arXiv (All)
open access
Non-variational scalar field cosmology: Exact Bianchi I solutions for near-minimal scalar fields
The purpose of this work is to investigate spatially homogeneous and flat cosmological solutions of the Einstein equations coupled to a non-variational ``near-minimal'' scalar field. This coupling model represents a minimal departure from standard theory by decoupling the scalar field's self-interac
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
- A four-dimensional lambda CDM-type cosmological model induced from higher dimensions using a kinematical constraint#954717
- Cosmological extra dimensions can mimic dark energy#998424
- Resonances in the early Universe#999699
- ADMISSIBILITY BEFORE DIMENSIONS A Structural Clarification on Higher-Dimensional Cosmology#83741
- Confront a dilaton model with the LHC measurements#1110074
Record · ID 999787
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