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Efficient waveforms for asymmetric-mass eccentric equatorial inspirals into rapidly spinning black holes

Christian E. A. Chapman-Bird ^1,2,*, Lorenzo Speri ³, Zachary Nasipak ⁴, Ollie Burke ^2,5, Michael L. Katz⁶, Alessandro Santini ⁷, Shubham Kejriwal ⁸, Philip Lynch ⁷, Josh Mathews ⁸ et al.

Hassan Khalvati ^9,10, Jonathan E. Thompson ^4,11, Soichiro Isoyama ⁸, Scott A. Hughes ¹², Niels Warburton ¹³, Alvin J. K. Chua ^8,14, and Maxime Pigou ⁵

¹Institute for Gravitational Wave Astronomy and School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, United Kingdom
²School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
³European Space Agency (ESA), European Space Research and Technology Centre (ESTEC), Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
⁴School of Mathematical Sciences and STAG Research Centre, University of Southampton, Southampton, United Kingdom, SO17 1BJ
⁵Laboratoire des 2 Infinis - Toulouse (L2IT-IN2P3), Université de Toulouse, CNRS, F-31062 Toulouse Cedex 9, France
⁶NASA Marshall Space Flight Center, Huntsville, Alabama 35811, USA
⁷Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, 14476 Potsdam, Germany
⁸Department of Physics, National University of Singapore, 21 Lower Kent Ridge Rd, Singapore 119077
⁹Perimeter Institute for Theoretical Physics, Ontario, N2L 2Y5, Canada
¹⁰University of Guelph, Guelph, Ontario N1G 2W1, Canada
¹¹Theoretical Astrophysics Group, California Institute of Technology, Pasadena, California 91125, USA
¹²Department of Physics and MIT Kavli Institute, MIT, Cambridge, Massachusetts 02139 USA
¹³School of Mathematics & Statistics, University College Dublin, Belfield, Dublin 4, Ireland
¹⁴Department of Mathematics, National University of Singapore, Singapore 119076

^*Contact author: c.chapman-bird@bham.ac.uk

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Articles Citing

Efficient waveforms for asymmetric-mass eccentric equatorial inspirals into rapidly spinning black holes

A multi-parameter expansion for the evolution of asymmetric binaries in astrophysical environments

Probing fundamental physics with extreme mass ratio inspirals: Full Bayesian inference for scalar charge

Single-harmonic search for extreme mass-ratio inspirals

Eccentricity distribution of extreme mass ratio inspirals

Transition-to-plunge self-force waveforms with a spinning primary

Hierarchical modeling of gravitational-wave populations for disentangling environmental and modified-gravity effects

Particles with precessing spin in Kerr spacetime: Analytic solutions for eccentric orbits and homoclinic motion near the equatorial plane

Postadiabatic self-force waveforms: Slowly spinning primary and precessing secondary

Hybrid waveform model for asymmetric spinning binaries: Self-force meets post-Newtonian theory

Extreme-mass-ratio inspirals in relativistic accretion discs

Systematic errors in fast relativistic waveforms for extreme mass ratio inspirals

Gravitational waves from the late inspiral, transition, and plunge of small-mass-ratio eccentric binaries

Gravitational radiation from hyperbolic orbits: Comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results

Constraining modified theories of gravity through the detection of one extremely large mass-ratio inspiral

First-time assessment of glitch-induced bias and uncertainty in inference of extreme mass ratio inspirals

Gravitational radiation from Kerr black holes using the Sasaki-Nakamura formalism: Waveforms and fluxes at infinity

Probing scalar field with generic extreme mass-ratio inspirals around Kerr black holes

Constraint on massive vector field with extreme-mass-ratio inspirals around a slowly rotating black hole

Assessing signal crosstalk between extreme-mass-ratio inspirals and Galactic binaries in LISA data

Extended mass distribution of PBHs during the QCD phase transition: Stochastic gravitational wave backgrounds and mini-extreme mass ratio inspirals

Spherical inspirals of spinning bodies into Kerr black holes

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