Black Hole Reactor — Hawking Radiation Power Cell

Sim Speed

½×

1×

5×

20×

Operator Controls

Mass Feed Rate
× equilibrium 1.00×

Containment Power 100%

Output Draw 70%

Converter Eff. 85%

Emergency

Scenarios

Physics

Hawking radiation: All black holes emit thermal radiation with temperature T ∝ 1/M. Smaller = hotter = more power.

Thermal runaway: Less mass → higher T → faster evaporation → even less mass → explosion.

Equilibrium: Maintain feed rate = evaporation rate to hold constant mass and stable power output.

BH Mass

—

Hawking Temperature

—

Peak gamma energy ∝ k_B T

Hawking Power Output

—

Electrical Output

—

η_converter × P_Hawking × draw

Net ΔM/dt

—

Feed − Evaporation

Containment Integrity

100%

Magnetic field stability

Gamma Flux

—

Converter saturation

Live Physics

r_Schwarzschild—

Evap rate—

Feed rate (abs)—

Evap time (rem)—

Luminosity ratio—

Evaporation Time (no feed)

—

Time until BH destroys itself