Neutrino Geoscience: Review, survey, future prospects
W. F. McDonough, H. Watanabe

TL;DR
Neutrino geoscience offers a promising approach to better understand Earth's internal heat sources by comparing physics measurements with geological models, addressing current uncertainties in radiogenic heat estimates.
Contribution
This review highlights the potential of neutrino detection to resolve discrepancies in Earth's radiogenic heat estimates and emphasizes future research directions in geoneutrino measurements.
Findings
Physics experiments suggest Earth's radiogenic heat is 15.3-38.2 TW.
Geological models estimate Earth's radiogenic heat at 20±10 TW.
Detection of oceanic geoneutrinos could clarify Earth's internal heat budget.
Abstract
The earth's surface heat flux is 463 TW (terrawatts, 10 watts). Although many assume we know the earth's abundance and distribution of radioactive heat producing elements (i.e., U, Th, and K), estimates for the mantle's heat production varying by an order of magnitude and recent particle physics findings challenge our dominant paradigm. Geologists predict the earth's budget of radiogenic power at 2010 TW, whereas particle physics experiments predict 15.3 TW (KamLAND, Japan) and 38.2 TW (Borexino, Italy). We welcome this opportunity to highlight the fundamentally important resource offered by the physics community and call attention to the shortcomings associated with the characterization of the geology of the earth. We review the findings from continent-based, physics experiments, the predictions from geology, and assess the degree of…
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Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Particle physics theoretical and experimental studies
