REVIEW ON SOLAR NEUTRINO STUDIES BOREXINO

Author(s):  
I. Drachnev ◽  
M. Agostini ◽  
K. Altenmuller ◽  
S. Appel ◽  
V. Atroshchenko ◽  
...  
Keyword(s):  
1992 ◽  
Author(s):  
K. Lande ◽  
B. Cleveland ◽  
T. Daily ◽  
R. Davis ◽  
J. Distel ◽  
...  
Keyword(s):  

1986 ◽  
Vol 177 (1) ◽  
pp. 47-50 ◽  
Author(s):  
R.N. Mohapatra ◽  
J.W.F. Valle

1993 ◽  
Vol 93 (3-4) ◽  
pp. 785-790 ◽  
Author(s):  
S. R. Bandler ◽  
C. Enss ◽  
G. Goldhaber ◽  
R. E. Lanou ◽  
H. J. Maris ◽  
...  

1993 ◽  
Vol 08 (14) ◽  
pp. 1273-1284 ◽  
Author(s):  
JOÃO PULIDO

The possibility of unconventional neutrino scattering in the Sun via flavor changing neutral currents as a possible source of the solar neutrino deficit is investigated. If the effect is really significant, a resonant process will occur. Taking into account the neutrino deficit reported by the solar neutrino experiments (Kamiokande II, SAGE Gallex), one finds Δ2m21 = (0.6–1.4) × 10−5 eV 2 with no vacuum mixing and 0.16 ≤ fex ≤ 0.34 where fex is the lepton violating coupling. Our understanding of the neutrino phenomenon in the Sun may be improved through accuracy improvements in experiments measuring νee− elastic scattering or others searching for exotic lepton decays.


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