25–28 Sept 2018
DESY Hamburg
Europe/Berlin timezone

Leptogenesis and light DM in the Scotogenic Model

27 Sept 2018, 16:35
15m
Seminar room 4a (SR 4a) (DESY Hamburg)

Seminar room 4a (SR 4a)

DESY Hamburg

Cosmology & Astroparticle Physics Parallel Session: Cosmo 5

Speaker

Mr Sven Baumholzer (Johannes Gutenberg-Universitaet Mainz)

Description

This talk is based on [arXiv:1806.06864][1]. We will present an extension of the Standard Model, including three right-handed neutrinos $N_i$ and a new Higgs doublet $\Sigma$, all charged under a exact $Z_2$ parity symmetry. This framework is also known as the "Scotogenic model". We will discuss how one can realize the SM neutrino masses + mixing angles and also generate the observed DM density and the baryon asymmetry of the universe (BAU) in this model framework. The DM is suppossed to be a keV right-handed neutrino which is mainly produced via a freeze-in mechanism given by decays of the new scalars. The BAU is generated via Leptogenesis, which relies on two CP violating mechanisms: 1) Oscillations among the RH neutrinos 2) Heavy scalar decays $\Sigma \to N L$ Combining everything, we found a quite constraint parameter region which places an upper bound on the allowed DM mass of $\mathcal{O} (20)\,\mathrm{keV}$ at most. [1]: https://arxiv.org/abs/1806.06864 "arXiv:1806.06864"

Primary author

Mr Sven Baumholzer (Johannes Gutenberg-Universitaet Mainz)

Co-authors

Prof. Pedro Schwaller (CERN) Mr Vedran Brdar (MPIK Heidelberg)

Presentation materials