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 Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We study direct detection bounds on cosmic ray-upscattered dark matter insimplified models including light mediators. We find that the energy dependencein the scattering cross section is significant, and produces stronger boundsthan previously found (which assumed constant cross sections) by many orders ofmagnitude at low DM mass. Finally, we compute the "neutrino-floor" that willlimit future direct detection searches for cosmic ray-upscattered dark matter.While we focus on vector interactions for illustration, we emphasize that theenergy dependence is critical in determining accurate bounds on any particlephysics model of Dark Matter-CR interactions from experimental data on thisscenario.

Bounds on Cosmic Ray-Boosted Dark Matter in Simplified Models and its Corresponding Neutrino-Floor