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双星和四极振子的引力波 被引量:1

Gravitational waves of the binary stars and the quadrupole oscillator
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摘要 按拉格朗日函数L =-g(λR +αRμνRμν +βR2 -Lm)的高导数引力理论研究力学系统的引力波问题 .在α>0 ,α +3 β <0的条件下 ,求出了双星和线性四极振子激发的引力辐射波 ,其结果当耦合常数α→ 0 ,β→ 0 时 ,与Einstein引力理论的结果相同 . The problems of the gravitational waves for the dynamic systems are studied in the higher-order theories of gravitation with Lagrangian L=-g(λR+αR μν R μν +βR 2+L m). In the case of α>0 and α+3β<0, the gravity radiating waves of the binary stars and the linear quadrupole oscillator are found. The results are the same as that of the Einstein theory of gravitation when α→0 and β→0.
作者 陈贻汉
出处 《湖北大学学报(自然科学版)》 CAS 2000年第1期40-43,48,共5页 Journal of Hubei University:Natural Science
关键词 R+R^2引力理论 引力波 双星 四极振子 R+R 2 gravitational theory gravitational wave binary stars quadrupole oscillator
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参考文献8

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