DEEP SPACE COMPUTING

Astrophysics & Cosmology

Modeling the evolution of the universe through billion-body N-Body simulations and relativistic ray-tracing.

The Digital Twin of the Universe

Astrophysics remains the ultimate testing ground for High-Performance Computing. By resolving the Null Geodesic Equations of curved spacetime and tracking the hierarchical growth of Dark Matter halos, we translate raw mathematical theory into visual scientific evidence.

Dark Matter Modeling

N-Body Simulations: Tracking billions of particles to model the "Cosmic Web."
Baryonic Feedback: Simulating supernova explosions and stellar winds.

Black Hole Dynamics

Accretion Ray-Tracing: Light-path visualization around Event Horizons using GPU solvers.
Gravitational Waves: Modeling binary mergers for LIGO/Virgo detection.

Galactic Evolution

SPH Modeling: Simulating the fluid-like behavior of interstellar gas and star formation.
Morphology: Tracking the structural evolution of spiral and elliptical galaxies.

Compute Logic: Theory -> Simulation -> ROI

Research Phase	HPC / AI Action	Scientific Outcome
Structure Formation	Fast Fourier Transforms (FFT) on $10,000^3$ particle grids.	Universal Matter Distribution Mapping
Relativistic Optics	GPU-accelerated ray-marching through Kerr-Metric manifolds.	Event Horizon Shadow Verification
Waveform Prediction	Solving Einstein’s equations via Numerical Relativity (BSSN).	LIGO/Virgo Data-Match Templates