Testing sub-gravitational forces on atoms from a miniature, in-vacuum source mass

TL;DR

This paper demonstrates the detection of gravitational forces between freely falling atoms and a miniature in-vacuum source mass using atom interferometry, advancing the search for new physics beyond the standard model.

Contribution

It introduces a novel in-vacuum, miniature source mass setup for atom interferometry, enabling sensitive measurements of sub-gravitational forces at the particle level.

Findings

Strengthened limits on scalar field models like chameleon and symmetron.

Achieved sensitivity to gravitational-strength coupling with atom interferometry.

Paved the way for future measurements of Newton's G and gravitational Aharonov-Bohm effect.

Abstract

Gravity is the weakest fundamental interaction and the only one that has not been measured at the particle level. Traditional experimental methods, from astronomical observations to torsion balances, use macroscopic masses to both source and probe gravitational fields. Matter wave interferometers have used neutrons, atoms and molecular clusters as microscopic test particles, but initially probed the field sourced by the entire earth. Later, the gravitational field arising from hundreds of kilograms of artificial source masses was measured with atom interferometry. Miniaturizing the source mass and moving it into the vacuum chamber could improve positioning accuracy, allow the use of monocrystalline source masses for improved gravitational measurements, and test new physics, such as beyond-standard-model ("fifth") forces of nature and non-classical effects of gravity. In this work, we detect the gravitational force between freely falling cesium atoms and an in-vacuum, centimeter-sized source mass using atom interferometry with state-of-the-art sensitivity. The ability to sense gravitational-strength coupling is conjectured to access a natural lower bound for fundamental forces, thereby representing an important milestone in searches for physics beyond the standard model. A local, in-vacuum source mass is particularly sensitive to a wide class of interactions whose effects would otherwise be suppressed beyond detectability in regions of high matter density. For example, our measurement strengthens limits on a number of cosmologically-motivated scalar field models, such as chameleon and symmetron fields, by over two orders of magnitude and paves the way toward novel measurements of Newton's gravitational constant G and the gravitational Aharonov-Bohm effect