Finite-N inertia and constrained link dynamics in a fuzzy-sphere black-hole matrix model
We prove the complete finite-N inertia of a published bifundamental-link Hessian in a fuzzy-sphere black-hole matrix model at xi=J: In(K)=(N+1,0,2N-1), N>=4, with low-rank exceptions. Under the source's covariantized temporal-gauge/A0 prescription, eliminating the auxiliary longitudinal sector yields a conditional Schur-complement inertia In(K_eff)=(1,0,2N-1); the unique negative mode is the outward extremal mode. This constrained-dynamics interpretation remains conditional on clarifying the transformation of rank-dependent projector weights under off-diagonal gauge transformations.
Authors
- Jason Davis (ORCID: https://orcid.org/0000-0002-0265-2219)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-11-03
- DOI
- https://doi.org/10.5281/zenodo.23925527
- Primary Topic
- Black Holes and Theoretical Physics
- Type
- preprint