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发表于 2025-3-23 11:53:39 | 显示全部楼层
Effect of Small Pulsar Distance Variations in Stochastic GW Background Searches with PTAs,in stochastic gravitational wave background searches with Pulsar Timing Arrays”, Phys. Rev. D 90, 062011 (2014). I calculated the magnitude of the overlap reduction functions presented here, the Taylor series expansion, wrote and executed all the numerical codes used to make Table 3.1 and all the fi
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Cultural Citizenship and Beyond,rlap reduction functions presented here, the Taylor series expansion, wrote and executed all the numerical codes used to make Table 3.1 and all the figures except for the contour plots. I wrote the draft of this paper, and all the text included here.
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Introduction,coherent superposition of the cosmic population of SMBHBs is expected to form a diffusive GW background, which has yet to be detected, cf. Hellings and Downs (1983), Rajagopal and Romani (.), Wyithe and Loeb (.), Sesana et al. (.), Jaffe and Backer (.), Jenet et al. (.), Sesana et al. (.), van Haast
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