scholarly journals Neutrino decay confronts the SNO data

2003 ◽  
Vol 555 (1-2) ◽  
pp. 33-42 ◽  
Author(s):  
Abhijit Bandyopadhyay ◽  
Sandhya Choubey ◽  
Srubabati Goswami
Keyword(s):  
2021 ◽  
Vol 2021 (5) ◽  
Author(s):  
Kaustav Chakraborty ◽  
Debajyoti Dutta ◽  
Srubabati Goswami ◽  
Dipyaman Pramanik

Abstract We study the physics potential of the long-baseline experiments T2HK, T2HKK and ESSνSB in the context of invisible neutrino decay. We consider normal mass ordering and assume the state ν3 as unstable, decaying into sterile states during the flight and obtain constraints on the neutrino decay lifetime (τ3). We find that T2HK, T2HKK and ESSνSB are sensitive to the decay-rate of ν3 for τ3/m3 ≤ 2.72 × 10−11s/eV, τ3/m3 ≤ 4.36 × 10−11s/eV and τ3/m3 ≤ 2.43 × 10−11s/eV respectively at 3σ C.L. We compare and contrast the sensitivities of the three experiments and specially investigate the role played by the mixing angle θ23. It is seen that for experiments with flux peak near the second oscillation maxima, the poorer sensitivity to θ23 results in weaker constraints on the decay lifetime. Although, T2HKK has one detector close to the second oscillation maxima, having another detector at the first oscillation maxima results in superior sensitivity to decay. In addition, we find a synergy between the two baselines of the T2HKK experiment which helps in giving a better sensitivity to decay for θ23 in the higher octant. We discuss the octant sensitivity in presence of decay and show that there is an enhancement in sensitivity which occurs due to the contribution from the survival probability Pμμ is more pronounced for the experiments at the second oscillation maxima. We also obtain the combined sensitivity of T2HK+ESSνSB and T2HKK+ESSνSB as τ3/m3 ≤ 4.36 × 10−11s/eV and τ3/m3 ≤ 5.53 × 10−11s/eV respectively at 3σ C.L.


1986 ◽  
Vol 180 (4) ◽  
pp. 347-352 ◽  
Author(s):  
K. Enqvist ◽  
J. Maalampi
Keyword(s):  

2015 ◽  
Vol 2015 (11) ◽  
Author(s):  
Thamys Abrahão ◽  
Hisakazu Minakata ◽  
Hiroshi Nunokawa ◽  
Alexander A. Quiroga

2018 ◽  
Vol 2018 (2) ◽  
Author(s):  
Sandhya Choubey ◽  
Srubabati Goswami ◽  
Dipyaman Pramanik
Keyword(s):  

1986 ◽  
Vol 166 (4) ◽  
pp. 479-483 ◽  
Author(s):  
G. Bernardi ◽  
G. Carugno ◽  
J. Chauveau ◽  
F. Dicarlo ◽  
M. Dris ◽  
...  
Keyword(s):  

2013 ◽  
Vol 76 (12) ◽  
pp. 1541-1545 ◽  
Author(s):  
R. A. Anikin ◽  
N. V. Mikheev

1989 ◽  
Vol 67 (9) ◽  
pp. 904-911 ◽  
Author(s):  
S. Weisnagel ◽  
J. Law

The process of inner bremsstrahlung is examined for the β− decay of 3H. These radiative effects are then combined with atomic corrections in a more complete theoretical reference spectrum consisting of both light and heavy neutrino decay in accordance with recently published results of neutrino mass experiments. Due to the unusual nature of the experimental detector, final density of states is modified to provide a decay rate as a function of recorded energy. This reference spectrum is compared with experimental data using the exact method employed in the original analysis. It is found that previously reported low energy Kurie spectrum deviations are still present in the sample data, corresponding to a best fit for neutrino mass mν = 17.2 keV and mixing probability R = 2.5%. The origin of the difference between the conclusions reached here and those of earlier cited works is briefly discussed.


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