Results 31 to 40 of about 35,525 (205)
Potential for a precision measurement of solar pp neutrinos in the Serappis experiment
The Serappis (SEarch for RAre PP-neutrinos In Scintillator) project aims at a precision measurement of the flux of solar pp neutrinos on the few-percent level.
Lukas Bieger +58 more
doaj +1 more source
Detecting the upturn of the solar 8B neutrino spectrum with LENA
LENA (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 ...
R. Möllenberg +7 more
doaj +1 more source
Highlight Talk from Super-Kamiokande
Super-Kamiokande (SK), a 50 kton water Cherenkov detector in Japan, is observing both atmospheric and solar neutrinos. It is also searching for supernova (relic) neutrinos, proton decays and dark matter-like particles. A three-flavor oscillation analysis
Yuuki Nakano +1 more
doaj +1 more source
Doublet-Singlet Oscillations and Dark Matter Neutrinos [PDF]
We examine the `singlet majoron model' first introduced by Chikashige, Mohapatra and Peccei as a simple extension of the standard model with massive Majorana neutrinos.
Okada, Nobuchika
core +2 more sources
Recent Borexino results and prospects for the near future
The Borexino experiment located in the Gran Sasso National Laboratory, is an organic liquid scintillator detector conceived for the real time spectroscopy of low energy solar neutrinos.
D’Angelo D. +95 more
doaj +1 more source
Solar neutrino spectroscopy [PDF]
More than forty years after the first detection of neutrinos from the Sun, the spectroscopy of solar neutrinos has proven to be an on-going success story. The long-standing puzzle about the observed solar neutrino deficit has been resolved by the discovery of neutrino flavor oscillations.
openaire +2 more sources
Projections for measuring the size of the solar core with neutrino-electron scattering [PDF]
We quantify the amount of data needed in order to measure the size and position of the $^8$B neutrino production region within the solar core, for experiments looking at elastic scattering between electrons and solar neutrinos.
Adams +43 more
core +2 more sources
ecCNO solar neutrinos: A challenge for gigantic ultra-pure liquid scintillator detectors
Neutrinos produced in the Sun by electron capture reactions on 13N, 15O and 17F, to which we refer as ecCNO neutrinos, are not usually considered in solar neutrino analysis since the expected fluxes are extremely low.
F.L. Villante
doaj +1 more source
Implications of CHOOZ results for the decoupling of solar and atmospheric neutrino oscillations
We have considered the results of solar and atmospheric neutrino oscillation experiments in the scheme of mixing of three neutrinos with a mass hierarchy.
Bilenky +13 more
core +1 more source
Possible tests of neutrino maximal mixing and comments on matter effects [PDF]
We show in a simple and general way that matter effects do not contribute to the averaged value of the probabilities of transition of solar $\nu_e$'s into other states in the case of maximal mixing of any number of massive neutrinos.
Bahcall +36 more
core +2 more sources

