arXiv (All)
open access
Gravitational Scattering of Oort Cloud Objects by Dark Matter: Constraints on the Primordial Black Hole Fraction
cosmology-and-nongalactic-astrophysicsearth-and-planetary-astrophysicssolar-and-stellar-astrophysics
Planetary systems can act as long-term gravitational detectors for dark matter. We investigate the gravitational scattering of Oort cloud objects by primordial black holes (PBHs) using celestial kinematics in the impulsive approximation. By evaluating the energy transfer during these encounters, we
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
- Dark ages bounds on nonaccreting massive compact halo objects#927285
- Small-Body Science with the Nautilus Space Observatory: From Cislunar Space Resilience to Mapping the Kuiper-Belt-to-Oort-Cloud Transition#997659
- Dark Matter Recoupling#925951
- Dynamical Tidal response of compact stars -- An EFT approach#1051453
- Lower central dark matter densities in nearby galaxies than predicted by simulations#1122747
Record · ID 974395
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