Total Black Hole Mass Recalibration and the Inverse Halo Problem

Paper II in the SMBH-DM Halo Framework series. We show that the coupling constant k = 4,120 from Paper I is an effective constant that absorbed the Milky Way's ratio of total black hole mass to SMBH mass. The true coupling (k_true ≈ 129) operates on total collapsed-object mass including the stellar black hole graveyard. Age-weighted contributions remove spin as a free parameter. The inverse halo problem recovers Gaia-Enceladus merger parameters from halo mass alone. Validated across four systems from dwarf galaxies to massive spirals. Resolves the Fornax dSph too-big-to-fail problem. Companion to Paper I: doi:10.5281/zenodo.15193025

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-04-17
DOI
https://doi.org/10.5281/zenodo.19631383
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
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article

Total Black Hole Mass Recalibration and the Inverse Halo Problem

Ronald Bibb
Zenodo (CERN European Organization for Nuclear Research)
Pulsars and Gravitational Waves Research
article

Total Black Hole Mass Recalibration and the Inverse Halo Problem

Ronald Bibb
article en

Abstract

Paper II in the SMBH-DM Halo Framework series. We show that the coupling constant k = 4,120 from Paper I is an effective constant that absorbed the Milky Way's ratio of total black hole mass to SMBH mass. The true coupling (k_true ≈ 129) operates on total collapsed-object mass including the stellar black hole graveyard. Age-weighted contributions remove spin as a free parameter. The inverse halo problem recovers Gaia-Enceladus merger parameters from halo mass alone. Validated across four systems from dwarf galaxies to massive spirals. Resolves the Fornax dSph too-big-to-fail problem. Companion to Paper I: doi:10.5281/zenodo.15193025

Zenodo (CERN European Organization for Nuclear Research)
Oldham Council (GB)
Openalex Percentile: Top 5%
Pulsars and Gravitational Waves Research
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