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HGUT
Harrison Grand
Unified Theory
Open ProblemsGreat Collision Dynamics
17Status: OpenFoundational

Cosmology

Model the Great Collision Outcome

Simulate the collision of the pre-universe structures and determine whether the event produced a rebound, complete merger, partial merger, fragmentation, or another outcome.

The Problem

Problem Statement

HGUT cosmology begins with a Great Collision involving pre-existing large-scale structures or phases. The open problem is to construct the dynamical model and map the outcome across impact parameter, velocity, angular momentum, material state, topology, and coupling values. Rebound, merger, partial merger, penetration, fragmentation, and asymmetric outcomes must be tested rather than assumed.

Scientific Importance

Why It Matters

The collision outcome determines the origin of the Graviton Mesh, the initial conditions of cosmology, the particle-debris spectrum, large-scale asymmetry, and the interpretation of the cosmic microwave background.

Progress Ledger

What Has Been Established So Far

1

The Great Collision is the organizing event of the current cosmological narrative.

2

Rebound, merger, and partial-merger interpretations have all been recognized as live possibilities.

3

The event has not yet been modeled with a completed field theory and systematic parameter scan.

Pass-or-Fail Structure

Research Gates

Every gate must be addressed before this problem can be considered closed. Partial success does not establish the complete identification.

GC-1Open

Initial-state model

Define the pre-collision objects, phases, fields, and boundary conditions.

GC-2Open

Collision solver

Evolve the nonlinear event with conserved energy, momentum, angular momentum, and topology.

GC-3Open

Outcome classification

Map rebound, merger, partial merger, penetration, and fragmentation regimes.

GC-4Open

Mesh formation

Show how the organized Graviton Mesh emerges from the event.

GC-5Dependent

Debris spectrum

Determine which stable and transient Harrison-Knot species are produced.

GC-6Open

Cosmological initial conditions

Extract expansion, contraction, density, temperature, perturbation, and asymmetry data.

Definition of Success

Exact Closure Criteria

This problem closes only when the following conditions are satisfied together.

  1. 1

    The pre-collision configuration is mathematically well defined.

  2. 2

    The nonlinear collision is simulated with convergent conservation diagnostics.

  3. 3

    The outcome regime is mapped across physically meaningful parameters.

  4. 4

    Mesh formation and collision debris emerge dynamically.

  5. 5

    The resulting state supplies consistent cosmological initial conditions.

  6. 6

    The model distinguishes among rebound, merger, and partial-merger histories.

  7. 7

    Predicted relics can be compared with CMB and large-scale-structure data.

Prerequisites

Dependencies

  • Completed cosmological field equations
  • Harrison-Knot particle spectrum
  • Sea-Time foundations
  • High-performance numerical framework
  • CMB interpretation

Open Collaboration

How Contributors Can Help

  • Initial-data construction
  • Nonlinear collision simulations
  • Parameter-space scans
  • Topology and debris diagnostics
  • Mesh-formation studies
  • Cosmological observable extraction

The Question Remains Open

Help test the candidate.

Successful arguments, failed attempts, independent simulations, corrections, and falsifying evidence all move the research program forward.