Theory and Experiment in Gravitational Physics
Abstract
The 2015 centenary of the publication of Einstein's general theory of relativity, and the first detection of gravitational waves have focused renewed attention on the question of whether Einstein was right. This review of experimental gravity provides a detailed survey of the intensive testing of Einstein's theory of gravity, including tests in the emerging strong-field dynamical regime. It discusses the theoretical frameworks needed to analyze gravitational theories and interpret experiments. Completely revised and updated, this new edition features coverage of new alternative theories of gravity, a unified treatment of gravitational radiation, and the implications of the latest binary pulsar observations. It spans the earliest tests involving the Solar System to the latest tests using gravitational waves detected from merging black holes and neutron stars. It is a comprehensive reference for researchers and graduate students working in general relativity, cosmology, particle physics and astrophysics.
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According to the general theory of relativity, a precise clock located at a position with higher geopotential runs quicker than a precise clock located at a position with lower geopotential.
“According to the GRT, a precise (atomic) clock located at the position P with higher geopotential runs quicker than a precise clock located at the position Q with lower geopotential [12,44,45].”
From Determination of the geopotential and orthometric height based on frequency shift equation (2011) · cites this paper as [45]
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“…probes near Earth, probes and relativistic corrections on the solar system scale, bound binaries producing gravitational waves in which at least one body is a compact object, and self-gravitating fluid dynamics plus post-Newtonian expansion for modeling the evolution of isolated stars (Will, 2018).”
- Authors
- Will, C. M.
- Affiliations
- Washington University in St. Louis (US)
- Corresponding author
- Will, Clifford M.
- ORCID
- Will, Clifford M.
- Venue
- Cambridge University Press eBooks
- Publisher
- Cambridge University Press
- Published
- 2018-09-07
- Volume
- 62
- Issue
- 12
- Pages
- 1153-1153
- OpenAlex
- W2058360989
- Cited by
- 3,637
- References
- 23
- Citations by year
- 2026: 56 · 2025: 95 · 2024: 119 · 2023: 86 · 2022: 98 · 2021: 168 · 2020: 137 · 2019: 115 · 2018: 157 · 2017: 122 · 2016: 125 · 2015: 111 · 2014: 120 · 2013: 139 · 2012: 105
- FWCI
- 55.20
- Type
- book
- Language
- en
- Open access
- closed
- Locations
- Cambridge University Press eBooks (publishedVersion)
- American Journal of Physics (publishedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Keywords
- tests of general relativity, modified gravity, gravitational waves, binary pulsars, strong-field tests, solar system tests, black hole mergers, neutron star mergers, Einstein's general relativity
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