“The abstractions of Einstein's curved space and time gave rise to analogies and pictures that played a new explanatory role.”
Cosmic Imagery: Key Images in the History of Science (2008)
Context: The abstractions of Einstein's curved space and time gave rise to analogies and pictures that played a new explanatory role. Space and time gave way to space-time, visible light was augmented by images across the rest of the electromagnetic spectrum, and we realised that we could see back towards the apparent beginnings of time.<!--part. 1, p. 8
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John D. Barrow58
British scientist 1952–2020Related quotes
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Source: 1900s, Notes d'un Peintre (Notes of a Painter) (1908), p. 410
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Source: 1942 - 1948, Arshile Gorky, – Goats on the roof' (2009), p. 357: in: 'A visit to the Metropolitan Museum with Gorky', Ethel Schwabacher, 1947
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Quote, 1919, as cited in Mondrian, -The Art of Destruction, Carel Blotkamp, Reaktion Books LTD. London 2001, p. 148
1910's
Gerald James Whitrow (1912–2000) British mathematician
p, 125
The Structure of the Universe: An Introduction to Cosmology (1949)
Laraine Day (1920–2007) American actress
The Independent, Obituaries, Laraine Day, November 13, 2007.
Roger Penrose book Fashion, Faith, and Fantasy in the New Physics of the Universe
Ch. 1, Mathematical Elegance as a Driving Force, p. 62 https://books.google.com/books?id=T09kCwAAQBAJ&pg=PA62. <br class="br">Fashion, Faith, and Fantasy in the New Physics of the Universe (2016)
Gerald James Whitrow (1912–2000) British mathematician
The Structure of the Universe: An Introduction to Cosmology (1949)
Context: The models of Einstein and de Sitter are static solutions of Einstein's modified gravitational equations for a world-wide homogeneous system. They both involve a positive cosmological constant λ, determining the curvature of space. If this constant is zero, we obtain a third model in classical infinite Euclidean space. This model is empty, the space-time being that of Special Relativity.
It has been shown that these are the only possible static world models based on Einstein's theory. In 1922, Friedmann... broke new ground by investigating non-static solutions to Einstein's field equations, in which the radius of curvature of space varies with time. This Possibility had already been envisaged, in a general sense, by Clifford in the eighties.<!--p.82