Radioactive heat production of six geologically important nuclides
arXiv:1710.06721 · doi:10.1002/2017GC006997
Abstract
Heat production rates for the geologically important nuclides Al, K, Fe, Th, U, and U are calculated on the basis of recent data on atomic and nuclear properties. The revised data differ by several per cent from some older values, but indicate that more recent analyses converge toward values with an accuracy sufficient for all common geoscience applications, although some possibilities for improvement still remain, especially in the case of K and with regard to the determination of half-lives. A Python script is provided for calculating heat production (https://github.com/trg818/radheat).
14 pages, 1 figure
References in corpus (2)
Cited by in corpus (6)
- The influence of bulk composition on long-term interior-atmosphere evolution of terrestrial exoplanets
- Radiogenic power and geoneutrino luminosity of the Earth and other terrestrial bodies through time
- Magma ocean evolution at arbitrary redox state
- Modification of the radioactive heat budget of Earth-like exoplanets by the loss of primordial atmospheres
- Unlocking planetesimal magnetic field histories: a refined, versatile model for thermal evolution and dynamo generation
- Evolution of Mercury's Earliest Atmosphere