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84922693328
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note
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The Roche lobe of a binary star is the innermost equipotential surface passing through the first Lagrangian point, L1. If a star fills its Roche lobe, the unbalanced pressure at L1 will cause mass transfer to the other star (2).
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84922746506
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The magnetospheric coupling parameter, 0:5 < φ < 1:4 is a numerical factor of order unity depending on the accretion flow, the disk model, and the magnetic inclination angle of the pulsar (10, 11, 32-34).
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84922727206
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This "turn-off problem" has previously been debated elsewhere (13, 33, 35).
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84922714913
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note
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This is the case if the pulsar spin period, P, is close to its initial spin period, P0.
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