 ↗ Measured the total solar-neutrino flux across all flavours, confirming the solar model.
  • Kajita, T. (2016). Nobel Lecture: discovery of atmospheric neutrino oscillations. Reviews of Modern Physics 88, 030501. doi:10.1103/RevModPhys.88.030501 ↗ Nobel laureate's own account of the atmospheric-oscillation discovery.
  • McDonald, A. B. (2016). Nobel Lecture: the Sudbury Neutrino Observatory — observation of flavor change for solar neutrinos. Reviews of Modern Physics 88, 030502. doi:10.1103/RevModPhys.88.030502 ↗ Companion Nobel lecture on the solar-neutrino flavour-change result.
  • NOvA Collaboration (Acero, M. A. et al.) (2022). Improved measurement of neutrino oscillation parameters by the NOvA experiment. Physical Review D 106, 032004. doi:10.1103/PhysRevD.106.032004 ↗ A recent long-baseline measurement refining the oscillation parameters.
  • Nobel Committee for Physics (2015). Scientific background: neutrino oscillations. Royal Swedish Academy of Sciences. link ↗ Establishes neutrino mass via oscillation — part of the framework's lineage.
  • Particle Data Group (Workman, R. L. et al.) (2022). Review of Particle Physics (cosmic-ray muon flux). Progress of Theoretical and Experimental Physics 2022, 083C01. doi:10.1093/ptep/ptac097 ↗ Reference values for one of the ambient input channels.
  • Formaggio, J. A. & Zeller, G. P. (2012). From eV to EeV: neutrino cross sections across energy scales. Reviews of Modern Physics 84, 1307. doi:10.1103/RevModPhys.84.1307 ↗ The standard review of measured neutrino cross-sections over all energies.
  • Scholberg, K. (2006). Prospects for measuring coherent elastic neutrino–nucleus scattering at a stopped-pion source. Physical Review D 73, 033005. doi:10.1103/PhysRevD.73.033005 ↗ Framed the experimental route later realised by COHERENT.
  • Sakurai, J. J. (1994). Modern Quantum Mechanics (rev. ed.). Addison-Wesley. Scattering amplitudes, partial waves and the optical theorem behind σ(E).
  • Mott, N. F. & Massey, H. S. W. (1965). The Theory of Atomic Collisions (3rd ed.). Oxford University Press. Foundational treatment of cross-sections and their energy dependence.

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