pith. sign in

arxiv: 1902.08604 · v1 · pith:JDFO2BC6new · submitted 2019-02-22 · 🌌 astro-ph.HE · gr-qc· hep-ph

Observing Eccentricity Oscillations of Binary Black Holes in LISA

classification 🌌 astro-ph.HE gr-qchep-ph
keywords oscillationsbinarykozai-lidovbinariesblackeccentricitylisaobserving
0
0 comments X
read the original abstract

The tidal force from a third body near a binary system could introduce long-term oscillations in the binary's eccentricity, known as Kozai-Lidov oscillations. We show that the Kozai-Lidov oscillations of stellar-mass black hole binaries have the potential to be observed by LISA. Detections of such binaries will give insights into binary formation channels and also provide an important benchmark of observing Kozai-Lidov oscillations directly.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 5 Pith papers

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

  1. An Enhanced Formation Channel for Galactic Dual-Line Gravitational-Wave Sources: von Zeipel-Lidov-Kozai Effect in Triples Involving Sgr A*

    astro-ph.HE 2026-02 unverdicted novelty 7.0

    ZLK oscillations in Sgr A* triples enhance dual-line GW source formation rates by a factor of 5-10.

  2. Dynamics of Binary System around a Supermassive Black Hole :Binary Scattering and Eccentric vZLK Oscillations

    gr-qc 2026-05 unverdicted novelty 6.0

    Binaries around supermassive black holes exhibit four periapsis-dependent scattering regimes in unbound orbits and scattering-type eccentric vZLK oscillations in bound orbits within Kerr spacetime.

  3. Eccentric Stellar-mass Binary Black Holes: Population, Detectability, and Waveform Analysis in the LISA and LIGO Era

    astro-ph.HE 2026-05 unverdicted novelty 5.0

    Simulations of dynamically formed eccentric stellar-mass BBHs predict dozens of LISA-detectable sources in the Milky Way, hundreds of low-SNR extragalactic mHz sources, a merger rate of ~9 Gpc^{-3} yr^{-1}, and potent...

  4. Eccentricity Without Measuring Eccentricity: Discriminating Among Stellar Mass Black Hole Binary Formation Channels

    astro-ph.HE 2019-07 unverdicted novelty 5.0

    Eccentricity influences LISA binary counts via peak frequency, required density for LIGO rate match, and SNR reduction, enabling formation channel discrimination through frequency-dependent number counts without direc...

  5. Retrieving the True Masses of Gravitational-wave Sources

    astro-ph.HE 2019-06 unverdicted novelty 5.0

    Hydrodynamic drag makes BBH waveforms resemble higher-mass vacuum sources, biasing matched-filter chirp-mass estimates upward for LISA sources.