arXiv (All)
open access
Quantum Field Theory Of Cosmological Perturbations Induced By Ultralight Dark Matter
cosmology-and-nongalactic-astrophysicsgeneral-relativity-and-quantum-cosmologyhigh-energy-physics-theory
The growth of primordial perturbations during the matter-dominated era is primarily driven by dark matter. Ultralight scalar fields (ULDM) are a promising candidate for this role, conventionally modeled as operating in a classical, high-occupation regime. In this work, we develop a first-principles
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
- Dark matter as higher-form fields#1012481
- High Energy Neutrinos, Gravitational Waves, and Dark Matter from a Cosmological First Order Phase Transition#1186734
- 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
- Emergent dark sector in group field theory cosmology#927624
Record · ID 1354203
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