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Coherent elastic neutrino-nucleus scattering: Terrestrial and astrophysical applications
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Coherent elastic neutrino-nucleus scattering: Terrestrial and astrophysical applications
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Coherent elastic neutrino-nucleus scattering (CE$\nu$NS) is a process in which neutrinos scatter on a nucleus which acts as a single particle. Though the total cross section is large by neutrino standards, CE$\nu$NS has long proven difficult to detect, since the deposited energy into the nucleus is $\sim$ keV. In 2017, the COHERENT collaboration announced the detection of CE$\nu$NS using a stopped-pion source with CsI detectors, followed up the detection of CE$\nu$NS using an Ar target. The detection of CE$\nu$NS has spawned a flurry of activities in high-energy physics, inspiring new constraints on beyond the Standard Model (BSM) physics, and new experimental methods. The CE$\nu$NS process has important implications for not only high-energy physics, but also astrophysics, nuclear physics, and beyond. This whitepaper discusses the scientific importance of CE$\nu$NS, highlighting how present experiments such as COHERENT are informing theory, and also how future experiments will provide a wealth of information across the aforementioned fields of physics.
Forward citations
Cited by 6 Pith papers
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Searches for heavy neutral lepton decays at spallation neutron sources
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$\texttt{SNuDD}$: Solar Neutrinos for Direct Detection
SNuDD computes solar-neutrino recoil spectra with non-standard interactions and derives NSI limits from xenon direct-detection data that are competitive with dedicated neutrino experiments.
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Refined extraction of electroweak and nuclear parameters from germanium CE$\nu$NS data
Combined fit of two germanium CEνNS datasets yields refined neutron radius, skin thickness, and sin²θ_W at low Q, presented versus Lindhard quenching variations and benchmarked against Shell Model form factors.
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Sterile Neutrino Mixing Parameters from Solar-Neutrino Coherent Scattering
Future dark matter detectors with ~3000 ton-yr exposure could probe sterile neutrino mixing with νμ and ντ in parameter space not reached by long-baseline or atmospheric searches.
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Cosmological dynamics and structure formation in a generalized mass-to-horizon entropy-inspired modified gravity
A thermodynamically inspired modified cosmology with parameter n changes expansion history and structure growth, claimed to falsify both flat and non-flat Lambda CDM while satisfying future thermodynamic equilibrium.
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