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Solar Neutrino Day-Night Effect
KTH, School of Engineering Sciences (SCI), Theoretical Physics, Theoretical Particle Physics.ORCID iD: 0000-0001-5948-9152
KTH, School of Engineering Sciences (SCI), Theoretical Physics, Theoretical Particle Physics.ORCID iD: 0000-0002-3525-8349
KTH, School of Engineering Sciences (SCI), Theoretical Physics, Theoretical Particle Physics.
2005 (English)In: NEUTRINO 2004 / [ed] Jacques Dumarchez, Thomas Patzak, François Vannucci, Elsevier Science B.V. , 2005, 578-578 p.Conference paper (Refereed)
Abstract [en]

We summarize the results of Ref. [M. Blennow, T. Ohlsson and H. Snellman, Phys. Rev. D 69 (2004) 073006, hep-ph/0311098] in which we determine the effects of three flavor mixing on the day-night asymmetry in the flux of solar neutrinos. Analytic methods are used to determine the difference in the day and night solar electron neutrino survival probabilites and numerical methods are used to determine the effect of three flavor mixing at detectors.

Place, publisher, year, edition, pages
Elsevier Science B.V. , 2005. 578-578 p.
Series
, Nuclear physics B, Proceedings supplements, ISSN 0920-5632
National Category
Subatomic Physics
Identifiers
URN: urn:nbn:se:kth:diva-34617DOI: 10.1016/j.nuclphysbps.2005.01.243ISI: 000228672500164OAI: oai:DiVA.org:kth-34617DiVA: diva2:423976
Conference
Neutrino 2004
Note
QC 20110617Available from: 2011-06-17 Created: 2011-06-10 Last updated: 2011-11-08Bibliographically approved

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