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




書(shū)目名稱Gravitational Waves from Coalescing Binaries影響因子(影響力)學(xué)科排名




書(shū)目名稱Gravitational Waves from Coalescing Binaries網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱Gravitational Waves from Coalescing Binaries網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱Gravitational Waves from Coalescing Binaries被引頻次




書(shū)目名稱Gravitational Waves from Coalescing Binaries被引頻次學(xué)科排名




書(shū)目名稱Gravitational Waves from Coalescing Binaries年度引用




書(shū)目名稱Gravitational Waves from Coalescing Binaries年度引用學(xué)科排名




書(shū)目名稱Gravitational Waves from Coalescing Binaries讀者反饋




書(shū)目名稱Gravitational Waves from Coalescing Binaries讀者反饋學(xué)科排名

爭(zhēng)議的蘋果

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

Amorous

侵略主義

小臼

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.

可觸知

可觸知

Daily-Value

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

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.

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