General relativity and conjugate ordinary differential equations
General relativity and conjugate ordinary differential equations
复制标题
广义相对论和共轭常微分方程
DOI:
10.1016/0022-0396(78)90012-8
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发表时间:
1978
影响因子:
2.4
通讯作者:
F. Tipler
中科院分区:
文献类型:
--
作者:
F. Tipler
This paper will essentially be concerned with a very aid problem in the theory of ordinary differential equations: what are sufficient conditions on the function F (t) in the equation d2x-p+ F (t) Jc;= 0 such that (I) has a solution with at least two zeros in an interval I? However, the sufficient conditions derived here are unusual in one respect: the motivation for the theorems comes from the physics of the gravitational field--General Relativity-and not from mathematical aesthetics. The notation and conventions of the equations and concepts from General Relativity theory will be the same as in [I]; see [2] for a more elementary introduction to General Relativity. Kecall that the object of study in Generai Relativity is a spacetime, which is a four-dimensional boundaryless Hausdorff manifold with a non-degenerate Lorentz metric g. A. timelike vector V is a vector satisfying g (V, V)< 0, a null vector satisfk g (V, V)=: 0 and a spacelike vector satisfies g (V, V)> 0. Latin indices label space and time dimensions and run from 1 to 4; Greek indices label space dimensions only and run from I to 3.