Improved global fit to Non-Standard neutrino Interactions using COHERENT energy and timing data

被引:76
作者
Coloma, Pilar [1 ,2 ]
Esteban, Ivan [3 ,4 ]
Gonzalez-Garcia, M. C. [3 ,4 ,5 ,6 ]
Maltoni, Michele [7 ]
机构
[1] Univ Valencia, Inst Fis Corpuscular, Edificio Inst Invest, E-46980 Valencia, Spain
[2] CSIC, Edificio Inst Invest, E-46980 Valencia, Spain
[3] Univ Barcelona, Dept Fis Quant & Astrofis, Diagonal 647, E-08028 Barcelona, Spain
[4] Univ Barcelona, Inst Ciencies Cosmos, Diagonal 647, E-08028 Barcelona, Spain
[5] ICREA, Pg Lluis Companys 23, E-08010 Barcelona, Spain
[6] SUNY Stony Brook, CN Yang Inst Theoret Phys, Stony Brook, NY 11794 USA
[7] Univ Autonoma Madrid, CSIC, Inst Fis Teor, Calle Nicolas Cabrera 13-15, E-28049 Madrid, Spain
基金
欧盟地平线“2020”;
关键词
Beyond Standard Model; Neutrino Physics; Solar and Atmospheric Neutrinos; MASSLESS NEUTRINOS; OSCILLATIONS; MATTER;
D O I
10.1007/JHEP02(2020)023
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We perform a global fit to neutrino oscillation and coherent neutrino-nucleus scattering data, using both timing and energy information from the COHERENT experiment. The results are used to set model-independent bounds on four-fermion effective operators inducing non-standard neutral-current neutrino interactions. We quantify the allowed ranges for their Wilson coefficients, as well as the status of the LMA-D solution, for a wide class of new physics models with arbitrary ratios between the strength of the operators involving up and down quarks. Our results are presented for the COHERENT experiment alone, as well as in combination with the global data from oscillation experiments. We also quantify the dependence of our results for COHERENT with respect to the choice of quenching factor, nuclear form factor, and the treatment of the backgrounds.
引用
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页数:30
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