Detecting supermassive black hole–induced binary eccentricity oscillations with LISA

Journal article

Stellar-mass black hole binaries (BHBs) near supermassive black holes (SMBH) in galactic nuclei undergo eccentricity oscillations due to gravitational perturbations from the SMBH. Previous works have shown that this channel can contribute to the overall BHB merger rate detected by the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo Interferometer. Significantly, the SMBH gravitational perturbations on the binary's orbit may produce eccentric BHBs which are expected to be visible using the upcoming Laser Interferometer Space Antenna (LISA) for a large fraction of their lifetime before they merge in the LIGO/Virgo band. For a proof of concept, we show that the eccentricity oscillations of these binaries can be detected with LISA for BHBs in the local universe up to a few megaparsecs, with observation periods shorter than the mission lifetime, thereby disentangling this merger channel from others. The approach presented here is straightforward to apply to a wide variety of compact object binaries with a tertiary companion.

Authors: Hoang, B-M; Naoz, S; Kocsis, B; Farr, WM; McIver, J

• Publication status: Published
• Peer review status: Peer reviewed
• Publisher: American Astronomical Society
• Journal: ASTROPHYSICAL JOURNAL LETTERS
• Volume: 875
• Issue: 2
• Pages: L31-L31
• Article number: ARTN L31
• Publication date: 2019-04-24
• DOI: 10.3847/2041-8213/ab14f7
• EISSN: 2041-8213
• ISSN: 2041-8205
• Keywords: FFR; galaxy: center; gravitational waves; quasars: supermassive black holes; galaxies: nuclei; stars: kinematics and dynamics; stars: black holes