arXiv (All)
open access
(Re)constructing Accurate Axion Oscillations
The cosmological evolution of ultralight axions typically involves rapid oscillations on the timescale of the inverse mass, making it challenging to resolve the dynamics at both the background and perturbation levels. In this study, we numerically implement a novel approach to this problem based on
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 Tale of Two Gauges: Effective Field Theory for Relativistic Behavior of Cosmological Axions#1013211
- A Unified Numerical Study of Axion Stars: From the Nonrelativistic Regime to General Relativity#1071408
- Cosmological Constrained Axion-Portal Inelastic Dark Matter for the LZ Event#1123777
- Does DESI prefer Damped Oscillating Dark Energy over Cosmological constant?#986276
- Axions as Dark Matter, Dark Energy, and Dark Radiation#925812
Record · ID 1013212
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