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Search for exotic contributions to atmospheric neutrino oscillations
INFN Sez. di Milano, Italy.
Universita’ di Bologna, Italy.ORCID iD: 0000-0002-2115-2930
Universita’ di Bologna, Italy ; INAF/IASF Sez. di Bologna, Italy.
Universita’ di Bologna, Italy.
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2005 (English)In: 29th International Cosmic Ray Conference: August 3 - 10, 2005, Pune, India, Mumbai: Tata Institute of Fundamental Research , 2005, p. 171-174Conference paper, Published paper (Other academic)
Abstract [en]

The energy spectrum of neutrino-induced upward-going muons in MACRO was analysed in terms of relativity principles violating effects, keeping standard mass-induced atmospheric neutrino oscillations as the dominant source of v(mu) -> v(tau) transitions. The data disfavor these possibilities even at a sub-dominant level; stringent 90% C.L. limits are placed on the Lorentz invariance violation parameter vertical bar Delta v vertical bar < 6 x 10(-24) at sin 2 theta(v) = 0 and vertical bar Delta v vertical bar < 2.5 divided by 5 x 10(-26) at sin 2 theta(v) = +/- 1. The limits can be re-interpreted as bounds on the Equivalence Principle violation parameters.

Place, publisher, year, edition, pages
Mumbai: Tata Institute of Fundamental Research , 2005. p. 171-174
National Category
Astronomy, Astrophysics and Cosmology
Research subject
Physics, Astroparticle Physics
Identifiers
URN: urn:nbn:se:lnu:diva-30286ISI: 000243522800044OAI: oai:DiVA.org:lnu-30286DiVA, id: diva2:706018
Conference
29th International Cosmic Ray Conference, August 3 - 10, 2005, Pune, India
Available from: 2014-03-18 Created: 2013-11-08 Last updated: 2015-05-12Bibliographically approved

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Becherini, Yvonne

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