scholarly journals Global analysis of Solar neutrino oscillation evidence including SNO and implications for Borexino

2002 ◽  
Vol 634 (1-2) ◽  
pp. 393-409 ◽  
Author(s):  
P Aliani ◽  
V Antonelli ◽  
M Picariello ◽  
E Torrente-Lujan
2020 ◽  
Vol 2020 (12) ◽  
Author(s):  
Ivan Esteban ◽  
M. C. Gonzalez-Garcia ◽  
Michele Maltoni ◽  
Ivan Martinez-Soler ◽  
Jordi Salvado

In this addendum we re-assess the constraints on Non-Standard Interactions (NSI) from the global analysis of neutrino oscillation data after including the new results released since the publication of ref. [1], in particular those presented at the Neutrino2020 conference. The new data considered here includes the total energy spectrum and the day-night asymmetry of the 2970-day SK4 solar neutrino sample [2], as well as the latest results from long-baseline (LBL) experiments T2K [3, 4] and NOvA [5, 6]. In addition, we have updated the reactor experiments Double-Chooz [7, 8] to 1276/587 days of far/near detector data and RENO [9, 10] to 2908 days of exposure.


2004 ◽  
Vol 69 (1) ◽  
Author(s):  
G. L. Fogli ◽  
E. Lisi ◽  
A. Marrone ◽  
D. Montanino ◽  
A. Palazzo ◽  
...  

2002 ◽  
Vol 17 (22) ◽  
pp. 1455-1464 ◽  
Author(s):  
ABHIJIT BANDYOPADHYAY ◽  
SANDHYA CHOUBEY ◽  
SRUBABATI GOSWAMI ◽  
D. P. ROY

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.


1999 ◽  
Vol 14 (12) ◽  
pp. 1953-1974 ◽  
Author(s):  
T. SAKAI ◽  
O. INAGAKI ◽  
T. TESHIMA

We analyze the solar, terrestrial and atmospheric neutrino experiments including SuperKamiokande data using the three-flavor neutrinos framework and obtain the allowed region for parameters [Formula: see text]. In solar neutrino experiments, we obtain the large angle solution [Formula: see text] and small angle solution (3×10-6-1.2×10-5 eV 2, 0.003-0.01) for θ13=0°-20°. From the terrestrial and atmospheric neutrino experiments including the sub-GeV and multi-GeV zenith angle dependence in SuperKamiokande 535 days data, we found that the νμ-ντ mixing is large and the range of [Formula: see text] as 0.02~0.0002  eV 2. There is no significant difference between large θ12 angle solution and small one.


2002 ◽  
Vol 2002 (04) ◽  
pp. 007-007 ◽  
Author(s):  
John N Bahcall ◽  
M. Concepcion Gonzalez-Garcia ◽  
Carlos Peña-Garay

2015 ◽  
Vol 2015 (9) ◽  
Author(s):  
Johannes Bergström ◽  
M. C. Gonzalez-Garcia ◽  
Michele Maltoni ◽  
Thomas Schwetz

2001 ◽  
Vol 2001 (08) ◽  
pp. 014-014 ◽  
Author(s):  
John N Bahcall ◽  
M. Concha Gonzalez-Garcia ◽  
Carlos Peña-Garay

1990 ◽  
Vol 65 (11) ◽  
pp. 1301-1304 ◽  
Author(s):  
K. Hirata ◽  
K. Inoue ◽  
T. Kajita ◽  
T. Kifune ◽  
K. Kihara ◽  
...  

2016 ◽  
Vol 2016 ◽  
pp. 1-6 ◽  
Author(s):  
Deniz Yilmaz

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.


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