The Measure of the Universe: A History of Modern CosmologyClarendon Press, 1965 - 436 síður |
From inside the book
Niðurstöður 1 - 3 af 74
Síða 123
... mass of the universe is not a conserved quantity , since mass is lost in the conversion of matter to radiation ( the rest mass of a light quantum being zero ) . Nor , according to Eddington , is the mass of the universe ' relative to ...
... mass of the universe is not a conserved quantity , since mass is lost in the conversion of matter to radiation ( the rest mass of a light quantum being zero ) . Nor , according to Eddington , is the mass of the universe ' relative to ...
Síða 203
... mass to change in time would require a mechanism of continuous mass - redistri- bution , over and above that of particle - creation - and this regardless of whether or not the total mass changes . ( Dirac , in the paper referred to ...
... mass to change in time would require a mechanism of continuous mass - redistri- bution , over and above that of particle - creation - and this regardless of whether or not the total mass changes . ( Dirac , in the paper referred to ...
Síða 233
... mass from a star which has broken up ' would provide the star with momentum , whilst ' a secular and statistical ... mass and , as a result , it was found that each galaxy must recede from our own with a velocity proportional to its ...
... mass from a star which has broken up ' would provide the star with momentum , whilst ' a secular and statistical ... mass and , as a result , it was found that each galaxy must recede from our own with a velocity proportional to its ...
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