MULTISCALE MODELING
From Singularity to Structure
Bridging the gap between subatomic quantum physics and galactic-scale gravitation.
The Methodology of Cosmic Expansion
The greatest challenge in modern cosmology is multi-scalability. Our architectural approach enables researchers to couple the quantum physics of the primordial universe with the complex gravitational dynamics of galaxy clusters.
Logic Layer: Phase -> Methodology -> Outcome
| Research Phase | HPC / AI Methodology | Scientific Outcome |
|---|---|---|
| Big Bang Era | Monte Carlo simulations for particle interactions at extreme energy densities. | Thermal History Reconstruction |
| The Dark Ages | Hydrodynamic Adaptive Mesh Refinement (AMR) of primordial gas clouds. | First Stars (Population III) Insights |
| Parameter Search | Bayesian Neural Networks for Likelihood analysis of cosmological parameters. | Hubble Tension ($H_0$) Resolution |
Quantum Scaling
Calculating the influence of subatomic fluctuations on the early distribution of matter.
Gravitational Coupling
Simulating massive-scale N-body structures across galactic manifolds.
AI Surrogates
Replacing traditional compute-heavy solvers with high-speed neural emulators.