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ON INCOMPATIBILITY OF GRAVITATIONAL RADIATION WITH THE 1915 EINSTEIN EQUATION |
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| ON INCOMPATIBILITY OF GRAVITATIONAL RADIATION WITH THE 1915 EINSTEIN EQUATION |
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| 作者：物理 文章来源：网上搜集 点击数： 更新时间：2005-8-18 11:36:56 |
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d and therefore cannot be associated with a dynamic source [11]. In other words, there is no evidence for the existence of a physical dynamic solution.
With the Hulse-Taylor binary pulsar experiment [16], it became easier to identify that the problem is in (1). Subsequently, it has been shown that (3), as a first-order approximation, can be derived from physical requirements which lead to general relativity [11]. Thus, (3) is on solid theoretical ground and general relativity remains a viable theory. Note, however, that the proof of the nonexistence of bounded dynamic solutions for (1) is essentially independent of the experimental supports for (3).
To prove this, it is sufficient to consider weak gravity since a physical solution must be compatible with Einstein's [2] notion of weak gravity (i.e., if there were a dynamic solution for a field equation, it should have a dynamic solution for a related weak gravity [11]). To calculate the radiation, consider further,
G(( ( G(1)(( + G(2)(( , where G(1)(( = (c(c(( + H(1)((, (2b)
H(1)(( ( -(c((((c + (((c( + ((((c(dcd , and ?(( 上一页 [1] [2] [3] [4] [5] [6] [7] [8] [9] [10] ... 下一页 >> |
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