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This paper was recently published in the Monthly Notices of the Royal Astronomical Society.
Batygin 2018, Schrödinger Evolution of Self-Gravitating Disks
I am posting this in here, but I am actually more interested in the implications of looking at this the other way around: namely, from a purely mathematical point of view, what are possible mathematical implications for generalizing the Schrödinger equation based on an unsimplified mathematical model of self-gravitating disks?
Batygin 2018, Schrödinger Evolution of Self-Gravitating Disks
Abstract said:An understanding of the long-term evolution of self-gravitating disks ranks among the classic outstanding problems of astrophysics. In this work, we show that the secular inclination dynamics of a geometrically thin quasi-Keplerian disk, with a surface density profile that scales as the inverse square-root of the orbital radius, are described by the time-dependent Schrödinger equation. Within the context of this formalism, nodal bending waves correspond to the eigenmodes of a quasiparticle's wavefunction, confined in an infinite square well with boundaries given by the radial extent of the disk. We further show that external secular perturbations upon self-gravitating disks exhibit a mathematical similarity to quantum scattering theory. Employing this framework, we derive an analytic criterion for the gravitational rigidity of a nearly-Keplerian disk under external perturbations. Applications of the theory to circumstellar disks and Galactic nuclei are discussed.
I am posting this in here, but I am actually more interested in the implications of looking at this the other way around: namely, from a purely mathematical point of view, what are possible mathematical implications for generalizing the Schrödinger equation based on an unsimplified mathematical model of self-gravitating disks?