PulseTrendingJournal ClubResearchersJournalsExplore
Instagram
HomeTrendingJournal ClubExplore
Synapse
⌘+K
Synapse
March 12, 2024Physical review. D/Physical review. D.Open Access

Extreme mass-ratio inspiral and waveforms for a spinning body into a Kerr black hole via osculating geodesics and near-identity transformations

View Full Paper
Ask AI
Bookmark
Share

Authors

LDLisa V. DrummondPLPhilip LynchAHAlexandra G. Hanselman

Discussion

Loading...

Member takes

Overview

Key Points

Key points are not available for this paper at this time.

Cite This Study

Drummond et al. (2024) studied this question.

synapsesocial.com/papers/68e745a1b6db6435876be72chttps://doi.org/10.1103/physrevd.109.064030
View Full Paper
Ask AI
Bookmark
Share

Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

  1. 1Spherical inspirals of spinning bodies into Kerr black holes2025
  2. 2Post-Newtonian expansions of extreme mass ratio inspirals of spinning bodies into Schwarzschild black holes2024
  3. 3Adiabatic inspirals under electromagnetic radiation reaction on Kerr spacetime2024 · 2 citations
  4. 4Chaos and Carter: Extreme-mass-ratio systems of relativistic rotating black holes in astrophysical environments2025
  5. 5Toward efficient effective-one-body models for generic, nonplanar orbits2024 · 45 citations