Exact Solution to Standard Model Hydrodynamic Cosmological Perturbation Theory and its Implications for Acoustic Oscillations
Philip D. Mannheim

TL;DR
This paper provides an exact hypergeometric function solution to cosmological perturbation theory during a matter-dominated era, revealing a maximum wavelength for acoustic oscillations that acts as a horizon.
Contribution
It offers a novel exact analytical solution to standard model cosmological perturbations, highlighting a fundamental limit on acoustic oscillation wavelengths.
Findings
Identifies a maximum wavelength for acoustic oscillations.
Provides an exact hypergeometric function solution.
Suggests a horizon for acoustic oscillations.
Abstract
We present an exact solution to standard model cosmological perturbation theory in a matter-dominated, adiabatic, hydrodynamic era. The solution is in the form of hypergeometric functions. While such functions can oscillate with the sound velocity, they can only do so at high frequency. There is thus a maximum wavelength to these oscillations, with this maximum wavelength serving to provide a horizon for acoustic oscillations.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsSolar and Space Plasma Dynamics · Geophysics and Gravity Measurements · Cosmology and Gravitation Theories
