Black Hole Merger Frustration in QSD: A Physically-Constrained Model for Jet Genesis,Scalar Emission, and Residual Dynamics

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Abstract Observational data from black hole mergers increasingly challenge classical gen-eral relativity (GR). Features such as asymmetric jets, prolonged ringdowns, andrepeating fast radio bursts (FRBs) suggest internal dynamics beyond GR’s scope.This manuscript introduces a physically grounded model based on QuantumSubstrate Dynamics (QSD), in which mass arises from phase-bound coherence within a Lorentz-invariant substrate field. In this framework, black hole mergers are not guaranteed. When internal phase,spin, or coherence conditions are misaligned, unification can fail—a scenario termed merger frustration. The result is a metastable dual-core system, or blackhole molecule, stabilized by a persistent coherence trench. This trench explainsjet asymmetries, post-merger emissions, and periodic scalar bursts. The Lorentz–Einstein Substrate (LESt) complements GR by modeling internal structure without contradicting external metric predictions. It provides falsifiable mechanisms for alternatives to singularity-driven collapse and reframes black hole thermodynamics as a structural, not horizon-based, process. The model predicts testable signatures across gravitational and electromagnetic channels, including jet precession without accretion, scalar yield, and delayed emissions. Observed systems such as GW190814, M87, SS 433, and FRB 180916 align with these behaviors.
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Black Hole Merger Frustration in QSD: A Physically-Constrained Model for Jet Genesis,Scalar Emission, and Residual Dynamics | Research Square window.SnipcartSettings = { analytics: { enabled: false } }; (function() { var accessVector = localStorage.getItem('access_vector') || ''; window.dataLayer = window.dataLayer || []; if (accessVector) { window.dataLayer.push({ user: { profile: { profileInfo: { snid: accessVector } } } }); } })(); (function(w,d,s,l,i){w[l]=w[l]||[];w[l].push({'gtm.start':new Date().getTime(),event:'gtm.js'});var f=d.getElementsByTagName(s)[0],j=d.createElement(s),dl=l!='dataLayer'?'&l='+l:'';j.async=true;j.src='https://www.googletagmanager.com/gtm.js?id='+i+dl;f.parentNode.insertBefore(j,f);})(window,document,'script','dataLayer','GTM-K279D39R'); Browse Preprints In Review Journals COVID-19 Preprints AJE Video Bytes Research Tools Research Promotion AJE Professional Editing AJE Rubriq About Preprint Platform In Review Editorial Policies Our Team Advisory Board Help Center Sign In Submit a Preprint Cite Share Download PDF Research Article Black Hole Merger Frustration in QSD: A Physically-Constrained Model for Jet Genesis,Scalar Emission, and Residual Dynamics Michael Bush This is a preprint; it has not been peer reviewed by a journal. https://doi.org/ 10.21203/rs.3.rs-6740268/v1 This work is licensed under a CC BY 4.0 License Status: Posted Version 1 posted You are reading this latest preprint version Abstract Observational data from black hole mergers increasingly challenge classical gen-eral relativity (GR). Features such as asymmetric jets, prolonged ringdowns, andrepeating fast radio bursts (FRBs) suggest internal dynamics beyond GR’s scope.This manuscript introduces a physically grounded model based on QuantumSubstrate Dynamics (QSD), in which mass arises from phase-bound coherence within a Lorentz-invariant substrate field. In this framework, black hole mergers are not guaranteed. When internal phase,spin, or coherence conditions are misaligned, unification can fail—a scenario termed merger frustration. The result is a metastable dual-core system, or blackhole molecule, stabilized by a persistent coherence trench. This trench explainsjet asymmetries, post-merger emissions, and periodic scalar bursts. The Lorentz–Einstein Substrate (LESt) complements GR by modeling internal structure without contradicting external metric predictions. It provides falsifiable mechanisms for alternatives to singularity-driven collapse and reframes black hole thermodynamics as a structural, not horizon-based, process. The model predicts testable signatures across gravitational and electromagnetic channels, including jet precession without accretion, scalar yield, and delayed emissions. Observed systems such as GW190814, M87, SS 433, and FRB 180916 align with these behaviors. black hole dual mergers jets substrate mass-phase QSD lest Full Text Additional Declarations No competing interests reported. Cite Share Download PDF Status: Posted Version 1 posted You are reading this latest preprint version Research Square lets you share your work early, gain feedback from the community, and start making changes to your manuscript prior to peer review in a journal. As a division of Research Square Company, we’re committed to making research communication faster, fairer, and more useful. We do this by developing innovative software and high quality services for the global research community. Our growing team is made up of researchers and industry professionals working together to solve the most critical problems facing scientific publishing. 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