Pulsar magnetosphere & spin-down

Layer 1 — Physicsin the Astrophysics subtree

Dipole radiation Ė = -(2/3c³)(μ sin α)²Ω⁴ gives Ω̇∝Ω³; braking index n ≡ Ω̈Ω/Ω̇² (≈3 for pure dipole, ~2-3 observed).

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