Cosmological fluid dynamics in the Schrödinger formalism

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

12 pages, 8 figures, submitted to MNRAS

Scientific paper

We investigate the dynamics of a cosmological dark matter fluid in the Schr\"odinger 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 Schr\"odinger formulation as a genuine alternative to standard methods in certain contexts, and a novel way to model multiple fluids.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Cosmological fluid dynamics in the Schrödinger formalism does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Cosmological fluid dynamics in the Schrödinger formalism, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmological fluid dynamics in the Schrödinger formalism will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-151194

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.