arXiv (All)
open access
Neutrino Emission from Proton Photon Jet Interactions in Microquasars
Microquasars are candidate sites for high energy particle production within our galaxy. Because their distances and compact emission regions limit direct observational constraints, numerical simulations are useful for connecting jet dynamics with possible multi messenger signatures. This work models
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 comparison of effective field theory models of redshift space galaxy power spectra for DESI 2024 and future surveys#609458
- The First Multi-Messenger Nova: External Shocks, TeV Photons, and Neutrinos in the Next Eruption of T CrB#973800
- A novel two loop inverse seesaw model#927197
- The Structural Abundance Crisis of Massive Galaxies in Current Cosmological Simulations#799146
- The Structural Abundance Crisis of Massive Galaxies in Current Cosmological Simulations#797723
Record · ID 1035686
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