Radiogenic power and geoneutrino luminosity of the Earth and other terrestrial bodies through time
arXiv:1912.04655 · doi:10.1029/2019GC008865
Abstract
We report the Earth's rate of radiogenic heat production and (anti)neutrino luminosity from geologically relevant short-lived radionuclides (SLR) and long-lived radionuclides (LLR) using decay constants from the geological community, updated nuclear physics parameters, and calculations of the spectra. We track the time evolution of the radiogenic power and luminosity of the Earth over the last 4.57 billion years, assuming an absolute abundance for the refractory elements in the silicate Earth and key volatile/refractory element ratios (e.g., Fe/Al, K/U, and Rb/Sr) to set the abundance levels for the moderately volatile elements. The relevant decays for the present-day heat production in the Earth ( TW) are from K, Rb, Sm, Th, U, and U. Given element concentrations in kg-element/kg-rock and density in kg/m, a simplified equation to calculate the present day heat production in a rock is: The radiogenic heating rate of Earth-like material at Solar System formation was some 10 to 10 times greater than present-day values, largely due to decay of Al in the silicate fraction, which was the dominant radiogenic heat source for the first Ma. Assuming instantaneous Earth formation, the upper bound on radiogenic energy supplied by the most powerful short-lived radionuclide Al ( = 0.7 Ma) is 5.510 J, which is comparable (within a factor of a few) to the planet's gravitational binding energy.
arXiv comment28 pages, 6 figures, 5 tables
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