arXiv (All)
open access
Hadronic Origin of Sub-PeV Gamma-Ray Emission from LHAASO J0621+3755
Very High Energy (VHE) gamma-rays in pulsars, and their surrounding halos, are interpreted to originate from the leptonic channel, electromagnetic interactions through electron inverse Compton (IC) scattering. In the hadronic scenario, TeV-PeV gamma-rays are generated from the decay of neutral pions
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
- Wolf–Rayet stars as tracers of gamma-ray emission - Isolated stars and stellar clusters or associations#445581
- CVE-2026-48100 — HIGH 8.7#1121058
- Pion radiative decays of excited hidden-charm pentaquark molecules: from $Σ_c^{(*)}\bar{D}^{(*)}(2S)$ molecules to the reported $P_c$ states#821913
- Observation of $ψ(3686)\to p K^- K_S^0 \bar Ξ^0+c.c.$#822458
- ROSAC: Studying the clustering properties of X-ray selected AGNs#639402
Record · ID 1232645
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