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- W4313304090 abstract "A precise and model-independent determination of the neutron distribution radius ${R}_{n}$ and thus the neutron skin thickness ${R}_{mathrm{skin}}$ of atomic nuclei is of fundamental importance in nuclear physics, particle physics, and astrophysics but remains a big challenge in terrestrial labs. We argue that the nearby core-collapse supernova (CCSN) in our Galaxy may render a neutrino flux with unprecedentedly high luminosity, offering the perfect opportunity to determine the ${R}_{n}$ and ${R}_{mathrm{skin}}$ through the coherent elastic neutrino-nucleus scattering ($mathrm{CE}ensuremath{nu}mathrm{NS}$). We evaluate the potential of determining the ${R}_{n}$ of lead (Pb) via $mathrm{CE}ensuremath{nu}mathrm{NS}$ with the nearby CCSN neutrinos in the RES-NOVA project which is designed to hunt CCSN neutrinos using an array of archaeological Pb based cryogenic detectors. We find that an ultimate precision of $ensuremath{sim}0.1%$ for the ${R}_{n}$ ($ensuremath{sim}0.006text{ }text{ }mathrm{fm}$ for the ${R}_{mathrm{skin}}$) of Pb can be achieved via RES-NOVA in the most optimistic case that the CCSN explosion were to occur at a distance of $ensuremath{sim}1text{ }text{ }mathrm{kpc}$ from the Earth." @default.
- W4313304090 created "2023-01-06" @default.
- W4313304090 creator A5067364245 @default.
- W4313304090 creator A5089253675 @default.
- W4313304090 date "2022-12-30" @default.
- W4313304090 modified "2023-10-14" @default.
- W4313304090 title "Supernova neutrinos as a precise probe of nuclear neutron skin" @default.
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- W4313304090 doi "https://doi.org/10.1103/physrevd.106.123034" @default.
- W4313304090 hasPublicationYear "2022" @default.
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