arXiv (All)
open access
Price's law for scalar waves on 1+4 dimensional subextremal Myers-Perry spacetimes
We consider Myers--Perry spacetimes $(M,g_{\mathbf{a},\mathbf{b},\mathfrak{m}})$ in $1+4$ dimensions with two spin parameters $(\mathbf{a},\mathbf{b})\in\mathbb{R}^2$, which are a direct generalization of the well known Kerr spacetime in $1+3$ dimensions. We prove that the Hamiltonian flow associate
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
- Regularized interacting scalar quantum field theories#1328273
- On flat pseudo-Euclidean solvable Malcev algebras#1083439
- An Effective $S$-Matrix Approach to Low-Frequency Waveforms from Black Hole Mergers#998456
- Tensor Calculus#1332405
- Tensor calculus#1330999
Record · ID 1456635
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