arXiv (All)
open access
The Cosmological $δ$-shift
We consider the extension of the $δ$-shift connecting Tr$(ϕ^3)$ and pion amplitudes to observables in cosmology. We start in flat-space and explain how one can extract the pion wavefunction and correlators from those of Tr$(ϕ^3)$ theory, via a simple kinematic deformation. As opposed to the amplitud
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 Celestial Sphere as an Ideal Benchmark for Quantum Gravity: Null-Geodesic Universality, Mass Generation, and Theory Discrimination with Existing Data#111545
- Three-Gluon Scattering Amplitude in de Sitter Spacetime#1202046
- Kinematic Flow for Banana Loops and Unparticles#1327364
- Loop integrals in de Sitter spacetime: The parity-split IBP system and $\mathrm{d}\log$-form differential equations#1297100
- Decreasing Universe Theory: The Tully-Fisher Relation#730660
Record · ID 1232943
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