Results 111 to 120 of about 2,129 (213)

Dark matter and rotation curves of stars in galaxies [PDF]

open access: yesAstronomische Nachrichten, 2001
The dark matter accretion theory (around a central body) of the author on the basis of his 5-dimensional Projective Unified Field Theory (PUFT) is applied to the orbital motion of stars around the center of the Galaxy. The departure of the motion from Newtonian mechanics leads to approximately flat rotation curves being in rough accordance with the ...
openaire   +4 more sources

Galaxy rotation curve

open access: yes
We present a complete framework for galactic dynamics based on the Energy-Space Emergence (ESE) paradigm. Space is not empty – it is a quantized energy lattice with fundamental spacing α0 = 1.2 5× 10−1 0m. Mass is a cluster of space nodes. Gravity is node density gradient. Galaxy shape is determined by cen-tral mass and its rotation.
openaire   +1 more source

Modified Gravity as a Common Cause for Cosmic Acceleration and Flat Galaxy Rotation Curves [PDF]

open access: yes, 2012
Flat galaxy rotation curves and the accelerating Universe both imply the existence of a critical accelera-tion, which is of the same order of magnitude in both the cases, in spite of the galactic and cosmic length scales being vastly different.
Priti Mishra, Tejinder P. Singh
core  

Galaxy rotation curves. The theory

open access: yes, 2013
The non-gauge vector field with as simple as possible Lagrangian (\ref{Lagrangian}) turned out an adequate tool for macroscopic description of the main properties of dark matter. The dependence of the velocity of a star on the radius of the orbit $V\left(r\right) $ -- galaxy rotation curve -- is derived analytically from the first principles ...
openaire   +2 more sources

Galaxy rotation curves with lognormal density distribution [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
Accepted for publication by MNRAS January 30 ...
openaire   +2 more sources

Mapping the dynamics, star-formation rates, and chemical properties of galaxies with integral field spectroscopy [PDF]

open access: yes, 2005
Major advances in the development of instruments for eight and ten meter class telescopes are revolutionising our understanding of galaxy formation. In particular, Integral Field Spectrographs (which produce a three dimensional {x, y, velocity) map of a ...
Swinbank, Anthony Mark   +1 more
core  

Relativistic correction in galaxy rotation curves [PDF]

open access: yes, 2022
Dark matter is one of the great unknowns in the world of science, as its existence is evidenced as necessary to explain astrophysical and cosmological phenomena related to gravitational forces, but its composition is unknown as it does not have non ...
Silva Junior, Ramon de Oliveira
core  

The inner structure of Λ CDM haloes - II. Halo mass profiles and low surface brightness galaxy rotation curves [PDF]

open access: yes, 2004
We use a set of high-resolution cosmological N-body simulations to investigate the inner mass profile of galaxy-sized cold dark matter (CDM) haloes.
Frenk, C.S.   +30 more
core   +1 more source

Global monopoles in Horndeski theory

open access: yesEuropean Physical Journal C: Particles and Fields
In this article, global monopole solutions will be presented for the Horndeski theory by solving linearized field equations. We obtain two different classes of solutions depending on whether the Horndeski scalar field is massless or massive.
M. Haluk Seçuk, Özgür Delice
doaj   +1 more source

Hydrostatic Equilibrium Constraints in X-COP Galaxy Clusters: Testing Hyperconical Modified Gravity in Hot-gas-dominated Regions

open access: yesThe Astrophysical Journal
Modified Newtonian dynamics (MOND) was originally proposed to model galaxy rotation curves without dark matter. However, MOND presents difficulties in explaining the radial acceleration relation observed in galaxy clusters, and moreover, it does not ...
Robert Monjo
doaj   +1 more source

Home - About - Disclaimer - Privacy