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The Gödel metric is an exact solution of the Einstein field equations in which the stress–energy tensor contains two terms, the first representing the matter density of a homogeneous distribution of swirling dust particles, and the second associated with a nonzero cosmological constant (see lambdavacuum solution). It is also known as the Gödel solution. This solution has many unusual properties—in particular, the existence of closed timelike curves that would allow a time travel in a universe described by the solution. Its definition is somewhat artificial in that the value of the cosmological constant must be carefully chosen to match the density of the dust grains, but this spacetime is an important pedagogical example. The solution was found in 1949 by Kurt Gödel. ==Definition== Like any other Lorentzian spacetime, the Gödel solution presents the metric tensor in terms of some local coordinate chart. It may be easiest to understand the Gödel universe using the cylindrical coordinate system (presented below), but this article uses the chart that Gödel originally used. In this chart, the line element is : where is a nonzero real constant, which turns out to be the angular velocity of the surrounding dust grains around the ''y'' axis, as measured by a "non-spinning" observer riding one of the dust grains. "Non-spinning" means that it doesn't feel centrifugal forces, but in this coordinate frame it would actually be turning on an axis parallel to the ''y'' axis. As we shall see, the dust grains stay at constant values of x, y, and z. Their density in this coordinate chart increases with ''x'', but their density in their own frames of reference is the same everywhere. 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「Gödel metric」の詳細全文を読む スポンサード リンク
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