SIAM Undergraduate Research Online

Volume 18

In This Volume

  • DOI: 10.1137/25S1739224

    Authors

    Vedant Ganesh (Corresponding author – Tanglin Trust School, Singapore)

    Project Advisors

    Alexander Mushtukov (University of Oxford)

    Abstract

    The dynamics of accretion in X-ray pulsars (XRPs) are shaped by the surrounding magnetic field. Charged material in the accretion disk impacts the magnetosphere and is constrained to the magnetic field lines due to the strength of the field. The particles’ dynamics are then influenced by extremely large gravitational forces due to high density and proximity, and centrifugal forces due to the corotation of the XRP magnetosphere. At higher mass accretion rates, radiative force appears which heavily influences the magnetic field flow. Accretion flows follow the magnetic field lines to impact the neutron star in a small region near the magnetic poles. We construct a numerical model to help determine the dynamics of accretion flow under these conditions and investigate its effects on the mass accretion rate and pulse profile of XRPs, assuming that the magnetic field is dominated by the dipole geometry. We show that variability in mass accretion rate, and hence pulse profile asymmetry, can be due to the misalignment between the accretion plane normal, rotational, and dipole axes, and we investigate the effects of each angle on pulse profile asymmetry.

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