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The deflection of light in the gravitational field of the Sun is one of the most fundamental consequences for general relativity as well as one of its classical tests first performed by Eddington a century ago.
Phys. Zeit
G. Nordström · 1912
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Ann. d. Phys
G. Nordström · 1913
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Ann. d. Phys
G. Nordström · 1913
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Ix. a determination of the deflection of light by the sun’s gravitational field, from observations made at the total eclipse of may 29, 1919
Frank Watson Dyson, Arthur Stanley Eddington, and Charles Davidson · 1920
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Apparent weight of photons
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D Kafri, JM Taylor, and GJ Milburn · 2014
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