Cosmology, Black Holes and Shock Waves Beyond the Hubble Length
Joel Smoller, Blake Temple

TL;DR
This paper develops exact shock wave solutions within Einstein's equations, proposing a novel cosmological model where the Big Bang originates from a localized explosion inside a black hole, with implications for universe expansion and uniformity.
Contribution
It introduces a new class of entropy satisfying shock wave solutions extending the OS model to non-zero pressure inside black holes, forming the basis for a novel cosmological scenario.
Findings
Shock waves lie beyond one Hubble length from the FRW center.
Shock wave eventually weakens and settles to a zero-pressure interface.
The Big Bang shock wave emerges at the speed of light for a specific equation of state.
Abstract
We construct exact, entropy satisfying shock wave solutions of the Einstein equations for a perfect fluid which extend the Oppeheimer-Snyder (OS) model to the case of non-zero pressure, {\it inside the Black Hole}. These solutions put forth a new Cosmological Model in which the expanding Friedmann-Robertson-Walker (FRW) universe emerges from the Big Bang with a shock wave at the leading edge of the expansion, analogous to a classical shock wave explosion. This explosion is large enough to account for the enormous scale on which the galaxies and the background radiation appear uniform. In these models, the shock wave must lie beyond one Hubble length from the FRW center, this threshhold being the boundary across which the bounded mass lies inside its own Schwarzshild radius, and thus the shock wave solution evolves inside a Black Hole. The entropy condition, which breaks the…
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
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Fluid Dynamics and Turbulent Flows
