2001/01/19 by V. A. Bednyakov, H. V. Klapdor‐Kleingrothaus, H. V. Klapdor-Kleingrothaus +2
Chemistry · Physics and Astronomy · #Annihilation #Boson #Chemistry #Dark Matter and Cosmic Phenomena #Elementary particle #Flux (metallurgy) #Higgs boson #Muon #Neutralino #Neutrino #Neutrino Physics Research #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Supersymmetry #hep-ph
paper · pdf · doi:10.1103/physrevd.64.075004
published as Phys.Rev. D64 (2001) 075004 · 10 pages, 4 figures. Talk given at Dark2000, Heidelberg, Germany, 10-15 July, 2000
arxiv created 2001/01/19 · openalex publication_date 2001/09/05 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We investigate the contribution of the minimal supersymmetric extension of the standard model Higgs bosons produced in the neutralino annihilation in the Earth and Sun to the total weakly interacting massive particles detection signal. We find that this contribution is important and results in a lower bound for the muon flux from the Sun of 10^\ensuremath-7--10^\ensuremath-8 m^\ensuremath-2 yr^\ensuremath-1 for neutralinos heavier than about 200 GeV. We notice that due to the SUSY charged Higgs bosons one can expect an energetic \ensuremathτ neutrino flux from the Sun at a level of 102 m^\ensuremath-2 yr^\ensuremath-1.