Question #55065
Pulsar astronomers parameterize pulsar spin-down in a model-independent way with the
relation O = On, where n is known as the braking index. Derive a functional form for n in terms of the three observables. What value is n for magnetic dipole radiation?
relation O = On, where n is known as the braking index. Derive a functional form for n in terms of the three observables. What value is n for magnetic dipole radiation?
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