# Harald P. Pfeiffer, Ph.D.

## Affiliations: | 2003-2009 | California Institute of Technology, Pasadena, CA | |

2009- | University of Toronto, Toronto, ON, Canada |

##### Area:

Gravitational Physics/Theoretical Astrophysics##### Website:

http://www.cita.utoronto.ca/~pfeiffer/##### Google:

"Harald Pfeiffer"##### Bio:

https://inspirehep.net/record/993523?ln=en

## Mean distance: 12.78 | S | N | B | C | P |

#### Parents

Sign in to add mentorSaul Arno Teukolsky | grad student | 2003 | Cornell | |

(Initial data for black hole evolutions.) |

#### Children

Sign in to add traineeGeoffrey Mark Lovelace | grad student | 2007 | Caltech |

Ilana R. MacDonald | grad student | 2013 | University of Toronto |

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#### Publications

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van de Meent M, Pfeiffer HP. (2020) Intermediate Mass-Ratio Black Hole Binaries: Applicability of Small Mass-Ratio Perturbation Theory. Physical Review Letters. 125: 181101 |

Abbott R, Abbott TD, Abraham S, et al. (2020) GW190521: A Binary Black Hole Merger with a Total Mass of 150 M_{⊙}. Physical Review Letters. 125: 101102 |

Abbott R, Abbott TD, Abraham S, et al. (2020) Properties and Astrophysical Implications of the 150 M ⊙ Binary Black Hole Merger GW190521 The Astrophysical Journal. 900 |

Abbott R, Abbott TD, Abraham S, et al. (2020) GW190814: Gravitational Waves from the Coalescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object The Astrophysical Journal. 896: 1-20 |

Abbott BP, Abbott R, Abbott TD, et al. (2020) GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M ⊙ The Astrophysical Journal. 892: L3 |

Monitor FGB, Hamburg R, Fletcher C, et al. (2020) A joint Fermi-GBM and LIGO/Virgo analysis of compact binary mergers from the first and second gravitational-wave observing runs The Astrophysical Journal. 893: 100 |

Ossokine S, Buonanno A, Marsat S, et al. (2020) Multipolar Effective-One-Body Waveforms for Precessing Binary Black Holes: Construction and Validation Physical Review D. 102 |

Matas A, Dietrich T, Buonanno A, et al. (2020) An aligned-spin neutron-star--black-hole waveform model based on the effective-one-body approach and numerical-relativity simulations Physical Review D. 102 |

Abbott R, Abbott TD, Abraham S, et al. (2020) GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses Physical Review D. 102: 4301501-4301529 |

Shaik FH, Lange J, Field SE, et al. (2020) Impact of subdominant modes on the interpretation of gravitational-wave signals from heavy binary black hole systems Physical Review D. 101 |