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書目名稱Gravitational Wave Astrophysics with Pulsar Timing Arrays影響因子(影響力)




書目名稱Gravitational Wave Astrophysics with Pulsar Timing Arrays影響因子(影響力)學(xué)科排名




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書目名稱Gravitational Wave Astrophysics with Pulsar Timing Arrays讀者反饋




書目名稱Gravitational Wave Astrophysics with Pulsar Timing Arrays讀者反饋學(xué)科排名

evasive

流浪者

吹牛需要藝術(shù)

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