The Measure of the Universe: A History of Modern CosmologyClarendon Press, 1965 - 436 síður |
From inside the book
Niðurstöður 1 - 3 af 46
Síða 118
... Lemaître . Although in point of time Lemaître's first great contribution to cosmology21 preceded this paper by Robertson , we have reserved mention of it until now because it marks the beginning of a new phase in cosmological thought ...
... Lemaître . Although in point of time Lemaître's first great contribution to cosmology21 preceded this paper by Robertson , we have reserved mention of it until now because it marks the beginning of a new phase in cosmological thought ...
Síða 120
... Lemaître's integral , which he himself did not discuss very fully , was carefully examined by de Sitter not long afterwards , 24 and a more complex integral , taking into account not only both open . and closed models but also positive ...
... Lemaître's integral , which he himself did not discuss very fully , was carefully examined by de Sitter not long afterwards , 24 and a more complex integral , taking into account not only both open . and closed models but also positive ...
Síða 122
... LEMAÎTRE MODEL Despite Robertson's contribution and its influence on American astronomy through Tolman , it was Lemaître who taught the majority how to avoid the dilemma involved in adopting either de Sitter's or Einstein's model . At a ...
... LEMAÎTRE MODEL Despite Robertson's contribution and its influence on American astronomy through Tolman , it was Lemaître who taught the majority how to avoid the dilemma involved in adopting either de Sitter's or Einstein's model . At a ...
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
Aðrar útgáfur - View all
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