88 research outputs found
Low energy neutrino astronomy with the large liquid scintillation detector LENA
The detection of low energy neutrinos in a large scintillation detector may
provide further important information on astrophysical processes as supernova
physics, solar physics and elementary particle physics as well as geophysics.
In this contribution, a new project for Low Energy Neutrino Astronomy (LENA)
consisting of a 50kt scintillation detector is presented.Comment: Proccedings of the International School of Nuclear Physics, Neutrinos
in Cosmology, in Astro, Particle and Nuclear Physics, Erice (SICILY) 16 - 24
Sept. 200
Optical Scattering Lengths in Large Liquid-Scintillator Neutrino Detectors
For liquid-scintillator neutrino detectors of kiloton scale, the transparency
of the organic solvent is of central importance. The present paper reports on
laboratory measurements of the optical scattering lengths of the organic
solvents PXE, LAB, and Dodecane which are under discussion for next-generation
experiments like SNO+, Hanohano, or LENA. Results comprise the wavelength range
from 415 to 440nm. The contributions from Rayleigh and Mie scattering as well
as from absorption/re-emission processes are discussed. Based on the present
results, LAB seems to be the preferred solvent for a large-volume detector.Comment: 9 pages, 3 figures, accepted for publication by Rev. Scient. Instr
Detection potential for the diffuse supernova neutrino background in the large liquid-scintillator detector LENA
The large-volume liquid-scintillator detector LENA (Low Energy Neutrino
Astronomy) will provide high-grade background discrimination and enable the
detection of diffuse supernova neutrinos (DSN) in an almost background-free
energy window from ~10 to 25 MeV. Within ten years of exposure, it will be
possible to derive significant constraints on both core-collapse supernova
models and the supernova rate in the near universe up to redshifts z<2.Comment: 11 pages, 8 figures. accepted for publication in Phys. Rev. D.
accepted for publication in Phys. Rev.
Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun
The Sun is fueled by a series of nuclear reactions that produce the energy
that makes it shine. The primary reaction is the fusion of two protons into a
deuteron, a positron and a neutrino. These neutrinos constitute the vast
majority of neutrinos reaching Earth, providing us with key information about
what goes on at the core of our star. Several experiments have now confirmed
the observation of neutrino oscillations by detecting neutrinos from secondary
nuclear processes in the Sun; this is the first direct spectral measurement of
the neutrinos from the keystone proton-proton fusion. This observation is a
crucial step towards the completion of the spectroscopy of pp-chain neutrinos,
as well as further validation of the LMA-MSW model of neutrino oscillations.Comment: Proceedings from NOW (Neutrino Oscillation Workshop) 201
Recommended from our members
Lifetime measurements of 214Po and 212Po with the CTF liquid scintillator detector at LNGS
We have studied the alpha decays of 214Po into 210Pb and of 212Po into 208Pb
tagged by the coincidence with the preceding beta decays from 214Bi and 212Bi,
respectively. The employed 222Rn, 232Th, and 220Rn sources were sealed inside
quartz vials and inserted in the Counting Test Facility at the underground Gran
Sasso National Laboratory in Italy. We find that the mean lifetime of 214Po is
(236.00 +- 0.42(stat) +- 0.15(syst)) \mu s and that of 212Po is (425.1 +-
0.9(stat) +- 1.2(syst)) ns. Our results, obtained from data with
signal-to-background ratio larger than 1000, reduce the overall uncertainties
and are compatible with previous measurements.Comment: RevTex, 11 pages, 5 figures, 3 tables. This second version matches
the one accepted for publication in EPJA: minor stylistic changes plus a
discussion of calibration of TDC time scal
Measurement of CNGS muon neutrino speed with Borexino
We have measured the speed of muon neutrinos with the Borexino detector using
short-bunch CNGS beams. The final result for the difference in time-of-flight
between a =17 GeV muon neutrino and a particle moving at the speed of light
in vacuum is {\delta}t = 0.8 \pm 0.7stat \pm 2.9sys ns, well consistent with
zero.Comment: 6 pages, 5 figure
Indication for the disappearance of reactor electron antineutrinos in the Double Chooz experiment
The Double Chooz Experiment presents an indication of reactor electron
antineutrino disappearance consistent with neutrino oscillations. A ratio of
0.944 0.016 (stat) 0.040 (syst) observed to predicted events was
obtained in 101 days of running at the Chooz Nuclear Power Plant in France,
with two 4.25 GW reactors. The results were obtained from a single 10
m fiducial volume detector located 1050 m from the two reactor cores. The
reactor antineutrino flux prediction used the Bugey4 measurement as an anchor
point. The deficit can be interpreted as an indication of a non-zero value of
the still unmeasured neutrino mixing parameter \sang. Analyzing both the rate
of the prompt positrons and their energy spectrum we find \sang = 0.086
0.041 (stat) 0.030 (syst), or, at 90% CL, 0.015 \sang 0.16.Comment: 7 pages, 4 figures, (new version after PRL referee's comments
JUNO Conceptual Design Report
The Jiangmen Underground Neutrino Observatory (JUNO) is proposed to determine
the neutrino mass hierarchy using an underground liquid scintillator detector.
It is located 53 km away from both Yangjiang and Taishan Nuclear Power Plants
in Guangdong, China. The experimental hall, spanning more than 50 meters, is
under a granite mountain of over 700 m overburden. Within six years of running,
the detection of reactor antineutrinos can resolve the neutrino mass hierarchy
at a confidence level of 3-4, and determine neutrino oscillation
parameters , , and to
an accuracy of better than 1%. The JUNO detector can be also used to study
terrestrial and extra-terrestrial neutrinos and new physics beyond the Standard
Model. The central detector contains 20,000 tons liquid scintillator with an
acrylic sphere of 35 m in diameter. 17,000 508-mm diameter PMTs with high
quantum efficiency provide 75% optical coverage. The current choice of
the liquid scintillator is: linear alkyl benzene (LAB) as the solvent, plus PPO
as the scintillation fluor and a wavelength-shifter (Bis-MSB). The number of
detected photoelectrons per MeV is larger than 1,100 and the energy resolution
is expected to be 3% at 1 MeV. The calibration system is designed to deploy
multiple sources to cover the entire energy range of reactor antineutrinos, and
to achieve a full-volume position coverage inside the detector. The veto system
is used for muon detection, muon induced background study and reduction. It
consists of a Water Cherenkov detector and a Top Tracker system. The readout
system, the detector control system and the offline system insure efficient and
stable data acquisition and processing.Comment: 328 pages, 211 figure
Measurements of extremely low radioactivity levels in BOREXINO
The techniques researched, developed and applied towards the measurement of
radioisotope concentrations at ultra-low levels in the real-time solar neutrino
experiment BOREXINO at Gran Sasso are presented and illustrated with specific
results of widespread interest. We report the use of low-level germanium gamma
spectrometry, low-level miniaturized gas proportional counters and low
background scintillation detectors developed in solar neutrino research. Each
now sets records in its field. We additionally describe our techniques of
radiochemical ultra-pure, few atom manipulations and extractions. Forefront
measurements also result from the powerful combination of neutron activation
and low-level counting. Finally, with our techniques and commercially available
mass spectrometry and atomic absorption spectroscopy, new low-level detection
limits for isotopes of interest are obtained.Comment: 27 pages, 5 figures. Submitted to Astroparticle Physics (17 Sep
2001). Spokesperson of the Borexino Collaboration: G. Bellini. Corresponding
author: W. Hampe
The SOX experiment in the neutrino physics
SOX (Short distance neutrino Oscillations with BoreXino) is a new experiment that takes place at the Laboratori Nazionali del Gran Sasso (LNGS) and it exploits the Borexino detector to study the neutrino oscillations at short distance. In different phases, by using two artificial sources Cr-51 and Ce-144-Pr-144, neutrino and antineutrino fluxes of measured intensity will be detected by Borexino in order to observe possible neutrino oscillations in the sterile state. In this paper an overview of the experiment is given and one of the two calorimeters that will be used to measure the source activity is described. At the end the expected sensitivity to determine the neutrino sterile mass is shown
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