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The astrophysical science case for a decihertz gravitational-wave detector

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arxiv 1710.11187 v1 pith:QMKCP7GE submitted 2017-10-30 astro-ph.HE astro-ph.SRgr-qc

Ilya Mandel , Alberto Sesana , Alberto Vecchio This is my paper · ORCID
classification astro-ph.HEastro-ph.SRgr-qc
keywords astrophysicalblackcasedecihertzgravitational-waveholessciencebinaries
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We discuss the astrophysical science case for a decihertz gravitational-wave mission. We focus on unique opportunities for scientific discovery in this frequency range, including probes of type IA supernova progenitors, mergers in the presence of third bodies, intermediate mass black holes, seeds of massive black holes, improved sky localization, and tracking the population of merging compact binaries.

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Cited by 5 Pith papers

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  1. Detecting White Dwarf Binary Mergers with Gravitational Waves

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    MAGIS Space and AEDGE could detect white-dwarf-binary mergers in the 10 mHz–1 Hz band, giving early warning of Type Ia supernova explosions at rates of roughly one every four years and a few hundred per year, respectively.

  2. Astrophysics and cosmology with a decihertz gravitational-wave detector: TianGO

    gr-qc 2019-08 conditional novelty 6.0 of 10

    A decihertz space gravitational-wave detector paired with a ground network would localize compact binary mergers far more precisely than the ground network alone, supporting standard-siren cosmology, early warning, an...

  3. Terrestrial Very-Long-Baseline Atom Interferometry: Summary of the Second Workshop

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    A workshop summary that compiles physics targets, technology advances, and a proto-collaboration roadmap for kilometer-scale atom interferometers aimed at dark matter and gravitational wave detection.

  4. 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.

  5. 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.

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