arXiv (All)
open access
Kink instability as a particle acceleration mechanism in X-ray binaries and the connection to the outburst cycle
We consider whether the kink instability can explain particle acceleration in hard state 'compact' X-ray binary jets. We apply a 1D model to assess the expected growth rate of the instability for a variety of jet models, then scale results from simulations to estimate a dissipation rate for the magn
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
- The enigmatic Soft X-ray AGN RX J0134.2--4258#639377
- Small-x effects in W + jets production at the Tevatron#303983
- AGNI: A differentiable MHD stability solver & optimizer for magnetic confinement fusion devices#677704
- AGNI: A differentiable MHD stability solver & optimizer for magnetic confinement fusion devices#674503
- Not enough stellar Mass Machos in the Galactic Halo#639499
Record · ID 1061470
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