Gravitational Waves, Volume 1: Theory and Experiments
By E. Poisson. 2008
589 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/71a6dc0b6375612bb2d6f9b077b7d5f3f24ab12b
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In Astronomy and Astrophysics
- J. Silk
- K. Saikawa
- Luis Lehner
- A. Arvanitaki
- S. Dimopoulos
- S. Mukherjee
- Benjamin Dan Wandelt
- André Großardt
Citations in the corpus
- Large-misalignment mechanism for the formation of compact axion structures: Signatures from the QCD axion to fuzzy dark matter (2019, background): “[222, 223] and [224, 225], and assuming that our signal is peaked around frequency fGW with a spread of ∆f ∼ fGW, the sensitivity of a pulsar network consisting of Np pulsars is given by:”
- The Schrödinger–Newton equation and its foundations (2014, background): “To be more specific, in the linearised theory of gravity (3), the interaction between gravity and matter is given by the Hamiltonian [36] Hint = − 1 2 ∫ d3r hµν T µν .”
- Dynamics of stellar black holes in young star clusters with different metallicities – II. Black hole–black hole binaries (2014, unknown): “The mass of the BHs affects both the frequency and the amplitude of the GW signal (e.g. Maggiore 2008).”
- Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo (2019, unknown): “They are generated y accelerated masses and more precisely, to lowest order, by ime changes of the mass quadrupole [1], such as in the orbital otion of a binary system of compact stars.”
- Probing the theory of gravity with gravitational lensing of gravitational waves and galaxy surveys (2019, background): “…binaries can be written in terms of the redshifted chirp mass Mz = (1+z)M as (Hawking & Israel 1987; Cutler & Flanagan 1994; Poisson & Will 1995; Maggiore 2008) h(fz) = Q(angles) √ 5 24 G5/6M2z(fzMz)−7/6 c3/2π2/3dL eiφz , (4) where M = (m1m2) 3/5 (m1+m2) 1/5 is the true chirp mass in terms of…”
- A Review of Gravitational Waves from Cosmic Domain Walls (2017, background): “We expect to obtain a lot of important information about physics at very high energies from direct observations of GWs due to the fact that they interact very weakly with matter and hence preserve almost all the features characterizing astrophysical or cosmological events [3,4].”