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arXiv · 1604.03151

The Fine Structure Constant and Habitable Planets

McCullen Sandora
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Abstract

We use the existence of habitable planets to impose anthropic requirements on the fine structure constant, $α$. To this effect, we present two considerations that restrict its value to be very near the one observed. The first, that the end product of stellar fusion is iron and not one of its neighboring elements, restricts $α^{-1}$ to be $145\pm 50$. The second, that radiogenic heat in the Earth's interior remains adequately productive for billions of years, restricts it to be $145\pm9$. A connection with the grand unified theory window is discussed, effectively providing a route to probe ultra-high energy physics with upcoming advances in planetary science.

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McCullen Sandora. 2016-04-04. The Fine Structure Constant and Habitable Planets. https://doi.org/10.1088/1475-7516%2F2016%2F08%2F048

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