Submitted:
09 April 2024
Posted:
09 April 2024
Read the latest preprint version here
Abstract
Keywords:
1. Introduction
even if we had a somewhat centrally distributed mass in the galaxy (the initial slow rise of the graph). Use of Gauss’ Law and a uniform, spherical distribution of matter would give
. A general distribution of matter (for non-relativistic considerations: Newtonian Gravity (NG), which is mostly the case) would involve this integral:
: mass dust, gas, stars, etc. but to obtain the Fisher-Tulley Law, additional “dark matter” is speculated as an extra gravitating source, other than matter already accounted for. This matter is most peculiar and only acts via the gravitational force. Some have postulated that dark matter may be primordial black holes[7]. Further speculation exists as to whether it is cold or hot and its distribution is expected to be a halo around galaxies out to several galactic radii.2. Is There Truly a Need for Dark Matter?
3. Conclusions
- ▪ Modify GR/NG and lose the mathematical structure of GR/NG
- ▪ Add elusive dark matter and hunt for that
- ▪ Modify the Cosmological “Constant” to vary with position/time and preserve the mathematical structure of GR/NG
References
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where a is the acceleration and is an area element normal to it. |


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