Rotation curves velocities obtained by warm low-density plasma simulating dark halos and dark matter
Y. Ben-Aryeh

TL;DR
This paper models warm low-density plasma as a potential explanation for galaxy rotation curves, suggesting it could account for the missing mass typically attributed to dark matter.
Contribution
It develops a new plasma-based model for galaxy halos, providing a novel approach to explain rotation curves without solely relying on dark matter.
Findings
Plasma density decreases exponentially with distance from galaxy center.
Large plasma mass can explain galaxy rotation curves.
Model suggests plasma halos are transparent in most electromagnetic spectra.
Abstract
The free electron model with Boltzmann statistics for spherical low-density plasmas is developed further with asymptotic relations obtaining the density of electrons, mass densities, and the potentials of such plasmas. Solutions are developed as function of a pure number proportional to the distance from the stellar plasma center (galaxy center) with extremely small coefficient, so that these solutions are essentially functions of large astronomical distances and masses. The present plasma is divided into a central part and very long tail, where the central part of the plasma shows an exponential dependence on the distance from the galaxy center, but a part of the large mass of this plasma is included in the long stellar plasma tail. The present model is specialized to completely ionized Hydrogen plasma (with a small correction factor considering its mixture with heavier atoms) where…
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
TopicsStellar, planetary, and galactic studies · Galaxies: Formation, Evolution, Phenomena · Astronomical Observations and Instrumentation
