pith. sign in

arxiv: hep-ph/0010117 · v2 · submitted 2000-10-11 · ✦ hep-ph

Remarks on models with singlet neutrino in large extra dimensions

classification ✦ hep-ph
keywords modelsneutrinodimensionsextragammagravityminimalneutrinos
0
0 comments X
read the original abstract

Small Dirac masses for neutrinos are natural in models with singlet fermions in large extra dimensions with quantum gravity scale M_{\ast} \sim 1- 100 TeV. We study two modifications of the minimal model in order to obtain the mass scale relevant for atmospheric neutrino oscillations with at most O(1) higher-dimensional Yukawa couplings and with M_{\ast} \sim a few TeV. 1) In models with singlet fermions in smaller number of extra dimensions than gravity, we find that the effects on BR (\mu \to e \gamma) and on charged-current universality in \pi^- \to e \bar{\nu}, \mu \bar{\nu} decays are suppressed as compared to that in the minimal model with neutrino and gravity in the same space. 2) If small Dirac masses for the singlets are added along with lepton number violating couplings, then the mass scales and mixing angles for neutrino oscillations can be different from those relevant for \mu \to e \gamma and \pi^- \to e \bar{\nu}, \mu \bar{\nu}. Thus, in both modified models the constraints on M_{\ast} from BR (\mu \to e \gamma) and \pi^- \to e \bar{\nu}, \mu \bar{\nu} decays can be significantly relaxed. Furthermore, constraints from supernova 1987a strongly disfavor oscillations of active neutrinos to sterile neutrinos in both the minimal and the modified models.

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. Dark Dimension Right-handed Neutrinos Confronted with Long-Baseline Oscillation Experiments

    hep-ph 2026-01 unverdicted novelty 3.0

    Dark dimension right-handed neutrino models are confronted with T2K and NOvA long-baseline oscillation data, yielding exclusion limits on model parameters while remaining compatible with standard three-neutrino oscillations.