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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

Secular Evolution of Orbital Parameters for General Bound Orbits in Kerr Spacetime

Eccentric binary black holes: A new framework for numerical relativity waveform surrogates

When Vacuum Breaks: A Self-Consistency Test for Astrophysical Environments in Extreme Mass Ratio Inspirals

Chase Orbits, Not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates

Pitching Cosmic Curveballs: Environmental Effects on Extreme-Mass-Ratio Inspirals with Spinning Secondaries

Black Hole Mergers beyond General Relativity: A Self-Force Approach

Relativistic tidal dissipation and the gravitational-wave signal of a white dwarf orbiting an intermediate-mass black hole

Measuring the neutron star equation of state from EMRIs in dark matter environments with LISA

Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis

Efficient and stable computation of gravitational-wave fluxes from generic Kerr orbits via a unified Heun-function framework

Adiabatic evolution of asymmetric binaries on generic orbits with new fundamental fields I: Characterization of gravitational wave fluxes

Probing Kerr symmetry breaking with LISA: Extreme-mass-ratio inspirals

Quantifying the scientific potential of intermediate and extreme mass ratio inspirals with the Laser Interferometer Space Antenna

Quadrupole and quadratic-in-spin effects in quasicircular, spinning, asymmetric binaries

New approach to the calculation of extreme-mass-ratio inspirals with a spinning secondary

Efficient eccentric effective-one-body dynamics via near-identity averaging transformations

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

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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

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