相持不下 发表于 2025-3-21 17:52:59
书目名称Gravitational Waves from Coalescing Binaries影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0388245<br><br> <br><br>书目名称Gravitational Waves from Coalescing Binaries影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0388245<br><br> <br><br>书目名称Gravitational Waves from Coalescing Binaries网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0388245<br><br> <br><br>书目名称Gravitational Waves from Coalescing Binaries网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0388245<br><br> <br><br>书目名称Gravitational Waves from Coalescing Binaries被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0388245<br><br> <br><br>书目名称Gravitational Waves from Coalescing Binaries被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0388245<br><br> <br><br>书目名称Gravitational Waves from Coalescing Binaries年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0388245<br><br> <br><br>书目名称Gravitational Waves from Coalescing Binaries年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0388245<br><br> <br><br>书目名称Gravitational Waves from Coalescing Binaries读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0388245<br><br> <br><br>书目名称Gravitational Waves from Coalescing Binaries读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0388245<br><br> <br><br>争议的苹果 发表于 2025-3-21 22:25:05
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 modAmorous 发表于 2025-3-22 02:13:30
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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.可触知 发表于 2025-3-22 14:26:02
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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.AER 发表于 2025-3-23 03:32:30
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.VOC 发表于 2025-3-23 09:32:51
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