The Irreversible Depletion of Dark Matter Spikes by Extreme-Mass-Ratio Inspirals
gr-qc, astro-ph.CO, astro-ph.GA, astro-ph.HE
Submitted: 2026-09-29
Updated: 2026-09-29
Terminology
Sources
- Dark matter annihilation at the galactic center
- Disks, spikes, and clouds: distinguishing environmental effects on BBH gravitational waveforms
- Circularization vs. Eccentrification in Intermediate Mass Ratio Inspirals inside Dark Matter Spikes
- The impact of relativistic corrections on the detectability of dark-matter spikes with gravitational waves
- Probing the Dark Matter density with gravitational waves from super-massive binary black holes
- Dynamical friction in dark matter spikes: corrections to Chandrasekhar's formula
- Dynamical friction from self-interacting dark matter
- Sharpening the dark matter signature in gravitational waveforms II: Numerical simulations with the NbodyIMRI code
- Self-interacting dark matter solves the final parsec problem of supermassive black hole mergers
- Sharpening the dark matter signature in gravitational waveforms I: Accretion and eccentricity evolution
- Fully Relativistic Treatment of Extreme Mass-Ratio Inspirals in Collisionless Environments
- Dark Drag Around Sagittarius A*
- Mass and spin coevolution of black holes inspiralling through dark matter
- Quantifying the Scientific Potential of Intermediate and Extreme Mass Ratio Inspirals with the Laser Interferometer Space Antenna
- LISA Definition Study Report
- Formation of Galactic Nuclei
- The Merger Rates and Mass Assembly Histories of Dark Matter Haloes in the Two Millennium Simulations
- EMERGE: Empirical predictions of galaxy merger rates since $z\sim6$
- The Depletion of Collisionless Dark Matter Spikes
- New Horizons for Fundamental Physics with LISA
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