2019
DOI: 10.48550/arxiv.1910.11878
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Grand Unified Neutrino Spectrum at Earth: Sources and Spectral Components

Edoardo Vitagliano,
Irene Tamborra,
Georg Raffelt

Abstract: We briefly review the dominant neutrino fluxes at Earth from different sources and present the Grand Unified Neutrino Spectrum ranging from meV to PeV energies. For each energy band and source, we discuss both theoretical expectations and experimental data. This compact review should be useful as a brief reference to those interested in neutrino astronomy, fundamental particle physics, dark-matter detection, high-energy astrophysics, geophysics, and other related topics.

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Cited by 13 publications
(29 citation statements)
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References 294 publications
(498 reference statements)
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“…The hep neutrinos are less studied experimentally because their flux is rather suppressed compared to that of 8 B neutrinos. The GS98 prediction for the flux of hep neutrinos is 0.8 × 10 4 cm −2 s −1 compared to 5.46 × 10 6 cm −2 s −1 for the 8 B neutrinos [27]. So apart from the magnitudes and spectral shapes of the fluxes, the physics for 8 B and hep neutrinos is essentially the same and we shall use the same formulas as in the previous section.…”
Section: Hep Neutrinosmentioning
confidence: 98%
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“…The hep neutrinos are less studied experimentally because their flux is rather suppressed compared to that of 8 B neutrinos. The GS98 prediction for the flux of hep neutrinos is 0.8 × 10 4 cm −2 s −1 compared to 5.46 × 10 6 cm −2 s −1 for the 8 B neutrinos [27]. So apart from the magnitudes and spectral shapes of the fluxes, the physics for 8 B and hep neutrinos is essentially the same and we shall use the same formulas as in the previous section.…”
Section: Hep Neutrinosmentioning
confidence: 98%
“…B. For the energy distribution we take in both cases the GS98 prediction taken from [27] with f 8B 0 = 5.46 × 10 6 cm −2 s −1 . We will also include neutrino oscillations into the picture at this point.…”
Section: Towards Realistic Picturesmentioning
confidence: 99%
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