arXiv (All)
open access
Observational constraints on Luciano-Saridakis holographic dark energy
Holographic dark energy (HDE) models provide a natural framework for linking gravitational thermodynamics to the late-time accelerated expansion of the Universe. In this work, we investigate the observational viability of an extended HDE scenario arising from a recently proposed generalized entropy.
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
- Observational constraints on Luciano-Saridakis holographic dark energy#921055
- Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae#973262
- The Spiral Model of Time: Direction, Span, and Self-Similarity#691327
- Entropy and the Scaffolding of Time: Decoherence, Cosmic Webs, and the Woven Tapestry of Spacetime#118818
- Time as Primary Substrate: A Unified Framework Cosmological Time Dilation, the Big Bang as Phase Transition, and the Temporal Field Origin of Gravity, Matter, and Dark Energy#170269
Record · ID 925291
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