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The Possible Role of PeP Weak Interactions in the Early History of the Earth

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Abstract

The p(pe− v)d, reaction (Q = 1.442 MeV) is examined in view of the possible Gamow Factor Cancellation (GFC) theorized by Kim and Zubarev (1995). The lifetime for the pep reaction in a metal hydride environment, such as FeH in the core of the earth, was calculated to be 2.54E(+12) yrs. The duration of the earth’s melting and degassing prior to the formation of the oceans can be calculated using the present ratio D/H = 1.5E(−4) for the oceanic value, the pep lifetime in Fe and the primordial ratio of D/H = 2.6E(−5). The time interval was calculated to be 630 ± 160 million years, yielding an oceanic formation age of 3.92 billion years ago. The d(pe−, v)t, reaction (Q = 5.474 MeV) was also examined in view of the subsequent decay of tritium to 3He and its possible role as a radiochronometer.

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Ward, T.E. (2002). The Possible Role of PeP Weak Interactions in the Early History of the Earth. In: Manuel, O. (eds) Origin of Elements in the Solar System. Springer, Boston, MA. https://doi.org/10.1007/0-306-46927-8_40

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  • DOI: https://doi.org/10.1007/0-306-46927-8_40

  • Publisher Name: Springer, Boston, MA

  • Print ISBN: 978-0-306-46562-8

  • Online ISBN: 978-0-306-46927-5

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