arXiv (All)
open access
The Geometry of Gravitational Radiation
We consider 4-dimensional asymptotically flat vacuum spacetimes near future null infinity endowed with the most general allowable Carroll geometry. We show that the near-boundary radial expansion (to a certain order) can be organised in terms of connections that can be obtained by gauging the confor
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
- Peeling property for the Einstein scalar field equations with the nonzero cosmological constant#798355
- Peeling property for the Einstein scalar field equations with the nonzero cosmological constant#796942
- A four-dimensional lambda CDM-type cosmological model induced from higher dimensions using a kinematical constraint#954717
- Perturbations of a Schwarzschild black hole and Newman-Unti gauge#1109699
- Stochastic motion of massless particles near event horizons in Schwarzschild and Reissner-Nordström spacetimes#1062366
Record · ID 998445
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