English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Non-zero neutrino mass and dark matter cast a shadow over the success of theStandard Model (SM) of Particle Physics. The most straightforward extension ofthe SM to explain these two phenomena is the Scotogenic model, where the SMparticle spectrum extends with three isospin singlet right-handed neutrinos andone doublet scalar while all of these being odd under $Z_2$ symmetry. In thiswork, we have considered the lightest right-handed neutrino as the dark mattercandidate and freeze-out mechanism for producing observed dark matter relicdensity. The observed dark matter relic density, neutrino oscillation data andlimits on the charged lepton flavor violation processes impose severeconstraints on the model. After satisfying all the constraints, we study thecollider signatures of the model at the proposed lepton collider experiments.

Radiative Neutrino Mass with Electroweak Scale Majorana Dark Matter in Scotogenic Model