Journal articles
Warping modes in discs around accreting neutron stars
Abstract : The origin and stability of a thin sheet of plasma in the magnetosphere of an accreting neutron star are investigated. First, the radial extension of such a magnetospheric disc is explored. Then a mechanism for magnetospheric accretion is proposed, reconsidering the bending wave explored by Agapitou, Papaloizou & Terquem, that was found to be stable in ideal magnetohydrodynamics. We show that this warping becomes unstable and can reach high amplitudes, in a variant of Pringle's radiation-driven model for the warping of active galactic nucleus accretion discs. Finally, we discuss how this mechanism might give a clue to explain the observed X-ray kilohertz quasi-periodic oscillation of neutron star binaries.
https://hal-insu.archives-ouvertes.fr/insu-03611754
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Submitted on : Thursday, March 17, 2022 - 1:43:22 PM
Last modification on : Tuesday, May 10, 2022 - 3:24:58 PM
Contributor : Nathalie Pothier Connect in order to contact the contributor
Submitted on : Thursday, March 17, 2022 - 1:43:22 PM
Last modification on : Tuesday, May 10, 2022 - 3:24:58 PM
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