The first turbulent combustion

TL;DR

This paper proposes that turbulent combustion initiated in the early universe's hot big bang, driven by quantum mechanics and fluid dynamics, influenced cosmic structure formation and is evidenced by cosmic microwave background anisotropies.

Contribution

It introduces a novel cosmological model where turbulence from the big bang seed structure formation, supported by CMB data, challenging traditional inflationary theories.

Findings

Turbulent patterns fossilized in the early universe influenced nucleosynthesis.

CMB anisotropies support a turbulence-based origin of cosmic structures.

Evidence from CMB spectra aligns with hydro-gravitational fragmentation models.

Abstract

The first turbulent combustion arises in a hot big bang cosmological model Gibson (2004) where nonlinear exothermic turbulence permitted by quantum mechanics, general relativity, multidimensional superstring theory, and fluid mechanics cascades from Planck to strong force freeze out scales with gravity balancing turbulent inertial-vortex forces. Interactions between Planck scale spinning and non-spinning black holes produce high Reynolds number turbulence and temperature mixing with huge Reynolds stresses driving the rapid inflation of space. Kolmogorovian turbulent temperature patterns are fossilized as strong-force exponential inflation stretches them beyond the scale of causal connection ct where c is light speed and t is time. Fossil temperature turbulence patterns seed nucleosynthesis, and then hydro-gravitational structure formation in the plasma epoch, Gibson (1996, 2000). Evidence about formation mechanisms is preserved by cosmic microwave background temperature anisotropies. CMB spectra indicate hydro-gravitational fragmentation at supercluster to galaxy masses in the primordial plasma with space stretched by \~10^50. Bershadskii and Sreenivasan (2002, 2003) CMB multi-scaling coefficients support a strong turbulence origin for the anisotropies prior to the plasma epoch.