Chandrasekhar Mass Limit
The Chandrasekhar mass limit (~1.4 M☉) separates white dwarfs from neutron stars. The τ-framework derives this from the degeneracy pressure sector of the f…
Physics
Domain level open problem
ASTRO
Book V
Public
Manuscript
Lean · Partial
Physics cascade
In plain language
The Chandrasekhar mass limit (~1.4 M☉) separates white dwarfs from neutron stars. The τ-framework derives this from the degeneracy pressure sector of the f…
Overview
The Chandrasekhar mass limit (~1.4 M☉) separates white dwarfs from neutron stars. The τ-framework derives this from the degeneracy pressure sector of the fiber T².
Result Statement
Chandrasekhar mass derived from degeneracy pressure sector. Status: Internally addressed.