Differences

This shows you the differences between two versions of the page.

--- un:equations-of-stellar-structure [2025/10/27 00:31] – asad
+++ un:equations-of-stellar-structure [2025/10/27 00:33] (current) – [Primary and secondary] asad
@@ Line 129: / Line 129: @@
   * They are **differential equations** that describe the **structural variation** of a star with radius \(r\).
   * They express the **fundamental conservation laws** of physics:
-  – (1) mechanical equilibrium,
+    * (1) mechanical equilibrium,
-  – (2) conservation of mass,
+    * (2) conservation of mass,
-  – (3) conservation of energy, and
+    * (3) conservation of energy, and
-  – (4–5) energy transport by radiation or convection.
+    * (4–5) energy transport by radiation or convection.
   * Their solutions give the radial profiles of \(P(r)\), \(\rho(r)\), \(T(r)\), \(M(r)\), and \(L(r)\).