Matches in SemOpenAlex for { <https://semopenalex.org/work/W1966771823> ?p ?o ?g. }
- W1966771823 endingPage "250" @default.
- W1966771823 startingPage "243" @default.
- W1966771823 abstract "The short review of theoretical aspects of ultra high energy (UHE) neutrinos. The accelerator sources, such as Supernovae remnants, Gamma Ray Bursts, AGN etc are discussed. The top-down sources include Topological Defects (TDs), Superheavy Dark Matter (SHDM) and Mirror Matter. The diffuse fluxes are considered accordingly as that of cosmogenic and top-down neutrinos. Much attention is given to the cascade upper limit to the diffuse neutrino fluxes in the light of Fermi-LAT data on diffuse high energy gamma radiation. This is most general and rigorous upper limit, valid for both cosmogenic and top-down models. At present upper limits from many detectors are close to the cascade upper limit, and 5 yr IceCube upper limit will be well below it." @default.
- W1966771823 created "2016-06-24" @default.
- W1966771823 creator A5070926062 @default.
- W1966771823 date "2012-08-01" @default.
- W1966771823 modified "2023-09-25" @default.
- W1966771823 title "High Energy Neutrino Astronomy" @default.
- W1966771823 cites W142989537 @default.
- W1966771823 cites W1630306512 @default.
- W1966771823 cites W1647766962 @default.
- W1966771823 cites W1967351450 @default.
- W1966771823 cites W1968174670 @default.
- W1966771823 cites W1970214299 @default.
- W1966771823 cites W1972776542 @default.
- W1966771823 cites W1974694458 @default.
- W1966771823 cites W1974848915 @default.
- W1966771823 cites W1975292641 @default.
- W1966771823 cites W1975906172 @default.
- W1966771823 cites W1976447431 @default.
- W1966771823 cites W1979847599 @default.
- W1966771823 cites W1981254463 @default.
- W1966771823 cites W1983278356 @default.
- W1966771823 cites W1998440977 @default.
- W1966771823 cites W2012922008 @default.
- W1966771823 cites W2016027253 @default.
- W1966771823 cites W2020834529 @default.
- W1966771823 cites W2021800636 @default.
- W1966771823 cites W2026678930 @default.
- W1966771823 cites W2030855972 @default.
- W1966771823 cites W2034776871 @default.
- W1966771823 cites W2037771611 @default.
- W1966771823 cites W2040363577 @default.
- W1966771823 cites W2040619705 @default.
- W1966771823 cites W2053003611 @default.
- W1966771823 cites W2061202128 @default.
- W1966771823 cites W2064491231 @default.
- W1966771823 cites W2066431612 @default.
- W1966771823 cites W2069926710 @default.
- W1966771823 cites W2081599663 @default.
- W1966771823 cites W2085023683 @default.
- W1966771823 cites W2086411872 @default.
- W1966771823 cites W2087508032 @default.
- W1966771823 cites W2088341276 @default.
- W1966771823 cites W2089313699 @default.
- W1966771823 cites W2104948382 @default.
- W1966771823 cites W2114752987 @default.
- W1966771823 cites W2132977758 @default.
- W1966771823 cites W2142689048 @default.
- W1966771823 cites W2147217332 @default.
- W1966771823 cites W2149383327 @default.
- W1966771823 cites W2157338954 @default.
- W1966771823 cites W2165977705 @default.
- W1966771823 cites W246292695 @default.
- W1966771823 cites W2986810904 @default.
- W1966771823 cites W3122948819 @default.
- W1966771823 cites W2062249906 @default.
- W1966771823 doi "https://doi.org/10.1016/j.nuclphysbps.2012.09.039" @default.
- W1966771823 hasPublicationYear "2012" @default.
- W1966771823 type Work @default.
- W1966771823 sameAs 1966771823 @default.
- W1966771823 citedByCount "3" @default.
- W1966771823 countsByYear W19667718232017 @default.
- W1966771823 countsByYear W19667718232019 @default.
- W1966771823 countsByYear W19667718232020 @default.
- W1966771823 crossrefType "journal-article" @default.
- W1966771823 hasAuthorship W1966771823A5070926062 @default.
- W1966771823 hasBestOaLocation W19667718232 @default.
- W1966771823 hasConcept C107966497 @default.
- W1966771823 hasConcept C121332964 @default.
- W1966771823 hasConcept C127592171 @default.
- W1966771823 hasConcept C1276947 @default.
- W1966771823 hasConcept C132221716 @default.
- W1966771823 hasConcept C134306372 @default.
- W1966771823 hasConcept C151201525 @default.
- W1966771823 hasConcept C159249277 @default.
- W1966771823 hasConcept C185544564 @default.
- W1966771823 hasConcept C185592680 @default.
- W1966771823 hasConcept C186453547 @default.
- W1966771823 hasConcept C186769553 @default.
- W1966771823 hasConcept C33923547 @default.
- W1966771823 hasConcept C34146451 @default.
- W1966771823 hasConcept C43617362 @default.
- W1966771823 hasConcept C44870925 @default.
- W1966771823 hasConcept C56623721 @default.
- W1966771823 hasConceptScore W1966771823C107966497 @default.
- W1966771823 hasConceptScore W1966771823C121332964 @default.
- W1966771823 hasConceptScore W1966771823C127592171 @default.
- W1966771823 hasConceptScore W1966771823C1276947 @default.
- W1966771823 hasConceptScore W1966771823C132221716 @default.
- W1966771823 hasConceptScore W1966771823C134306372 @default.
- W1966771823 hasConceptScore W1966771823C151201525 @default.
- W1966771823 hasConceptScore W1966771823C159249277 @default.
- W1966771823 hasConceptScore W1966771823C185544564 @default.
- W1966771823 hasConceptScore W1966771823C185592680 @default.
- W1966771823 hasConceptScore W1966771823C186453547 @default.
- W1966771823 hasConceptScore W1966771823C186769553 @default.
- W1966771823 hasConceptScore W1966771823C33923547 @default.
- W1966771823 hasConceptScore W1966771823C34146451 @default.
- W1966771823 hasConceptScore W1966771823C43617362 @default.