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14 papers
New experimental limits on the Pauli forbidden transitions in C nuclei obtained with 485 days Borexino data
The Borexino Collaboration
The Pauli exclusion principle (PEP) has been tested for nucleons () in with the Borexino detector.The approach consists of a search for , , and emit…
Solar neutrino results from Borexino and main future perspectives
M. Pallavicini
Borexino is a solar neutrino experiment running at the Laboratori Nazionali del Gran Sasso, Italy. The radioactive background levels in the liquid scintillator target meet or even…
Measurement of the solar 8B neutrino rate with a liquid scintillator target and 3 MeV energy threshold in the Borexino detector
The Borexino Collaboration
We report the measurement of electron neutrino elastic scattering from 8B solar neutrinos with 3 MeV energy threshold by the Borexino detector in Gran Sasso (Italy). The rate of so…
The Borexino detector at the Laboratori Nazionali del Gran Sasso
Borexino Collaboration, G. Alimonti
Borexino, a large volume detector for low energy neutrino spectroscopy, is currently running underground at the Laboratori Nazionali del Gran Sasso, Italy. The main goal of the exp…
New results on solar neutrino fluxes from 192 days of Borexino data
The Borexino Collaboration
We report the direct measurement of the ^7Be solar neutrino signal rate performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso. The interaction rate of the…
Discovery of underground argon with low level of radioactive 39Ar and possible applications to WIMP dark matter detectors
C. Galbiati, R. Purtschert
We report on the first measurement of 39Ar in argon from underground natural gas reservoirs. The gas stored in the US National Helium Reserve was found to contain a low level of 39…
First real time detection of Be7 solar neutrinos by Borexino
Borexino Collaboration
This paper reports a direct measurement of the Be7 solar neutrino signal rate performed with the Borexino low background liquid scintillator detector. This is the first real-time s…
Pulse-Shape discrimination with the Counting Test Facility
H. O. Back et al.
Pulse shape discrimination (PSD) is one of the most distinctive features of liquid scintillators. Since the introduction of the scintillation techniques in the field of particle de…
A Search for Neutrinos from the Solar hep Reaction and the Diffuse Supernova Neutrino Background with the Sudbury Neutrino Observatory
The SNO Collaboration
A search has been made for neutrinos from the hep reaction in the Sun and from the diffuse supernova neutrino background (DSNB) using data collected during the first operational ph…
Electron Energy Spectra, Fluxes, and Day-Night Asymmetries of B Solar Neutrinos from the 391-Day Salt Phase SNO Data Set
SNO Collaboration
Results are reported from the complete salt phase of the Sudbury Neutrino Observatory experiment in which NaCl was dissolved in the DO target. The addition of salt enhanced the…
Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity
SNO Collaboration
The Sudbury Neutrino Observatory (SNO) has precisely determined the total active (nu_x) 8B solar neutrino flux without assumptions about the energy dependence of the nu_e survival…
Measurement of 222Rn dissolved in water at the Sudbury Neutrino Observatory
I. Blevis
The technique used at the Sudbury Neutrino Observatory (SNO) to measure the concentration of 222Rn in water is described. Water from the SNO detector is passed through a vacuum deg…
Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory
SNO Collaboration
Solar neutrinos from the decay of B have been detected at the Sudbury Neutrino Observatory (SNO) via the charged current (CC) reaction on deuterium and by the elastic scatterin…
The Sudbury Neutrino Observatory
The SNO Collaboration
The Sudbury Neutrino Observatory is a second generation water Cherenkov detector designed to determine whether the currently observed solar neutrino deficit is a result of neutrino…