《从零学相对论》连载26
发布时间:2018-10-17 17:54
【摘要】:正§8.8伯克霍夫定理正如§6.5所云,史瓦西之所以能够很快就求得真空爱因斯坦方程的第一个精确解,是因为他巧妙地利用了问题本身的对称性——恒星既是球对称的,又是静态的.然而,任何恒星都不是永恒不变的,它们也像人一样要经历生、老、病、死等各个演化阶段,恒星在许多阶段中并不处于静态之中,这时恒星外部的时空几何还可用史瓦西真空线元式(8-7-1)描述吗?如果有人向史瓦西提出这个问题,恐怕
[Abstract]:8. 8. Birkhoff Theorem, as in 搂6.5, Schwartz was able to quickly find the first exact solution to the vacuum Einstein equation because he skilfully took advantage of the symmetry of the problem itself-stars are spherical symmetry. It's static again. However, no star is permanent, and like a human being, it has to go through many stages of evolution, such as life, old age, sickness, death, and stars are not static in many stages. Can the space-time geometry outside the star be described by Swarthy's vacuum line element (8-7-1)? If this question were to be raised with Schwarzenegger, I am afraid
【作者单位】: 北京师范大学物理系;中科院应用数学所;
【分类号】:P159
本文编号:2277486
[Abstract]:8. 8. Birkhoff Theorem, as in 搂6.5, Schwartz was able to quickly find the first exact solution to the vacuum Einstein equation because he skilfully took advantage of the symmetry of the problem itself-stars are spherical symmetry. It's static again. However, no star is permanent, and like a human being, it has to go through many stages of evolution, such as life, old age, sickness, death, and stars are not static in many stages. Can the space-time geometry outside the star be described by Swarthy's vacuum line element (8-7-1)? If this question were to be raised with Schwarzenegger, I am afraid
【作者单位】: 北京师范大学物理系;中科院应用数学所;
【分类号】:P159
【相似文献】
相关会议论文 前1条
1 张双南;;对Birkhoff定理的理解、引力透镜的计算问题、物质向黑洞的塌缩问题、“冻结星”问题、史瓦西度规的奇异性问题[A];新观点新学说学术沙龙文集34:高能天体物理中的热点问题[C];2009年
相关博士学位论文 前1条
1 王富军;霍金辐射和黑洞熵[D];大连理工大学;2010年
相关硕士学位论文 前6条
1 苏沛;双黑洞引力场中电子辐射[D];上海师范大学;2013年
2 邓峻峰;黑洞时空中的量子纠缠提纯[D];湖南师范大学;2011年
3 陈秀武;2+1维旋转Dilaton黑洞的几何热力学研究[D];兰州大学;2012年
4 周盛;用等效势的方法分析膜理论中有径向密度分布的球对称黑洞的测地线[D];湖南师范大学;2012年
5 尹芬芬;圈量子修正黑洞的霍金辐射[D];湖南师范大学;2013年
6 畅伟伟;对流超射对5M_& 恒星演化的影响[D];浙江师范大学;2013年
,本文编号:2277486
本文链接:https://www.wllwen.com/kejilunwen/tianwen/2277486.html