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Hypothesis 01 · Astrophysics / Propulsion
Soliton Wave Propulsion: A Directed Research Hypothesis
Jeffery Reed · Independent Researcher · Version 2.0 · April 2026

Proposes that naturally occurring spacetime soliton waves; potentially generated by magnetar starquakes; may be detectable in existing gravitational wave observatory data and could serve as the physical foundation for a novel propulsion concept.

Abstract

This document presents a directed research hypothesis proposing that naturally occurring spacetime soliton waves, potentially generated by magnetar starquakes, may be detectable in existing gravitational wave observatory data and could serve as the physical foundation for a soliton wave propulsion system.

Rather than generating a spacetime distortion from scratch, the proposed concept involves coupling a vessel to a naturally propagating soliton wave in the same way a surfer rides an existing wave. The hypothesis is grounded in a coherent stack of peer-reviewed research spanning soliton stability, steering, energy conversion, and spacetime soliton geometry.

A specific gap in the existing literature is identified: no research team has yet searched for the gravitational wave burst signature produced at the moment of soliton formation from a magnetar starquake event, using magnetar catalogues to correlate timing with existing unmodeled burst data. This document establishes the conceptual framework, the corrected experimental target, and the priority of that research direction.

The Core Premise

Current warp drive theory, including the Alcubierre metric and its successors, focuses on generating a spacetime distortion artificially; a problem that requires exotic energy conditions and remains practically unsolvable with known physics.

This hypothesis takes a different approach. If spacetime soliton waves occur naturally; as they may during magnetar starquake events; then the engineering problem shifts from generation to detection and coupling. A vessel does not need to create the wave. It needs to find one and ride it.

The analogy to ocean wave surfing is intentional and precise. A surfer does not generate the energy that moves them. They position themselves correctly relative to a wave that already exists and couple their motion to it. The energy expenditure required is orders of magnitude lower than generating equivalent motion independently.

The Identified Research Gap

LIGO and Virgo maintain an unmodeled burst search pipeline specifically designed to detect gravitational wave events that do not match known templates. Magnetar starquakes are monitored and catalogued in real time. The gravitational wave burst signature produced at the moment of soliton formation from a magnetar event has a predictable character; compact, shape-preserving, non-chirping, constant velocity.

No research team has applied a Lentz soliton template to magnetar-correlated unmodeled LIGO burst data. That search has not been performed. This is a concrete, falsifiable claim about a missing experiment, not a theoretical assertion. The data exists. The infrastructure exists. The correlation methodology exists. The search does not.

The strongest counterargument to this hypothesis involves the Celmaster 2025 paper challenging Lentz's weak energy condition compliance. This is directly engaged in the full document. Bobrick-Martire and Fuchs 2024 provide alternative positive-energy frameworks that do not rely on Lentz specifically, and the core observational gap identified here does not depend on any single theoretical framework being correct.
Filed with the Library of Congress. Developed through independent research by Jeffery Reed, April 2026.

This is a documented hypothesis identifying a research gap, not a peer-reviewed publication. Full document available upon request.

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Hypothesis 02 · Astrophysics / Color Science
What Color Is a Black Hole? Challenging the Unexamined Assumption
Jeffery Reed · Independent Researcher · April 2026

Challenges the widely repeated orange-gold color assignment of black holes; arguing that this representation reflects radio intensity mapping methodology rather than any physical color property, and that blackbody emission physics suggests a different plausible visible appearance.

Abstract

The 2019 Event Horizon Telescope image of M87* introduced the orange-gold black hole into public consciousness. This color has since been repeated across science communication, textbooks, and visual media as if it were a measured physical property of the object.

It is not. The orange-gold representation is the product of a specific false color methodology; radio wave intensity mapped to a visible color scale; applied without the planetary correction process that has been standard practice in solar system imaging for decades. This document identifies that methodological inconsistency, traces its origin, and proposes a more defensible characterization of what a black hole's accretion disk would likely appear to the human eye under direct observation.

The False Color Problem

When imaging planetary bodies, the standard methodology involves capturing raw telescope data and then applying a calibration process to restore what the human eye would actually perceive. The Voyager images of Neptune, for example, went through this correction process. The resulting blue is not arbitrary; it reflects the actual scattering properties of Neptune's atmosphere.

The EHT image of M87* did not go through this process. The orange-gold color was selected to represent radio wave intensity; hotter regions mapped to brighter orange; using a color scale optimized for human readability of the data, not for visual accuracy. This is a documented and legitimate scientific choice for data visualization. It has been misrepresented as a depiction of the object's actual color.

The parallel is direct. If Neptune had been released with the same false color methodology applied to M87*, it would appear orange. It doesn't appear orange. We know this because the correction was applied. No equivalent correction has been applied to or discussed in the context of the black hole image.

A More Defensible Characterization

Blackbody radiation physics and accretion disk temperature modeling suggest that the inner regions of an actively accreting black hole disk operate at temperatures in the range of millions of degrees Kelvin. At these temperatures, peak emission falls in the X-ray range; far outside human visible perception. The visible light component of this emission would shift toward the blue-white end of the spectrum.

The outer disk, at lower temperatures, would produce emission closer to yellow-white. Gravitational lensing effects would further distort the apparent shape and color distribution. The honest answer to "what color is a black hole" is that we do not have a corrected visible-light image of one; and the orange-gold that dominates science communication is a data visualization artifact, not a measurement.

The strongest part of this document is the methodology critique, which is independently valid regardless of what the correct color turns out to be. The specific color prediction carries more uncertainty due to the synchrotron complication and M87*'s unusual low-Eddington radiatively inefficient accretion regime. Both limitations are documented honestly in the full paper.
Filed with the Library of Congress. Developed through independent research by Jeffery Reed, April 2026.

This is a documented hypothesis challenging an unexamined methodological assumption, not a peer-reviewed publication. Full document available upon request.