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 Tools annual

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 Tools monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

The lightest $Z_2$ odd particle in the scotogenic model, referred to asscotogenic dark matter (DM), is a widely studied candidate for DM. Thisscotogenic DM is generated through well-known thermal processes as well as viathe evaporation of primordial black holes (PBHs). Recent reports suggested thatthe curvature fluctuations of PBHs during an epoch dominated by these entitiesin the early universe can serve as the source of so-called inducedgravitational waves (GWs). In this study, we demonstrate that stringentconstraints on the mass of scotogenic DM and PBHs can be obtained through thedetection of induced GWs using future detectors.

Constraining scotogenic dark matter and primordial black holes using gravitational waves