One Hundred Years of General Relativity 2017
DOI: 10.1142/9789814635134_0002
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Genesis of general relativity — A concise exposition

Abstract: This short exposition starts with a brief discussion of situation before the completion of special relativity (Le Verrier's discovery of the Mercury perihelion advance anomaly, Michelson-Morley experiment, Eötvös experiment, Newcomb's improved observation of Mercury perihelion advance, the proposals of various new gravity theories and the development of tensor analysis and differential geometry) and accounts for the main conceptual developments leading to the completion of the general relativity: gravity has f… Show more

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“…If the Sun acts as a lens, the deflection angle of light 1°away from the Sun (which is favorable for successful observations; see Titov et al 2018) can reach ∼500 mas, and the number of sources within 1°is ∼63. Therefore, the measurement precision of γ with 10 epochs of observations is expected to reach ∼10 −8 , achieving the advanced level in the next few decades (see chapter 8 in Ni 2017). In such a case, using measurements of light deflection caused by the gravitational fields of celestial bodies in the solar system via SKA-VLBI may allow astronomers to test the (noninertial) motion and multipole moment effect of celestial bodies, and test and develop secondorder or higher PPN formalisms and/or different metric theories of gravity (e.g., Damour & Nordtvedt 1993;Kopeikin & Makarov 2007;Fomalont et al 2009;Li et al 2022c).…”
Section: Solar System Tests Of Relativistic Gravitymentioning
confidence: 99%
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“…If the Sun acts as a lens, the deflection angle of light 1°away from the Sun (which is favorable for successful observations; see Titov et al 2018) can reach ∼500 mas, and the number of sources within 1°is ∼63. Therefore, the measurement precision of γ with 10 epochs of observations is expected to reach ∼10 −8 , achieving the advanced level in the next few decades (see chapter 8 in Ni 2017). In such a case, using measurements of light deflection caused by the gravitational fields of celestial bodies in the solar system via SKA-VLBI may allow astronomers to test the (noninertial) motion and multipole moment effect of celestial bodies, and test and develop secondorder or higher PPN formalisms and/or different metric theories of gravity (e.g., Damour & Nordtvedt 1993;Kopeikin & Makarov 2007;Fomalont et al 2009;Li et al 2022c).…”
Section: Solar System Tests Of Relativistic Gravitymentioning
confidence: 99%
“…where G is the gravitational constant, M e and R e are the solar mass and radius, respectively, a and e are the semimajor axis and the eccentricity of the orbit of Mercury, respectively, c is the speed of light, and J 2 , the solar quadrupole moment, is ∼10 −7 (see chapter 8 in Ni 2017). The second term is smaller than the first term by a factor of ∼6 × 10 −4 , and the precision of J 2 can currently reach ∼10 −2 (e.g., Pitjeva et al 2022).…”
Section: Solar System Tests Of Relativistic Gravitymentioning
confidence: 99%
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