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FERN

书目名称Gravitational Wave Astrophysics with Pulsar Timing Arrays影响因子(影响力)




书目名称Gravitational Wave Astrophysics with Pulsar Timing Arrays影响因子(影响力)学科排名




书目名称Gravitational Wave Astrophysics with Pulsar Timing Arrays网络公开度




书目名称Gravitational Wave Astrophysics with Pulsar Timing Arrays网络公开度学科排名




书目名称Gravitational Wave Astrophysics with Pulsar Timing Arrays被引频次




书目名称Gravitational Wave Astrophysics with Pulsar Timing Arrays被引频次学科排名




书目名称Gravitational Wave Astrophysics with Pulsar Timing Arrays年度引用




书目名称Gravitational Wave Astrophysics with Pulsar Timing Arrays年度引用学科排名




书目名称Gravitational Wave Astrophysics with Pulsar Timing Arrays读者反馈




书目名称Gravitational Wave Astrophysics with Pulsar Timing Arrays读者反馈学科排名

evasive

流浪者

吹牛需要艺术

https://doi.org/10.1007/978-3-642-51337-4articular, they provide a new means of addressing open questions in astrophysics and fundamental physics and for studying black holes: from their formation, evolution and demographics, to the assembly history of galactic structures and the dynamical behaviour of gravitational fields in the strong no

gusher

RAGE

Cultural Citizenship and Beyond,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

RAGE

Introduction and Overview: Who, What, Whyk hole binary using Pulsar Timing Arrays”, Physical Review Letters, Volume 109, Issue 8 (2012), cited as Mingarelli et al. (2012). Minor modifications here have been made to the paper: Figs. 4.1 and 4.2 have been added to clarify the geometry and the importance of the precession effects respectively

agenda

https://doi.org/10.1007/978-3-031-27473-2an anisotropic stochastic GW background, based on the formalism introduced in Mingarelli et al. (2013) (equivalently Chap. 2). Indeed, in Mingarelli et al. (2013) we show that the stochastic GWB may have a fractional degree of anisotropy of around 20 . at high frequencies, while Taylor and Gair (201

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FLACK