IceCube-22 Solar WIMP Data: Searching for Muon Neutrinos from Dark Matter Annihilations in the Sun
Relic dark matter in the galactic halo may become gravitationally trapped in the Sun and accumulate in its center, where it can annihilate each other, producing standard model particles, which may decay creating neutrinos. A search was performed using data from the IceCube detector in its 22 string...
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IceCube Neutrino Observatory
2009
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ftdatacite:10.21234/b4g59s 2023-05-15T18:22:06+02:00 IceCube-22 Solar WIMP Data: Searching for Muon Neutrinos from Dark Matter Annihilations in the Sun IceCube Collaboration 2009 https://dx.doi.org/10.21234/b4g59s https://icecube.wisc.edu/science/data/ic22-solar-wimp unknown IceCube Neutrino Observatory https://dx.doi.org/10.1103/physrevlett.102.201302 neutrino astronomy dark matter dataset Dataset 2009 ftdatacite https://doi.org/10.21234/b4g59s https://doi.org/10.1103/physrevlett.102.201302 2021-11-05T12:55:41Z Relic dark matter in the galactic halo may become gravitationally trapped in the Sun and accumulate in its center, where it can annihilate each other, producing standard model particles, which may decay creating neutrinos. A search was performed using data from the IceCube detector in its 22 string configuration. The experimental dataset consists of 104.26 days livetime, corresponding to a set of runs recorded during the period when the Sun was below the horizon at the South Pole, between March 21st and September 23rd. Dataset South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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DataCite Metadata Store (German National Library of Science and Technology) |
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unknown |
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neutrino astronomy dark matter |
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neutrino astronomy dark matter IceCube Collaboration IceCube-22 Solar WIMP Data: Searching for Muon Neutrinos from Dark Matter Annihilations in the Sun |
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neutrino astronomy dark matter |
description |
Relic dark matter in the galactic halo may become gravitationally trapped in the Sun and accumulate in its center, where it can annihilate each other, producing standard model particles, which may decay creating neutrinos. A search was performed using data from the IceCube detector in its 22 string configuration. The experimental dataset consists of 104.26 days livetime, corresponding to a set of runs recorded during the period when the Sun was below the horizon at the South Pole, between March 21st and September 23rd. |
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Dataset |
author |
IceCube Collaboration |
author_facet |
IceCube Collaboration |
author_sort |
IceCube Collaboration |
title |
IceCube-22 Solar WIMP Data: Searching for Muon Neutrinos from Dark Matter Annihilations in the Sun |
title_short |
IceCube-22 Solar WIMP Data: Searching for Muon Neutrinos from Dark Matter Annihilations in the Sun |
title_full |
IceCube-22 Solar WIMP Data: Searching for Muon Neutrinos from Dark Matter Annihilations in the Sun |
title_fullStr |
IceCube-22 Solar WIMP Data: Searching for Muon Neutrinos from Dark Matter Annihilations in the Sun |
title_full_unstemmed |
IceCube-22 Solar WIMP Data: Searching for Muon Neutrinos from Dark Matter Annihilations in the Sun |
title_sort |
icecube-22 solar wimp data: searching for muon neutrinos from dark matter annihilations in the sun |
publisher |
IceCube Neutrino Observatory |
publishDate |
2009 |
url |
https://dx.doi.org/10.21234/b4g59s https://icecube.wisc.edu/science/data/ic22-solar-wimp |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.1103/physrevlett.102.201302 |
op_doi |
https://doi.org/10.21234/b4g59s https://doi.org/10.1103/physrevlett.102.201302 |
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1766201459461849088 |