Search: onr:"20186400" > Multipole analysis ...
Fältnamn | Indikatorer | Metadata |
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000 | 13510naa a22041653a 4500 | |
001 | 20186400 | |
003 | SE-LIBR | |
005 | 20170322161936.0 | |
007 | cr|||||||||||| | |
008 | 170322s2015 sw |||| o |||| ||eng c | |
024 | 7 | a http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-2474312 uri |
024 | 7 | a urn:nbn:se:uu:diva-2474312 urn |
024 | 7 | a 10.1140/epjc/s10052-014-3224-52 doi |
040 | a S | |
041 | 0 | a eng |
042 | 9 EPLK | |
100 | 1 | a Aartsen, M. G.4 aut |
245 | 1 0 | a Multipole analysis of IceCube data to search for dark matter accumulated in the Galactic haloh [Elektronisk resurs] |
260 | c 2015 | |
500 | a Published | |
506 | 0 | a gratis |
520 | a Dark matter which is bound in the Galactic halo might self-annihilate and produce a flux of stable final state particles, e. g. high energy neutrinos. These neutrinos can be detected with IceCube, a cubic-kilometer sized Cherenkov detector. Given IceCube's large field of view, a characteristic anisotropy of the additional neutrino flux is expected. In this paper we describe a multipole method to search for such a large-scale anisotropy in IceCube data. This method uses the expansion coefficients of a multipole expansion of neutrino arrival directions and incorporates signal-specific weights for each expansion coefficient. We apply the technique to a high-purity muon neutrino sample from the Northern Hemisphere. The final result is compatible with the null-hypothesis. As no signal was observed, we present limits on the self-annihilation cross-section averaged over the relative velocity distribution <sigma(A)v > down to 1.9x10(-23) cm(3) s(-1) for a dark matter particle mass of 700-1,000 GeV and direct annihilation into nu(nu) over bar. The resulting exclusion limits come close to exclusion limits from gamma-ray experiments, that focus on the outer Galactic halo, for high dark matter masses of a few TeV and hard annihilation channels. | |
650 | 7 | a Natural Sciences2 hsv |
650 | 7 | a Physical Sciences2 hsv |
650 | 7 | a Other Physics Topics2 hsv |
650 | 7 | a Naturvetenskap2 hsv0 264446 |
650 | 7 | a Fysik2 hsv0 274895 |
650 | 7 | a Annan fysik2 hsv |
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710 | 1 2 | a Uppsala universitetb Teknisk-naturvetenskapliga vetenskapsområdet4 pbl |
772 | 1 8 | i channel recordw 19753896 |
773 | 0 8 | i Värdpublikationt European Physical Journal Cg 75:1x 1434-6044 |
856 | 4 0 | u http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-247431 |
856 | 4 0 | u http://dx.doi.org/10.1140/epjc/s10052-014-3224-5 |
856 | 4 0 | u http://uu.diva-portal.org/smash/get/diva2:797128/FULLTEXT01 |
950 | k | 6 650a Naturvetenskapw gu Fysik |
950 | k | 6 650a Atomerw hu Naturvetenskap |
950 | k | 6 650a Experimentw hu Naturvetenskap |
950 | k | 6 650a Fysikw hu Naturvetenskap |
950 | k | 6 650a Kemiw hu Naturvetenskap |
950 | k | 6 650a Kloningw hu Naturvetenskap |
950 | k | 6 650a Laboratorierw hu Naturvetenskap |
950 | k | 6 650a Marinbiologiw hu Naturvetenskap |
950 | k | 6 650a Matematikw hu Naturvetenskap |
950 | k | 6 650a Medicinska experimentw hu Naturvetenskap |
950 | k | 6 650a Tyngdlagenw hu Naturvetenskap |
950 | k | 6 650a Utvecklingsläraw hu Naturvetenskap |
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024 | 7 | 5 APISa urn:nbn:se:uu:diva-2474312 urn |
852 | 5 APISb APIS | |
856 | 4 0 | 5 APISu http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-247431 |
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