Planets and Dark Energy
Carl H. Gibson (Univ. Cal. San Diego), Rudolph E. Schild (Harvard)

TL;DR
This paper presents a fluid mechanical model called hydro-gravitational-dynamics (HGD) that explains the formation of cosmic structures from the early universe to galaxy clusters, challenging standard dark energy interpretations.
Contribution
It introduces HGD as a new framework for understanding cosmic structure formation, emphasizing plasma fragmentation and fluid dynamics over traditional dark matter and dark energy models.
Findings
Proposes plasma fragmentation at 0.03 Myr forming large-scale structures.
Explains star and planet formation via binary mergers of primordial gas planets.
Suggests supernovae and planetary nebulae influence distance measurements and dark energy hypotheses.
Abstract
Self gravitational fluid mechanical methods termed hydro-gravitational-dynamics (HGD) predict plasma fragmentation 0.03 Myr after the turbulent big bang to form protosuperclustervoids, turbulent protosuperclusters, and protogalaxies at the 0.3 Myr transition from plasma to gas. Linear protogalaxyclusters fragment at 0.003 Mpc viscous-inertial scales along turbulent vortex lines or in spirals, as observed. The plasma protogalaxies fragment on transition into white-hot planet-mass gas clouds (PFPs) in million-solar-mass clumps (PGCs) that become globular-star-clusters (GCs) from tidal forces or dark matter (PGCs) by freezing and diffusion into 0.3 Mpc halos with 97% of the galaxy mass. The weakly collisional non-baryonic dark matter diffuses to > Mpc scales and fragments to form galaxy cluster halos. Stars and larger planets form by binary mergers of the trillion PFPs per PGC, mostly on…
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
TopicsGamma-ray bursts and supernovae · Stellar, planetary, and galactic studies · Astro and Planetary Science
