The Measure of the Universe: A History of Modern CosmologyClarendon Press, 1965 - 436 síður |
From inside the book
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Síða 179
... relativistic cosmology , ( 2 / Rc2 ) R " + ( R ' / cR ) 2 + ( k / R2 ) = 0 , ( 46 ) the connexion requiring the identification of k with -AB2 / 3 / c2.105 This last equation is that which describes an expanding relativistic universe of ...
... relativistic cosmology , ( 2 / Rc2 ) R " + ( R ' / cR ) 2 + ( k / R2 ) = 0 , ( 46 ) the connexion requiring the identification of k with -AB2 / 3 / c2.105 This last equation is that which describes an expanding relativistic universe of ...
Síða 184
... relativistic cosmology ' , and as one which makes for clarity in so far as it avoids ' the cumbrous tensor calculus'.123 Despite these remarks he adds , rather wistfully , that it is hardly worth while nowadays to compare Newtonian ...
... relativistic cosmology ' , and as one which makes for clarity in so far as it avoids ' the cumbrous tensor calculus'.123 Despite these remarks he adds , rather wistfully , that it is hardly worth while nowadays to compare Newtonian ...
Síða 359
... cosmic time 7 , Robertson purported to equate Milne's model to a relativistic model with a metric of the sort he and Walker derived for relativistic cosmology . Milne's answer was that he objected to the use of the ' cosmic time ' 7 as ...
... cosmic time 7 , Robertson purported to equate Milne's model to a relativistic model with a metric of the sort he and Walker derived for relativistic cosmology . Milne's answer was that he objected to the use of the ' cosmic time ' 7 as ...
Efni
COSMOLOGICAL DIFFICULTIES WITH | 16 |
FIELD THEORIES AND THE WISH TO | 24 |
The Le SageThomson explanation of gravitation | 38 |
Höfundarréttur | |
19 aðrir hlutar ekki sýndir
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The Measure of the Universe: A History of Modern Cosmology John David North Engin sýnishorn í boði - 1965 |
Common terms and phrases
absolute apparent magnitude appear argument assumption astronomical Bondi chapter clusters concept constant coordinates corresponding Cosmological Principle cosmological theories cosmologists covariant creation curvature density derived distance Eddington Einstein energy equivalent Euclidean Euclidean geometry example expanding universe expansion explained fact field equations finite formula function galactic galaxies geodesics geometry given gravitational field homogeneous Hubble Hubble's Hubble's Law hypothesis ibid idea infinite infinity interpretation isotropy Leibniz Lemaître light line-element Mach's Principle mass Math mathematical matter McCrea McVittie mean metric Milne Milne's motion nebulae Newton's Newtonian non-Euclidean geometry objects observer P. G. Tait parallax particles Phys physical possible problem radial reason regarded relation relativistic cosmology result Riemannian scientific seems sense simple Sitter solution space space-time spatial spectral spherical stars steady-state theories supposed tensor theoretical theory of gravitation Theory of Relativity tion Tolman universe velocity Weyl's Principle Whitehead Whitrow