4.5 Article

Dark matter in the type Ib seesaw model

Journal

JOURNAL OF HIGH ENERGY PHYSICS
Volume -, Issue 5, Pages -

Publisher

SPRINGER
DOI: 10.1007/JHEP05(2021)129

Keywords

Cosmology of Theories beyond the SM; Neutrino Physics

Funding

  1. program PRIN 2017 - Italian Ministero dell'Universita e della Ricerca (MUR) [2017W4HA7S]
  2. research project TAsP (Theoretical Astroparticle Physics) - Istituto Nazionale di Fisica Nucleare (INFN)
  3. Chinese Scholarship Council (CSC) [201809210011, [2018]3101, [2019]536]
  4. STFC Consolidated Grant [ST/L000296/1]
  5. European Union's Horizon 2020 Research and Innovation programme under Marie Sklodowska-Curie grant agreement HIDDeN European ITN project [H2020-MSCA-ITN-2019//860881-HIDDeN]

Ask authors/readers for more resources

This paper presents a minimal type Ib seesaw model and proposes an extension introducing dark matter into the model, exploring the parameter space for dark matter production. The connection between dark matter production and laboratory experiments is discussed, especially in relation to the mixing between standard model neutrinos and heavy neutrinos. Parameters related to dark matter production are constrained by experimental results and can be tested further in future experiments such as SHiP.
We consider a minimal type Ib seesaw model where the effective neutrino mass operator involves two different Higgs doublets, and the two right-handed neutrinos form a heavy Dirac mass. We propose a minimal dark matter extension of this model, in which the Dirac heavy neutrino is coupled to a dark Dirac fermion and a dark complex scalar field, both charged under a discrete Z(2) symmetry, where the lighter of the two is a dark matter candidate. Focussing on the fermionic dark matter case, we explore the parameter space of the seesaw Yukawa couplings, the neutrino portal couplings and dark scalar to dark fermion mass ratio, where correct dark matter relic abundance can be produced by the freeze-in mechanism. By considering the mixing between the standard model neutrinos and the heavy neutrino, we build a connection between the dark matter production and current laboratory experiments ranging from collider to lepton flavour violating experiments. For a GeV mass heavy neutrino, the parameters related to dark matter production are constrained by the experimental results directly and can be further tested by future experiments such as SHiP.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.5
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available