Matches in SemOpenAlex for { <https://semopenalex.org/work/W4300656559> ?p ?o ?g. }
- W4300656559 abstract "Since the recent results of direct detection experiments at low mass, many authors have revisited the case of light (1--10) GeV weakly interacting massive particles. In particular, there have been a few attempts to explain the results from the DAMA/LIBRA, CDMS and/or CoGeNT experiments by invoking neutralinos lighter than 15 GeV. Here we show that in the minimal supersymmetric standard mode (MSSM), such light particles are completely ruled out by the Tevatron limits on the mass of the pseudoscalar Higgs. On the contrary, in the next-to-minimal supersymmetric standard model (NMSSM), we find that light neutralinos could still be viable candidates. In fact, in some cases, they may even have an elastic scattering cross section on nucleons in the range that is needed to explain either the DAMA/LIBRA, CoGeNT or CDMS recent results. Finally, we revisit the lowest limit on the neutralino mass in the MSSM and find that neutralinos should be heavier than $ensuremath{sim}28text{ }text{ }mathrm{GeV}$ to evade present experimental bounds." @default.
- W4300656559 created "2022-10-03" @default.
- W4300656559 creator A5005380504 @default.
- W4300656559 creator A5034956580 @default.
- W4300656559 creator A5042629460 @default.
- W4300656559 creator A5082125000 @default.
- W4300656559 creator A5085693529 @default.
- W4300656559 date "2010-12-27" @default.
- W4300656559 modified "2023-09-30" @default.
- W4300656559 title "Can neutralinos in the MSSM and NMSSM scenarios still be light?" @default.
- W4300656559 cites W1556403580 @default.
- W4300656559 cites W1967863527 @default.
- W4300656559 cites W1975574756 @default.
- W4300656559 cites W1986436958 @default.
- W4300656559 cites W1997339944 @default.
- W4300656559 cites W2006782725 @default.
- W4300656559 cites W2016310977 @default.
- W4300656559 cites W2029297603 @default.
- W4300656559 cites W2032823467 @default.
- W4300656559 cites W2036836787 @default.
- W4300656559 cites W2044649624 @default.
- W4300656559 cites W2046874742 @default.
- W4300656559 cites W2051170596 @default.
- W4300656559 cites W2068671056 @default.
- W4300656559 cites W2068736126 @default.
- W4300656559 cites W2068995455 @default.
- W4300656559 cites W2078266073 @default.
- W4300656559 cites W2088318212 @default.
- W4300656559 cites W2089002844 @default.
- W4300656559 cites W2094027398 @default.
- W4300656559 cites W2099449022 @default.
- W4300656559 cites W2105683921 @default.
- W4300656559 cites W2106624583 @default.
- W4300656559 cites W2110651113 @default.
- W4300656559 cites W2116293249 @default.
- W4300656559 cites W2123725669 @default.
- W4300656559 cites W2127331794 @default.
- W4300656559 cites W2142454375 @default.
- W4300656559 cites W2143701114 @default.
- W4300656559 cites W2146784204 @default.
- W4300656559 cites W2160253850 @default.
- W4300656559 cites W2165739256 @default.
- W4300656559 cites W2949841305 @default.
- W4300656559 cites W3098750462 @default.
- W4300656559 cites W3099247730 @default.
- W4300656559 cites W3102862371 @default.
- W4300656559 cites W3104412157 @default.
- W4300656559 cites W3104953676 @default.
- W4300656559 cites W3105509403 @default.
- W4300656559 cites W3106293764 @default.
- W4300656559 cites W3121360198 @default.
- W4300656559 cites W3135806615 @default.
- W4300656559 cites W4297156282 @default.
- W4300656559 doi "https://doi.org/10.1103/physrevd.82.115027" @default.
- W4300656559 hasPublicationYear "2010" @default.
- W4300656559 type Work @default.
- W4300656559 citedByCount "57" @default.
- W4300656559 countsByYear W43006565592012 @default.
- W4300656559 countsByYear W43006565592013 @default.
- W4300656559 countsByYear W43006565592014 @default.
- W4300656559 countsByYear W43006565592015 @default.
- W4300656559 countsByYear W43006565592016 @default.
- W4300656559 countsByYear W43006565592017 @default.
- W4300656559 countsByYear W43006565592018 @default.
- W4300656559 countsByYear W43006565592019 @default.
- W4300656559 countsByYear W43006565592020 @default.
- W4300656559 countsByYear W43006565592021 @default.
- W4300656559 countsByYear W43006565592022 @default.
- W4300656559 countsByYear W43006565592023 @default.
- W4300656559 crossrefType "journal-article" @default.
- W4300656559 hasAuthorship W4300656559A5005380504 @default.
- W4300656559 hasAuthorship W4300656559A5034956580 @default.
- W4300656559 hasAuthorship W4300656559A5042629460 @default.
- W4300656559 hasAuthorship W4300656559A5082125000 @default.
- W4300656559 hasAuthorship W4300656559A5085693529 @default.
- W4300656559 hasBestOaLocation W43006565592 @default.
- W4300656559 hasConcept C101454708 @default.
- W4300656559 hasConcept C101583263 @default.
- W4300656559 hasConcept C109214941 @default.
- W4300656559 hasConcept C116674579 @default.
- W4300656559 hasConcept C121332964 @default.
- W4300656559 hasConcept C158129726 @default.
- W4300656559 hasConcept C166957645 @default.
- W4300656559 hasConcept C172695262 @default.
- W4300656559 hasConcept C185544564 @default.
- W4300656559 hasConcept C200006409 @default.
- W4300656559 hasConcept C21265024 @default.
- W4300656559 hasConcept C2778144533 @default.
- W4300656559 hasConcept C40976572 @default.
- W4300656559 hasConcept C95457728 @default.
- W4300656559 hasConceptScore W4300656559C101454708 @default.
- W4300656559 hasConceptScore W4300656559C101583263 @default.
- W4300656559 hasConceptScore W4300656559C109214941 @default.
- W4300656559 hasConceptScore W4300656559C116674579 @default.
- W4300656559 hasConceptScore W4300656559C121332964 @default.
- W4300656559 hasConceptScore W4300656559C158129726 @default.
- W4300656559 hasConceptScore W4300656559C166957645 @default.
- W4300656559 hasConceptScore W4300656559C172695262 @default.
- W4300656559 hasConceptScore W4300656559C185544564 @default.
- W4300656559 hasConceptScore W4300656559C200006409 @default.