arXiv (All)
open access
Warm inflation beyond the Gaussian limit: primordial black holes and induced gravitational waves
In warm inflation, the primordial fluctuations are driven by random kicks from a hot radiation bath. Two features of these kicks matter: how long the bath remembers them, which shapes the power spectrum, and how their strengths are spread, which controls the rare, extreme fluctuations. In this paper
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
- Impact of Heavy Modes on Primordial Black Hole Formation#1077670
- Lukewarm inflation, primordial black holes and gravitational waves#1013868
- Primordial Black Holes from Inflation with a Spectator Field#1388316
- Analyzing $μ$ Parameter Range and the Duration of Reheating in the Polynomial $α$-attractor Models using CMB Observations#1104589
- Spectator Composes a Gravitational Canon: Spectator-field-triggered Phase Transition During Inflation and its Anisotropic Gravitational Wave Signals#1123001
Record · ID 1467915
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