The Measure of the Universe: A History of Modern CosmologyClarendon Press, 1965 - 436 síður |
From inside the book
Niðurstöður 1 - 3 af 66
Síða 211
... theory of Bondi and Gold was the so - called ' Perfect Cosmological Principle ' . This will be discussed again in Part II . For the present we notice that whereas Milne's Cosmological Principle required the large - scale aspect of the ...
... theory of Bondi and Gold was the so - called ' Perfect Cosmological Principle ' . This will be discussed again in Part II . For the present we notice that whereas Milne's Cosmological Principle required the large - scale aspect of the ...
Síða 305
A History of Modern Cosmology John David North. combination of the sample principle , 31 the principle of spherical symmetry about each fundamental observer , 32 and criteria for the geometry of light paths ... COSMOLOGICAL PRINCIPLES 305.
A History of Modern Cosmology John David North. combination of the sample principle , 31 the principle of spherical symmetry about each fundamental observer , 32 and criteria for the geometry of light paths ... COSMOLOGICAL PRINCIPLES 305.
Síða 311
... Principle . Adding the similar solution of ( 1 ) and ( 3 ) : - με Ма ( 5 ) this becomes the ' perfect ' cosmological principle . Traditionally this interpretation was ... COSMOLOGICAL PRINCIPLES 311 Cosmological theories and models.
... Principle . Adding the similar solution of ( 1 ) and ( 3 ) : - με Ма ( 5 ) this becomes the ' perfect ' cosmological principle . Traditionally this interpretation was ... COSMOLOGICAL PRINCIPLES 311 Cosmological theories and models.
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