A proposed guided Bose-Einstein condensate interferometer could improve constraints on chameleon dark energy models by up to 3 orders of magnitude and on symmetron models by up to 26 orders of magnitude.
For the field to evolve to its vacuum minimum within the chamber, the Compton wavelength 15 must be smaller than the vacuum chamber radius
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Quantum-enhanced screened dark energy detection
A proposed guided Bose-Einstein condensate interferometer could improve constraints on chameleon dark energy models by up to 3 orders of magnitude and on symmetron models by up to 26 orders of magnitude.