Authors: Gene H Barbee
Fusion determines the abundance of elements measured throughout space. It powers the sun and underlies the aging cycle of the stars. The author developed an atomic binding energy model [2] and this paper extends the model to the abundance of the elements. The model is largely independent of measured parameters and based on probabilities. The early universe consists of plasma until the temperature drops enough to allow electrons to form orbits around protons. Later, acoustic and gravitational forces become dominant and accumulation of mass into clusters, galaxies and clusters begins. The concentration process allows stars to “light up” with fusion when they become dense and hot. This is known in the literature as re-ionization. Early stars burn hydrogen and follow a well-documented aging cycle that depends on the kinetics of progressive fusion reactions. Literature contains the measured abundance of the heavy elements [8][7][11] produced by these reactions. Review
Comments: 17 Pages. Comments appreciated genebarbee@msn.coom
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[v1] 2013-08-01 21:25:22
[v2] 2014-06-04 15:47:04
[v3] 2015-01-09 17:50:24
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