The Measure of the Universe: A History of Modern CosmologyClarendon Press, 1965 - 436 síður |
From inside the book
Niðurstöður 1 - 3 af 28
Síða 80
... spherical in order to avoid the necessity of assigning boundary conditions . 25 This was not developed at the time . The seemingly paradoxical ' curvature of space - time ' , and the ana- logies between spherical surfaces and ...
... spherical in order to avoid the necessity of assigning boundary conditions . 25 This was not developed at the time . The seemingly paradoxical ' curvature of space - time ' , and the ana- logies between spherical surfaces and ...
Síða 108
... spherical contingencies was drawn . This was a distinction neither Riemann nor any of his early followers ( such as Beltrami ) seems to have appreciated . De Sitter also made use of Schwarzschild's paper of 1900 , where the distinction ...
... spherical contingencies was drawn . This was a distinction neither Riemann nor any of his early followers ( such as Beltrami ) seems to have appreciated . De Sitter also made use of Schwarzschild's paper of 1900 , where the distinction ...
Síða 305
... spherical symmetry about each fundamental observer , 32 and criteria for the geometry of light paths similar to those of Helmholtz and Lie.33 ' Cosmological principles ' returned to the limelight with the advent of the series of papers ...
... spherical symmetry about each fundamental observer , 32 and criteria for the geometry of light paths similar to those of Helmholtz and Lie.33 ' Cosmological principles ' returned to the limelight with the advent of the series of papers ...
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