Weak gravity at micron scales from dark bubble cosmology and its cosmological consequences
Ulf Danielsson, Suvendu Giri

TL;DR
This paper explores a dark bubble cosmology model predicting weaker gravity at micron scales, with implications for experimental tests, early universe inflation, and the universe's matter content, offering novel insights into cosmological constant problems.
Contribution
It introduces a dark bubble model that predicts weaker gravity at small scales and explains early inflation and matter content without new fields, connecting quantum origins with observable phenomena.
Findings
Gravity weakens at micron scales, measurable via tabletop experiments.
The model predicts a period of early inflation driven by reduced gravity at high densities.
It provides a cosmological explanation for the matter content and the cosmological constant's timing.
Abstract
The dark bubble model makes a positive cosmological constant natural in string theory, and predicts several new physical phenomena within reach in the near future. In this paper we study the experimental consequences of the model for the strength of gravity at scales of order m. Contrary to other models of gravity involving extra dimensions, the dark bubble model predicts gravity to become weaker rather than stronger at small scales, compared to Newtonian gravity. In particular, we provide explicit predictions of measurable deviations using table top experiments. We also show how the same effect reduces the effective force of gravity at high energy densities in cosmology, leading to a period of early inflation without the need for anything beyond radiation. We also discuss the quantum origin of the universe with a 5D black hole acting as a catalyst for the nucleation of the…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories
