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Cosmic rays, gamma rays and neutrinos from point sources

dc.contributor.authorTomozawa, Yukioen_US
dc.date.accessioned2011-11-15T16:06:12Z
dc.date.available2011-11-15T16:06:12Z
dc.date.issued1993-06-15en_US
dc.identifier.citationTomozawa, Yukio (1993). "Cosmic rays, gamma rays and neutrinos from point sources." AIP Conference Proceedings 276(1): 490-495. <http://hdl.handle.net/2027.42/87672>en_US
dc.identifier.otherAPCPCS-276-1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87672
dc.description.abstractThe suggestion has been made that the energy spectrum from point sources such as AGN (Active Galactic Nuclei) and GBHC (Galactic Black Hole Candidates) is universal, irrespective of the nature of the emitted particles. A comparison of the energy spectrum for cosmic rays at the source and γ‐rays from quasars obtained recently by CGRO (Compton Gamma Ray Observatory) indicates that the prediction is in agreement with the data in the average sense. This suggests that neutrinos from point sources should have a spectral index identical to that of γ‐rays for an individual point source. This prediction is also consistent with the recent observation of neutrinos by Kamiokande and IMB in which the ratio of νμ/νe is close to 1, instead of 2 as expected from atmospheric neutrinos. For a further test of the model, analysis of the time variation of γ‐ray spectra from quasars is suggested.en_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleCosmic rays, gamma rays and neutrinos from point sourcesen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumRandall Lab. of Physics, University of Michigan, Ann Arbor, Michigan 48109‐1120en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87672/2/490_1.pdf
dc.identifier.doi10.1063/1.43872en_US
dc.identifier.sourceThe seventh international symposium on very high energy cosmic‐ray interactionsen_US
dc.owningcollnamePhysics, Department of


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