IndisputableMonolith.Astrophysics.ChandrasekharMassStructure
The ChandrasekharMassStructure module establishes that mass-scale anchors remain positive and finite on the RS phi-ladder for astrophysical mass limits. Researchers deriving white dwarf structure from Recognition Science principles would cite it. The module organizes four declarations that extend the upstream MassToLight derivation of the mass-to-light ratio.
claimMass-scale anchors for the Chandrasekhar limit satisfy $0 < M_{Ch} < M_{max}$ as positive finite values on the recognition ladder, with structure derived from the mass-to-light ratio $M/L$ in RS units.
background
This module operates in the astrophysics domain and imports 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' with three independent derivations including stellar assembly via recognition cost weighting. The local setting applies the unified forcing chain to stellar structure, adding the constraint that mass-scale anchors stay positive and finite in the RS ladder range.
proof idea
This is a definition module, no proofs. The overall structure consists of four sibling declarations that supply chandrasekhar_mass_from_ledger and the two implications for mass-to-light bounds, extending the three derivations already present in the upstream MassToLight module.
why it matters in Recognition Science
The module supplies structural anchors for the Chandrasekhar mass in the Recognition Science framework, supporting the mass formula yardstick * phi^(rung - 8 + gap(Z)) and the constant G = phi^5 / pi. It extends the MassToLight module for M/L derivation but lists no downstream theorems.
scope and limits
- Does not derive explicit numerical values for the Chandrasekhar mass.
- Does not address dynamical stability or evolution of white dwarfs.
- Does not incorporate general relativity corrections outside the RS ladder.