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Status of non-standard neutrino interactions
KTH, School of Engineering Sciences (SCI), Theoretical Physics, Theoretical Particle Physics.ORCID iD: 0000-0002-3525-8349
2013 (English)In: Reports on progress in physics (Print), ISSN 0034-4885, E-ISSN 1361-6633, Vol. 76, no 4, 044201- p.Article, review/survey (Refereed) Published
Abstract [en]

The phenomenon of neutrino oscillations has been established as the leading mechanism behind neutrino flavor transitions, providing solid experimental evidence that neutrinos are massive and lepton flavors are mixed. Here we review sub-leading effects in neutrino flavor transitions known as non-standard neutrino interactions (NSIs), which is currently the most explored description for effects beyond the standard paradigm of neutrino oscillations. In particular, we report on the phenomenology of NSIs and their experimental and phenomenological bounds as well as an outlook for future sensitivity and discovery reach.

Place, publisher, year, edition, pages
Institute of Physics Publishing (IOPP), 2013. Vol. 76, no 4, 044201- p.
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-122115DOI: 10.1088/0034-4885/76/4/044201ISI: 000317032800001Scopus ID: 2-s2.0-84875919004OAI: oai:DiVA.org:kth-122115DiVA: diva2:621264
Funder
Swedish Research Council, 621-2011-3985
Note

QC 20130514

Available from: 2013-05-14 Created: 2013-05-13 Last updated: 2017-12-06Bibliographically approved

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Ohlsson, Tommy

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  • apa
  • harvard1
  • ieee
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More styles
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  • de-DE
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