High-energy neutrinos from astrophysical accelerators of cosmic ray
nuclei

High-energy neutrinos from astrophysical accelerators of cosmic ray nuclei

Ongoing experimental efforts to detect cosmic sources of high energy neutrinos are guided by the expectation that astrophysical accelerators of cosmic ray protons would also generate neutrinos through interactions with ambient matter and/or photons. However there will be a reduction in the predicted...

Bibliografski detalji
Glavni autori:	Anchordoqui, L, Hooper, D, Sarkar, S, Taylor, A
Format:	Journal article
Jezik:	English
Izdano:	2007

Slični predmeti

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The intergalactic propagation of ultra-high energy cosmic ray nuclei
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Astrophysical origin of high-energy cosmic neutrinos
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Intergalactic propagation of ultrahigh energy cosmic ray nuclei: An analytic approach
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od: Mertsch, P, i dr.
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Astrophysical neutrinos and cosmic rays observed by IceCube
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The Impact of Heavy Nuclei on the Cosmogenic Neutrino Flux
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Implications of cosmic ray results for UHE neutrinos
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High-Energy and Ultra-High-Energy Neutrino Astrophysics
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Astrophysical Sources of Cosmic Rays and Related Measurements with the Pierre Auger Observatory
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Cosmic ray acceleration by multiple shocks in the jets of Active Galactic Nuclei
od: Müller Ana Laura, i dr.
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Neutrino Telescopes and High-Energy Cosmic Neutrinos
od: Andrea Palladino, i dr.
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COSMIC-RAY NEUTRINOS IN THE ATMOSPHERE
od: Gaisser, T, i dr.
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Information Technologies on High-Energy Astrophysics: Cosmic Ray Anisotropy using HAWC Observatory
od: de la Fuente Eduardo, i dr.
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od: Böser Sebastian
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od: Aartsen, MG, i dr.
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Observation of high-energy astrophysical neutrinos in three years of IceCube data
od: Aartsen, MG, i dr.
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Exotic Neutrino Interactions at the Pierre Auger Observatory
od: Anchordoqui, L, i dr.
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Differential limit on the extremely-high-energy cosmic neutrino flux in the presence of astrophysical background from nine years of IceCube data
od: Aartsen, M. G., i dr.
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High Energy Neutrino Emission from Astrophysical Jets in the Galaxy
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Continuous solutions of cosmic-rays and waves in astrophysical environments
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Differential limit on the extremely-high-energy cosmic neutrino flux in the presence of astrophysical background from nine years of IceCube data
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