scholarly journals Improved short-baseline neutrino oscillation search and energy spectrum measurement with the PROSPECT experiment at HFIR

2021 ◽  
Vol 103 (3) ◽  
Author(s):  
M. Andriamirado ◽  
A. B. Balantekin ◽  
H. R. Band ◽  
C. D. Bass ◽  
D. E. Bergeron ◽  
...  
2010 ◽  
Vol 22 (3) ◽  
pp. 639-641
Author(s):  
廖树清 Liao Shuqing ◽  
张开志 Zhang Kaizhi ◽  
石金水 Shi Jinshui

2010 ◽  
Vol 22 (4) ◽  
pp. 918-922
Author(s):  
张信军 Zhang Xinjun ◽  
王亮平 Wang Liangping ◽  
呼义翔 Hu Yixiang ◽  
吴撼宇 Wu Hanyu ◽  
李岩 Li Yan

2019 ◽  
Vol 55 (8) ◽  
Author(s):  
Yonghao Chen ◽  
Guangyuan Luan ◽  
Jie Bao ◽  
Hantao Jing ◽  
Liying Zhang ◽  
...  

2015 ◽  
Vol 30 (20) ◽  
pp. 1530015
Author(s):  
Carlo Giunti

We consider the extension of standard three-neutrino mixing with the addition of one or two light sterile neutrinos which can explain the anomalies found in short-baseline neutrino oscillation experiments. We review the results of the global analyses of short-baseline neutrino oscillation data in [Formula: see text] and [Formula: see text] neutrino mixing schemes.


2016 ◽  
Vol 31 (01) ◽  
pp. 1650003 ◽  
Author(s):  
C. Giunti ◽  
E. M. Zavanin

We derive the relation between the amplitudes of short-baseline appearance and disappearance oscillations in [Formula: see text] neutrino mixing schemes which is the origin of the appearance–disappearance tension that is found from the analysis of the existing data in any [Formula: see text] neutrino mixing scheme. We illustrate the power of the relation to reveal the appearance–disappearance tension in the cases of [Formula: see text] and [Formula: see text] mixing using the results of global fits of short-baseline neutrino oscillation data.


2005 ◽  
Vol 20 (14) ◽  
pp. 3055-3058
Author(s):  
◽  
RICHARD GRAN

The K2K long-baseline neutrino oscillation experiment has analyzed all data including the period ending in February 2004. The total data sample is from 8.9 × 1019 protons on target. We observe 108 events at the far detector, Super-Kamiokande, when 150.9 + 11.6 - 10.0 were expected. Further, we observe a distortion of the neutrino energy spectrum which is consistent with νμ to ντ oscillation. The probability that we would observe these results if there is no neutrino oscillation is 0.011%, a 3.9 σ significance.


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