# Diagnosing the Reactor Antineutrino Anomaly with Global Antineutrino   Flux Data

**Authors:** C. Giunti, Y. F. Li, B. R. Littlejohn, P. T. Surukuchi

arXiv: 1901.01807 · 2019-04-24

## TL;DR

This paper analyzes recent reactor antineutrino measurements to understand the anomaly, finding that data favor incorrect isotope flux models over sterile neutrino explanations, with no strong preference for oscillations.

## Contribution

It provides a comprehensive global fit of new antineutrino flux data, evaluating hypotheses about the anomaly and the role of sterile neutrinos and isotope flux modeling.

## Key findings

- Global fits favor isotope flux mis-modeling over sterile neutrino oscillations.
- No significant preference for sterile neutrino oscillations when considering new data.
- Hybrid models with both oscillations and flux inaccuracies are only mildly favored.

## Abstract

We have examined the impact of new Daya Bay, Double Chooz, and RENO measurements on global fits of reactor antineutrino flux data to a variety of hypotheses regarding the origin of the reactor antineutrino anomaly. In comparing RENO and Daya Bay measurements of inverse beta decay (IBD) yield versus $^{239}$Pu fission fraction, we find differing levels of precision in measurements of time-integrated yield and yield slope, but similar central values, leading to modestly enhanced isotopic IBD yield measurements in a joint fit of the two datasets. In the absence of sterile neutrino oscillations, global fits to all measurements now provide 3{\sigma} preference for incorrect modeling of specific fission isotopes over common mis-modeling of all beta-converted isotopes. If sterile neutrino oscillations are considered, global IBD yield fits provide no substantial preference between oscillation-including and oscillation-excluding hypotheses: hybrid models containing both sterile neutrino oscillations and incorrect $^{235}$U or $^{239}$Pu flux predictions are favored at only 1-2{\sigma} with respect to models where $^{235}$U, $^{238}$U, and $^{239}$Pu are assumed to be incorrectly predicted.

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1901.01807/full.md

## References

54 references — full list in the complete paper: https://tomesphere.com/paper/1901.01807/full.md

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Source: https://tomesphere.com/paper/1901.01807