Abstract
We compute the full $\mathcal{O}({\ensuremath{\alpha}}_{s})$ SUSY-QCD corrections to dark matter annihilation in the Higgs-funnel, resumming potentially large $\ensuremath{\mu}\mathrm{tan}\ensuremath{\beta}$ and ${A}_{b}$ contributions and keeping all finite $\mathcal{O}({m}_{b},s,1/{tan}^{2}\ensuremath{\beta})$ terms. We demonstrate numerically that these corrections strongly influence the extraction of SUSY mass parameters from cosmological data and must therefore be included in common analysis tools such as darksusy or micromegas.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
