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We study binary systems in which a stellar mass compact object spirals into a massive black hole, known as extreme mass ratio inspirals, in scenarios with a new fundamental scalar field.
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P. Amaro-Seoane, J. R. Gair, M. Freitag, M. Coleman Miller, I. Mandel, C. J. Cutler, and S. Babak, “Astrophysics, detection and science applications of intermediate- and extreme mass-ratio inspirals,” Class. Quant. Grav
2007
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L. Barack and C. Cutler, “Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes,” Phys. Rev. D
2007
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2008
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S. Alexander and N. Yunes, “Chern-Simons Modified General Relativity,” Phys. Rept
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F.-L. Julié, “On the motion of hairy black holes in Einstein-Maxwell-dilaton theories,” JCAP
2018
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L. Barack and A. Pound, “Self-force and radiation reaction in general relativity,” Rept. Prog. Phys
2019
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L. Speri and J. R. Gair, “Assessing the impact of transient orbital resonances,” Phys. Rev. D
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T. Damour and G. Esposito-Farese, “Tensor multiscalar theories of gravitation,” Class. Quant. Grav
2093
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