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Pulsar efficiency, defined as the ratio of the pulsed bolometric luminosity to the spin-down power, is calculated to be about 15% (averaged over the spin-dipole inclination angle, ranging between about 50% for the aligned and 10% for the orthogonal).
Goldreich, P., Julian, W. H., 1969, Ap.J. 157, 869
1969
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Ruderman, M.A., Sutherland, P.G., 1975, Ap.J. 196, 51
1975
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Abdo, A.A., et al, 2010, Ap. J. S. 187, 460
2010
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Gruzinov, A., 2012, arXiv:1205.3367
2012
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