The Measure of the Universe: A History of Modern CosmologyClarendon Press, 1965 - 436 síður |
From inside the book
Niðurstöður 1 - 3 af 32
Síða 181
... McCrea , maintaining that Newtonian mechanics cannot be applied in a self - consistent way to a uniform unbounded distribution of matter . In the light of this criticism McCrea modified his position.113 Taking the case of a pressure ...
... McCrea , maintaining that Newtonian mechanics cannot be applied in a self - consistent way to a uniform unbounded distribution of matter . In the light of this criticism McCrea modified his position.113 Taking the case of a pressure ...
Síða 183
... McCrea's modified theory is compared with Bondi's it is found that though one is for an ' arbitrarily large ' and the other for an unbounded material system , they give otherwise similar results . One such result concerns the status of ...
... McCrea's modified theory is compared with Bondi's it is found that though one is for an ' arbitrarily large ' and the other for an unbounded material system , they give otherwise similar results . One such result concerns the status of ...
Síða 216
... McCrea questioned the classical interpre- tation , for ' in classical mechanics the absolute value of the stress does not enter into the equations of motion . The latter depend only upon the gradient of the stress , so the stress may be ...
... McCrea questioned the classical interpre- tation , for ' in classical mechanics the absolute value of the stress does not enter into the equations of motion . The latter depend only upon the gradient of the stress , so the stress may be ...
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