English

The Fine Structure Constant and Habitable Planets

Cosmology and Nongalactic Astrophysics 2016-10-18 v1 Earth and Planetary Astrophysics High Energy Physics - Theory

Abstract

We use the existence of habitable planets to impose anthropic requirements on the fine structure constant, α\alpha. 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 α1\alpha^{-1} to be 145±50145\pm 50. The second, that radiogenic heat in the Earth's interior remains adequately productive for billions of years, restricts it to be 145±9145\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.

Keywords

Cite

@article{arxiv.1604.03151,
  title  = {The Fine Structure Constant and Habitable Planets},
  author = {McCullen Sandora},
  journal= {arXiv preprint arXiv:1604.03151},
  year   = {2016}
}

Comments

24 pages, 4 figures

R2 v1 2026-06-22T13:29:50.691Z