FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2952803852> ?p ?o ?g. }

• W2952803852 abstract "We discuss the extent to which models of Weakly Interacting Massive Particle (WIMP) Dark Matter (DM) at and above the electroweak scale can be probed conclusively in future high energy and astroparticle physics experiments. We consider simplified models with bino-like dark matter and slepton-like coannihilation partners, and find that perturbative models yield the observed relic abundance up to at least 10 TeV. We emphasise that coannihilation can either increase or decrease the dark matter relic abundance. We compute the sensitivity of direct detection experiments to DM-nucleus scattering, consider indirect detection bounds and estimate the sensitivity of future proton colliders to slepton pair production. We find that current and future experiments will be able to probe the Dirac DM models up to at least 10 TeV. However, current and future searches will not be sensitive to models of Majorana dark matter for masses above 2 or 4 TeV, for one or ten coannihilation partners respectively, leaving around 70 % of the parameter space unconstrained. This demonstrates the need for new experimental ideas to access models of coannihilating Majorana dark matter." @default.
• W2952803852 created "2019-06-27" @default.
• W2952803852 creator A5020787240 @default.
• W2952803852 creator A5085387224 @default.
• W2952803852 date "2018-10-01" @default.
• W2952803852 modified "2023-09-26" @default.
• W2952803852 title "Leptonic WIMP coannihilation and the current dark matter search strategy" @default.
• W2952803852 cites W1933364091 @default.
• W2952803852 cites W1987435915 @default.
• W2952803852 cites W2013416637 @default.
• W2952803852 cites W2099725150 @default.
• W2952803852 cites W2110999179 @default.
• W2952803852 cites W2119625101 @default.
• W2952803852 cites W2124464017 @default.
• W2952803852 cites W2125449845 @default.
• W2952803852 cites W2131034562 @default.
• W2952803852 cites W2133715515 @default.
• W2952803852 cites W2150261371 @default.
• W2952803852 cites W2159938857 @default.
• W2952803852 cites W2165854509 @default.
• W2952803852 cites W2242731797 @default.
• W2952803852 cites W2258584306 @default.
• W2952803852 cites W2592020519 @default.
• W2952803852 cites W2606553439 @default.
• W2952803852 cites W2780166815 @default.
• W2952803852 cites W2949920378 @default.
• W2952803852 cites W2963376959 @default.
• W2952803852 cites W2964127341 @default.
• W2952803852 cites W2992592221 @default.
• W2952803852 cites W3084106382 @default.
• W2952803852 cites W3094773677 @default.
• W2952803852 cites W3098061607 @default.
• W2952803852 cites W3098307845 @default.
• W2952803852 cites W3098372271 @default.
• W2952803852 cites W3098475895 @default.
• W2952803852 cites W3098991547 @default.
• W2952803852 cites W3099587139 @default.
• W2952803852 cites W3099660382 @default.
• W2952803852 cites W3099757056 @default.
• W2952803852 cites W3100491724 @default.
• W2952803852 cites W3102198902 @default.
• W2952803852 cites W3102782745 @default.
• W2952803852 cites W3104866921 @default.
• W2952803852 cites W3105142934 @default.
• W2952803852 cites W3105283976 @default.
• W2952803852 cites W3121642222 @default.
• W2952803852 cites W3123750486 @default.
• W2952803852 cites W4250614887 @default.
• W2952803852 doi "https://doi.org/10.1007/jhep10(2018)187" @default.
• W2952803852 hasPublicationYear "2018" @default.
• W2952803852 type Work @default.
• W2952803852 sameAs 2952803852 @default.
• W2952803852 citedByCount "21" @default.
• W2952803852 countsByYear W29528038522018 @default.
• W2952803852 countsByYear W29528038522019 @default.
• W2952803852 countsByYear W29528038522020 @default.
• W2952803852 countsByYear W29528038522021 @default.
• W2952803852 countsByYear W29528038522022 @default.
• W2952803852 countsByYear W29528038522023 @default.
• W2952803852 crossrefType "journal-article" @default.
• W2952803852 hasAuthorship W2952803852A5020787240 @default.
• W2952803852 hasAuthorship W2952803852A5085387224 @default.
• W2952803852 hasBestOaLocation W29528038521 @default.
• W2952803852 hasConcept C101454708 @default.
• W2952803852 hasConcept C109214941 @default.
• W2952803852 hasConcept C113840448 @default.
• W2952803852 hasConcept C121332964 @default.
• W2952803852 hasConcept C159249277 @default.
• W2952803852 hasConcept C166957645 @default.
• W2952803852 hasConcept C168173289 @default.
• W2952803852 hasConcept C172790937 @default.
• W2952803852 hasConcept C17863212 @default.
• W2952803852 hasConcept C184748400 @default.
• W2952803852 hasConcept C186453547 @default.
• W2952803852 hasConcept C26405456 @default.
• W2952803852 hasConcept C2778144533 @default.
• W2952803852 hasConcept C2778761060 @default.
• W2952803852 hasConcept C2780397496 @default.
• W2952803852 hasConcept C40976572 @default.
• W2952803852 hasConcept C44870925 @default.
• W2952803852 hasConcept C57853336 @default.
• W2952803852 hasConcept C66157390 @default.
• W2952803852 hasConcept C78470386 @default.
• W2952803852 hasConcept C95457728 @default.
• W2952803852 hasConceptScore W2952803852C101454708 @default.
• W2952803852 hasConceptScore W2952803852C109214941 @default.
• W2952803852 hasConceptScore W2952803852C113840448 @default.
• W2952803852 hasConceptScore W2952803852C121332964 @default.
• W2952803852 hasConceptScore W2952803852C159249277 @default.
• W2952803852 hasConceptScore W2952803852C166957645 @default.
• W2952803852 hasConceptScore W2952803852C168173289 @default.
• W2952803852 hasConceptScore W2952803852C172790937 @default.
• W2952803852 hasConceptScore W2952803852C17863212 @default.
• W2952803852 hasConceptScore W2952803852C184748400 @default.
• W2952803852 hasConceptScore W2952803852C186453547 @default.
• W2952803852 hasConceptScore W2952803852C26405456 @default.
• W2952803852 hasConceptScore W2952803852C2778144533 @default.
• W2952803852 hasConceptScore W2952803852C2778761060 @default.
• W2952803852 hasConceptScore W2952803852C2780397496 @default.
• W2952803852 hasConceptScore W2952803852C40976572 @default.

• next