scholarly journals Measurement of reactor antineutrino flux and spectrum at RENO

2021 ◽  
Vol 104 (11) ◽  
Author(s):  
S. G. Yoon ◽  
H. Seo ◽  
Z. Atif ◽  
J. H. Choi ◽  
H. I. Jang ◽  
...  
2017 ◽  
Vol 118 (25) ◽  
Author(s):  
F. P. An ◽  
A. B. Balantekin ◽  
H. R. Band ◽  
M. Bishai ◽  
S. Blyth ◽  
...  

2021 ◽  
Vol 2021 (3) ◽  
Author(s):  
Guillermo Fernandez-Moroni ◽  
Pedro A. N. Machado ◽  
Ivan Martinez-Soler ◽  
Yuber F. Perez-Gonzalez ◽  
Dario Rodrigues ◽  
...  

Abstract We analyze in detail the physics potential of an experiment like the one recently proposed by the vIOLETA collaboration: a kilogram-scale Skipper CCD detector deployed 12 meters away from a commercial nuclear reactor core. This experiment would be able to detect coherent elastic neutrino nucleus scattering from reactor neutrinos, capitalizing on the exceptionally low ionization energy threshold of Skipper CCDs. To estimate the physics reach, we elect the measurement of the weak mixing angle as a case study. We choose a realistic benchmark experimental setup and perform variations on this benchmark to understand the role of quenching factor and its systematic uncertainties, background rate and spectral shape, total exposure, and reactor antineutrino flux uncertainty. We take full advantage of the reactor flux measurement of the Daya Bay collaboration to perform a data driven analysis which is, up to a certain extent, independent of the theoretical un- certainties on the reactor antineutrino flux. We show that, under reasonable assumptions, this experimental setup may provide a competitive measurement of the weak mixing angle at few MeV scale with neutrino-nucleus scattering.


2019 ◽  
Author(s):  
Hyunkwan Seo

The smallest neutrino mixing angle \theta_{13}θ13 has been successfully measured by the disappearance of reactor antineutrinos at RENO, Daya Bay, and Double Chooz. The oscillation frequency is also measured based on energy and baseline dependent disappearance probability of reactor antineutrinos. Recent results find a variation in the observed reactor antineutrino flux as a function of the reactor fuel evolution. We report more precisely measured values of \theta_{13}θ13 and \Delta m_{ee}^2Δmee2 and results on the evolution of observed reactor antineutrino yield and spectrum.


2021 ◽  
Vol 2021 (1) ◽  
Author(s):  
Jeffrey M. Berryman ◽  
Patrick Huber

Abstract We present results from global fits to the available reactor antineutrino dataset, as of Fall 2019, to determine the global preference for a fourth, sterile neutrino. We have separately considered experiments that measure the integrated inverse-beta decay (IBD) rate from those that measure the energy spectrum of IBD events at one or more locations. The evidence that we infer from rate measurements varies between ≲ 3σ and negligible depending on the reactor antineutrino flux model employed. Moreover, we find that spectral ratios ostensibly imply ≳ 3σ evidence, consistent with previous work, though these measurements are known to be plagued by issues related to statistical interpretation; these results should therefore be viewed cautiously. The software used is the newly developed GLoBESfit tool set which is based on the publicly available GLoBES framework and will be released as open-source software.


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