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Intermediate/Extreme mass ratio inspiral (I/EMRI) system provides a good tool to test the nature of gravity in strong field.
LIGO Scientific and Virgo Collaborations
1903
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2003
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2003
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C. M. Will and N. Yunes, Testing alternative theories of gravity using LISA , Class. Quant. Grav. 21
2004
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M. C. Miller, Probing general relativity with mergers of supermassive and intermediate-mass black holes , Astrophys. J. 618
2004
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L. Barack and C. Cutler, LISA capture sources: Approximate waveforms, signal-to-noise ratios, and parameter estimation accuracy , Phys. Rev. D 69
2016
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2004
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E. Berti, A. Buonanno and C. M. Will, Estimating spinning binary parameters and testing alternative theories of gravity with LISA , Phys. Rev. D 71
2005
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2005
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2006
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2007
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S. Babak, H. Fang, J. R. Gair, K. Glampedakis and S. A. Hughes, ’Kludge’ gravitational waveforms for a test-body orbiting a Kerr black hole , Phys. Rev. D 75
2007
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T. S. Keidl, J. L. Friedman and A. G. Wiseman, On finding fields and self-force in a gauge appropriate to separable wave equations , Phys. Rev. D 75
2007
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2007
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2016
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LIGO Scientific, Virgo, Fermi-GBM and INTEGRAL Collaborations
2017
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2017
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2017
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P. Creminelli and F. Vernizzi, Dark Energy after GW170817 and GRB170817A , Phys. Rev. Lett. 119
2017
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2017
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2017
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W.-R. Hu and Y.-L. Wu, The Taiji Program in Space for gravitational wave physics and the nature of gravity , Natl. Sci. Rev. 4
2017
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2017
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2017
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2017
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LIGO Scientific and Virgo Collaborations
2017
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2018
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M. Van De Meent and N. Warburton, Fast Self-forced Inspirals , Class. Quant. Grav. 35
2018
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LIGO Scientific and Virgo Collaborations
2019
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LIGO Scientific and Virgo Collaborations
2019
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2019
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2019
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2021
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2022
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2022
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C. M. Will, Bounding the mass of the graviton using gravitational wave observations of inspiralling compact binaries , Phys. Rev. D 57
2061
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A. Krolak, K. D. Kokkotas and G. Schaefer, On estimation of the postNewtonian parameters in the gravitational wave emission of a coalescing binary , Phys. Rev. D 52
2089
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T. Damour and G. Esposito-Farese, Tensor multiscalar theories of gravitation , Class. Quant. Grav. 9
2093
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