AbstractLENA (Low Energy Neutrino Astronomy) has been proposed as a next generation 50 kt liquid scintillator detector. The large target mass allows a high precision measurement of the solar 8B neutrino spectrum, with an unprecedented energy threshold of 2 MeV. Hence, it can probe the MSW-LMA prediction for the electron neutrino survival probability in the transition region between vacuum and matter-dominated neutrino oscillations. Based on Monte Carlo simulations of the solar neutrino and the corresponding background spectra, it was found that the predicted upturn of the solar 8B neutrino spectrum can be detected with 5σ significance after 5 years
Dark matter detectors will soon be sensitive to Solar neutrinos via two distinct channels: coherent ...
Neutrinos produced in the Sun by electron capture reactions on 13 N, 15 O and 17 F, to which we refe...
Thanks to the excellent levels of achieved radiopurity and to the accurate data analysis techniques,...
LENA ( L ow E nergy N eutrino A stronomy) has been proposed as a next generation 50 kt liquid scinti...
AbstractLENA (Low Energy Neutrino Astronomy) has been proposed as a next generation 50 kt liquid sci...
LENA (Low Energy Neutrino Astronomy) has been proposed as a next generation 50 kt liquid scintillato...
LENA (Low Energy Neutrino Astronomy) is a proposed next-generation neutrino detector based on 50 kil...
The detection of low energy neutrinos in a large scintillation detector may provide further importan...
AbstractLENA (Low Energy Neutrino Astronomy) is a proposed next-generation neutrino detector based o...
As part of the European LAGUNA design study on a next-generation neutrino detector, we propose the ...
AbstractScintillator detectors are known for their good light yield, energy resolution, timing chara...
Low-energy solar neutrino detection plays a fundamental role in understanding both solar astrophysic...
AbstractWe show that liquid organic scintillator detectors (e.g., KamLAND and Borexino) can measure ...
Several proposals for studying neutrinos with large detectors are currently under discussion. We sug...
We show that liquid organic scintillator detectors (e.g., KamLAND and Borexino) can measure the 8B s...
Dark matter detectors will soon be sensitive to Solar neutrinos via two distinct channels: coherent ...
Neutrinos produced in the Sun by electron capture reactions on 13 N, 15 O and 17 F, to which we refe...
Thanks to the excellent levels of achieved radiopurity and to the accurate data analysis techniques,...
LENA ( L ow E nergy N eutrino A stronomy) has been proposed as a next generation 50 kt liquid scinti...
AbstractLENA (Low Energy Neutrino Astronomy) has been proposed as a next generation 50 kt liquid sci...
LENA (Low Energy Neutrino Astronomy) has been proposed as a next generation 50 kt liquid scintillato...
LENA (Low Energy Neutrino Astronomy) is a proposed next-generation neutrino detector based on 50 kil...
The detection of low energy neutrinos in a large scintillation detector may provide further importan...
AbstractLENA (Low Energy Neutrino Astronomy) is a proposed next-generation neutrino detector based o...
As part of the European LAGUNA design study on a next-generation neutrino detector, we propose the ...
AbstractScintillator detectors are known for their good light yield, energy resolution, timing chara...
Low-energy solar neutrino detection plays a fundamental role in understanding both solar astrophysic...
AbstractWe show that liquid organic scintillator detectors (e.g., KamLAND and Borexino) can measure ...
Several proposals for studying neutrinos with large detectors are currently under discussion. We sug...
We show that liquid organic scintillator detectors (e.g., KamLAND and Borexino) can measure the 8B s...
Dark matter detectors will soon be sensitive to Solar neutrinos via two distinct channels: coherent ...
Neutrinos produced in the Sun by electron capture reactions on 13 N, 15 O and 17 F, to which we refe...
Thanks to the excellent levels of achieved radiopurity and to the accurate data analysis techniques,...