Results 31 to 40 of about 6,622 (234)
Next generation direct dark matter detection experiments are favorable facilities to probe neutrino properties and light mediators beyond the Standard Model.
ShivaSankar K.A. +4 more
doaj +1 more source
Calculated Event Rates for Axion Detection via Atomic and Nuclear Processes
The possibility of detection of 5.5 MeV and 14.4 keV solar axions by observing axion‐induced nuclear and atomic transitions is investigated. The presence of nuclear transitions between spin orbit partners can be manifested by the subsequent deexcitation via gamma ray emissions.
John D. Vergados +3 more
wiley +1 more source
The couplings between the neutrinos and exotic fermion can be probed in both neutrino scattering experiments and dark matter direct detection experiments.
Zikang Chen, Tong Li, Jiajun Liao
doaj +1 more source
Erstmalige Beobachtung des CNO‐Zyklus
Vor 80 Jahren schlugen Carl Friedrich von Weizsäcker und Hans Bethe den sogenannten CNO‐Zyklus als mögliche Energiequelle für die Sterne vor. Bis vor kurzem ließ sich dieser Fusionsmechanismus in der Sonne jedoch experimentell nicht nachweisen. Dies gelang jetzt mit dem Neutrinodetektor Borexino.
Kai Zuber
wiley +1 more source
Correlated and integrated directionality for sub-MeV solar neutrinos in Borexino [PDF]
Liquid scintillator detectors play a central role in the detection of neutrinos from various sources. In particular, it is the only technique used so far for the precision spectroscopy of sub-MeV solar neutrinos, as demonstrated by the Borexino ...
M. Agostini +96 more
semanticscholar +1 more source
Understanding the Sun: Borexino [PDF]
Solar neutrinos have been detected over the past 40 years providing the first evidence of physics beyond the Standard Model for elementary particle interactions. The hypothesis of neutrino oscillations has offered a solution to the long-standing solar neutrino problem (missing solar neutrinos).
Aldo Ianni
openalex +2 more sources
Solar neutrinos from the CNO fusion cycle: Borexino discovery and implications for the solar physics
Our Sun is powered by the fusion of hydrogen into helium that proceeds in the solar core via two distinct mechanisms: dominant proton-proton ( pp ) chain and sub-dominant Carbon-Nitrogen-Oxygen (CNO) cycle. Solar neutrinos are emitted in electron-flavour
L. Ludhova
semanticscholar +1 more source
We explore the implications of the Borexino experiment’s real time measurements of the lowest energy part of the neutrino spectrum from the primary pp fusion process up to 0.420 MeV through the 7Be decay at 0.862 MeV to the pep reaction at 1.44 MeV.
Amir N. Khan, Douglas W. McKay
doaj +1 more source
Updating neutrino magnetic moment constraints
In this paper we provide an updated analysis of the neutrino magnetic moments (NMMs), discussing both the constraints on the magnitudes of the three transition moments Λi and the role of the CP violating phases present both in the mixing matrix and in ...
B.C. Cañas +4 more
doaj +1 more source
Low background techniques for the Borexino nylon vessels [PDF]
Borexino is an organic liquid scintillator underground detector for low energy solar neutrinos. The experiment has to satisfy extremely stringent low background requirements.
Pocar, A.
core +3 more sources

