Can A Star Be Born From Chaos a Theory
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| Formato: | Recurso digital |
| Lenguaje: | inglés |
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2025
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| _version_ | 1866901896575320064 |
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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 |