Search engine for discovering works of Art, research articles, and books related to Art and Culture
ShareThis
Javascript must be enabled to continue!

An introduction of Universal Basic Mass Density for dark matter halos

View through CrossRef
Abstract In this work we propose a universal basic mass density and a universal basic metric inside dark matter halos in the framework of Einstein equations providing an analytical ground for learning about dark matter. In a previous work the authors have proposed a simplified model for galaxies: a Schwarzschild black hole (that contains all the baryonic matter of the galaxy) immersed inside a dark matter halo. The solution solved the Einstein equations perturbatively and successfully gave the flat rotation curve and the baryonic Tully-Fisher relation, the two signatures of spiral galaxies. In this work we take the black hole mass (the baryonic mass) of the solution to be zero in order to focus our study on the dark matter halo exclusively. Among the results (1) is the prediction of a universal basic mass density of dark matter, ρ = a0/2πGr, where a0 ≈ 2.8 × 10−11 m/s2 is a universal constant whose value was deduced from observations, (2) we show that the mass and velocity curve of the dark halo agree excellently with observational data at intermediate distances where the baryonic matter contribution is negligible, (3) we show that the constant a0 is the origin of the constant surface density of dark matter and the origin of the scale-radius/scale-density scaling relation of the Navarro-Frenk-White profile (4) we show how the inclusion of baryonic matter in our model solves the core-cusp problem.
Springer Science and Business Media LLC
Title: An introduction of Universal Basic Mass Density for dark matter halos
Description:
Abstract In this work we propose a universal basic mass density and a universal basic metric inside dark matter halos in the framework of Einstein equations providing an analytical ground for learning about dark matter.
In a previous work the authors have proposed a simplified model for galaxies: a Schwarzschild black hole (that contains all the baryonic matter of the galaxy) immersed inside a dark matter halo.
The solution solved the Einstein equations perturbatively and successfully gave the flat rotation curve and the baryonic Tully-Fisher relation, the two signatures of spiral galaxies.
In this work we take the black hole mass (the baryonic mass) of the solution to be zero in order to focus our study on the dark matter halo exclusively.
Among the results (1) is the prediction of a universal basic mass density of dark matter, ρ = a0/2πGr, where a0 ≈ 2.
8 × 10−11 m/s2 is a universal constant whose value was deduced from observations, (2) we show that the mass and velocity curve of the dark halo agree excellently with observational data at intermediate distances where the baryonic matter contribution is negligible, (3) we show that the constant a0 is the origin of the constant surface density of dark matter and the origin of the scale-radius/scale-density scaling relation of the Navarro-Frenk-White profile (4) we show how the inclusion of baryonic matter in our model solves the core-cusp problem.

Related Results

The Black Mass as Play: Dennis Wheatley's The Devil Rides Out
The Black Mass as Play: Dennis Wheatley's The Devil Rides Out
Literature—at least serious literature—is something that we work at. This is especially true within the academy. Literature departments are places where workers labour over texts c...
Spin Alignment of Dark Matter Halos: Fast Halos
Spin Alignment of Dark Matter Halos: Fast Halos
Abstract We investigate the spin alignment of dark matter halos by considering a mechanism somewhat similar to tidal locking; we dub it tidal-locking theory (TLT). W...
Evolution and statistics of non-sphericity of dark matter halos from cosmological N-body simulation
Evolution and statistics of non-sphericity of dark matter halos from cosmological N-body simulation
Abstract We revisit the non-sphericity of cluster-mass-scale halos from cosmological N-body simulation on the basis of triaxial modeling. In order to understand the ...
Faint and Extended Galaxies as Probes for Understanding the Nature of Dark Matter Particles
Faint and Extended Galaxies as Probes for Understanding the Nature of Dark Matter Particles
Dark matter remains one of the most enigmatic components of the universe, constituting approximately 27% of its total mass-energy content, yet its fundamental nature is still poorl...
Dark QED from inflation
Dark QED from inflation
Abstract One contribution to any dark sector’s abundance comes from its gravitational production during inflation. If the dark sector is weakly coupled to the ...
The dark matter and dark energy
The dark matter and dark energy
The dark matter and dark energy are one of the biggest challenges facing contemporary physics and astronomy. Dark energy and dark matter play an important role the universe. The am...
KONTESTASI TASAWUF SUNNÎ DAN TASAWUF FALSAFÎ DI NUSANTARA
KONTESTASI TASAWUF SUNNÎ DAN TASAWUF FALSAFÎ DI NUSANTARA
<p>This article scrutinizes the history of Islamic development in Nusantara between 15th to 18th centuries, which has been colored from theological mysticism thought. Uniquel...

Back to Top