Gravitational radiation from relativistic phase transitions
Gravitational radiation from relativistic phase transitions
复制标题
相对论相变产生的引力辐射
DOI：
10.1086/152193
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发表时间：
1973
期刊：
影响因子：
--
通讯作者：
J. Winicour
中科院分区：
文献类型：
--
作者：
J. Winicour
对引力波的产生和探测提出了半牛顿的处理方法。这被用来估计压力的相对论性增加带来的引力辐射。这些结果适用于各种天体物理过程，并与之相对应。结论是，在银河系中心可观测到的事件的产率必须超过1 M次太阳。(认证)
A semi-Newtonian treatment of the generation and detection of gravitational waves is presented. This is used to estimate the gravitational radiation from relativistic increases in pressure. The results are applied to various astrophysical processes, and the corresponding ed. It is concluded that observable events at the galactic center must have yields in excess of 1 M sub solar . (auth)