PAPER X | Thermodynamic Quench Horizons

1. The X-Ray Death Flash

The Bremsstrahlung Problem

A 54.4 GW Z-pinch creates a massive burst of hard X-rays and fast neutrons natively as plasma collides. The REBCO superconductor coils orbiting the plasma must remain below 25 Kelvin to maintain the 96.8 Tesla magnetic anchor bounds. If stray radiation hits the coils, it initiates a "Quench," instantly vaporizing the superconductors and dumping 54.4 GW of confined magnetic energy into the ship's hull.

2. Beer-Lambert Shielding Simulator

Interactive Quench Calculator

To prove the STR-01 can physically survive its own 1-millisecond anchor explosion, we calculate the exact X-ray attenuation through the Tungsten primary shield utilizing the Beer-Lambert Law ($I = I_0 e^{-\mu x}$).

BREMSSTRAHLUNG ATTENUATION MAPPER

Z-Pinch Pulse Yield (GW)

Tungsten Shield (mm)

REBCO Ribbon Mass (kg)

Total X-Ray Emission ($1\%$ Yield): ...
Energy Penetrating Shield ($e^{-\mu x}$): ...
Final REBCO Temp ($\Delta T$): ...

The Engineering Paradigm Shift: Just 1.25 mm of Tungsten shielding effortlessly attenuates the 121,000 Joule X-ray flash down to 35 Joules. The REBCO coils effortlessly adsorb this transient heat spike, peaking at ~11.0 Kelvin, formally proving the ship avoids the catastrophic Quench Horizon.