Can A Star Be Born From Chaos a Theory

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Autor principal: McEvoy, Adam L
Formato: Recurso digital
Lenguaje:inglés
Publicado: Zenodo 2025
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author McEvoy, Adam L
author_facet McEvoy, Adam L
contents <p>This research presents a novel approach to energy amplification and astrophysical engineering using chaos-based predictive leverage in three-body stellar systems. By recursively measuring orbital curvature and applying a pi-scaled fractal forecasting method, the study models how precise momentum injections can be used to amplify kinetic output during chaotic gravitational interactions.</p> <p>Simulations demonstrate that when three neutron stars orbit near a supermassive Kerr black hole, predictive energy inputs—timed at gravitational inflection points—can trigger net energy gains between 2× to 4.5× the input. Beyond harvesting energy from chaos, the model introduces the <strong>Fractal Star Genesis Hypothesis</strong>: under specific timing and alignment conditions, a blast event near an event horizon can stabilize into a long-lived, star-like radiative object. This may offer an alternative mechanism for stellar formation in the early universe.</p> <p>Applications include stellar reignition, entropy inversion, and gravitational resonance engineering. This paper lays the groundwork for further simulation and exploration of high-energy systems, controlled spacetime feedback, and chaos-tempered energy control at cosmic scale.</p>
format Recurso digital
id zenodo_https___doi_org_10_5281_zenodo_15366884
institution Zenodo
language eng
publishDate 2025
publisher Zenodo
record_format zenodo
spellingShingle Can A Star Be Born From Chaos a Theory
McEvoy, Adam L
blackhole
space
energy
cosmos
entropy
thedr
<p>This research presents a novel approach to energy amplification and astrophysical engineering using chaos-based predictive leverage in three-body stellar systems. By recursively measuring orbital curvature and applying a pi-scaled fractal forecasting method, the study models how precise momentum injections can be used to amplify kinetic output during chaotic gravitational interactions.</p> <p>Simulations demonstrate that when three neutron stars orbit near a supermassive Kerr black hole, predictive energy inputs—timed at gravitational inflection points—can trigger net energy gains between 2× to 4.5× the input. Beyond harvesting energy from chaos, the model introduces the <strong>Fractal Star Genesis Hypothesis</strong>: under specific timing and alignment conditions, a blast event near an event horizon can stabilize into a long-lived, star-like radiative object. This may offer an alternative mechanism for stellar formation in the early universe.</p> <p>Applications include stellar reignition, entropy inversion, and gravitational resonance engineering. This paper lays the groundwork for further simulation and exploration of high-energy systems, controlled spacetime feedback, and chaos-tempered energy control at cosmic scale.</p>
title Can A Star Be Born From Chaos a Theory
topic blackhole
space
energy
cosmos
entropy
thedr
url https://doi.org/10.5281/zenodo.15366884