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R. Gandhi, C. Quigg, M. H. Reno and I. Sarcevic, Phys. Rev. D 58
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W. de Boer, M. Herold, C. Sander, V. Zhukov, A. V. Gladyshev and D. I. Kazakov, arXiv:astro-ph/0408272; W. de Boer, C. Sander, V. Zhukov, A. V. Gladyshev and D. I. Kazakov, Phys. Rev. Lett. 95

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2009

High Energy Neutrinos As A Test of Leptophilic Dark Matter

Spolyar, Douglas, Buckley, Matthew, Freese, Katherine et al.

Understand

Recently, observations by PAMELA, the Fermi Gamma Ray Space Telescope, and other cosmic ray experiments have generated a great deal of interest in dark matter (DM) particles which annihilate at a high rate to leptons.

In this letter, we explore the possibility of using large volume neutrino telescopes, such as IceCube, to constrain such models; specifically we consider signals due to DM annihilation in the inner Milky Way.
We find that, if Dark Matter annihilations are responsible for the signals observed by PAMELA and FGST, then IceCube (in conjunction with the planned low threshold extension, DeepCore) should detect or exclude the corresponding neutrino signal from the inner Milky Way with a few years of observation.

Built on

A. Sommerfeld, Annalen der Physik 403, 257 (1931); N. Arkani-Hamed, D. P. Finkbeiner, T. Slatyer and N. Weiner, arXiv:0810.0713 [hep-ph]; M. Cirelli and A. Strumia, arXiv:0808.3867 [astro-ph];
Original
1931
Earlier work this paper cites.
G. Jungman and M. Kamionkowski, Phys. Rev. D 51
Original
1951
Earlier work this paper cites.
J. R. Ellis, R. A. Flores, K. Freese, S. Ritz, D. Seckel and J. Silk, Phys. Lett. B 214
1984
Earlier work this paper cites.
K. Freese, Phys. Lett. B 167
1986
Earlier work this paper cites.
M. Srednicki, K. A. Olive and J. Silk, Nucl. Phys. B 279
1987
Earlier work this paper cites.
J. R. Primack, D. Seckel and B. Sadoulet, Ann. Rev. Nucl. Part. Sci. 38
1988
Earlier work this paper cites.
G. Jungman, M. Kamionkowski and K. Griest, Phys. Rept. 267
1996
Earlier work this paper cites.
J. D. Lewin and P. F. Smith, Astropart. Phys. 6
1996
Earlier work this paper cites.
S. W. Barwick et al
1997
Earlier work this paper cites.

Similar

R. Gandhi, C. Quigg, M. H. Reno and I. Sarcevic, Phys. Rev. D 58
1998
Cited alongside, same era.
P. Gondolo and J. Silk, Phys. Rev. Lett. 83
2002
Cited alongside, same era.
N. W. Evans, F. Ferrer and S. Sarkar, Phys. Rev. D 69
2004
Cited alongside, same era.
P. Jean et al
2004
Cited alongside, same era.
M. Honda, T. Kajita, K. Kasahara, S. Midorikawa and T. Sanuki, Phys. Rev. D 75
2004
Cited alongside, same era.
G. Bertone, D. Hooper and J. Silk, Phys. Rept. 405
2005
Cited alongside, same era.
W. de Boer, M. Herold, C. Sander, V. Zhukov, A. V. Gladyshev and D. I. Kazakov, arXiv:astro-ph/0408272; W. de Boer, C. Sander, V. Zhukov, A. V. Gladyshev and D. I. Kazakov, Phys. Rev. Lett. 95