pith. sign in

arxiv: hep-ph/9604403 · v1 · pith:YVOF6NKHnew · submitted 1996-04-25 · ✦ hep-ph · astro-ph· gr-qc

Neutrino Oscillations in Strong Gravitational Fields

Dardo P\'iriz , Mou Roy , Jos\'e Wudka This is my paper
classification ✦ hep-ph astro-phgr-qc
keywords gravitationaleffectsfieldsneutrinoneutrinososcillationspresencestrong
0
0 comments X
read the original abstract

Neutrino oscillations in the presence of strong gravitational fields are studied. We look at very high energy neutrinos ($\sim $1 TeV) emanating from Active Galactic Nuclei (AGN). It is observed that spin flavor resonant transitions of such neutrinos may occur in the vicinity of AGN due to {\it gravitational} effects and due to the presence of a large magnetic field ($\sim $1 Tesla). A point to note is that matter effects (normal MSW transitions) become negligible in comparison o gravitational effects in our scenario.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Mass Varying Neutrino Oscillation in Teleparallel Gravity

    hep-ph 2026-06 unverdicted novelty 4.0

    Torsion-coupled scalar in teleparallel gravity induces density-dependent neutrino masses that alter MSW resonance and yield constraints on coupling parameters from Super-Kamiokande, Borexino and SNO data.