Comparison of a new type of Dark Matter with the Milky Way and M31 grand rotation curves

In the electron Born self-energy (eBse) model, free electrons are of finite-size and possess both a rest mass, m e , as well as, a Born mass, m e B = 74,000 m e . The Born mass, which originates from the energy contained within the electric field that surrounds a finite-sized electron, serves as a D...

Full description

Saved in:
Bibliographic Details
Published inScientific reports Vol. 14; no. 1; pp. 24090 - 16
Main Author Law, Bruce M.
Format Journal Article
LanguageEnglish
Published London Nature Publishing Group UK 15.10.2024
Nature Publishing Group
Nature Portfolio
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary:In the electron Born self-energy (eBse) model, free electrons are of finite-size and possess both a rest mass, m e , as well as, a Born mass, m e B = 74,000 m e . The Born mass, which originates from the energy contained within the electric field that surrounds a finite-sized electron, serves as a Dark Matter (DM) particle in this theory (designated eBDM, electron Born Dark Matter). The equation of state for m e B is w = -1 , which implies that two Born masses experience a repulsive gravitational interaction. This repulsive gravitational interaction stabilizes the formation of a DM halo of m e B particles, of typical halo size ~ 100 kpc, around a central mass M (e.g. a galaxy), where this gravitational stability arises from the competing attractive M - m e B and repulsive m e B - m e B interactions. A solution of the linearized Poisson-Boltzmann equation, for this system, allows one to derive an expression for the rotational velocity V eBDM (R) , as a function of radius R from the galactic center. A composite model composed of rotational velocity contributions from the galactic bulge, galactic disk, as well as, V eBDM (R) is found to provide a good description of the Grand Rotation Curves for the Milky Way and M31 galaxies.
Bibliography:ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:2045-2322
2045-2322
DOI:10.1038/s41598-024-74884-6