Gravity Resonance Spectroscopy and Dark Energy Symmetron Fields
arXiv:2012.07472 · doi:10.1140/epjs/s11734-021-00088-y
Abstract
Spectroscopic methods allow to measure energy differences with unrivaled precision. In the case of gravity resonance spectroscopy, energy differences of different gravitational states are measured without recourse to the electromagnetic interaction. This provides a very pure and background free look at gravitation and topics related to the central problem of dark energy and dark matter at short distances. In this article we analyse the effect of additional dark energy scalar symmetron fields, a leading candidate for a screened dark energy field, and place limits in a large volume of parameter space.
arXiv commentFQMT'19 conference proceedings, 9 pages, 8 figures
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Cited by in corpus (13)
- Testing Screened Modified Gravity
- Tests of Fundamental Quantum Mechanics and Dark Interactions with Low Energy Neutrons -- Extended Version
- Screened Scalar Fields in the Laboratory and the Solar System
- Next generation design and prospects for CANNEX
- Quantum gravitational states of ultracold neutrons as a tool for probing of beyond-Riemann gravity
- SELCIE: A tool for investigating the chameleon field of arbitrary sources
- Quantum-enhanced screened dark energy detection
- Search for dark energy with neutron interferometry
- Imprints of screened dark energy on nonlocal quantum correlations
- Dynamical Casimir effect with screened scalar fields
- Green's function analysis of the Neutron Lloyd interferometer
- Quantum and thermal pressures from light scalar fields
- Equivalence of scalar-tensor theories and scale-dependent gravity