Stellar energy conservation during evolution
A stellar shell's luminosity divergence accounts for local energy production, change in specific internal energy and compression or expansion work.
Key knowledge
A stellar shell's luminosity divergence accounts for local energy production, change in specific internal energy and compression or expansion work. Nuclear production need not equal surface luminosity during contraction or post-main-sequence evolution.
Values and equations
∂L/∂m = εnet − du/dt − P d(1/ρ)/dt
- L
- luminosity W
- m
- mass coordinate kg
- εnet
- net energy production per mass W kg⁻¹
- u
- specific internal energy J kg⁻¹
- P
- pressure Pa
- ρ
- density kg m⁻³
- t
- time following a mass shell s
Conditions and scope
- Derivatives follow the mass shell in the displayed quasistatic thermodynamic equation.
- The net local production term must include relevant losses, such as escaping neutrino energy, in the adopted model.
Sources · 1
References
Sources retain their recorded scope. A source link alone does not establish verification of every statement.
Evidence and review
Read equation 242 and explicit warning that thermal equilibrium fails during pre/post-main-sequence stages; did not reproduce the notes' missing 3/2 in an ideal-gas internal-energy expression.
2026-10-10 · Independent AI editorial review: All26 Life-authored Cosmos compact statements, conditions, displayed equations and all56 origin semantic links read. Entire26-entry author statement/source matrix and explicit exclusions assessed. Targeted independent primary sections are listed below; this does not claim every referenced source body or proof was independently re-read. This is scoped AI reference-content review, not human disciplinary certification or whole-field completion. Receipt: cosmos-life-independent-content-review.1.
Entry details
Permanent link to this entry ↗- Record identity
- uni-cosmos-stellar-energy
- Revision
- core.1
- Structured reference record
- University core expansion