LID-1166 Dual Black Hole Growth Simulator

Epoch: 0.0 Myr (z ≈ 6.80)

Sep: 400.0 pc | Decay Rate: 1.42 pc/Myr

Total Mass: 80.00 M_sun × 10⁶

Primary BH₁ (LID-A)

Secondary BH₂ (LID-B)

Astrophysical Benchmarks

Orbital & Reservoir Dynamics

Initial Separation 400 pc

Ambient Gas Reservoir (n_H) 10,000 cm⁻³

Accretion Mode Super-Eddington (3.5x)

Mass Ratio (q = M₂/M₁) 0.60

Coalescence Telemetry Inspiral Active

Orbital Period

2.41 Myr

GW Frequency

2.63 nHz

Est. Coalescence

148 Myr

Accretion Rate

0.82 M_sun/yr

Cosmological Context

The Early SMBH Paradox: Quasars observed at z > 6 harbor black holes > 10⁹ M_sun just ~800 Myr after the Big Bang. Standard Eddington-limited accretion cannot grow stellar seeds quickly enough.

LID-1166 Discovery: Confirms tight binary SMBHs embedded in dense circum-nuclear gas disks. Dynamical friction drains orbital energy, funneling massive gas streams directly into both event horizons to trigger runaway super-Eddington growth.