Built on

E. Waxman and J. N. Bahcall, “High-energy neutrinos from astrophysical sources: An Upper bound,” Phys. Rev. D 59
1999
Earlier work this paper cites.
F. W. Stecker, “A note on high energy neutrinos from agn cores,” Phys. Rev. D 72
2005
Earlier work this paper cites.
J. K. Becker, M. Stamatikos, F. Halzen and W. Rhode, “Coincident grb neutrino flux predictions: implications for experimental uhe neutrino physics,” Astropart. Phys. 25
2005
Earlier work this paper cites.
A. Loeb and E. Waxman, “The Cumulative background of high energy neutrinos from starburst galaxies,” JCAP 0605
2006
Earlier work this paper cites.
F. W. Stecker, “Are Diffuse High Energy Neutrinos from Starburst Galaxies Observable?,” Astropart. Phys. 26
2006
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.
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
Earlier work this paper cites.
A. A. Abdo et al
Original
2009
Earlier work this paper cites.
P. Huntemeyer [Milagro Collaboration], “Galactic TeV gamma ray sources and diffuse emission: Results from Milagro,” PoS TEXAS 2010
2010
Earlier work this paper cites.
F. Vissani, F. Aharonian and N. Sahakyan, “On the Detectability of High-Energy Galactic Neutrino Sources,” Astropart. Phys. 34
Original
2011
Earlier work this paper cites.

Similar

F. W. Stecker, “PeV neutrinos observed by IceCube from cores of active galactic nuclei,” Phys. Rev. D 88
Original
2013
Cited alongside, same era.
K. Murase, M. Ahlers and B. C. Lacki, “Testing the Hadronuclear Origin of PeV Neutrinos Observed with IceCube,” Phys. Rev. D 88
Original
2013
Cited alongside, same era.
P. Padovani and E. Resconi, “Are both BL Lacs and pulsar wind nebulae the astrophysical counterparts of IceCube neutrino events?,” Mon. Not. Roy. Astron. Soc. 443
Original
2014
Cited alongside, same era.
I. Tamborra, S. Ando and K. Murase, “Star-forming galaxies as the origin of diffuse high-energy backgrounds: Gamma-ray and neutrino connections, and implications for starburst history,” JCAP 1409
Original
2014
Cited alongside, same era.
K. Asano and P. Mészáros, “Neutrino and Cosmic-Ray Release from Gamma-Ray Bursts: Time-Dependent Simulations,” Astrophys. J. 785

Then

A. Palladino, G. Pagliaroli, F. L. Villante and F. Vissani, “What is the Flavor of the Cosmic Neutrinos Seen by IceCube?,” Phys. Rev. Lett. 114
Original
2015
Later among the works it cites.
M. G. Aartsen et al
Original
2015
Later among the works it cites.
M. G. Aartsen et al
Original
2015
Later among the works it cites.
M. G. Aartsen et al
Original
2015
Later among the works it cites.
K. Murase, “On the Origin of High-Energy Cosmic Neutrinos,” AIP Conf. Proc. 1666
Original
2015
Later among the works it cites.

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2016

Extragalactic plus Galactic model for IceCube neutrino events

Palladino, Andrea, Vissani, Francesco

Understand

The hypothesis that high energy cosmic neutrinos are power law distributed is critically analyzed.

We propose a model with two components that explains better the observations.
The extragalactic component of the high energy neutrino flux has a canonical $E_\nu^{-2}$ spectrum while the galactic component has a $E_\nu^{-2.7}$ spectrum; both of them are significant.
This model has several implications, that can be tested by IceCube and ANTARES in the next years.

Built on

E. Waxman and J. N. Bahcall, “High-energy neutrinos from astrophysical sources: An Upper bound,” Phys. Rev. D 59
1999
Earlier work this paper cites.
F. W. Stecker, “A note on high energy neutrinos from agn cores,” Phys. Rev. D 72
2005
Earlier work this paper cites.
J. K. Becker, M. Stamatikos, F. Halzen and W. Rhode, “Coincident grb neutrino flux predictions: implications for experimental uhe neutrino physics,” Astropart. Phys. 25
2005
Earlier work this paper cites.
A. Loeb and E. Waxman, “The Cumulative background of high energy neutrinos from starburst galaxies,” JCAP 0605
2006
Earlier work this paper cites.
F. W. Stecker, “Are Diffuse High Energy Neutrinos from Starburst Galaxies Observable?,” Astropart. Phys. 26
2006
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.
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
Earlier work this paper cites.
A. A. Abdo et al
Original
2009
Earlier work this paper cites.
P. Huntemeyer [Milagro Collaboration], “Galactic TeV gamma ray sources and diffuse emission: Results from Milagro,” PoS TEXAS 2010
2010
Earlier work this paper cites.
F. Vissani, F. Aharonian and N. Sahakyan, “On the Detectability of High-Energy Galactic Neutrino Sources,” Astropart. Phys. 34
Original
2011
Earlier work this paper cites.