# Dressed dense atomic gases

**Authors:** Igor Lesanovsky, Beatriz Olmos, William Guerin, Robin Kaiser

arXiv: 1902.02989 · 2019-09-04

## TL;DR

This paper develops a theoretical framework for understanding how weakly excited dense atomic gases exhibit collective many-body interactions and how these effects can be probed through microwave spectroscopy, revealing complex non-equilibrium physics.

## Contribution

It introduces a novel theory for dressed many-body states in dense atomic gases and demonstrates how collective excitations lead to emergent many-body potentials beyond binary interactions.

## Key findings

- Collective excitations cause many-body interactions in dense gases.
- Microwave spectroscopy can detect time-dependent line-shifts related to these interactions.
- The phase pattern of the dressing laser influences the observed signals.

## Abstract

In dense atomic gases the interaction between transition dipoles and photons leads to the formation of many-body states with collective dissipation and long-ranged forces. Despite decades of research, a full understanding of this paradigmatic many-body problem is still lacking. Here, we put forward and explore a scenario in which a dense atomic gas is weakly excited by an off-resonant laser field. We develop the theory for describing such dressed many-body ensembles and show that collective excitations are responsible for the emergence of many-body interactions, i.e. effective potentials that cannot be represented as a sum of binary terms. We illustrate how interaction effects may be probed through microwave spectroscopy via the analysis of time-dependent line-shifts, and show that these signals are sensitive to the phase pattern of the dressing laser. Our study offers a new perspective on dense atomic ensembles interacting with light and promotes this platform as a setting for the exploration of rich non-equilibrium many-body physics.

## Full text

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## Figures

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## References

35 references — full list in the complete paper: https://tomesphere.com/paper/1902.02989/full.md

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Source: https://tomesphere.com/paper/1902.02989