arXiv (All)
open access
AdS - de Sitter transition in interacting dark energy models
Recent cosmological results, including the persistent $H_0$ tension and indications of dynamical dark energy, have raised the possibility that the standard $Λ$-Cold Dark Matter ($Λ$CDM) model may be incomplete. At the same time, theoretical developments based on swampland conjectures indicate that t
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
- Interpreting the Hubble tension with a cascade decaying dark matter sector#927141
- Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data#998267
- Cosmological anatomy of interacting dark energy#1013733
- Scalaron-driven dark matter during warm inflation via UV freeze-in#448808
- Non-minimally Coupled Running Curvaton for DESI-motivated Dynamical Dark Energy#1108998
Record · ID 1143023
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