Constraining the solar neutrino survival probability curve by using Li6 , Li7 , C12 , O18 , F19 , and Ca42 nuclear targets

2021 ◽  
Vol 104 (1) ◽  
Author(s):  
Y. Fujita ◽  
K. Zuber ◽  
H. Fujita
Keyword(s):  
Solar Neutrino ◽  
Survival Probability ◽  
Probability Curve ◽  
Nuclear Targets

scholarly journals WHAT CAN SNO NEUTRAL CURRENT RATE TEACH US ABOUT THE SOLAR NEUTRINO ANOMALY

2002 ◽  
Vol 17 (22) ◽  
pp. 1455-1464 ◽  
Author(s):  
ABHIJIT BANDYOPADHYAY ◽  
SANDHYA CHOUBEY ◽  
SRUBABATI GOSWAMI ◽  
D. P. ROY
Keyword(s):  
Neutrino Oscillation ◽  
Solar Neutrino ◽  
Survival Probability ◽  
Neutral Current ◽  
Neutrino Flux ◽  
Mixing Parameters ◽  
Active Neutrino ◽  
Quantitative Analyses

We investigate how the anticipated neutral current rate from SNO will sharpen our understanding of the solar neutrino anomaly. Quantitative analyses are performed with representative values of this rate in the expected range of 0.8–1.2. This would provide a 5–10σ signal for νe transition into a state containing an active neutrino component. Assuming this state to be purely active one can estimate both the 8 B neutrino flux and the νe survival probability to a much higher precision than currently possible. Finally the measured value of the NC rate will have profound implications for the mass and mixing parameters of the solar neutrino oscillation solution.

scholarly journals Combined Effect of NSI and SFP on Solar Electron Neutrino Oscillation

2016 ◽  
Vol 2016 ◽  
pp. 1-6 ◽  
Author(s):  
Deniz Yilmaz
Keyword(s):  
Neutrino Oscillation ◽  
Solar Neutrino ◽  
Survival Probability ◽  
Low Energy ◽  
Electron Neutrino ◽  
Combined Effect ◽  
Neutrino Interaction ◽  
Dirac Particles ◽  
Electron Neutrinos ◽  
Neutrino Experiments

The combined effect of spin-flavor precession (SFP) and the nonstandard neutrino interaction (NSI) on the survival probability of solar electron neutrinos (assumed to be Dirac particles) is examined for various values ofϵ11,ϵ12, andμB. It is found that the neutrino survival probability curves affected by SFP and NSI effects individually for some values of the parameters (ϵ11,ϵ12, andμB) get close to the standard MSW curve when both effects are combined. Therefore, the combined effect of SFP and NSI needs to be taken into account when the solar electron neutrino data obtained by low energy solar neutrino experiments is investigated.

THE SOLAR NEUTRINO PROBLEM WITHIN MSW THEORY

1993 ◽  
Vol 08 (17) ◽  
pp. 1557-1562 ◽  
Author(s):  
S. ESPOSITO
Keyword(s):  
Solar Neutrino ◽  
Survival Probability ◽  
High Energy ◽  
Solar Neutrinos ◽  
Low Energy ◽  
Solar Neutrino Problem ◽  
High Energy Neutrinos

It is shown that the experiments on solar neutrinos can be accounted in terms of the Mikheyev-Smirnov-Wolfestein theory with ∆m2=6×10−6 eV 2 and sin 2 2θ=7×10−3. In the scenario proposed here the high energy neutrinos, from 8 B , have a survival probability around 1/3, the intermediate ones, around the 7 Be line a very small one ~ 2×10−3 and the low energy neutrinos, the ones coming from pp reactions, do not oscillate.

scholarly journals Study of the Solar Neutrino Survival Probability

1998 ◽  
Vol 81 (23) ◽  
pp. 5056-5059 ◽  
Author(s):  
C. M. Bhat ◽  
P. C. Bhat ◽  
M. Paterno ◽  
H. B. Prosper
Keyword(s):  
Solar Neutrino ◽  
Survival Probability

Temporal variation in annual survival probability of the Eurasian woodcock Scolopax rusticola wintering in France

2002 ◽  
Vol 8 (1) ◽  
pp. 21-30 ◽  
Author(s):  
Giacomo Tavecchia ◽  
Roger Pradel ◽  
François Gossmann ◽  
Claudine Bastat ◽  
Yves Ferrand ◽  
...  
Keyword(s):  
Temporal Variation ◽  
Survival Probability ◽  
Annual Survival ◽  
Scolopax Rusticola
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