Preprint PUBDB-2023-07201

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Waveform Modelling for the Laser Interferometer Space Antenna

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2023

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Report No.: arXiv:2311.01300

Abstract: LISA, the Laser Interferometer Space Antenna, will usher in a new era in gravitational-wave astronomy. As the first anticipated space-based gravitational-wave detector, it will expand our view to the millihertz gravitational-wave sky, where a spectacular variety of interesting new sources abound: from millions of ultra-compact binaries in our Galaxy, to mergers of massive black holes at cosmological distances; from the beginnings of inspirals that will venture into the ground-based detectors' view to the death spiral of compact objects into massive black holes, and many sources in between. Central to realising LISA's discovery potential are waveform models, the theoretical and phenomenological predictions of the pattern of gravitational waves that these sources emit. This white paper is presented on behalf of the Waveform Working Group for the LISA Consortium. It provides a review of the current state of waveform models for LISA sources, and describes the significant challenges that must yet be overcome.

Keyword(s): LISA ; gravitational radiation: frequency ; black hole: binary: coalescence ; gravitational radiation detector ; binary: compact ; capture ; galaxy ; wave function ; black hole: mass


Note: 237 pages, 11 figures, white paper from the LISA Consortium Waveform Working Group, invited for submission to Living Reviews in Relativity

Contributing Institute(s):
  1. Theoretische Astroteilchenphysik (Z_THAT)
Research Program(s):
  1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2023
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Creative Commons Attribution CC BY 4.0 ; OpenAccess
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 Record created 2023-11-27, last modified 2024-03-01


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