arXiv (All)
open access
Investigating the coincidence problem with Interacting Dark Energy Models
Interacting dark energy (IDE) models within the framework of general relativity (GR) provide a possible extension of the standard $Λ$CDM model and may alleviate the coincidence problem. In this paper, we investigate three phenomenological interacting dark energy models using a combination of cosmic
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
- Cosmological anatomy of interacting dark energy#1013733
- Is DESI Seeing Dynamical Dark Energy, or a Cosmic Glitch in Gravity?#1154442
- Simulations of dark energy cosmologies#387504
- Comparing Mass-Varying Neutrino Dark Energy Models with DESI DR2: Cosmological Constraints and Bayesian Evidence#1051583
- Appendix: Deficit Distribution Function and Effective Gravitational Constant – A Closed Algebraic Model (Final Version)#692157
Record · ID 927536
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