FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2034787735> ?p ?o ?g. }

• W2034787735 abstract "The recent observation by the PAMELA satellite of a rising positron fraction up to ∼100 GeV has triggered a considerable amount of putative interpretations in terms of dark matter (DM) annihilation or decay. Here, we make a critical reassessment of such a possibility, recalling the elementary conditions with respect to the standard astrophysical background that would make it likely, showing that they are not fulfilled. Likewise, we argue that, as now well accepted, DM would need somewhat contrived properties to contribute significantly to the observed positron signal, even when including e.g. clumpiness effects. This means that most of natural DM candidates arising in particle physics beyond the standard model are not expected to be observed in the cosmic antimatter spectrum, unfortunately. However, this does not prevent them from remaining excellent DM candidates, this only points towards the crucial need of developing much more complex detection strategies (multimessenger, multiwavelength, multiscale searches)." @default.
• W2034787735 created "2016-06-24" @default.
• W2034787735 creator A5019510510 @default.
• W2034787735 creator A5071247285 @default.
• W2034787735 creator A5081613664 @default.
• W2034787735 date "2010-01-01" @default.
• W2034787735 modified "2023-10-06" @default.
• W2034787735 title "Cosmic ray positron excess: is the dark matter solution a good bet?" @default.
• W2034787735 cites W1514857296 @default.
• W2034787735 cites W1623274452 @default.
• W2034787735 cites W1681318429 @default.
• W2034787735 cites W1969779370 @default.
• W2034787735 cites W1971277862 @default.
• W2034787735 cites W1988045362 @default.
• W2034787735 cites W1989512487 @default.
• W2034787735 cites W2010519206 @default.
• W2034787735 cites W2013416637 @default.
• W2034787735 cites W2016527243 @default.
• W2034787735 cites W2019889489 @default.
• W2034787735 cites W2020913145 @default.
• W2034787735 cites W2055046332 @default.
• W2034787735 cites W2056111576 @default.
• W2034787735 cites W2058899596 @default.
• W2034787735 cites W2094401251 @default.
• W2034787735 cites W2098710805 @default.
• W2034787735 cites W2107415832 @default.
• W2034787735 cites W2114603802 @default.
• W2034787735 cites W2115528245 @default.
• W2034787735 cites W2120574945 @default.
• W2034787735 cites W2122658693 @default.
• W2034787735 cites W2128476026 @default.
• W2034787735 cites W2129713777 @default.
• W2034787735 cites W2130927785 @default.
• W2034787735 cites W2132875692 @default.
• W2034787735 cites W2135403967 @default.
• W2034787735 cites W2136000363 @default.
• W2034787735 cites W2165070955 @default.
• W2034787735 cites W2986810904 @default.
• W2034787735 cites W3011160802 @default.
• W2034787735 cites W3041586415 @default.
• W2034787735 cites W3097984739 @default.
• W2034787735 cites W3098823536 @default.
• W2034787735 cites W3100110286 @default.
• W2034787735 cites W3100264914 @default.
• W2034787735 cites W3100762204 @default.
• W2034787735 cites W3101208491 @default.
• W2034787735 cites W3102921613 @default.
• W2034787735 cites W3105727495 @default.
• W2034787735 cites W3124821660 @default.
• W2034787735 doi "https://doi.org/10.1063/1.3462661" @default.
• W2034787735 hasPublicationYear "2010" @default.
• W2034787735 type Work @default.
• W2034787735 sameAs 2034787735 @default.
• W2034787735 citedByCount "1" @default.
• W2034787735 countsByYear W20347877352013 @default.
• W2034787735 crossrefType "proceedings-article" @default.
• W2034787735 hasAuthorship W2034787735A5019510510 @default.
• W2034787735 hasAuthorship W2034787735A5071247285 @default.
• W2034787735 hasAuthorship W2034787735A5081613664 @default.
• W2034787735 hasBestOaLocation W20347877352 @default.
• W2034787735 hasConcept C101454708 @default.
• W2034787735 hasConcept C109214941 @default.
• W2034787735 hasConcept C110916831 @default.
• W2034787735 hasConcept C111309251 @default.
• W2034787735 hasConcept C121332964 @default.
• W2034787735 hasConcept C147120987 @default.
• W2034787735 hasConcept C159249277 @default.
• W2034787735 hasConcept C166957645 @default.
• W2034787735 hasConcept C179203047 @default.
• W2034787735 hasConcept C184748400 @default.
• W2034787735 hasConcept C185544564 @default.
• W2034787735 hasConcept C194172872 @default.
• W2034787735 hasConcept C201941533 @default.
• W2034787735 hasConcept C202100949 @default.
• W2034787735 hasConcept C2985595821 @default.
• W2034787735 hasConcept C40976572 @default.
• W2034787735 hasConcept C44870925 @default.
• W2034787735 hasConcept C59375849 @default.
• W2034787735 hasConcept C95457728 @default.
• W2034787735 hasConceptScore W2034787735C101454708 @default.
• W2034787735 hasConceptScore W2034787735C109214941 @default.
• W2034787735 hasConceptScore W2034787735C110916831 @default.
• W2034787735 hasConceptScore W2034787735C111309251 @default.
• W2034787735 hasConceptScore W2034787735C121332964 @default.
• W2034787735 hasConceptScore W2034787735C147120987 @default.
• W2034787735 hasConceptScore W2034787735C159249277 @default.
• W2034787735 hasConceptScore W2034787735C166957645 @default.
• W2034787735 hasConceptScore W2034787735C179203047 @default.
• W2034787735 hasConceptScore W2034787735C184748400 @default.
• W2034787735 hasConceptScore W2034787735C185544564 @default.
• W2034787735 hasConceptScore W2034787735C194172872 @default.
• W2034787735 hasConceptScore W2034787735C201941533 @default.
• W2034787735 hasConceptScore W2034787735C202100949 @default.
• W2034787735 hasConceptScore W2034787735C2985595821 @default.
• W2034787735 hasConceptScore W2034787735C40976572 @default.
• W2034787735 hasConceptScore W2034787735C44870925 @default.
• W2034787735 hasConceptScore W2034787735C59375849 @default.
• W2034787735 hasConceptScore W2034787735C95457728 @default.
• W2034787735 hasLocation W20347877351 @default.
• W2034787735 hasLocation W20347877352 @default.

• next