Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6596
Title: A modified WKB formulation for linear eigenmodes of a collisionless self-gravitating disc in the epicyclic approximation
Authors: Gulati, Mamta
Saini, T.D.
Keywords: analytical galaxies
kinematics and dynamics
galaxies nuclei
Issue Date: 21-Jul-2016
Publisher: Oxford University Press for the RAS
Citation: Monthly Notices of the Royal Astronomical Society, 2016, Vol.460, p1019-1032
Abstract: The short-wave asymptotics (WKB) of spiral density waves in self-gravitating stellar discs is well suited for the study of the dynamics of tightly-wound wavepackets. But the textbook WKB theory is not well adapted to the study of the linear eigenmodes in a collisionless self-gravitating disc because of the transcendental nature of the dispersion relation. We present a modified WKB theory of spiral density waves, for collisionless discs in the epicyclic limit, in which the perturbed gravitational potential is related to the perturbed surface density by the Poisson integral in Kalnaj's logarithmic spiral form. An integral equation is obtained for the surface density perturbation, which is seen to also reduce to the standard WKB dispersion relation. Although our formulation is general and applies to all discs, we present our analysis only for nearly Keplerian, low-mass, self-gravitating discs revolving around massive central objects, and derive an integral equation governing the slow precessional modes of such discs. For a prograde disc, the integral kernel turns out be real and symmetric, implying that all slow modes are stable. We apply the slow mode integral equation to two unperturbed disc profiles, the Jalali–Tremaine annular discs, and the Kuzmin disc. We determine eigenvalues and eigenfunctions for both m = 1 and m = 2 slow modes for these profiles and discuss their properties. Our results compare well with those of Jalali–Tremaine.
Description: Open access
URI: http://hdl.handle.net/2289/6596
ISSN: 1365-2966 - (online)
0035-8711
Alternative Location: http://adsabs.harvard.edu/abs/2016MNRAS.460.1019G
http://arxiv.org/abs/1601.04148
http://dx.doi.org/10.1093/mnras/stw970
Copyright: 2016 The authors & the Royal Astronomical Society.
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
2016_MNRAS_460_1019.pdf
  Restricted Access
Open Access1.72 MBAdobe PDFView/Open Request a copy


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.