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We study extreme mass ratio inspirals occurring in modified gravity, for which the system is modeled by a small compact object with scalar charge spiraling into a supermassive Kerr black hole.
1909
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1910
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M. Vallisneri, Use and abuse of the Fisher information matrix in the assessment of gravitational-wave parameter-estimation prospects , Phys. Rev. D 77
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2016
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K. Yagi and L. C. Stein, Black Hole Based Tests of General Relativity , Class. Quant. Grav. 33
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F. M. Ramazanoğlu and F. Pretorius, Spontaneous Scalarization with Massive Fields , Phys. Rev. D 93
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2009
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2009
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2009
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2009
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LIGO Scientific
2010
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2010
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2010
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2010
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2016
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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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2018
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2018
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F.-L. Julié, On the motion of hairy black holes in Einstein-Maxwell-dilaton theories , JCAP 01
2018
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2018
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2018
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2018
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2019
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2019
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2019
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2019
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A. Kuntz, R. Penco and F. Piazza, Extreme mass ratio inspirals with scalar hair , Journal of Cosmology and Astroparticle Physics 2020
2020
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E. Barausse, E. Berti, T. Hertog, S. A. Hughes, P. Jetzer, P. Pani et al., Prospects for fundamental physics with lisa , General Relativity and Gravitation 52
2020
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2021
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2021
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T. Damour and G. Esposito-Farese, Tensor multiscalar theories of gravitation , Class. Quant. Grav. 9
2093
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