SYSTEM_ACTIVE
COMMAND_CENTER_v6.1
MALTHEN_OS_>
REFRESH
EXPERIMENTAL ENGINEERING // MAL_LAB_v3.0

Malthen Laboratory.

An experimental playground where complex algorithms, relativistic physics, and digital aesthetics meet.

DURUM: AKTİF_DENEY
LEFT CLICK: Add | HOLD: Scale Up | RIGHT CLICK: Scale Down
SYSTEM MASS: 0
ENTROPY (PARTICLES): 0
PHYSICS: RELATIVISTIC
AVG. SPEED: 0.0 v
OBJECTS: 0
DATA_STREAM // LIVE_LOG
[SYSTEM] Core initialized...
[DATA] Connection established.
[READY] Awaiting interaction.

Physics Engine.

Newtonian Gravity

N-body gravity simulation. Every body accelerates in the gravitational field of others according to Newton's universal gravity law.

F = G · m₁m₂ / r²   |   a = F/m

Keplerian Accretion Disk

In black hole accretion disks, inner orbit particles rotate much faster than outer ones. Temperature gradient: inner region is blue-white, outer is red.

ω ∝ r−3/2   |   T ∝ r−3/4

Roche & Tidal Physics

When smaller bodies approach massive objects, tidal forces shred the body. Remnants spiral down into the accretion disk.

dR ≈ R · (2M/m)1/3

Lorentz Speed Limit

No body can exceed the speed of light. As speed increases, the Lorentz factor limits acceleration asymptotically.

veff = c · v / √(v² + c²)

HR Diagram & Photon Sphere

Star colors shift from red to blue depending on mass. A thin light ring that captures photons forms at a radius of 1.5×rs of black holes.

rph = 1.5 × rs   |   L ∝ M3.5

Momentum & Supernova

Momentum is conserved in mergers. In a supernova, 75% of the star is ejected into space as nebula, and the remnant collapses into a neutron star or black hole.

pf = Σ(mi·vi)   |   Mremnant ≈ 0.25M