arXiv (All)
open access
Cusp regularization with spin structures and gravitational anomalies
The family of $SL(2,\mathbb Z)$ black holes has an accumulation point corresponding to a cusped geometry, which causes the sum over black holes to diverge. We extend cusp regularization to the sum over geometries compatible with a fixed boundary spin structure. For $c_L=c_R$, including the cusp as a
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
- Regular black holes from Oppenheimer-Snyder collapse#1399708
- Stationary Rotating Geometries Associated with Nonsingular Pulsating Collapse#793087
- Stationary Rotating Geometries Associated with Nonsingular Pulsating Collapse#789083
- Signatures of Novikov-Thorne accretion disks around rotating black holes in semiclassical gravity with trace anomaly#1050454
- $Spin(n,n)\times\mathbb{R}^+$ Generalised Geometry and Consistent Truncations on Branes#1110205
Record · ID 1467352
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