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翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク Static universe ： ウィキペディア英語版 Static universe A static universe, also referred to as a "stationary" or "infinite" or "static infinite" universe, is a cosmological model in which the universe is both spatially infinite and temporally infinite, and space is neither expanding nor contracting. Such a universe does not have spatial curvature; that is to say that it is 'flat'. A static infinite universe was first proposed by Giordano Bruno. In contrast to this model, Albert Einstein proposed a temporally infinite but spatially finite model as his preferred cosmology in 1917, in his paper ''Cosmological Considerations in the General Theory of Relativity''. After the discovery of the redshift–distance relationship (deduced by the inverse correlation of galactic brightness to redshift) by Vesto Slipher and Edwin Hubble, the Roman Catholic priest Georges Lemaître interpreted the redshift as proof of universal expansion and thus a Big Bang, whereas Fritz Zwicky proposed that the redshift was caused by the photons losing energy as they passed through the matter and/or forces in intergalactic space. Zwicky's proposal would come to be called 'tired light'- a term coined by the leading Big Bang proponent Richard Tolman. ==Einstein's universe== Albert Einstein added a positive cosmological constant to his equations of general relativity to counteract the attractive effects of gravity on ordinary matter, which would otherwise cause a spatially finite universe to either collapse or expand forever. This motivation evaporated after the proposal by the astrophysicist and Roman Catholic priest Georges Lemaître that the universe appears to be not static, but expanding. Edwin Hubble had researched data from the observations made by astronomer Vesto Slipher to confirm a relationship between redshift and distance, which forms the basis for the modern expansion paradigm that was introduced by Lemaître. According to George Gamow this led Einstein to declare this cosmological model, and especially the introduction of the cosmological constant, his "biggest blunder". Einstein's static universe is closed (i.e. has hyperspherical topology and positive spatial curvature), and contains uniform dust and a positive cosmological constant with value precisely $\backslash Lambda\_E\; =\; 4\backslash pi\; G\backslash rho/c^2$, where $G$ is Newtonian gravitational constant, $\backslash rho$ is the energy density of the matter in the universe and $c$ is the speed of light. The radius of curvature of space of the Einstein universe is equal to :$R\_E\; =\; \backslash Lambda\_E^\; =\; \{c\; \backslash over\; \backslash sqrt\{4\backslash pi\; G\backslash rho\}\}.$ The Einstein universe is one of Friedmann's solutions to Einstein's field equation for dust with density $\backslash rho$, cosmological constant $\backslash Lambda\_E$, and radius of curvature $R\_E$. It is the only non-trivial static solution to Friedmann's equations. Because the Einstein universe soon was recognized to be inherently unstable, it was shortly abandoned as a viable model for the universe. It is unstable in the sense that any slight change in either the value of the cosmological constant, the matter density, or the spatial curvature will result in a universe that either expands and accelerates forever or re-collapses to a big crunch. After Einstein renounced his cosmological constant, and embraced the Friedmann-LeMaitre model of an expanding universe, most physicists of the twentieth century assumed that the cosmological constant is zero. If so (absent some other form of dark energy), the expansion of the universe would be decelerating. However, after Saul Perlmutter, Brian P. Schmidt, and Adam G. Riess introduced the theory of an accelerating universe in 1998, a positive cosmological constant has been revived as a simple explanation for dark energy. 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Static universe」の詳細全文を読む スポンサード リンク 翻訳と辞書 : 翻訳のためのインターネットリソース Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.