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Indirect dark matter searches in gamma and cosmic rays
Stockholm University, Faculty of Science, Department of Physics. Stockholm University, Faculty of Science, The Oskar Klein Centre for Cosmo Particle Physics (OKC).
Number of Authors: 2
2017 (English)In: Nature Physics, ISSN 1745-2473, E-ISSN 1745-2481, Vol. 13, no 3, 224-231 p.Article, review/survey (Refereed) Published
Abstract [en]

Dark matter candidates such as weakly interacting massive particles are predicted to annihilate or decay into Standard Model particles, leaving behind distinctive signatures in gamma rays, neutrinos, positrons, antiprotons, or even antinuclei. Indirect dark matter searches, and in particular those based on gamma-ray observations and cosmic-ray measurements, could detect such signatures. Here we review the strengths and limitations of this approach and look into the future of indirect dark matter searches.

Place, publisher, year, edition, pages
2017. Vol. 13, no 3, 224-231 p.
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:su:diva-141224DOI: 10.1038/NPHYS4049ISI: 000395814000011OAI: oai:DiVA.org:su-141224DiVA: diva2:1089301
Available from: 2017-04-19 Created: 2017-04-19 Last updated: 2017-04-19Bibliographically approved

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