Weak-field limit of Kaluza-Klein models with spherical compactification: experimental constraints
Alexey Chopovsky, Maxim Eingorn, Alexander Zhuk

TL;DR
This paper examines six-dimensional Kaluza-Klein models with spherical compactification, analyzing their gravitational behavior and experimental constraints, and finds that certain parameter choices align with observed gravitational tests.
Contribution
It provides the first detailed analysis of weak-field gravitational tests for this specific Kaluza-Klein model with spherical internal space and derives experimental bounds on model parameters.
Findings
Yukawa-type corrections to Newtonian potential for certain parameters
Model satisfies Solar system gravitational tests with high accuracy
Stable compactification achieved for positive internal space equation of state parameter
Abstract
We investigate the classical gravitational tests for the six-dimensional Kaluza-Klein model with spherical (of a radius ) compactification of the internal space. The model contains also a bare multidimensional cosmological constant . The matter, which corresponds to this ansatz, can be simulated by a perfect fluid with the vacuum equation of state in the external space and an arbitrary equation of state with the parameter in the internal space. For example, and correspond to the monopole two-forms and the Casimir effect, respectively. In the particular case , the parameter is also absent: . In the weak-field approximation, we perturb the background ansatz by a point-like mass. We demonstrate that in the case the perturbed metric coefficients have the Yukawa type corrections with respect…
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