scholarly journals Solar neutrino flare, megaton neutrino detectors and human space journey

2019 ◽  
Author(s):  
Daniele Fargion ◽  
Pietro Oliva ◽  
P. G. De Sanctis Lucentini ◽  
Silvia Pietroni ◽  
Fabio La Monaca ◽  
...  
Keyword(s):  
Solar Neutrino ◽  
Neutrino Detectors

(6Li,6He) measurements as an alternative calibration for solar neutrino detectors

1991 ◽  
Vol 44 (6) ◽  
pp. 2771-2775 ◽  
Author(s):  
E. Aschenauer ◽  
H. Dennert ◽  
W. Eyrich ◽  
A. Lehmann ◽  
M. Moosburger ◽  
...  
Keyword(s):  
Solar Neutrino ◽  
Neutrino Detectors

Development of In-loaded liquid scintillators for solar neutrino detectors

2005 ◽  
Vol 143 ◽  
pp. 487 ◽  
Author(s):  
C. Buck ◽  
I. Barabanov ◽  
O. Besida ◽  
L. Bezrukov ◽  
C. Cattadori ◽  
...  
Keyword(s):  
Solar Neutrino ◽  
Neutrino Detectors

SOLAR NEUTRINO DETECTORS AND (3He, t) CHARGE-EXCHANGE REACTIONS

News 99 ◽  
2002 ◽  
Author(s):  
M. FUJIWARA ◽  
H. AKIMUNE ◽  
I. DAITO ◽  
H. EJIRI ◽  
H. FUJIMURA ◽  
...  
Keyword(s):  
Charge Exchange ◽  
Solar Neutrino ◽  
Exchange Reactions ◽  
Neutrino Detectors

scholarly journals Accelerator calibration of solar neutrino detectors

1993 ◽  
Vol 314 (2) ◽  
pp. 185-189
Author(s):  
E.G. Adelberger ◽  
L. DeBraeckeleer ◽  
W.C. Haxton ◽  
K.A. Snover
Keyword(s):  
Solar Neutrino ◽  
Neutrino Detectors

Study of GaAs as a material for solar neutrino detectors

2000 ◽  
Vol 439 (2-3) ◽  
pp. 651-661 ◽  
Author(s):  
A.V. Markov ◽  
A.Y. Polyakov ◽  
N.B. Smirnov ◽  
A.V. Govorkov ◽  
V.K. Eremin ◽  
...  
Keyword(s):  
Solar Neutrino ◽  
Neutrino Detectors

NEUTRINOS FROM SUPERNOVA EXPLOSION AND THE MIKHEYEV-SMIRNOV-WOLFENSTEIN EFFECT

1987 ◽  
Vol 02 (11) ◽  
pp. 827-834 ◽  
Author(s):  
HISAKAZU MINAKATA ◽  
HIROSHI NUNOKAWA ◽  
KIYOSHI SHIRAISHI ◽  
HIROSHI SUZUKI
Keyword(s):  
Solar Neutrino ◽  
Supernova Explosion ◽  
Mixing Angles ◽  
Neutrino Detectors ◽  
Electron Neutrinos ◽  
The Earth

It is shown that by taking the effect of the Earth into account the possible observation of electron neutrinos from the supernova SN1987A at the Kamiokande II is compatible with the solution of the solar neutrino puzzle by the Mikheyev-Smirnov-Wolfenstein mechanism. Our scenario requires relatively large mixing angles sin 2 2θ ≳ 0.3 and, most probably, ∆m2 of the order of 10−6 ~ 10−5 (eV) 2. The implications of possible observation in other neutrino detectors are briefly discussed.

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