FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1778333042> ?p ?o ?g. }

• W1778333042 abstract "The latest IceCube data suggest that the all-flavor cosmic neutrino flux may be as large as 10^-7 GeV/cm^2/s/sr around 30 TeV. We show that, if sources of the TeV-PeV neutrinos are transparent to gamma rays with respect to two-photon annihilation, strong tensions with the isotropic diffuse gamma-ray background measured by Fermi are unavoidable, independently of the production mechanism. We further show that, if the IceCube neutrinos have a photohadronic (pgamma) origin, the sources are expected to be opaque to 1-100 GeV gamma rays. With these general multimessenger arguments, we find that the latest data suggest a population of cosmic-ray accelerators hidden in GeV-TeV gamma rays as a neutrino origin. Searches for x-ray and MeV gamma-ray counterparts are encouraged, and TeV-PeV neutrinos themselves will serve as special probes of dense source environments." @default.
• W1778333042 created "2016-06-24" @default.
• W1778333042 creator A5004308379 @default.
• W1778333042 creator A5007068870 @default.
• W1778333042 creator A5085798900 @default.
• W1778333042 date "2016-02-18" @default.
• W1778333042 modified "2023-10-14" @default.
• W1778333042 title "Hidden Cosmic-Ray Accelerators as an Origin of TeV-PeV Cosmic Neutrinos" @default.
• W1778333042 cites W1530183786 @default.
• W1778333042 cites W1560975535 @default.
• W1778333042 cites W1572313312 @default.
• W1778333042 cites W1575265700 @default.
• W1778333042 cites W1647766962 @default.
• W1778333042 cites W1669035376 @default.
• W1778333042 cites W1680468302 @default.
• W1778333042 cites W1685552061 @default.
• W1778333042 cites W1700467429 @default.
• W1778333042 cites W1703498629 @default.
• W1778333042 cites W1867972542 @default.
• W1778333042 cites W1886185970 @default.
• W1778333042 cites W1931086765 @default.
• W1778333042 cites W1947464863 @default.
• W1778333042 cites W1953981590 @default.
• W1778333042 cites W1968990802 @default.
• W1778333042 cites W1971214100 @default.
• W1778333042 cites W1980042166 @default.
• W1778333042 cites W1981037855 @default.
• W1778333042 cites W1984598861 @default.
• W1778333042 cites W1990948132 @default.
• W1778333042 cites W1992214959 @default.
• W1778333042 cites W1992960149 @default.
• W1778333042 cites W1995305986 @default.
• W1778333042 cites W1998290692 @default.
• W1778333042 cites W1999663363 @default.
• W1778333042 cites W1999798079 @default.
• W1778333042 cites W2003360851 @default.
• W1778333042 cites W2003518429 @default.
• W1778333042 cites W2006171159 @default.
• W1778333042 cites W2006876891 @default.
• W1778333042 cites W2007403924 @default.
• W1778333042 cites W2015750713 @default.
• W1778333042 cites W2020489162 @default.
• W1778333042 cites W2020834529 @default.
• W1778333042 cites W2022539726 @default.
• W1778333042 cites W2029010726 @default.
• W1778333042 cites W2038561135 @default.
• W1778333042 cites W2040923262 @default.
• W1778333042 cites W2043129109 @default.
• W1778333042 cites W2050276909 @default.
• W1778333042 cites W2050755767 @default.
• W1778333042 cites W2051627582 @default.
• W1778333042 cites W2056832236 @default.
• W1778333042 cites W2063384422 @default.
• W1778333042 cites W2073750316 @default.
• W1778333042 cites W2083055131 @default.
• W1778333042 cites W2088107666 @default.
• W1778333042 cites W2089091546 @default.
• W1778333042 cites W2096521050 @default.
• W1778333042 cites W2099604834 @default.
• W1778333042 cites W2111348189 @default.
• W1778333042 cites W2117778658 @default.
• W1778333042 cites W2119729316 @default.
• W1778333042 cites W2120758231 @default.
• W1778333042 cites W2123046843 @default.
• W1778333042 cites W2126588894 @default.
• W1778333042 cites W2136262096 @default.
• W1778333042 cites W2151427614 @default.
• W1778333042 cites W2156054267 @default.
• W1778333042 cites W2167428831 @default.
• W1778333042 cites W2190595503 @default.
• W1778333042 cites W2225354912 @default.
• W1778333042 cites W2336225215 @default.
• W1778333042 cites W2592598485 @default.
• W1778333042 cites W2949096495 @default.
• W1778333042 cites W2949416507 @default.
• W1778333042 cites W2963177337 @default.
• W1778333042 cites W2963641739 @default.
• W1778333042 cites W3099714470 @default.
• W1778333042 cites W3100242372 @default.
• W1778333042 cites W3101198806 @default.
• W1778333042 cites W3101677647 @default.
• W1778333042 cites W3102729550 @default.
• W1778333042 cites W3103211113 @default.
• W1778333042 cites W3104561109 @default.
• W1778333042 cites W3104856020 @default.
• W1778333042 cites W3104882501 @default.
• W1778333042 cites W3105676301 @default.
• W1778333042 cites W3105987168 @default.
• W1778333042 cites W3106087154 @default.
• W1778333042 cites W3122118387 @default.
• W1778333042 cites W2010166940 @default.
• W1778333042 doi "https://doi.org/10.1103/physrevlett.116.071101" @default.
• W1778333042 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/26943524" @default.
• W1778333042 hasPublicationYear "2016" @default.
• W1778333042 type Work @default.
• W1778333042 sameAs 1778333042 @default.
• W1778333042 citedByCount "222" @default.
• W1778333042 countsByYear W17783330422016 @default.
• W1778333042 countsByYear W17783330422017 @default.
• W1778333042 countsByYear W17783330422018 @default.

• next