首页 | 本学科首页   官方微博 | 高级检索  
     检索      

太阳系天体的后牛顿重力
引用本文:钟鸣乾.太阳系天体的后牛顿重力[J].西北大学学报,1999,29(5):381-383.
作者姓名:钟鸣乾
作者单位:西北大学物理学系!陕西西安710069
基金项目:中国科学技术大学天体物理和宇宙学基金
摘    要:计算和讨论了太阳和某些行星产生的广义相对论的后牛顿重力改正,并与牛顿引潮力进行了比较。结果表明,重力的后牛顿效应可能影响太阳系某些天体的运动和演化

关 键 词:后牛顿重力改正  广义相对论  太阳系天体  引潮力

Post Newtonian gravity of celestial bodies in solar system
ZHONG Ming,qian.Post Newtonian gravity of celestial bodies in solar system[J].Journal of Northwest University(Natural Science Edition),1999,29(5):381-383.
Authors:ZHONG Ming  qian
Abstract:Post Newtonian gravity correction to the acceleration of gravity in general relativity, produced by the sun and some planets,is calculated and discussed,and is compared with Newtonian tidal force.It is stated that the motion and evolution for some celestial bodies in the solar system may be influenced by the post Newtonian effect due to gravity.
Keywords:post-Newtonian gravity correction  general relativity  celestial bodies in solar system  tidal force
本文献已被 CNKI 维普 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号