Status: CANONICAL Paper: 05 — Segmented Spacetime: Infalling Matter and Radiowaves
In SSZ, infalling matter approaching a dark star is never lost behind an event horizon. Instead, it encounters a region of extreme segmentation where time dilation is finite (D(r_s) = 0.555) rather than zero. Light emitted by infalling matter is transformed into highly redshifted radio waves.
| Observable | SSZ Prediction | GR Prediction |
|---|---|---|
| Matter fate at r_s | Slowed but not frozen | Frozen / lost |
| Light from r_s | Radio waves (z = 0.802) | No escape |
| Information | Preserved | Lost (paradox) |
| Radio emission | Detectable with SKA | None expected |
Infalling matter has two velocity components (Paper 02):
v_total = v_fall + v_eigen
- v_fall: gravitational infall velocity
- v_eigen: intrinsic velocity of matter
- At r_s, both are finite and well-defined
- SKA (Square Kilometre Array): Radio emission from infalling matter near compact objects
- Next-generation EHT: Resolve radio structures near BH shadows
- LIGO/LISA: Modified ringdown from finite D(r_s)
- Paper 02 (Dual Velocities): Kinematic framework
- Paper 09 (Dark Star): Dark star properties
- Paper 16 (Singularities): No singularity resolution
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