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LISA sources in Milky Way globular clusters

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arxiv 1802.05661 v5 pith:VGBCKYWA submitted 2018-02-15 astro-ph.HE astro-ph.GA

Kyle Kremer , Sourav Chatterjee , Katelyn Breivik , Carl L. Rodriguez , Shane L. Larson , Frederic A. Rasio This is my paper · ORCID
classification astro-ph.HEastro-ph.GA
keywords detectablesourcesbinarieslisabh-bhclusterscontainglobular
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abstract

We explore the formation of double-compact-object binaries in Milky Way (MW) globular clusters (GCs) that may be detectable by the Laser Interferometer Space Antenna (LISA). We use a set of 137 fully evolved GC models that, overall, effectively match the properties of the observed GCs in the MW. We estimate that, in total, the MW GCs contain $\sim21$ sources that will be detectable by LISA. These detectable sources contain all combinations of black hole (BH), neutron star, and white dwarf components. We predict $\sim7$ of these sources will be BH-BH binaries. Furthermore, we show that some of these BH-BH binaries can have signal-to-noise ratios large enough to be detectable at the distance of the Andromeda galaxy or even the Virgo cluster.

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Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Analytic Waveforms for Eccentric Gravitational Wave Bursts

    gr-qc 2019-09 conditional novelty 7.0 of 10

    A new analytic 'effective fly-by' waveform family for eccentric gravitational wave bursts, validated against numerical and numerical-relativity waveforms.

  2. The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range

    gr-qc 2019-08 accept novelty 3.0 of 10

    A Decihertz Observatory would fill the gap between LISA and ground detectors, enabling early-warning multimessenger astronomy and measurements of intermediate-mass black hole populations.

  3. Waveform Modelling for the Laser Interferometer Space Antenna

    gr-qc 2023-11 unverdicted novelty 2.0 of 10

    A review of existing waveform models for LISA sources and the challenges that must still be overcome.

  4. Population Synthesis of Gravitational Wave Sources

    astro-ph.HE 2025-02 accept novelty 1.0 of 10

    A review of population synthesis: the codes, the environments, and the predicted rates and features of gravitational wave sources, with an emphasis on breaking degeneracies.

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