English

Unbroken B-L Symmetry

High Energy Physics - Phenomenology 2014-11-11 v2 Cosmology and Nongalactic Astrophysics High Energy Physics - Experiment

Abstract

The difference between baryon number B and lepton number L is the only anomaly-free global symmetry of the Standard Model, easily promoted to a local symmetry by introducing three right-handed neutrinos, which automatically make neutrinos massive. The non-observation of any (B-L)-violating processes leads us to scrutinize the case of unbroken gauged B-L; besides Dirac neutrinos, the model contains only three parameters, the gauge coupling strength g', the Stueckelberg mass MZM_{Z'}, and the kinetic mixing angle χ\chi. The new force could manifest itself at any scale, and we collect and derive bounds on g' over the entire testable range MZM_{Z'} = 0 - 101310^{13} eV, also of interest for the more popular case of spontaneously broken B-L or other new light forces. We show in particular that successful Big Bang nucleosynthesis provides strong bounds for masses 10 eV < MZM_{Z'} < 10 GeV due to resonant enhancement of the rate fˉfνˉRνR\bar{f} f \leftrightarrow \bar{\nu}_R \nu_R. The strongest limits typically arise from astrophysics and colliders, probing scales MZ/gM_{Z'}/g' from TeV up to 101010^{10} GeV.

Keywords

Cite

@article{arxiv.1408.6845,
  title  = {Unbroken B-L Symmetry},
  author = {Julian Heeck},
  journal= {arXiv preprint arXiv:1408.6845},
  year   = {2014}
}

Comments

8 pages, 3 figures; added reference, matches published version

R2 v1 2026-06-22T05:43:20.698Z