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樓主
發(fā)表于 2025-3-21 17:52:59 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Gravitational Waves from Coalescing Binaries
編輯Stanislav Babak
視頻videohttp://file.papertrans.cn/389/388245/388245.mp4
叢書名稱Synthesis Lectures on Wave Phenomena in the Physical Sciences
圖書封面Titlebook: ;
出版日期Book 2020
版次1
doihttps://doi.org/10.1007/978-3-031-02612-6
isbn_softcover978-3-031-01484-0
isbn_ebook978-3-031-02612-6Series ISSN 2690-2346 Series E-ISSN 2690-2354
issn_series 2690-2346
The information of publication is updating

書目名稱Gravitational Waves from Coalescing Binaries影響因子(影響力)




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沙發(fā)
發(fā)表于 2025-3-21 22:25:05 | 只看該作者
James A. Baker,Frederick Z. Culverhouseng binary systems. We start with the leading order description and then discuss the post-Newtonian approximation. Next, we describe the extreme mass ratio inspirals (EMRIs) and the basis for the effective-one-body approach. Finally, we touch the numerical relativity and its role in the GW signal mod
板凳
發(fā)表于 2025-3-22 02:13:30 | 只看該作者
地板
發(fā)表于 2025-3-22 06:31:07 | 只看該作者
5#
發(fā)表于 2025-3-22 08:54:01 | 只看該作者
https://doi.org/10.1057/9780230374409We start with remembering the basic statistical notions, then we will give a brief overview of the frequentist and Bayesian approaches. We apply this theory to a problem of GW data analysis; there we overview common techniques used in different frequency bands—LIGO, LISA, PTA.
6#
發(fā)表于 2025-3-22 14:26:02 | 只看該作者
7#
發(fā)表于 2025-3-22 20:04:47 | 只看該作者
8#
發(fā)表于 2025-3-23 00:14:22 | 只看該作者
GW Sources and Observatories,In this chapter we consider the specific aspects of GWs search in three frequency bands: (i) 101000 Hz with the ground-based laser interferometric observatories; (ii) 10.-0.1 Hz with the space-based observatory LISA; and (iii) 10.-10. Hz with the Pulsar Timing Array.
9#
發(fā)表于 2025-3-23 03:32:30 | 只看該作者
James A. Baker,Frederick Z. Culverhouseng binary systems. We start with the leading order description and then discuss the post-Newtonian approximation. Next, we describe the extreme mass ratio inspirals (EMRIs) and the basis for the effective-one-body approach. Finally, we touch the numerical relativity and its role in the GW signal modeling.
10#
發(fā)表于 2025-3-23 09:32:51 | 只看該作者
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