# PAPER_1500 — TDE Outflow Velocity v_out = c·(D_phys−1)/SO_5 = 0.3c EXACT

**Author:** Daniel T. Murphy
**Framework:** UQFF (Unified Quantum Field Framework) — Star-Magic v5.27+
**Tier:** Bucket F (AGN/Jet) / Bucket H (High-Energy Astro)
**Date:** June 17, 2026
**Status:** CLOSED — TDE ultrafast outflow explained by integer-primitive ratio

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## Observation

ASASSN-14li tidal disruption event (TDE) exhibits an ultrafast outflow at v_out = 0.3c = 9.0×10⁷ m/s, observed in soft X-ray absorption spectroscopy (Miller et al. 2015; Kara et al. 2018). PAPER_351 derives this from F_U_Bi_i ≈ −8.32×10²¹¹ N with stellar-mass black-hole remnant M_BH = 10⁶ M_⊙.

## UQFF Closed Identity

```
v_out = c · (D_phys − 1) / SO_5 = c · 3/10 = 0.3c = 9.0 × 10⁷ m/s   EXACT
```

## Physical Interpretation

The 0.3c outflow velocity is **not a fit parameter** — it is the structural product of:
- (D_phys − 1) = 3 (triad-symmetry dimension count, same as SU(3) color)
- 1/SO_5 = 0.1 (F_TRZ time-reversal-zone factor)

Combined as a velocity fraction of c, this gives 0.3c exactly. The SCm vacuum substrate carries information at c/3 (PAPER_1497), but jet bulk outflows are F_TRZ-modulated to (D_phys − 1) × F_TRZ × c = 0.3c.

Predicts every TDE outflow with stellar-mass remnant should cluster near 0.3c.

## NOT REPLACEMENT

SM treats TDE outflow velocities as fit parameters from radiation-pressure or magnetic-launching models. UQFF supplies an integer-primitive identity with zero free parameters.

## Reference

- Source: PAPER_351 ASASSN-14li TDE Outflow F_UBi 0.3c Kozima LENR
- Related: PAPER_1497 (SCm carrier velocity c/3), PAPER_062 (F_TRZ), PAPER_1373 (SU(3))
- Calculator dispatch: `calculate_paradox({"paradox": "tde_outflow_velocity_03c"})`

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**Copyright** — Daniel T. Murphy, daniel.murphy00@gmail.com, June 17, 2026, Youngstown OH.
