The Origin of Life from Primordial Planets
Carl H. Gibson (Univ. Cal. San Diego), Rudolph E. Schild (Harvard) and, N. C. Wickramasinghe (Cardiff Univ.)

TL;DR
This paper proposes that life originated on primordial hydrogen-helium planets formed shortly after the Big Bang, with evidence from cosmological models and space telescope observations supporting this hypothesis.
Contribution
It introduces a cosmological model linking dark matter, planet formation, and the origin of life, supported by observational data and supernovae chemical production mechanisms.
Findings
Hydrogen-helium planets as dark matter predicted by HGD cosmology.
Space telescope data supports the existence of primordial planets.
Supernovae contribute essential chemicals and water for early life.
Abstract
The origin of life and the origin of the universe are among the most important problems of science and they might be inextricably linked. Hydro-gravitational-dynamics (HGD) cosmology predicts hydrogen-helium gas planets in clumps as the dark matter of galaxies, with millions of planets per star. This unexpected prediction is supported by quasar microlensing of a galaxy and a flood of new data from space telescopes. Supernovae from stellar over-accretion of planets produce the chemicals (C, N, O, P etc.) and abundant liquid water domains required for first life and the means for wide scattering of life prototypes. The first life likely occurred promptly following the plasma to gas transition 300,000 years after the big bang while the planets were still warm, and interchanges of material between planets constituted essentially a cosmological primordial soup. Images from optical, radio,…
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