English

Modified majoron model for cosmological anomalies

High Energy Physics - Phenomenology 2021-07-21 v2 Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena

Abstract

The vacuum expectation value vsv_s of a Higgs triplet field Δ\Delta carrying two units of lepton number LL induces neutrino masses vs\propto v_s. The neutral component of Δ\Delta gives rise to two Higgs particles, a pseudoscalar AA and a scalar SS. The most general renormalizable Higgs potential VV for Δ\Delta and the Standard-Model Higgs doublet Φ\Phi does not permit the possibility that the mass of either AA or SS is small, of order vsv_s, while the other mass is heavy enough to forbid the decay ZASZ\to A S to comply with LEP 1 data. We present a model with additional dimension-6 terms in VV, in which this feature is absent and either AA or SS can be chosen light. Subsequently we propose the model as a remedy to cosmological anomalies, namely the tension between observed and predicted tensor-to-scalar mode ratios in the cosmic microwave background and the different values of the Hubble constant measured at different cosmological scales. Furthermore, if Δ\Delta dominantly couples to the third-generation doublet Lτ=(ντ,τ)L_\tau=(\nu_\tau,\tau), the deficit of ντ\nu_\tau events at IceCube can be explained. The singly and doubly charged triplet Higgs bosons are lighter than 280 GeV and 400 GeV respectively, and could be found at the LHC.

Keywords

Cite

@article{arxiv.2005.13280,
  title  = {Modified majoron model for cosmological anomalies},
  author = {Gabriela Barenboim and Ulrich Nierste},
  journal= {arXiv preprint arXiv:2005.13280},
  year   = {2021}
}

Comments

5 pages, 2 figures. More pedagogical explanation of model and UV completion (with extra figure), typos fixed

R2 v1 2026-06-23T15:50:57.269Z