PulseJournal ClubResearchersJournalsExplore
Instagram
HomeJournal ClubExplore
Synapse
⌘+K
Synapse
October 16, 2025Open Access

Spherical inspirals of spinning bodies into Kerr black holes

View Full Paper
Ask AI
Bookmark
Share

Authors

VSViktor SkoupýGPGabriel Andres PiovanoVWVojtěch Witzany

Discussion

Loading...

Member takes

Overview

Analysis of gravitational wave signals from EMRIs in spherical orbits, highlighting the importance of secondary spin effects.

Key Points

  • Gravitational wave signals from extreme mass-ratio inspirals are significantly affected by the secondary spin.
  • For spherical inspirals into Kerr black holes, neglecting spin leads to detectable waveform mismatches.
  • The study models flux-driven spherical orbits of spinning bodies with a focus on precise gravitational wave detection.
  • This framework enhances predictions for future gravitational wave observatories like LISA, improving astrophysical parameter extraction.

Cite This Study

Skoupý et al. (2025) studied this question.

synapsesocial.com/papers/68f04918e559138a1a06d421https://doi.org/10.48550/arxiv.2506.20726
View Full Paper
Ask AI
Bookmark
Share