The possibility to use large amount of CdWO4 crystal scintillators to detect solar neutrino of low energies via neutrino capture reactions on 116Cd is investigated. The detector concept is based on placing CdWO4 crystals in liquid scintillator inside the sphere of 18 m in diameter, on which 9500 photomultipliers are installed. Such design makes possible event to place reconstruction inside CdWO4 crystal with accuracy 1 mm for 1 MeV electrons. Thus, expected background from random signal coincidences can be reduced to the rate ~300 events per year, which is of the same order magnitude as expected neutrino signal (260 ± 65 events per year in 30 ton of CdWO4), taking into account neutrino detection efficiency
New challenging questions in astro-particle physics are opened with the discovery of neu- trino mass...
The Jiangmen Underground Neutrino Observatory (JUNO) features a 20 kt multi-purpose underground liqu...
Neutrinos produced in the Sun by electron capture reactions on 13N, 15O and 17F, to which we refer a...
The usage of a large amount of CdTe(CdZnTe) semiconductor detectors for solar neutrino spectroscopy ...
A first measurement of neutrinos from the CNO fusion cycle in the Sun would allow a resolution to th...
In this paper, an application of silicon drift detectors (SDDs) as photodetectors for large inorgani...
This paper describes the main features of the proposed low energy solar neutrino detector Borexino, ...
The LENS project aims at the real-time spectroscopy of low energy solar neutrinos. Detection would p...
We show that liquid organic scintillator detectors (e.g., KamLAND and Borexino) can measure the 8B s...
Although it is well known that CaWO4 is a scintillator it is not often used, mainly because it has a...
The spectroscopy of solar neutrinos is now entering the precision era, after a golden age which has ...
Two methods are discussed for the solar neutrino spectroscopy in the sub-MeV region: absorption in a...
International audienceThe next generation of dark matter direct detection experiments will besensiti...
AbstractWe show that liquid organic scintillator detectors (e.g., KamLAND and Borexino) can measure ...
The LENS project aims at the real-time spectroscopy of low energy solar neutrinos. Detection would p...
New challenging questions in astro-particle physics are opened with the discovery of neu- trino mass...
The Jiangmen Underground Neutrino Observatory (JUNO) features a 20 kt multi-purpose underground liqu...
Neutrinos produced in the Sun by electron capture reactions on 13N, 15O and 17F, to which we refer a...
The usage of a large amount of CdTe(CdZnTe) semiconductor detectors for solar neutrino spectroscopy ...
A first measurement of neutrinos from the CNO fusion cycle in the Sun would allow a resolution to th...
In this paper, an application of silicon drift detectors (SDDs) as photodetectors for large inorgani...
This paper describes the main features of the proposed low energy solar neutrino detector Borexino, ...
The LENS project aims at the real-time spectroscopy of low energy solar neutrinos. Detection would p...
We show that liquid organic scintillator detectors (e.g., KamLAND and Borexino) can measure the 8B s...
Although it is well known that CaWO4 is a scintillator it is not often used, mainly because it has a...
The spectroscopy of solar neutrinos is now entering the precision era, after a golden age which has ...
Two methods are discussed for the solar neutrino spectroscopy in the sub-MeV region: absorption in a...
International audienceThe next generation of dark matter direct detection experiments will besensiti...
AbstractWe show that liquid organic scintillator detectors (e.g., KamLAND and Borexino) can measure ...
The LENS project aims at the real-time spectroscopy of low energy solar neutrinos. Detection would p...
New challenging questions in astro-particle physics are opened with the discovery of neu- trino mass...
The Jiangmen Underground Neutrino Observatory (JUNO) features a 20 kt multi-purpose underground liqu...
Neutrinos produced in the Sun by electron capture reactions on 13N, 15O and 17F, to which we refer a...