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To accrete or not to accrete: the dilemma of the recycling scenario

L. Burderi·F. D'Antona·T. Di Salvo·G. Lavagetto·R. Iaria·N. R. Robba
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Abstract

We study the evolution of a low-mass X-ray binary by coupling a binary stellar evolution code with a general relativistic code that describes the behaviour of the neutron star. We find that non-conservative mass transfer scenarios are required to prevent the formation of submillisecond pulsars and/or the collapse to a black hole. We discuss the sweeping effects of an active magneto-dipole rotator on the transferred matter as a promising mechanism to obtain highly non-conservative evolutions.

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L. Burderi, F. D'Antona, T. Di Salvo, G. Lavagetto, R. Iaria, N. R. Robba. 2004-04-15. To accrete or not to accrete: the dilemma of the recycling scenario. https://arxiv.org/abs/astro-ph/0404303

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