Matters of Gravity: Dark Matter and the Cosmological Constant
Burra G.Sidharth

TL;DR
This paper explores solutions to longstanding issues in cosmology by proposing a time-varying gravitational constant to address dark matter detection problems and using average universe density to explain the cosmological constant's value.
Contribution
It introduces a novel approach where a varying gravitational constant and universe density considerations resolve two major cosmological problems.
Findings
A varying gravitational constant could explain the non-detection of dark matter.
Average universe density can account for the observed value of the cosmological constant.
Proposes a unified framework for addressing dark matter and dark energy issues.
Abstract
We consider two problems that have vexed physicists for several decades -- dark matter and the cosmological constant. The problem has been that the former has not been detected while the latter gives a far higher value than detected by observation. We argue that a time varying gravitational constant obviates the former problem, while the latter problem can be circumvented by considering the average density of the universe.
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Taxonomy
TopicsRelativity and Gravitational Theory · Quantum and Classical Electrodynamics · Quantum Mechanics and Applications
