Simulating the pre-cosmological collision and determining whether it produced rebound, merger, partial merger, fragmentation, or another outcome.
Programme Overview
This program converts the Great Collision cosmology from a qualitative origin narrative into a nonlinear computational problem. The simulations must establish the initial state, collision regime, Mesh formation, debris spectrum, asymmetry, and resulting cosmological initial conditions.
Immediate Milestone
Build the first controlled reduced-dimensional collision model that distinguishes rebound from merger while conserving energy and momentum.
Active Objectives
Define the pre-collision structures.
Construct conserved nonlinear initial data.
Simulate rebound, merger, and partial-merger regimes.
Track Mesh formation.
Classify generated Harrison-Knot debris.
Extract thermal and perturbation initial conditions.
Connect collision outcomes to the CMB.
Evidence Trail
This ledger records the mathematical, computational, conceptual, and numerical work already completed within this programme.
The Great Collision has been identified as the central cosmological formation event.
Rebound, merger, and partial merger remain explicit competing outcomes.
The Great Collision is linked to Mesh formation.
The collision-debris spectrum has been connected to particle formation.
CMB interpretation has been defined as a downstream validation program.
The required parameter-space scan has been specified.
Shared Mathematical Foundation
The master Lagrangian and baseline displacement, phase, interaction, and conservation equations are already established. The work on this page concerns solving, validating, extending, and testing their consequences in this specific physical sector.
Active Research
Successful derivations, failed simulations, replications, corrections, and falsifying evidence all belong in the evidence trail.
