Built on

S. Baker and R. D. Cousins, Clarification of the use of chi square and likelihood functions in fits to histograms
1984
Earlier work this paper cites.
K. Griest and M. Kamionkowski, Unitarity Limits on the Mass and Radius of Dark Matter Particles
1990
Earlier work this paper cites.
T. K. Gaisser, Cosmic rays and particle physics
1990
Earlier work this paper cites.
F. W. Stecker, C. Done, M. H. Salamon and P. Sommers, High-energy neutrinos from active galactic nuclei
1992
Earlier work this paper cites.
E. Waxman and J. N. Bahcall, High-energy neutrinos from cosmological gamma-ray burst fireballs
1997
Earlier work this paper cites.
D. J. Chung, E. W. Kolb and A. Riotto, Nonthermal supermassive dark matter
1998
Earlier work this paper cites.
E. Waxman and J. N. Bahcall, High-energy neutrinos from astrophysical sources: An Upper bound
1999
Earlier work this paper cites.
D. J. Chung, E. W. Kolb, and A. Riotto, Production of massive particles during reheating
1999
Earlier work this paper cites.
A. Mucke, R. Engel, J. P. Rachen, R. J. Protheroe and T. Stanev, SOPHIA: Monte Carlo simulations of photohadronic processes in astrophysics
2000
Earlier work this paper cites.
G. F. Giudice, E. W. Kolb, and A. Riotto, Largest temperature of the radiation era and its cosmological implications
2001
Earlier work this paper cites.
F. Halzen and D. Hooper, High-energy neutrino astronomy: The Cosmic ray connection
2002
Earlier work this paper cites.
R. Allahverdi and M. Drees, Production of massive stable particles in inflaton decay
2002
Earlier work this paper cites.
P. H. Frampton, S. L. Glashow and D. Marfatia, Zeroes of the neutrino mass matrix
2002
Earlier work this paper cites.
T. Stanev, High energy cosmic rays
2004
Earlier work this paper cites.
M. Cirelli, N. Fornengo, and A. Strumia, Minimal dark matter
2006
Earlier work this paper cites.
A. Loeb and E. Waxman, The Cumulative background of high energy neutrinos from starburst galaxies
2006
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
2006
Earlier work this paper cites.

Similar

G. B. Gelmini and P. Gondolo, Neutralino with the right cold dark matter abundance in (almost) any supersymmetric model
2006
Cited alongside, same era.
N. Haba, Y. Kajiyama, S. Matsumoto, H. Okada, and K. Yoshioka, Universally Leptophilic Dark Matter From Non-Abelian Discrete Symmetry
Original
2011
Cited alongside, same era.
P. Ciafaloni, M. Cirelli, D. Comelli, A. De Simone, A. Riotto and A. Urbano, On the Importance of Electroweak Corrections for Majorana Dark Matter Indirect Detection
Original
2011
Cited alongside, same era.
H. Fritzsch, Z. z. Xing and S. Zhou, Two-zero Textures of the Majorana Neutrino Mass Matrix and Current Experimental Tests
Original
2011
Cited alongside, same era.
H. N. He, R. Y. Liu, X. Y. Wang, S. Nagataki, K. Murase and Z. G. Dai, Icecube non-detection of GRBs: Constraints on the fireball properties

Then

K. Agashe, Y. Cui, L. Necib, and J. Thaler, (In)direct Detection of Boosted Dark Matter
Original
2014
Later among the works it cites.
T. K. Gaisser, K. Jero, A. Karle and J. van Santen, Generalized self-veto probability for atmospheric neutrinos
Original
2014
Later among the works it cites.
H. Baer, K.-Y. Choi, J. E. Kim, and L. Roszkowski, Dark matter production in the early Universe: beyond the thermal WIMP paradigm
Original
2014
Later among the works it cites.
K. Harigaya, M. Kawasaki, K. Mukaida and M. Yamada, Dark Matter Production in Late Time Reheating
Original
2014
Later among the works it cites.
M. G. Aartsen et al
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…

Reading the bibliography…

2015

Decaying Leptophilic Dark Matter at IceCube

Boucenna, Sofiane M., Chianese, Marco, Mangano, Gianpiero et al.

Understand

We present a novel interpretation of IceCube high energy neutrino events (with energy larger than 60 TeV) in terms of an extraterrestrial flux due to two different contributions: a flux originated by known astrophysical sources and dominating IceCube observations up to few hundreds TeV, and a new flux component where the most energetic neutrinos come from the leptophilic three-body decays of dark matter particles with a mass of few PeV.

Differently from other approaches, we provide two examples of elementary particle models that do not require extremely tiny coupling constants.
We find the compatibility of the theoretical predictions with the IceCube results when the astrophysical flux has a cutoff of the order of 100 TeV (broken power law).
In this case the most energetic part of the spectrum (PeV neutrinos) is due to an extra component such as the decay of a very massive dark matter component.