arXiv (All)
open access
Kinetic-theory derivation and Bayesian analysis of the finite-temperature shifted CMB power spectrum
cosmology-and-nongalactic-astrophysicsgeneral-relativity-and-quantum-cosmologyhigh-energy-physics-theory
Finite-temperature quantum-gravitational corrections to the cosmological constant introduce two additional density parameters, $Ω_{Λ_2}$ and $Ω_{Λ_3}$, the associated terms of which scale as $a^{-4}$ and $a^{-2}$, respectively. In previous work (Papers I and II), these parameters were studied using
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
- Direct Observational Analysis of the Cosmic Microwave Background Angular Power Spectrum from Planck Data#87977
- From quantum fluctuations to galaxy power spectrum multipoles#987037
- Influence of finite-temperature effects on CMB power spectrum#1012004
- Scalar Photon Coupling and Modified Photon Evolution: CMB Signatures and Cosmological Constraints#635900
- Scalar Photon Coupling and Modified Photon Evolution: CMB Signatures and Cosmological Constraints#633551
Record · ID 1201448
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