The Emergence of Negative Superhumps in Cataclysmic Variables: Smoothed Particle Hydrodynamics Simulations
David M. Thomas, Matt A. Wood

TL;DR
This paper demonstrates through simulations that magnetic fields in cataclysmic variables can induce disk tilts leading to negative superhumps, providing a physical mechanism for their emergence.
Contribution
The study integrates Lai's magnetic tilt instability model into SPH simulations, showing how magnetic fields cause disk tilts and generate negative superhumps.
Findings
Negative superhumps emerge in simulations with magnetic fields in the kilogauss range.
Period deficits of negative superhumps match those from tilted disk models.
Disks are tilted and precess retrogradely, consistent with observations.
Abstract
Negative superhumps are believed to arise in cataclysmic variable systems when the accretion disk is tilted with respect to the orbital plane. Slow retrograde precession of the line-of-nodes results in a signal---the negative superhump---with a period slightly less than the orbital period. Previous studies have shown that tilted disks exhibit negative superhumps, but a consensus on how a disk initially tilts has not been reached. Analytical work by Lai suggests that a magnetic field on the primary can lead to a tilt instability in a disk when the dipole moment is offset in angle from the spin axis of the primary and when the primary's spin axis is, itself, not aligned with the angular momentum axis of the binary orbit. However, Lai did not apply his work to the formation of negative superhumps. In this paper, we add Lai's model to an existing smoothed particle hydrodynamics code. Using…
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