Experimental parameters for a Cerium 144 based intense electron antineutrino generator experiment at very short baselines
Experimental parameters for a Cerium 144 based intense electron antineutrino generator experiment at very short baselines
复制标题
极短基线下基于铈 144 的强电子反中微子发生器实验的实验参数
DOI:
--
复制
发表时间:
2014
期刊:
影响因子:
--
通讯作者:
G. Tikhomirov
中科院分区:
文献类型:
--
作者:
J. Gaffiot;T. Lasserre;G. Mention;M. Vivier;M. Cribier;M. Durero;V. Fischer;A. Letourneau;Eric Dumonteil;I. Saldikov;G. Tikhomirov
The standard three-neutrino oscillation paradigm, associated with small squared mass splittings Δm 2 ≪ 0.1 eV 2 , has been successfully built up over the last 15 years using solar, atmospheric, long baseline accelerator and reactor neutrino experiments. However, this well-established picture might suffer from anomalous results reported at very short baselines in some of these experiments. If not experimental artifacts, such results could possibly be interpreted as the existence of at least an additional fourth sterile neutrino species, mixing with the known active flavors with an associated mass splitting Δm 2 new ≫ 0.01 eV 2 and being insensitive to standard weak interactions. Precision measurements at very short baselines (5–15 m) with intense MeV ¯ ν e emitters can be used to probe these anomalies. In this article, the expected ¯ ν e signal and backgrounds of a generic experiment which consists of deploying an intense β − radioactive source inside or in the vicinity of a large liquid scintillator detector are studied. The technical challenges to perform such an experiment are identified, along with quantifying the possible source-and detector-induced systematics and their impact on the sensitivity to the observation of neutrino oscillations at short baselines.