Tully–Fisher relations and retardation theory for galaxies
Author:
- 17 September 2021
- journal article
- research article
- Published by World Scientific Pub Co Pte Ltd in International Journal of Modern Physics D
- Vol. 30 (14)
Abstract
Galaxies are huge physical systems having dimensions of many tens of thousands of light years. Thus any change at the galactic center will be noticed at the rim only tens of thousands of years later. Those retardation effects seem to be neglected in present day galactic modeling used to calculate rotational velocities of matter in the rims of the galaxy. The significant differences between the predictions of Newtonian theory and observed velocities are usually explained by either assuming dark matter or by modifying the laws of gravity (MOND). In this essay, we will show that taking retardation effects into account one can explain the azimuthal velocities of galactic matter and the well known Tully–Fisher relations of galaxies.Keywords
All Related Versions
This publication has 10 references indexed in Scilit:
- Lorentz Symmetry Group, Retardation, Intergalactic Mass Depletion and Mechanisms Leading to Galactic Rotation CurvesSymmetry, 2020
- The Effect of Retardation on Galactic Rotation CurvesJournal of Physics: Conference Series, 2019
- Gravity, stability and cosmological modelsInternational Journal of Modern Physics D, 2017
- GRAVITY AND THE COMPLEXITY OF COORDINATES IN FISHER INFORMATIONInternational Journal of Modern Physics D, 2010
- THE GRAVITATIONAL ORIGIN OF THE DISTINCTION BETWEEN SPACE AND TIMEInternational Journal of Modern Physics D, 2009
- The Geometrical Meaning of TimeFoundations of Physics, 2008
- Dark matter and visible baryons in M33Monthly Notices of the Royal Astronomical Society, 2003
- Rotational properties of 21 SC galaxies with a large range of luminosities and radii, from NGC 4605 /R = 4kpc/ to UGC 2885 /R = 122 kpc/The Astrophysical Journal, 1980
- Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission RegionsThe Astrophysical Journal, 1970
- On a New Cluster of Nebulae in PiscesProceedings of the National Academy of Sciences, 1937