A test of general relativity using radio links with the Cassini spacecraft
Abstract
According to general relativity, photons are deflected and delayed by the curvature of space-time produced by any mass. The bending and delay are proportional to gamma + 1, where the parameter gamma is unity in general relativity but zero in the newtonian model of gravity. The quantity gamma - 1 measures the degree to which gravity is not a purely geometric effect and is affected by other fields; such fields may have strongly influenced the early Universe, but would have now weakened so as to produce tiny--but still detectable--effects. Several experiments have confirmed to an accuracy of approximately 0.1% the predictions for the deflection and delay of photons produced by the Sun. Here we report a measurement of the frequency shift of radio photons to and from the Cassini spacecraft as they passed near the Sun. Our result, gamma = 1 + (2.1 +/- 2.3) x 10(-5), agrees with the predictions of standard general relativity with a sensitivity that approaches the level at which, theoretically, deviations are expected in some cosmological models.
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Cassini-Huygens mission sets constraints so Brans-Dicke must be very close to GR; unless screening at small scales, this bound makes it difficult for Brans-Dicke theories to depart from GR at cosmological scales.
“The Cassini–Huygens mission (Bertotti et al. 2003) sets the constraints so Brans–Dicke must be very close to GR. Unless there is a successful screening mechanism at work at small scales, this bound makes it difficult for Brans–Dicke theories to depart from GR at cosmological scales.”
From Testing general relativity in cosmology (2019) · cites this paper as Bertotti et al. 2003
The most stringent constraint on Brans-Dicke theory comes from solar system tests, where the Cassini mission put the bound |ω_BD| > 40000.
“The most stringent constraint on Brans–Dicke (BD) theory comes from solar system tests where the Cassini mission put the bound (Bertotti et al. 2003; Will 2014).”
From Testing general relativity in cosmology (2019) · cites this paper as Bertotti et al. 2003
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- Authors
- Bertotti, B., Iess, L., & Tortora, P.
- Affiliations
- University of Pavia (IT)
- Sapienza University of Rome (IT)
- University of Bologna (IT)
- Corresponding author
- Iess, L.
- ORCID
- Venue
- Nature
- Published
- 2003-09
- Volume
- 425
- Issue
- 6956
- Pages
- 374-376
- ISSN
- 0028-0836 (ISSN-L)
- 1476-4687
- OpenAlex
- W2154120281
- Cited by
- 2,017
- References
- 1
- Citations by year
- 2026: 86 · 2025: 103 · 2024: 81 · 2023: 80 · 2022: 82 · 2021: 90 · 2020: 106 · 2019: 162 · 2018: 105 · 2017: 104 · 2016: 109 · 2015: 90 · 2014: 97 · 2013: 83 · 2012: 77
- FWCI
- 30.07
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Nature (publishedVersion)
- PubMed (publishedVersion)
- RePEc: Research Papers in Economics (submittedVersion)
- Archivio istituzionale della ricerca (Alma Mater Studiorum Università di Bologna) (submittedVersion)
- IRIS Research product catalog (Sapienza University of Rome) (submittedVersion)
- Funders
- Jet Propulsion Laboratory
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
- Keywords
- general relativity, gamma parameter, photon deflection, Cassini spacecraft, radio links, solar gravity, frequency shift, modified gravity, cosmological models
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