pith. sign in
module module moderate

IndisputableMonolith.Cosmology.Inflation

show as:
view Lean formalization →

This module identifies the inflaton potential with the J-cost function and defines associated slow-roll and e-folding quantities for Recognition Science cosmology. Cosmologists modeling early-universe dynamics would cite these definitions to link standard inflation observables to the recognition framework. The module consists of definitions and short lemmas built directly on the imported Cost and Constants modules.

claimThe inflaton potential is given by $V = J$, where $J$ denotes the J-cost. Slow-roll parameters are defined as slowRollEpsilon and slowRollEta, with eFoldings computed from the potential; the horizon, flatness, and monopole problems are addressed via sixty_efolds and related statements.

background

The module imports Constants, which fixes the RS time quantum as τ₀ = 1 tick, and Cost, which supplies the J-cost function. The supplied doc-comment states that the inflaton potential in RS is just the J-cost. Sibling declarations introduce inflatonPotential, potential_min_at_one, slowRollEpsilon, slowRollEta, eFoldings, and the three problem-solving statements.

proof idea

This is a definition module, no proofs.

why it matters in Recognition Science

The module supplies the core objects used by the sibling declarations horizon_problem_solved, flatness_problem_solved, monopole_problem_solved, and powerSpectrum. It places the standard inflationary toolkit inside the Recognition Science setting that begins from the J-uniqueness and phi fixed-point steps of the forcing chain.

scope and limits

depends on (2)

Lean names referenced from this declaration's body.

declarations in this module (24)