Publications (5)
Factorization vs. Non-Factorization: S-Matrix Corrections for Precision Neutrino Physics
D. Delepine, A. Yebra
The standard treatment of neutrino oscillations usually relies on factorization which assumes neutrino production, propagation, and detection are independent processes. As a conseq…
Distinguishing Dirac and Majorana neutrinos with astrophysical fluxes
J. Barranco, D. Delepine, M. Napsuciale +1
Massive neutrinos can have helicity . Neutrino helicity changes when the neutrino interacts with an external magnetic field and it is possible that the left-h…
The Dirac Majorana Confusion Theorem in the Presence of Flavor-Changing Neutral Currents: A CP-Filter Mechanism
David Delepine, A. Yebra
The Practical Dirac Majorana Confusion Theorem(PDMCT) asserts that phenomenological differences between Dirac and Majorana neutrinos are kinematically suppressed by (neutrino mass/…
Solar Flares as a Probe of Neutrino Nature: Distinguishing Dirac and Majorana via Resonant Spin-Flavor Precession
D. Delepine, A. Yebra
Resonant Spin-Flavor Precession (RSFP) of solar neutrinos is studied using the quantum density matrix formalism, explicitly taking into account collisional decoherence and solar ma…
Distinguishing Dirac and Majorana Neutrinos: Resonant Spin-Flavor Precession of GeV-Scale Astrophysical Transients
D. Delepine, A. Yebra
We present a unified formalism to study the Resonant Spin-Flavor Precession (RSFP) of high-energy ( GeV) transient astrophysical neutrinos as a probe of their fundamental D…