Measuring solar neutrinos over gigayear timescales with paleo detectors

dc.contributor.authorTapia-Arellano, Nataliaen
dc.contributor.authorHoriuchi, Shunsakuen
dc.contributor.departmentCenter for Neutrino Physicsen
dc.date.accessioned2021-07-22T14:48:04Zen
dc.date.available2021-07-22T14:48:04Zen
dc.date.issued2021-06-15en
dc.description.abstractMeasuring the solar neutrino flux over gigayear timescales could provide a new window to inform the solar standard model as well as studies of the Earth's long-term climate. We demonstrate the feasibility of measuring the time evolution of the B-8 solar neutrino flux over gigayear timescales using paleo detectors, naturally occurring minerals which record neutrino-induced recoil tracks over geological times. We explore suitable minerals and identify track lengths of 15-30 nm to be a practical window to detect the B-8 solar neutrino flux. A collection of ultraradiopure minerals of different ages, each some 0.1 kg by mass, can be used to probe the rise of the B-8 solar neutrino flux over the recent gigayear of the Sun's evolution. We also show that the time-integrated tracks are sensitive to models of the Sun.en
dc.description.versionPublished versionen
dc.format.mimetypeapplication/pdfen
dc.identifier.doihttps://doi.org/10.1103/PhysRevD.103.123016en
dc.identifier.eissn2470-0029en
dc.identifier.issn2470-0010en
dc.identifier.issue12en
dc.identifier.other123016en
dc.identifier.urihttp://hdl.handle.net/10919/104256en
dc.identifier.volume103en
dc.language.isoenen
dc.rightsCreative Commons Attribution 4.0 Internationalen
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en
dc.titleMeasuring solar neutrinos over gigayear timescales with paleo detectorsen
dc.title.serialPhysical Review Den
dc.typeArticle - Refereeden
dc.type.dcmitypeTexten
dc.type.dcmitypeStillImageen

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