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

The vanishing of the Higgs quartic coupling at a high energy scale may beexplained by Intermediate Scale Supersymmetry, where supersymmetry breaks at$(10^9$-$10^{12})$ GeV. The possible range of supersymmetry breaking scales canbe narrowed down by precise measurements of the top quark mass and the strongcoupling constant. On the other hand, nuclear recoil experiments can probeHiggsino or sneutrino dark matter up to a mass of $10^{12}$ GeV. We derive thecorrelation between the dark matter mass and precision measurements of standardmodel parameters, including supersymmetric threshold corrections. The darkmatter mass is bounded from above as a function of the top quark mass and thestrong coupling constant. The top quark mass and the strong coupling constantare bounded from above and below respectively for a given dark matter mass. Wealso discuss how the observed dark matter abundance can be explained byfreeze-out or freeze-in during a matter-dominated era after inflation, with theinflaton condensate being dissipated by thermal effects.

Dark Matter Detection, Standard Model Parameters, and Intermediate Scale Supersymmetry