arXiv (All)
open access
Cosmic Heterogeneity Shapes the Evolution of Dark Energy and Time
Early- and late-Universe measurements of the Hubble constant disagree, a puzzle known as the Hubble tension. We derive cosmological parameters from first principles, using only the dynamics of cosmic volume and the possibility that matter can be unevenly distributed. Within this framework, three of
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
- Partial Relief of the Hubble Tension and a Natural Self-Interacting Dark Matter Candidate From Staged Symmetry Breaking#1104955
- Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data#998267
- Alleviating cosmological tensions with a hybrid dark sector#257757
- Resonant Coupled Dark Sector (RCDS): A Phenomenological Interacting Cosmology with Early-Time Modulation#307791
Record · ID 1106242
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