arXiv (All)
open access
Tracing the Evolution of $Ω_m(z)$ over the Last 10 Billion Years with Non-parametric Methods
We investigate the redshift evolution of the matter density parameter, $Ω_m(z)$, using galaxy cluster gas mass fraction measurements combined with cosmic chronometer $H(z)$ data and type Ia supernova luminosity distances. This provides a non-parametric probe of the normalization of the cosmological
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
- Testing a cosmological teleparallel modified f(T) model with parametric H(z)#629848
- Testing a cosmological teleparallel modified f(T) model with parametric H(z)#627986
- Investigating the $H_0$ Tension and Expansion-History Mismatch with Diverse Dark Energy Parametrization Frameworks#1105969
- Untangling dust emission and cosmic infrared background anisotropies with the scattering transform statistics#1079409
- Probing cosmic anisotropy from galaxy clusters via the dipole fitting method#974326
Record · ID 1062866
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