Built on

S. L. Glashow, “Resonant Scattering of Antineutrinos,” Phys. Rev. 118
1960
Earlier work this paper cites.
V. S. Berezinsky and A. Z. Gazizov, “Cosmic Neutrinos and Possibility to Search for W Bosons Having 30-GeV-100-GeV Masses in Underwater Experiments,” JETP Lett. 25
1977
Earlier work this paper cites.
A. M. Dziewonski and D. L. Anderson, “Preliminary reference earth model,” Phys. Earth Planet. Interiors 25
1981
Earlier work this paper cites.
J. G. Learned and S. Pakvasa, “Detecting tau-neutrino oscillations at PeV energies,” Astropart. Phys. 3
1995
Earlier work this paper cites.
R. Gandhi, C. Quigg, M. H. Reno and I. Sarcevic, “Neutrino interactions at ultrahigh-energies,” Phys. Rev. D 58
1998
Earlier work this paper cites.
J. F. Beacom, et al
2005
Earlier work this paper cites.
L. A. Anchordoqui, H. Goldberg, F. Halzen and T. J. Weiler, “Neutrinos as a diagnostic of high energy astrophysical processes,” Phys. Lett. B 621
2005
Earlier work this paper cites.
C. Moura, “Detection of ultra-high energy tau-neutrino by double-bang event,” AIP Conf. Proc. 809
2006
Earlier work this paper cites.
D. F. Cowen [IceCube Collaboration], “Tau neutrinos in IceCube,” J. Phys. Conf. Ser. 60
2007
Earlier work this paper cites.
F. L. Villante and F. Vissani, “How precisely neutrino emission from supernova remnants can be constrained by gamma ray observations?,” Phys. Rev. D 78
Original
2008
Earlier work this paper cites.

Similar

P. Lipari, “Hadronic interactions modeling, and the calculation of the inclusive fluxes of atmospheric muons and neutrinos,” Nucl. Phys. Proc. Suppl. 175-176
2008
Cited alongside, same era.
G. Battistoni et al
2008
Cited alongside, same era.
S. R. Kelner, F. A. Aharonian and V. V. Bugayov, “Energy spectra of gamma-rays, electrons and neutrinos produced at proton-proton interactions in the very high energy regime,” Phys. Rev. D 74
2009
Cited alongside, same era.
S. R. Kelner and F. A. Aharonian, “Energy spectra of gamma-rays, electrons and neutrinos produced at interactions of relativistic protons with low energy radiation,” Phys. Rev. D 78
2010
Cited alongside, same era.
S. Hummer, M. Ruger, F. Spanier and W. Winter, “Simplified models for photohadronic interactions in cosmic accelerators,” Astrophys. J. 721
Original
2010

Then

M. G. Aartsen et al
Original
2013
Later among the works it cites.
F. Vissani, G. Pagliaroli and F. L. Villante, “The fraction of muon tracks in cosmic neutrinos,” JCAP 1309
Original
2013
Later among the works it cites.
V. Barger, J. Learned and S. Pakvasa, “IceCube PeV Cascade Events Initiated by Electron-Antineutrinos at Glashow Resonance,” Phys. Rev. D 87
Original
2013
Later among the works it cites.
M. G. Aartsen et al
Original
2014
Later among the works it cites.
V. Barger, L. Fu, J. G. Learned, D. Marfatia, S. Pakvasa and T. J. Weiler, “Glashow resonance as a window into cosmic neutrino sources,” Phys. Rev. D 90
Original

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2015

Double pulses and cascades above 2 PeV in IceCube

Palladino, Andrea, Pagliaroli, Giulia, Villante, Francesco L. et al.

Understand

IceCube collaboration has seen an unexpected population of high energy neutrinos compatible with an astrophysical origin.

We consider two categories of events that can help to diagnose cosmic neutrinos: double pulse, that may allow us to clearly discriminate the cosmic component of tau neutrinos; cascades with deposited energy above 2 PeV, including events produced by electron antineutrinos at the Glashow resonance, that can be used to investigate the neutrino production mechanisms.
We show that one half of the double pulse signal is due to the neutrinos spectral region already probed by IceCube.
By normalizing to HESE data, we find that 10 more years are required to obtain 90% probability to observe a double pulse.

Built on

S. L. Glashow, “Resonant Scattering of Antineutrinos,” Phys. Rev. 118
1960
Earlier work this paper cites.
V. S. Berezinsky and A. Z. Gazizov, “Cosmic Neutrinos and Possibility to Search for W Bosons Having 30-GeV-100-GeV Masses in Underwater Experiments,” JETP Lett. 25
1977
Earlier work this paper cites.
A. M. Dziewonski and D. L. Anderson, “Preliminary reference earth model,” Phys. Earth Planet. Interiors 25
1981
Earlier work this paper cites.
J. G. Learned and S. Pakvasa, “Detecting tau-neutrino oscillations at PeV energies,” Astropart. Phys. 3
1995
Earlier work this paper cites.
R. Gandhi, C. Quigg, M. H. Reno and I. Sarcevic, “Neutrino interactions at ultrahigh-energies,” Phys. Rev. D 58
1998
Earlier work this paper cites.
J. F. Beacom, et al
2005
Earlier work this paper cites.
L. A. Anchordoqui, H. Goldberg, F. Halzen and T. J. Weiler, “Neutrinos as a diagnostic of high energy astrophysical processes,” Phys. Lett. B 621
2005
Earlier work this paper cites.
C. Moura, “Detection of ultra-high energy tau-neutrino by double-bang event,” AIP Conf. Proc. 809
2006
Earlier work this paper cites.
D. F. Cowen [IceCube Collaboration], “Tau neutrinos in IceCube,” J. Phys. Conf. Ser. 60
2007
Earlier work this paper cites.
F. L. Villante and F. Vissani, “How precisely neutrino emission from supernova remnants can be constrained by gamma ray observations?,” Phys. Rev. D 78
Original
2008
Earlier work this paper cites.

Similar

P. Lipari, “Hadronic interactions modeling, and the calculation of the inclusive fluxes of atmospheric muons and neutrinos,” Nucl. Phys. Proc. Suppl. 175-176
2008
Cited alongside, same era.
G. Battistoni et al
2008
Cited alongside, same era.
S. R. Kelner, F. A. Aharonian and V. V. Bugayov, “Energy spectra of gamma-rays, electrons and neutrinos produced at proton-proton interactions in the very high energy regime,” Phys. Rev. D 74
2009
Cited alongside, same era.
S. R. Kelner and F. A. Aharonian, “Energy spectra of gamma-rays, electrons and neutrinos produced at interactions of relativistic protons with low energy radiation,” Phys. Rev. D 78
2010
Cited alongside, same era.
S. Hummer, M. Ruger, F. Spanier and W. Winter, “Simplified models for photohadronic interactions in cosmic accelerators,” Astrophys. J. 721
Original
2010

Then

M. G. Aartsen et al
Original
2013
Later among the works it cites.
F. Vissani, G. Pagliaroli and F. L. Villante, “The fraction of muon tracks in cosmic neutrinos,” JCAP 1309
Original
2013
Later among the works it cites.
V. Barger, J. Learned and S. Pakvasa, “IceCube PeV Cascade Events Initiated by Electron-Antineutrinos at Glashow Resonance,” Phys. Rev. D 87
Original
2013
Later among the works it cites.
M. G. Aartsen et al
Original
2014
Later among the works it cites.
V. Barger, L. Fu, J. G. Learned, D. Marfatia, S. Pakvasa and T. J. Weiler, “Glashow resonance as a window into cosmic neutrino sources,” Phys. Rev. D 90
Original

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Cited alongside, same era.

S. Hummer, M. Maltoni, W. Winter and C. Yaguna, “Energy dependent neutrino flavor ratios from cosmic accelerators on the Hillas plot,” Astropart. Phys. 34

Original

2010

Cited alongside, same era.

A. Bhattacharya, R. Gandhi, W. Rodejohann and A. Watanabe, “The Glashow resonance at IceCube: signatures, event rates and p p pp vs. p γ p\gamma interactions,” JCAP 1110

Original

2011

Cited alongside, same era.

Z. z. Xing and S. Zhou, “The Glashow resonance as a discriminator of UHE cosmic neutrinos originating from p-gamma and p-p collisions,” Phys. Rev. D 84

2011

Cited alongside, same era.

R. Abbasi et al

Original

2012

Cited alongside, same era.

F. Vissani and F. Aharonian, “Galactic Sources of High-Energy Neutrinos: Highlights,” Nucl. Instrum. Meth. A 692

2012

Cited alongside, same era.

Olga Botner slides from https://events.icecube.wisc.edu/conferenceDisplay.py?confId=68

Cited in the paper.

M. G. Aartsen et al