A Model for Frequency-Dependent Negentropic Gravity: Astrophysical Signatures of a Dynamic Coherence Field
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2025
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| _version_ | 1866902287580921856 |
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| author | Brandon Dick |
| author_facet | Brandon Dick |
| contents | <p> I propose a modification to the Einstein Field Equations based on the postulate that<br>the quantum informational state of matter, or its negentropy, is sourced by a dynamic scalar<br>field—the Coherence Field. I have theorized that this field's coupling to spacetime curvature,<br>represented by the constant \kappa, is not a fundamental constant but is instead<br>frequency-dependent, \kappa(f). This single hypothesis elegantly resolves a major theoretical<br>paradox while preserving the successes of General Relativity in static or low-frequency regimes.<br>In this framework, \kappa(f) \approx 0 for static phenomena, yielding predictions for gravitational<br>lensing and black hole shadows that are identical to General Relativity, in agreement with<br>current observations. However, in high-frequency, dynamic events such as a compact binary<br>merger, \kappa(f) becomes significant, leading to a cascade of new, testable predictions.<br>Through a suite of high-fidelity numerical simulations, I demonstrate three such signatures: (1)<br>the generation of a composite gravitational waveform containing both tensor and scalar<br>components, (2) an accelerated rate of binary inspiral due to an additional scalar energy-loss<br>channel, and (3) a unique distortion of the post-merger black hole ringdown "chord," where<br>high-frequency Quasi-Normal Modes are preferentially damped. This model of<br>Frequency-Dependent Negentropic Gravity offers a comprehensive and falsifiable framework<br>that is consistent with all known observations while providing a rich new phenomenology for<br>gravitational wave astronomy.</p> |
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| id | zenodo_https___doi_org_10_5281_zenodo_17278294 |
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| publishDate | 2025 |
| publisher | Zenodo |
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| spellingShingle | A Model for Frequency-Dependent Negentropic Gravity: Astrophysical Signatures of a Dynamic Coherence Field Brandon Dick General relativity Modified gravity Gravitational waves Cosmology Scaler-tensor theroy Negentropy <p> I propose a modification to the Einstein Field Equations based on the postulate that<br>the quantum informational state of matter, or its negentropy, is sourced by a dynamic scalar<br>field—the Coherence Field. I have theorized that this field's coupling to spacetime curvature,<br>represented by the constant \kappa, is not a fundamental constant but is instead<br>frequency-dependent, \kappa(f). This single hypothesis elegantly resolves a major theoretical<br>paradox while preserving the successes of General Relativity in static or low-frequency regimes.<br>In this framework, \kappa(f) \approx 0 for static phenomena, yielding predictions for gravitational<br>lensing and black hole shadows that are identical to General Relativity, in agreement with<br>current observations. However, in high-frequency, dynamic events such as a compact binary<br>merger, \kappa(f) becomes significant, leading to a cascade of new, testable predictions.<br>Through a suite of high-fidelity numerical simulations, I demonstrate three such signatures: (1)<br>the generation of a composite gravitational waveform containing both tensor and scalar<br>components, (2) an accelerated rate of binary inspiral due to an additional scalar energy-loss<br>channel, and (3) a unique distortion of the post-merger black hole ringdown "chord," where<br>high-frequency Quasi-Normal Modes are preferentially damped. This model of<br>Frequency-Dependent Negentropic Gravity offers a comprehensive and falsifiable framework<br>that is consistent with all known observations while providing a rich new phenomenology for<br>gravitational wave astronomy.</p> |
| title | A Model for Frequency-Dependent Negentropic Gravity: Astrophysical Signatures of a Dynamic Coherence Field |
| topic | General relativity Modified gravity Gravitational waves Cosmology Scaler-tensor theroy Negentropy |
| url | https://doi.org/10.5281/zenodo.17278294 |