Cosmological fluid dynamics in the Schrödinger formalism

dc.creatorJohnston, Rebecca
dc.creatorLasenby, A. N.
dc.creatorHobson, M. P.
dc.date2009-04-03
dc.date.accessioned2026-07-07T13:00:21Z
dc.date.available2026-07-07T13:00:21Z
dc.descriptionWe investigate the dynamics of a cosmological dark matter fluid in the Schrödinger formulation, seeking to evaluate the approach as a potential tool for theorists. We find simple wave-mechanical solutions of the equations for the cosmological homogeneous background evolution of the dark matter field, and use them to obtain a piecewise analytic solution for the evolution of a compensated spherical overdensity. We analyse this solution from a `quantum mechanical' viewpoint, and establish the correct boundary conditions satisfied by the wavefunction. Using techniques from multi-particle quantum mechanics, we establish the equations governing the evolution of multiple fluids and then solve them numerically in such a system. Our results establish the viability of the Schrödinger formulation as a genuine alternative to standard methods in certain contexts, and a novel way to model multiple fluids.
dc.description12 pages, 8 figures, submitted to MNRAS
dc.identifierhttps://arxiv.org/abs/0904.0611
dc.identifierhttp://arxiv.org/abs/0904.0611
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/225818
dc.subjectCosmology and Nongalactic Astrophysics
dc.titleCosmological fluid dynamics in the Schrödinger formalism
dc.typetext

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