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

In this paper we perform for the first time an in-depth analysis ofthe spectra in the phenomenological supersymmetric Standard Model thatsimultaneously offer an explanation for the   (g-2)_{\mu}    (  g  −  2   )  μdiscrepancy    \Delta a_{\mu}    Δ   a  μ,result in the right dark-matter relic density   \Omega_{DM} h^2Ω   D  Mh  2and are minimally fine-tuned. The resulting spectra may be obtainedfrom [1]. To discuss the experimental exclusion potential for ourmodels, we analyse the resulting LHC phenomenology as well as thesensitivity of dark-matter direct detection experiments to thesespectra. We find that the latter type of experiments with sensitivity tothe spin-dependent dark-matter–nucleon scattering cross section   \sigma_{SD,p}    σ   S  D  ,  pwill probe all of our found solutions.

Dark matter, fine-tuning and (g-2)_{\mu} in the pMSSM