Search for dark matter annihilation in the Galactic Center with IceCube-79
The Milky Way is expected to be embedded in a halo of dark matter particles, with the highest density in the central region, and decreasing density with the halo-centric radius. Dark matter might be indirectly detectable at Earth through a flux of stable particles generated in dark matter annihilati...
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Stockholms universitet, Fysikum
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ftstockholmuniv:oai:DiVA.org:su-125815 2023-05-15T18:22:50+02:00 Search for dark matter annihilation in the Galactic Center with IceCube-79 Ahrens, Maryon Bohm, Christian Dumm, Jonathan P. Finley, Chad Flis, Samuel Hulth, Per Olof Hultqvist, Klas Walck, Christian Wolf, Martin Zoll, Marcel 2015 application/pdf http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-125815 https://doi.org/10.1140/epjc/s10052-015-3713-1 eng eng Stockholms universitet, Fysikum Stockholms universitet, Oskar Klein-centrum för kosmopartikelfysik (OKC) European Physical Journal C, 1434-6044, 2015, 75:10, orcid:0000-0001-6105-7762 orcid:0000-0001-8879-7031 http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-125815 doi:10.1140/epjc/s10052-015-3713-1 ISI:000366311800002 info:eu-repo/semantics/openAccess Physical Sciences Fysik Article in journal info:eu-repo/semantics/article text 2015 ftstockholmuniv https://doi.org/10.1140/epjc/s10052-015-3713-1 2023-02-23T21:43:45Z The Milky Way is expected to be embedded in a halo of dark matter particles, with the highest density in the central region, and decreasing density with the halo-centric radius. Dark matter might be indirectly detectable at Earth through a flux of stable particles generated in dark matter annihilations and peaked in the direction of the Galactic Center. We present a search for an excess flux of muon (anti-) neutrinos from dark matter annihilation in the Galactic Center using the cubic-kilometer-sized IceCube neutrino detector at the South Pole. There, the Galactic Center is always seen above the horizon. Thus, new and dedicated veto techniques against atmospheric muons are required to make the southern hemisphere accessible for IceCube. We used 319.7 live-days of data from IceCube operating in its 79-string configuration during 2010 and 2011. No neutrino excess was found and the final result is compatible with the background. We present upper limits on the self-annihilation cross-section, < sAv >, for WIMP masses ranging from 30GeV up to 10TeV, assuming cuspy (NFW) and flat-cored (Burkert) dark matter halo profiles, reaching down to similar or equal to 4 . 10(-24) cm(3) s(-1), and similar or equal to 2.6 . 10(-23) cm(3) s(-1) for the nu(nu) over bar channel, respectively. Article in Journal/Newspaper South pole Stockholm University: Publications (DiVA) Milky Way ENVELOPE(-68.705,-68.705,-71.251,-71.251) Sav’ ENVELOPE(156.400,156.400,68.817,68.817) South Pole The European Physical Journal C 75 10 |
institution |
Open Polar |
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Stockholm University: Publications (DiVA) |
op_collection_id |
ftstockholmuniv |
language |
English |
topic |
Physical Sciences Fysik |
spellingShingle |
Physical Sciences Fysik Ahrens, Maryon Bohm, Christian Dumm, Jonathan P. Finley, Chad Flis, Samuel Hulth, Per Olof Hultqvist, Klas Walck, Christian Wolf, Martin Zoll, Marcel Search for dark matter annihilation in the Galactic Center with IceCube-79 |
topic_facet |
Physical Sciences Fysik |
description |
The Milky Way is expected to be embedded in a halo of dark matter particles, with the highest density in the central region, and decreasing density with the halo-centric radius. Dark matter might be indirectly detectable at Earth through a flux of stable particles generated in dark matter annihilations and peaked in the direction of the Galactic Center. We present a search for an excess flux of muon (anti-) neutrinos from dark matter annihilation in the Galactic Center using the cubic-kilometer-sized IceCube neutrino detector at the South Pole. There, the Galactic Center is always seen above the horizon. Thus, new and dedicated veto techniques against atmospheric muons are required to make the southern hemisphere accessible for IceCube. We used 319.7 live-days of data from IceCube operating in its 79-string configuration during 2010 and 2011. No neutrino excess was found and the final result is compatible with the background. We present upper limits on the self-annihilation cross-section, < sAv >, for WIMP masses ranging from 30GeV up to 10TeV, assuming cuspy (NFW) and flat-cored (Burkert) dark matter halo profiles, reaching down to similar or equal to 4 . 10(-24) cm(3) s(-1), and similar or equal to 2.6 . 10(-23) cm(3) s(-1) for the nu(nu) over bar channel, respectively. |
format |
Article in Journal/Newspaper |
author |
Ahrens, Maryon Bohm, Christian Dumm, Jonathan P. Finley, Chad Flis, Samuel Hulth, Per Olof Hultqvist, Klas Walck, Christian Wolf, Martin Zoll, Marcel |
author_facet |
Ahrens, Maryon Bohm, Christian Dumm, Jonathan P. Finley, Chad Flis, Samuel Hulth, Per Olof Hultqvist, Klas Walck, Christian Wolf, Martin Zoll, Marcel |
author_sort |
Ahrens, Maryon |
title |
Search for dark matter annihilation in the Galactic Center with IceCube-79 |
title_short |
Search for dark matter annihilation in the Galactic Center with IceCube-79 |
title_full |
Search for dark matter annihilation in the Galactic Center with IceCube-79 |
title_fullStr |
Search for dark matter annihilation in the Galactic Center with IceCube-79 |
title_full_unstemmed |
Search for dark matter annihilation in the Galactic Center with IceCube-79 |
title_sort |
search for dark matter annihilation in the galactic center with icecube-79 |
publisher |
Stockholms universitet, Fysikum |
publishDate |
2015 |
url |
http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-125815 https://doi.org/10.1140/epjc/s10052-015-3713-1 |
long_lat |
ENVELOPE(-68.705,-68.705,-71.251,-71.251) ENVELOPE(156.400,156.400,68.817,68.817) |
geographic |
Milky Way Sav’ South Pole |
geographic_facet |
Milky Way Sav’ South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
European Physical Journal C, 1434-6044, 2015, 75:10, orcid:0000-0001-6105-7762 orcid:0000-0001-8879-7031 http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-125815 doi:10.1140/epjc/s10052-015-3713-1 ISI:000366311800002 |
op_rights |
info:eu-repo/semantics/openAccess |
op_doi |
https://doi.org/10.1140/epjc/s10052-015-3713-1 |
container_title |
The European Physical Journal C |
container_volume |
75 |
container_issue |
10 |
_version_ |
1766202256317743104 |