IndisputableMonolith.Astrophysics.ChandrasekharMassStructure
The ChandrasekharMassStructure module establishes structural properties ensuring mass-scale anchors remain positive and finite inside the RS phi-ladder range. Astrophysicists deriving white-dwarf limits from first principles would cite it to close the mass-anchor step. The module consists of definitions that import and extend the MassToLight module's three M/L derivations.
claimMass-scale anchors $M$ satisfy $0 < M < \infty$ for rung values inside the RS phi-ladder; the Chandrasekhar mass structure is the collection of ledger-based and implication statements realizing this positivity and finiteness.
background
The module resides in the Astrophysics domain and imports only Mathlib plus the MassToLight module. The upstream doc-comment states: 'This module provides the unified derivation of the stellar mass-to-light ratio (M/L) from Recognition Science principles, eliminating the last external calibration input.' It supplies three independent derivations via stellar assembly, recognition cost weighting, and related strategies. The local setting is the RS ladder for mass scales, where anchors are expressed via phi-powers and must remain positive and finite.
proof idea
This is a definition module, no proofs.
why it matters in Recognition Science
The module supplies the required structural content that mass-scale anchors are positive and finite in the RS ladder range, thereby completing the mass-anchor step before applications of the mass formula. It feeds the Chandrasekhar-related siblings inside the same module and supports downstream use of the MassToLight derivations in stellar structure calculations.
scope and limits
- Does not compute numerical values of the Chandrasekhar mass.
- Does not address dynamical stability or collapse equations.
- Does not import external observational calibrations.
- Does not extend mass anchors outside the phi-ladder range.