Same framework, applied to Exoplanets
The framework's value lies in its universality across disparate domains. The brake operator \(\mathcal{B}\), dispersion \(\mathcal{S}\), consensus \(\mathcal{M}\), spectral primitive \(\mathcal{P}\), anti-shadow detector \(\mathfrak{A}\), and scope-reporter \(\mathscr{A}\) — together with Theorems 1–13 — are applied here exactly as on every other domain. Source code: github.com/senuamedia/uniformity. No per-domain calibration. No imported threshold. No bespoke fit.
Cross-domain catalogue — \(\beta\)-strip
This domain's primitive is BLS bump-hunt over period grid rather than the brake operator \(\mathcal{B}\). The cross-domain catalogue below shows brake-exponent readings from the other domains — the same framework, the same code, different operator.
Click any point for the full reading: instance, domain, \(\beta\) value, and a link to the source code.
What the framework provides for exoplanet detection
Transit detection has a domain-standard primitive (Box-Least-Squares periodogram). The framework's bump-hunt operates over the same period grid, recovering known transits with millisecond precision. Where the framework's cascade-style probes (PELT, EMD, wavelet) do not improve BLS at the operative level, the framework reports that honestly under Law V — they are at best secondary diagnostics.
Headline results (catalogue instance 4)
- WASP-43b period 0.81336 d (literature 0.81348 d, 0.015% error).
- HD 209458b: exact match.
- Dataset: TESS via lightkurve, full-cadence light curves.
Experiments
Scripts: domains/exoplanets/experiments/ (4 scripts).
tess_exoplanet_test.py— primary recovery experiment.
Framework reading
Theorem 1 reading: each transit is a sub-cascade returning to baseline in finite time within the orbital period. The framework's bump-hunt transfers cleanly from particle-physics resonance hunting to stellar photometry — same primitive, different domain.