Matches in SemOpenAlex for { <https://semopenalex.org/work/W4386364893> ?p ?o ?g. }
Showing items 1 to 71 of
71
with 100 items per page.
- W4386364893 abstract "The flux of neutrinos from annihilation of gravitationally captured dark matter in the Sun has significant constraints from direct-detection experiments. However, these constraints are relaxed for inelastic dark matter as inelastic dark matter interactions generate less energetic nuclear recoils compared to elastic dark matter interactions. In this paper, we explore the possibility for large volume underground neutrino experiments to detect the neutrino flux from captured inelastic dark matter in the Sun. The neutrino spectrum has two components: a mono-energetic spike from pion and kaon decays at rest and a broad-spectrum shoulder from prompt primary meson decays. We focus on detecting the shoulder neutrinos from annihilation of hadrophilic inelastic dark matter with masses in the range 4-100 GeV and the mass splittings in up to 300 keV. We determine the event selection criterion for DUNE to identify GeV-scale muon neutrinos and anti-neutrinos originating from hadrophilic dark matter annihilation in the Sun, and forecast the sensitivity from contained events. We also map the current bounds from Super-Kamiokande and IceCube on elastic dark matter, as well as the projected limits from Hyper-Kamiokande, to the parameter space of inelastic dark matter. We find that there is a region of parameter space that these neutrino experiments are more sensitive to than the direct-detection experiments. For dark matter annihilation to heavy-quarks, the projected sensitivity of DUNE is weaker than current (future) Super (Hyper) Kamiokande experiments. However, for the light-quark channel, only the spike is observable and DUNE will be the most sensitive experiment." @default.
- W4386364893 created "2023-09-02" @default.
- W4386364893 creator A5062207150 @default.
- W4386364893 creator A5079824432 @default.
- W4386364893 creator A5081913495 @default.
- W4386364893 creator A5091276419 @default.
- W4386364893 date "2023-08-30" @default.
- W4386364893 modified "2023-09-28" @default.
- W4386364893 title "Neutrino constraints on inelastic dark matter captured in the Sun" @default.
- W4386364893 doi "https://doi.org/10.48550/arxiv.2308.16134" @default.
- W4386364893 hasPublicationYear "2023" @default.
- W4386364893 type Work @default.
- W4386364893 citedByCount "0" @default.
- W4386364893 crossrefType "posted-content" @default.
- W4386364893 hasAuthorship W4386364893A5062207150 @default.
- W4386364893 hasAuthorship W4386364893A5079824432 @default.
- W4386364893 hasAuthorship W4386364893A5081913495 @default.
- W4386364893 hasAuthorship W4386364893A5091276419 @default.
- W4386364893 hasBestOaLocation W43863648931 @default.
- W4386364893 hasConcept C103193775 @default.
- W4386364893 hasConcept C105795698 @default.
- W4386364893 hasConcept C107966497 @default.
- W4386364893 hasConcept C109214941 @default.
- W4386364893 hasConcept C113840448 @default.
- W4386364893 hasConcept C121332964 @default.
- W4386364893 hasConcept C159249277 @default.
- W4386364893 hasConcept C172790937 @default.
- W4386364893 hasConcept C185544564 @default.
- W4386364893 hasConcept C186453547 @default.
- W4386364893 hasConcept C201941533 @default.
- W4386364893 hasConcept C26405456 @default.
- W4386364893 hasConcept C33923547 @default.
- W4386364893 hasConcept C44870925 @default.
- W4386364893 hasConcept C57853336 @default.
- W4386364893 hasConcept C66157390 @default.
- W4386364893 hasConcept C73586568 @default.
- W4386364893 hasConcept C7602139 @default.
- W4386364893 hasConceptScore W4386364893C103193775 @default.
- W4386364893 hasConceptScore W4386364893C105795698 @default.
- W4386364893 hasConceptScore W4386364893C107966497 @default.
- W4386364893 hasConceptScore W4386364893C109214941 @default.
- W4386364893 hasConceptScore W4386364893C113840448 @default.
- W4386364893 hasConceptScore W4386364893C121332964 @default.
- W4386364893 hasConceptScore W4386364893C159249277 @default.
- W4386364893 hasConceptScore W4386364893C172790937 @default.
- W4386364893 hasConceptScore W4386364893C185544564 @default.
- W4386364893 hasConceptScore W4386364893C186453547 @default.
- W4386364893 hasConceptScore W4386364893C201941533 @default.
- W4386364893 hasConceptScore W4386364893C26405456 @default.
- W4386364893 hasConceptScore W4386364893C33923547 @default.
- W4386364893 hasConceptScore W4386364893C44870925 @default.
- W4386364893 hasConceptScore W4386364893C57853336 @default.
- W4386364893 hasConceptScore W4386364893C66157390 @default.
- W4386364893 hasConceptScore W4386364893C73586568 @default.
- W4386364893 hasConceptScore W4386364893C7602139 @default.
- W4386364893 hasLocation W43863648931 @default.
- W4386364893 hasOpenAccess W4386364893 @default.
- W4386364893 hasPrimaryLocation W43863648931 @default.
- W4386364893 hasRelatedWork W1595487980 @default.
- W4386364893 hasRelatedWork W1730956029 @default.
- W4386364893 hasRelatedWork W2009258843 @default.
- W4386364893 hasRelatedWork W2099448775 @default.
- W4386364893 hasRelatedWork W3098284633 @default.
- W4386364893 hasRelatedWork W3099074417 @default.
- W4386364893 hasRelatedWork W3101683297 @default.
- W4386364893 hasRelatedWork W3102172971 @default.
- W4386364893 hasRelatedWork W4309956472 @default.
- W4386364893 hasRelatedWork W4322717467 @default.
- W4386364893 isParatext "false" @default.
- W4386364893 isRetracted "false" @default.
- W4386364893 workType "article" @default.