The Measure of the Universe: A History of Modern CosmologyClarendon Press, 1965 - 436 síður |
From inside the book
Niðurstöður 1 - 3 af 42
Síða 70
... spatial infinity , if it is essential that we treat the universe as of infinite spatial extent'.2 We have seen that , in another problem , both he and Schwarzschild had found similar boundary con- ditions to be necessary , both taking ...
... spatial infinity , if it is essential that we treat the universe as of infinite spatial extent'.2 We have seen that , in another problem , both he and Schwarzschild had found similar boundary con- ditions to be necessary , both taking ...
Síða 98
... spatial distance ' ( A ) between two points was then defined by A = R sin d cos ( y + d ) ( 36 ) ( y is a constant and R is the radius of curvature of the space ) and it was shown that ' a freely moving star and a freely moving observer ...
... spatial distance ' ( A ) between two points was then defined by A = R sin d cos ( y + d ) ( 36 ) ( y is a constant and R is the radius of curvature of the space ) and it was shown that ' a freely moving star and a freely moving observer ...
Síða 168
... spatial intervals in terms of spatial coordinates in the conventional Euclidean manner either in r - measure or in R - measure . If the former , that is to say if he uses the metric de2 = dr2 + r2 ( d02 + sin2 0 dp2 ) , ( 29 ) then the ...
... spatial intervals in terms of spatial coordinates in the conventional Euclidean manner either in r - measure or in R - measure . If the former , that is to say if he uses the metric de2 = dr2 + r2 ( d02 + sin2 0 dp2 ) , ( 29 ) then the ...
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