arXiv (All)
open access
Chiral Carroll string near Schwarzschild black hole
We obtain the action for the chiral Carroll string moving in a curved string-Carroll target spacetime from a Carroll expansion, in powers of the speed of light $c$, of the action for the relativistic closed bosonic string. Applying this setup to a classical closed bosonic string approaching the $4$-
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
- The Geometry of Gravitational Radiation#998445
- The Lemniscate Soliton: Phi as the Unique Stable Resonance of Self-Referential Curvature in Spacetime#167430
- Stochastic motion of massless particles near event horizons in Schwarzschild and Reissner-Nordström spacetimes#1062366
- Quasi-local Hamiltonian for generalized Kerr-Schild black holes in the Iyer-Wald formalism#625118
- Quasi-local Hamiltonian for generalized Kerr-Schild black holes in the Iyer-Wald formalism#622845
Record · ID 1051334
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