arXiv (All)
open access
Predictions on the abundance of primordial black holes: results from the SMILE VLBI milli-lensing sample
Primordial black holes (PBHs) formed in the early universe represent a well-motivated dark matter candidate. However, their abundance in the intermediate-to-high mass range ($10^6$-$10^9\,M_\odot$) remains relatively less constrained. In this mass regime, the corresponding Einstein radii on the mill
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
- Reconstructing Early Primordial Black Hole Domination from Gravitational-Wave Backgrounds#999569
- Primordial Black Hole Seeds for Little Red Dots in $f(R)$ Gravity#798359
- Primordial Black Hole Seeds for Little Red Dots in $f(R)$ Gravity#796946
- Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe#1122902
- Shape Degeneracies: the likely culprit for the differences between lens mass models of galaxy clusters#1063358
Record · ID 1034094
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