arXiv (All)
open access
Black Holes as Frequency-Dependent Filters of Stochastic Gravitational Waves
cosmology-and-nongalactic-astrophysicsgeneral-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomenahigh-energy-physics-phenomenologyhigh-energy-physics-theory
Black holes ring when perturbed, whereas their response to a stationary gravitational-wave background is a real-frequency scattering problem, not a source of additional quasi-normal-mode lines. We make this standard distinction quantitative by treating a black hole as a frequency-, angle-, and polar
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- A semicoherent resampling method for long-transient gravitational wave searches with applications to subsolar-mass primordial black-hole binaries#1069974
- Constraining the geometry of rotating black holes with eikonal QNMs#1051223
- Relic gravitational waves from primordial gravitational collapses#1014502
- Comparing the Detectability of the Baryon Acoustic Oscillation through Gravitational-Wave Autocorrelation and Cross-Correlation with Galaxies#1034947
- Angular power spectrum of induced gravitational waves: breaking model and parameter degeneracies in PTA observations#821158
Record · ID 1037327
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive