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P. Bernardini

Researcher at University of Salento

Publications -  16
Citations -  1124

P. Bernardini is an academic researcher from University of Salento. The author has contributed to research in topics: Neutrino & Neutrino oscillation. The author has an hindex of 16, co-authored 16 publications receiving 1087 citations.

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Journal ArticleDOI

Measurement of the atmospheric neutrino-induced upgoing muon flux using MACRO

M. Ambrosio, +135 more
- 27 Aug 1998 - 
TL;DR: In this article, a measurement of the flux of neutrino-induced upgoing muons ( ν >∼ 100 GeV) using the MACRO detector is presented, where the ratio of the observed to expected events integrated over all zenith angles is 0.74 ± 0.036 (stat) ±0.13 (theoretical).
Journal ArticleDOI

Final results of magnetic monopole searches with the MACRO experiment

M. Ambrosio, +128 more
TL;DR: In this article, the authors present the final results obtained by the MACRO experiment in the search for GUT magnetic monopoles in the penetrating cosmic radiation, for the range 4×10 −5 <β < 1.
Journal ArticleDOI

Matter effects in upward-going muons and sterile neutrino oscillations

M. Ambrosio, +127 more
- 27 Sep 2001 - 
TL;DR: The angular distribution of upward-going muons produced by atmospheric neutrinos in the rock below the MACRO detector shows anomalies in good agreement with two flavor ν μ → ν τ oscillations with maximum mixing and Δm 2 around 0.0024 eV 2.
Journal ArticleDOI

Seasonal variations in the underground muon intensity as seen by MACRO

M. Ambrosio, +133 more
TL;DR: In this article, the authors search for a correlation between variations in the underground muon rate, Nμ, and seasonal temperature variation in the atmosphere with high statistical significance and find that these correlations are present with high significance.
Journal ArticleDOI

Low energy atmospheric muon neutrinos in MACRO

M. Ambrosio, +123 more
- 06 Apr 2000 - 
TL;DR: In this article, the authors present the measurement of two event samples induced by atmospheric ν μ of average energy E ν ∼4 GeV with an angular distribution similar to that expected from the Bartol atmospheric neutrino flux.