Solar System Experiments in the Search for Dark Energy and Dark Matter
arXiv:2509.05910 · doi:10.1103/cmwl-xnhz
Abstract
We reassess the realistic discovery reach of Solar-System experiments for dark energy (DE) and dark matter (DM), making explicit the bridge from cosmology-level linear responses to local, screened residuals. In scalar-tensor frameworks with a universal conformal coupling and chameleon/Vainshtein screening, we map cosmological responses inferred by DESI and \emph{Euclid} to thin-shell or Vainshtein residuals in deep Solar potentials . We emphasize a two-branch strategy. In a detection-first branch, a verified local anomaly -- an Einstein equivalence principle (EEP) violation, a Shapiro-delay signal with , an AU-scale Yukawa tail, or a ultralight DM (ULDM) line in clocks/atom interferometers in space (AIS) -- triggers a joint refit of cosmology and Solar-System data under a common microphysical parameterization . In a guardrail branch, Solar-System tests enforce constraints (EEP; PPN parameters ; and ) and close unscreened or weakly screened corners indicated by cosmology. We forecast, per conjunction, (Ka-/X-band or optical Shapiro), $η_{EEP}\sim (1\mbox{--}10)\times 10^{-17}$ (drag-free AIS), (sub-mm-class LLR), a uniform ~2x tightening of AU-scale Yukawa/DM-density bounds, and improved ULDM-coupling reach from clocks. For a conformal benchmark, implies and a Sun thin shell at ; Vainshtein screening at 1 AU yields , naturally below near-term reach. We recommend a cost-effective guardrail+discovery portfolio with explicit triggers for escalation to dedicated missions.
32 pages, 4 figures, 12 tables
References in corpus (29)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- The Confrontation between General Relativity and Experiment
- Multi-messenger Observations of a Binary Neutron Star Merger
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- Causality, Analyticity and an IR Obstruction to UV Completion
- Dark Energy after GW170817: dead ends and the road ahead
- Strong constraints on cosmological gravity from GW170817 and GRB 170817A
- Searching for dilaton dark matter with atomic clocks
- Equivalence Principle Violations and Couplings of a Light Dilaton
- Search for ultralight scalar dark matter with atomic spectroscopy
- Searching for dark matter and variation of fundamental constants with laser and maser interferometry
- MICROSCOPE mission: final results of the test of the Equivalence Principle
- Matter-wave Atomic Gradiometer Interferometric Sensor (MAGIS-100)
- DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements
- Screening Modifications of Gravity through Disformally Coupled Fields
- Disformal Theories of Gravity: From the Solar System to Cosmology
- The Laser Astrometric Test of Relativity (LATOR) Mission
- Dark energy interactions near the galactic centre
- Testing Theories of Gravity with Planetary Ephemerides
- DESI results: Hint towards coupled dark matter and dark energy
- Screened Scalar Fields in the Laboratory and the Solar System
- Estimates of the change rate of solar mass and gravitational constant based on the dynamics of the Solar System
- Testing modified gravity via Yukawa potential in two body problem: Analytical solution and observational constraints
- Dilaton Solutions for Laboratory Constraints and Lunar Laser Ranging
- A Search for New Physics with the BEACON Mission
- The BepiColombo solar conjunction experiments revisited
- Multioscillating black holes
- Lunar Laser Ranging with High-Power CW Lasers
- Searching for new physics in the solar system with tetrahedral spacecraft formations