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Title: Reactor antineutrino anomaly

Journal Article · · Physical Review. D, Particles Fields
;  [1]; ;  [1]; ; ;  [2]
  1. CEA, Irfu, SPP, Centre de Saclay, F-91191 Gif-sur-Yvette (France)
  2. CEA, Irfu, SPhN, Centre de Saclay, F-91191 Gif-sur-Yvette (France)

Recently, new reactor antineutrino spectra have been provided for {sup 235}U, {sup 239}Pu, {sup 241}Pu, and {sup 238}U, increasing the mean flux by about 3%. To a good approximation, this reevaluation applies to all reactor neutrino experiments. The synthesis of published experiments at reactor-detector distances <100 m leads to a ratio of observed event rate to predicted rate of 0.976{+-}0.024. With our new flux evaluation, this ratio shifts to 0.943{+-}0.023, leading to a deviation from unity at 98.6% C.L. which we call the reactor antineutrino anomaly. The compatibility of our results with the existence of a fourth nonstandard neutrino state driving neutrino oscillations at short distances is discussed. The combined analysis of reactor data, gallium solar neutrino calibration experiments, and MiniBooNE-{nu} data disfavors the no-oscillation hypothesis at 99.8% C.L. The oscillation parameters are such that |{Delta}m{sub new}{sup 2}|>1.5 eV{sup 2} (95%) and sin{sup 2}(2{theta}{sub new})=0.14{+-}0.08 (95%). Constraints on the {theta}{sub 13} neutrino mixing angle are revised.

OSTI ID:
21537700
Journal Information:
Physical Review. D, Particles Fields, Vol. 83, Issue 7; Other Information: DOI: 10.1103/PhysRevD.83.073006; (c) 2011 American Institute of Physics; ISSN 0556-2821
Country of Publication:
United States
Language:
English