Coherent elastic neutrino-nucleus scattering at the European Spallation Source

被引:0
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作者
D. Baxter
J. I. Collar
P. Coloma
C. E. Dahl
I. Esteban
P. Ferrario
J. J. Gomez-Cadenas
M.C. Gonzalez-Garcia
A. R. L. Kavner
C. M. Lewis
F. Monrabal
J. Munõz Vidal
P. Privitera
K. Ramanathan
J. Renner
机构
[1] University of Chicago,Enrico Fermi Institute, Kavli Institute for Cosmological Physics, and Department of Physics
[2] Instituto de Física Corpuscular,Department of Physics and Astronomy
[3] Universitat de Valéncia and CSIC,undefined
[4] Edificio Institutos Investigación,undefined
[5] Northwestern University,undefined
[6] Fermi National Accelerator Laboratory,undefined
[7] Departament de Fisica Quantica i Astrofisica and Institut de Ciencies del Cosmos,undefined
[8] Universitat de Barcelona,undefined
[9] Donostia International Physics Center (DIPC),undefined
[10] Ikerbasque,undefined
[11] Basque Foundation for Science,undefined
[12] Institució Catalana de Recerca i Estudis Avancats (ICREA),undefined
[13] C.N. Yang Institute for Theoretical Physics,undefined
[14] Stony Brook University,undefined
[15] Donostia International Physics Center (DIPC),undefined
[16] Instituto Gallego de Física de Altas Energías,undefined
[17] Univ. de Santiago de Compostela,undefined
关键词
Neutrino Detectors and Telescopes (experiments); Beyond Standard Model; Electroweak interaction;
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摘要
The European Spallation Source (ESS), presently well on its way to completion, will soon provide the most intense neutron beams for multi-disciplinary science. Fortuitously, it will also generate the largest pulsed neutrino flux suitable for the detection of Coherent Elastic Neutrino-Nucleus Scattering (CEνNS), a process recently measured for the first time at ORNL’s Spallation Neutron Source. We describe innovative detector technologies maximally able to profit from the order-of-magnitude increase in neutrino flux provided by the ESS, along with their sensitivity to a rich particle physics phenomenology accessible through high-statistics, precision CEνNS measurements.
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