2019
DOI: 10.1103/physrevd.99.105002
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Quantum simulation of dark energy candidates

Abstract: Additional scalar fields from scalar-tensor, modified gravity or higher dimensional theories beyond general relativity may account for dark energy and the accelerating expansion of the Universe.These theories have led to proposed models of screening mechanisms, such as chameleon and symmetron fields, to account for the tight experimental bounds on fifth-force searches. Cold atom systems have been very successfully used to constrain the parameters of these screening models, and may in future eliminate the inter… Show more

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Cited by 10 publications
(6 citation statements)
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References 78 publications
(107 reference statements)
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“…Any topological defect passing through atomic clocks within the network would lead to a desynchronisation of the clocks with respect to a reference clock on the ground [468]. BECs can also be used to search for ultralight dark‐matter particles [469], constraining dark energy models [470], and testing physical regimes where quantum mechanics and GR may interact.…”
Section: Fundamental Physics Experimentsmentioning
confidence: 99%
“…Any topological defect passing through atomic clocks within the network would lead to a desynchronisation of the clocks with respect to a reference clock on the ground [468]. BECs can also be used to search for ultralight dark‐matter particles [469], constraining dark energy models [470], and testing physical regimes where quantum mechanics and GR may interact.…”
Section: Fundamental Physics Experimentsmentioning
confidence: 99%
“…Ref. [1]) At low values of the density ρ, the potential allows for spontaneous breaking of the Z 2 symmetry and therefore gives a nonvanishing vacuum expectation value to the symmetron (blue line). However, for ρ µ 2 M 2 , the symmetron can only have a vanishing vacuum expectation value and is therefore screened (orange line).…”
Section: Symmetronsmentioning
confidence: 99%
“…as points with an infinitely high mass density. Certainly, such an infinity can only be of a mathematical nature and must hint at a limitation of the theory 1 . Removing this limitation could be achieved by a UV-completion of GR, which is commonly assumed to be quantum gravity -a theory that reconciles quantum physics with GR.…”
Section: Introductionmentioning
confidence: 99%
“…Many scalar-tensor theories assume a conformal coupling between the metric tensor and the scalar field, and cold atom systems have been found to be well suited to studying these particular models in experiments (e.g. in atom interferometers [17,18]) and analogue gravity simulations [19]. Atom interferometry experiments currently provide the tightest constraints on some of these models [12,20].…”
mentioning
confidence: 99%
“…We begin by modelling our BEC as an interacting massive scalar Bose field Φ (x, t) in a covariant formalism to introduce the background metric in a natural way, following the approach of [19,57,58]. Note that we do not assume that the BEC has "relativistic" properties such as large excitation energies (i.e.…”
mentioning
confidence: 99%