The double pulsar -- A new testbed for relativistic gravity
The double pulsar -- A new testbed for relativistic gravity
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双脉冲星——相对论引力的新试验台
DOI：
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发表时间：
2004
期刊：
影响因子：
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通讯作者：
P. Freire
中科院分区：
文献类型：
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作者：
Michael Kramer;A. Lyne;M. Burgay;A. Possenti;R. Manchester;F. Camilo;M. Mclaughlin;D. Lorimer;N. D'Amico;B. C. Joshi;J. Reynolds;P. Freire
我们的团队几个月前发现的第一颗双脉冲星由两颗双脉冲星组成，一颗周期为22 ms，另一颗周期为2.7 s。这个周期只有2.4小时的双星系统为相对论引力物理提供了一个真正独特的实验室。在这篇文章中，我们总结了已发表的结果，并展望了未来观测的前景。
The first ever double pulsar, discovered by our team a few months ago, consists of two pulsars, one with period of 22 ms and the other with a period of 2.7 s. This binary system with a period of only 2.4-hr provides a truly unique laboratory for relativistic gravitational physics. In this contribution we summarize the published results and look at the prospects of future observations.