Probing dark energy with atom interferometry
Theories of dark energy require a screening mechanism to explain why the associated scalar fields do not mediate observable long range fifth forces. The archetype of this is the chameleon field. Here we show that individual atoms are too small to screen the chameleon field inside a large high-vacuum...
| Main Authors: | Burrage, Clare, Copeland, Edmund J., Hinds, E. A. |
|---|---|
| Format: | Article |
| Published: |
IOP Science
2015
|
| Online Access: | https://eprints.nottingham.ac.uk/42099/ |
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