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Zenodo
2026
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| Online Access: | https://doi.org/10.5281/zenodo.19521163 |
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Table of Contents:
- <p><span class="s11"><span class="bumpedFont15">We propose that the flat brane (</span></span><span class="s12"><span class="bumpedFont15">κ</span></span><span class="s11"><span class="bumpedFont15"> = 0, {3,6} triangular tiling</span></span><span class="s11"><span class="bumpedFont15">) is the cosmological equilibrium state of the One-Octonion Brane-Bulk Framework, but that in regions of sufficiently strong gravitational acceleration (</span></span><span class="s12"><span class="bumpedFont15">a</span></span><span class="s11"><span class="bumpedFont15"> ≫ </span></span><span class="s12"><span class="bumpedFont15">a</span></span><span class="s11"><span class="bumpedFont15">₀), the brane locally relaxes toward its hyperbolic parent geometry (</span></span><span class="s12"><span class="bumpedFont15">κ</span></span><span class="s11"><span class="bumpedFont15"> → −1, {7,3} heptagonal tiling). This </span></span><span class="s13"><span class="bumpedFont15">T1 brane relaxation</span></span><span class="s11"><span class="bumpedFont15"> is physically distinct from the T2* dephasing (gravitomagnetic lensing) discussed in §2. Together they predict a novel form of </span></span><span class="s13"><span class="bumpedFont15">geometrically induced birefringence</span></span><span class="s11"><span class="bumpedFont15"> wherever the brane curvature transitions between regimes. We demonstrate that this framework — with zero free parameters beyond </span></span><span class="s12"><span class="bumpedFont15">a</span></span><span class="s11"><span class="bumpedFont15">₀ = cH₀/2π = 1.042 × 10⁻¹⁰ m/s² — simultaneously explains: (i) the upper kHz quasi-periodic oscillation (QPO) of 4U 1636-536 to 0.1% accuracy; (ii) the 3:2 twin-peak ratio of high-frequency QPOs in GRS 1915+105 to 0.9% accuracy; (iii) the universal occurrence of QPOs in all compact accreting systems via an exact theorem (κₐᵩᵩ = −1 at the ISCO for all masses); (iv) the repeating/non-repeating FRB dichotomy; and (v) the mass-dependent GW birefringence hinted at in GW190521. New observational predictions are made for polarimetric monitoring of Betelgeuse's companion Siwarha (November 2027 window) and for polarimetric decomposition of the SN 2024afav magnetar light curve</span></span></p>