Fast extreme-mass-ratio-inspiral waveforms: New tools for millihertz gravitational-wave data analysis

  title={Fast extreme-mass-ratio-inspiral waveforms: New tools for millihertz gravitational-wave data analysis},
  author={Michael L. Katz and Alvin J. K. Chua and Lorenzo Speri and Niels Warburton and Scott A. Hughes},
  journal={Physical Review D},
Michael L. Katz, Alvin J. K. Chua, Lorenzo Speri, Niels Warburton, and Scott A. Hughes Max-Planck-Institut für Gravitationsphysik, Albert-Einstein-Institut, Am Mühlenberg 1, 14476 Potsdam-Golm, Germany∗ Theoretical Astrophysics Group, California Institute of Technology, Pasadena, CA 91125, United States School of Mathematics and Statistics, University College Dublin, Belfield, Dublin 4, Ireland Department of Physics and MIT Kavli Institute, Massachusetts Institute of Technology, Cambridge, MA… 
Resonance crossing of a charged body in a magnetized Kerr background: an analogue of extreme mass ratio inspiral
We investigate resonance crossings of a charged body moving around a Kerr black hole immersed in an external homogeneous magnetic field. This system can serve as an electromagnetic analogue of a
Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity
Tousif Islam,1, 2, 3, 4, ∗ Scott E. Field,2, 3 Scott A. Hughes,5 Gaurav Khanna,6, 1, 3 Vijay Varma,7, † Matthew Giesler,8 Mark A. Scheel,9 Lawrence E. Kidder,8 and Harald P. Pfeiffer7 1Department of
Extreme mass-ratio inspirals as probes of scalar fields: eccentric equatorial orbits around Kerr black holes
Susanna Barsanti, 2 Nicola Franchini, 4 Leonardo Gualtieri, 2 Andrea Maselli, 6 and Thomas P. Sotiriou 8 Dipartimento di Fisica, “Sapienza” Università di Roma, Piazzale Aldo Moro 5, 00185, Roma,
Detection of scalar fields by extreme mass ratio inspirals with a Kerr black hole
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. Besides
Adiabatic equatorial inspirals of a spinning body into a Kerr black hole
The detection of gravitational waves from Extreme mass Ratio Inspirals (EMRIs) by the future space-based gravitational-wave detectors demands the generation of accurate enough waveform templates.
On Detecting Equatorial Symmetry Breaking with LISA
The equatorial symmetry of the Kerr black hole is generically broken in models of quantum gravity. Nevertheless, most phenomenological models start from the assumption of equatorial symmetry, and
Highly eccentric extreme-mass-ratio-inspiral waveforms via fast self-forced inspirals
Jonathan McCart, 2, ∗ Thomas Osburn, 3, † and Justin Y. J. Burton 1 Department of Physics and Astronomy, State University of New York at Geneseo, New York 14454, USA Machine Learning Center, Georgia
Detecting new fundamental fields with LISA
Andrea Maselli, Nicola Franchini, Leonardo Gualtieri, Thomas P. Sotiriou, Susanna Barsanti, Paolo Pani Gran Sasso Science Institute (GSSI), I-67100 L’Aquila, Italy INFN, Laboratori Nazionali del Gran
Assessing the impact of transient orbital resonances
One of the primary sources for the future space-based gravitational wave detector, the Laser Interferometer Space Antenna, are the inspirals of small compact objects into massive black holes in the


arXiv e-prints
  • arXiv:2102.02713
  • 2021
  • Rev. D 93, 064024
  • 2016
arXiv e-prints
  • arXiv:2008.06071
  • 2020
Contributors, “GSL - GNU scientific library - GNU project - free software foundation (FSF),
  • 2010
  • Rev. D 101, 064007
  • 2020
Classical and Quantum Gravity 32
  • 232002
  • 2015
  • Rev. D 78, 64028
  • 2008
  • J. 185, 635
  • 1973
  • Rev. D 75, 4005
  • 2007
Classical and Quantum Gravity 21
  • S1595
  • 2004