Resonant Spacetime Hypothesis 2.0

     where \( d(t) \) is detector data.  

2. Sensitivity Estimate

   - For \( h_0 \sim 10^{-24} \) (predicted amplitude), LIGO O4 can detect SNR > 5 with 1 yr integration.  

Validation

- Null Test: Inject synthetic signals into noise to verify recovery.  

- Frequency Binning: Search for excess power in 32--38 Hz bins (Fig. 5a).  

CMB Spiral-Phase Correlations

Prediction

Spiral harmonics \( \psi_{nlm} \propto e^{im\phi + \beta \ln r} \) imprint helical phase patterns in CMB polarization:  

\[B_\ell^m \sim \int \psi_{nlm} \cdot \nabla T \, d\Omega,\]  

where \( T \) is the temperature anisotropy. These generate: