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发表于 2025-3-21 16:15:29 | 显示全部楼层 |阅读模式
书目名称Gravitational Wave Astrophysics
编辑Carlos F. Sopuerta
视频video
丛书名称Astrophysics and Space Science Proceedings
图书封面Titlebook: ;
出版日期Conference proceedings 2015
版次1
doihttps://doi.org/10.1007/978-3-319-10488-1
isbn_softcover978-3-319-38292-0
isbn_ebook978-3-319-10488-1Series ISSN 1570-6591 Series E-ISSN 1570-6605
issn_series 1570-6591
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发表于 2025-3-21 21:36:29 | 显示全部楼层
https://doi.org/10.1007/978-3-476-02811-2f the expected GW signal, highlighting its dependence on the overall binary population, the relation between SMBHs and their hosts, and their coupling with the stellar and gaseous environment. I describe the status of current PTA efforts, and prospect of future detection and SMBH binary astrophysics.
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The Coalescence Rates of Compact Object Binaries,ulations of binary evolution. The two methods give consistent results, yet the uncertainties are still quite large. Nevertheless the current estimates point that the probability of detection of gravitational waves in the coming years is quite high.
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Biofeedback in der Narbentherapie,stant specific angular momentum profile that we study, we observe a significant change of the disk shape after a few orbits. This change is more pronounced the larger the initial inclination angle is.
发表于 2025-3-23 07:50:34 | 显示全部楼层
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