Search for dark matter from the Galactic halo with the IceCube Neutrino Telescope
- Abbasi, R.
- Abdou, Y.
- Abu-Zayyad, T.
- Adams, J.
- Aguilar, J.A.
- Ahlers, M.
- Andeen, K.
- Auffenberg, J.
- Bai, X.
- Baker, M.
- Barwick, S.W.
- Bay, R.
- Alba, J.L.B.
- Beattie, K.
- Beatty, J.J.
- Bechet, S.
- Becker, J.K.
- Becker, K.H.
- Benabderrahmane, M.L.
- BenZvi, S.
- Berdermann, J.
- Berghaus, P.
- Berley, D.
- Bernardini, E.
- Bertrand, D.
- Besson, D.Z.
- Bindig, D.
- Bissok, M.
- Blaufuss, E.
- Blumenthal, J.
- Boersma, D.J.
- Bohm, C.
- Bose, D.
- Boser, S.
- Botner, O.
- Braun, J.
- Brown, A.M.
- Buitink, S.
- Carson, M.
- Chirkin, D.
- Christy, B.
- Clem, J.
- Clevermann, F.
- Cohen, S.
- Colnard, C.
- Cowen, D.F.
- D'Agostino, M.V.
- Danninger, M.
- Daughhetee, J.
- Davis, J.C.
- Clercq, C. De
- Demirors, L.
- Denger, T.
- Depaepe, O.
- Descamps, F.
- Desiati, P.
- Vries-Uiterweerd, G. de
- DeYoung, T.
- Diaz-Velez, J.C.
- Dierckxsens, M.
- Dreyer, J.
- Dumm, J.P.
- Ehrlich, R.
- Eisch, J.
- Ellsworth, R.W.
- Engdegard, O.
- Euler, S.
- Evenson, P.A.
- Fadiran, O.
- Fazely, A.R.
- Fedynitch, A.
- Feusels, T.
- Filimonov, K.
- Finley, C.
- Fischer-Wasels, T.
- Foerster, M.M.
- Fox, B.D.
- Franckowiak, A.
- Franke, R.
- Gaisser, T.K.
- Gallagher, J.
- Geisler, M.
- Gerhardt, L.
- Gladstone, L.
- Glusenkamp, T.
- Goldschmidt, A.
- Goodman, J.A.
- Grant, D.
- Griesel, T.
- Gross, A.
- Grullon, S.
- Gurtner, M.
- Ha, C.
- Hallgren, A.
- Halzen, F.
- Han, K.
- Hanson, K.
- Heinen, D.
- Helbing, K.
- Herquet, P.
- Lafebre, S.J.
- et al.
DOIAbstract
Contains fulltext : 96327.pdf (preprint version ) (Open Access) Contains fulltext : 96327-1.pdf (publisher's version ) (Open Access)Self-annihilating or decaying dark matter in the Galactic halo might produce high energy neutrinos detectable with neutrino telescopes. We have conducted a search for such a signal using 276 days of data from the IceCube 22-string configuration detector acquired during 2007 and 2008. The effect of halo model choice in the extracted limit is reduced by performing a search that considers the outer halo region and not the Galactic Center. We constrain any large-scale neutrino anisotropy and are able to set a limit on the dark matter self-annihi...
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