Key Concepts

Summary

This paper simulates how galaxies and cosmic structure form in CPP. Lattice defects from incomplete Capotauro

Capotauro

Chiral nucleation event that froze the lattice

View in map → breaking seed density perturbations that grow through gravitational collapse. Monte Carlo simulations with up to 2 billion defects on a \(256^3\) grid (running on H200 GPU in 60.9 seconds) produce power spectra that are scale-invariant at low \(k\) (matching \(\Lambda\)CDM) with distinctive lattice oscillations at high \(k\) — a testable prediction.

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MC structure formation from lattice defects. Runs: 100k to 2B defects on \(256^3\) grid (H200 GPU). \(P(k) \sim k^{-3}\) at low-\(k\) (scale-invariant), lattice oscillations at high-\(k\). 2B run: 60.9 s, mean density 119.2, \(P(k) \sim 4 \times 10^9\). Slope \(-2.95\) to \(-3.05\). Low-\(k\) matches \(\Lambda\)CDM. High-\(k\) oscillations are unique CPP signature.

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Full MC methodology, GPU implementation, power spectrum analysis, comparison with \(\Lambda\)CDM, testable predictions for future surveys.

🔊 Audio reading — coming soon

PDF & Paper

Abstract

Large-scale Monte Carlo simulations of structure formation from lattice defects are performed on GPU, scaling up to 2 billion defects. The resulting power spectra are scale-invariant at low \(k\) and exhibit distinctive lattice oscillations at high \(k\), providing a unique testable CPP signature.