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Improved methods for solar Dark Matter searches with the IceCube neutrino telescope
Stockholm University, Faculty of Science, Department of Physics. (The IceCube Collaboration)ORCID iD: 0000-0001-8879-7031
2015 (English)In: The IceCube Neutrino Observatory - Contributions to ICRC 2015: Part IV: Searches for Dark Matter and Exotic Particles, 2015, 17-24 p.Conference paper (Refereed)
Abstract [en]

Gravitationally captured Dark Matter in the form of Weakly Interacting Massive Particles(WIMPs) can annihilate into standard-model particles, such as neutrinos. The IceCube neutrinodetector at the South Pole is an excellent instrument to search for such a neutrino signal fromthe Sun. We present an alternative analysis which improves on previous approaches, in particularin background-dominated regions. Newly developed techniques based on hit clustering and hit-based vetos allow a more accurate reconstruction and identification of events in the detector andthereby a stronger rejection of background. These techniques are also applicable to other IceCubeanalyses and event filters. We present results for a solar WIMP search using the first year of datataken with the completed IceCube detector with 86 strings.

Place, publisher, year, edition, pages
2015. 17-24 p.
Keyword [en]
IceCube, neutrino, sun, WIMP, dark matter, cluster analysis
National Category
Astronomy, Astrophysics and Cosmology
Research subject
Physics
Identifiers
URN: urn:nbn:se:su:diva-125092OAI: oai:DiVA.org:su-125092DiVA: diva2:891768
Conference
The 34th International Cosmic Ray Conference, 30 July - 6 August, 2015, The Hague, The Netherlands
Available from: 2016-01-07 Created: 2016-01-07 Last updated: 2016-01-26Bibliographically approved
In thesis
1. A search for solar dark matter with the IceCube neutrino detector: Advances in data treatment and analysis technique
Open this publication in new window or tab >>A search for solar dark matter with the IceCube neutrino detector: Advances in data treatment and analysis technique
2016 (English)Doctoral thesis, comprehensive summary (Other academic)
Abstract [en]

There is compelling observational evidence for the existence of dark matter in the Universe, including our own Galaxy, which could possibly consist of weakly interacting massive particles (WIMPs) not contained in the standard model (SM) of particle physics. WIMPs may get gravitationally trapped inside heavy celestial bodies of ordinary matter. The Sun is a nearby candidate for such a capture process which is driven by the scattering of WIMPs on its nuclei. Forming an over-density at the Sun's core the WIMPs would self-annihilate yielding energetic neutrinos, which leave the Sun and can be detected in experiments on Earth. The cubic-kilometer sized IceCube neutrino observatory, constructed in the clear glacial ice at the Amundsen-Scott South Pole Station in Antarctica offers an excellent opportunity to search for this striking signal.

This thesis is dedicated to the search for these solar dark matter signatures in muon neutrinos from the direction of the Sun. Newly developed techniques based on hit clustering and hit-based vetos allow more accurate reconstruction and identification of events in the detector and thereby a stronger rejection of background. These techniques are also applicable to other IceCube analyses and event filters. In addition, new approaches to the analysis without seasonal cuts lead to improvements in sensitivity especially in the low-energy regime (<=100 GeV), the target of the more densely instrumented DeepCore sub-array.

This first analysis of 369 days of data recorded with the completed detector array of 86 strings revealed no significant excess above the expected background of atmospheric neutrinos. This allows us to set strong limits on the annihilation rate of WIMPs in the Sun for the models probed in this analysis. The IceCube limits for the spin-independent WIMP-proton scattering cross-section are the most stringent ones for WIMP masses above 100 GeV.

Place, publisher, year, edition, pages
Stockholm: Department of Physics, Stockholm University, 2016. 189 p.
Keyword
neutrino, WIMP, dark matter, cluster analysis, sun, IceCube, IC86
National Category
Astronomy, Astrophysics and Cosmology
Research subject
Physics
Identifiers
urn:nbn:se:su:diva-125341 (URN)978-91-7649-329-8 (ISBN)
Public defence
2016-02-29, sal FB42, AlbaNova universitetscentrum, Roslagstullsbacken 21, Stockholm, 14:00 (English)
Opponent
Supervisors
Projects
IceCube
Available from: 2016-02-04 Created: 2016-01-10 Last updated: 2016-01-27Bibliographically approved

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Zoll, Marcel
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