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We perform tests of General Relativity (GR) with gravitational waves (GWs) from the inspiral stage of compact binaries using a theory-independent framework, which adds generic phase corrections to each multipole of a GR waveform model in frequency domain.
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2004
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2004
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K. G. Arun, Bala R. Iyer, M. S. S. Qusailah, and B. S. Sathyaprakash, “Probing the non-linear structure of general relativity with black hole binaries,” Phys. Rev. D74
2006
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2015
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Thomas P. Sotiriou, “Black Holes and Scalar Fields,” Class. Quant. Grav. 32
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Benjamin D. Lackey, Mohit Nayyar, and Benjamin J. Owen, “Observational constraints on hyperons in neutron stars,” Phys. Rev. D73
2006
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Alessandra Buonanno, Yan-bei Chen, and Michele Vallisneri, “Detecting gravitational waves from precessing binaries of spinning compact objects: Adiabatic limit,” Phys. Rev. D 67
2006
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Y. Wiaux, L. Jacques, and P. Vandergheynst, “Fast spin 2 spherical harmonics transforms and application in cosmology,” Journal of Computational Physics 226
2007
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Noah Sennett, Probing Fundamental Physics With Gravitational Waves From Inspiraling Binary Systems , Ph.D. thesis , Maryland U., Maryland U. (2021)
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M. Kramer et al. , “Strong-Field Gravity Tests with the Double Pulsar,” Phys. Rev. X 11
2021
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