{"about":{"site":"https://codewithpapers.app","non_affiliation":"Code with Papers and Syntology are not affiliated with, endorsed by, or sponsored by Papers with Code, Meta, or the pwc-archive mirror.","licence":"CC BY-SA 4.0","licence_url":"https://creativecommons.org/licenses/by-sa/4.0/legalcode","attribution":"https://codewithpapers.app/attribution","modified":"archive material modified by Syntology; see the attribution page"},"url":"/paper/neutrino-emission-from-magnetized-micro","title":"Neutrino emission from magnetized micro-quasar jets","arxiv_id":"1706.03087","date":"2017-06-09","proceeding":null,"authors":["Theodoros Smponias","Odysseas Kosmas"],"abstract":"The hadronic jets in a micro-quasar stellar system are modelled with the relativistic hydrocode PLUTO. We focus on neutrino emission from such jets produced by fast proton (non-thermal) collisions on thermal ones within the hadronic jet. We adopt a semi-analytical approximation for the description of the secondary particles produced from p-p collisions and develop appropriate algorithms using the aforementioned injected protons as input. As a concrete example we consider the SS-433 X-ray binary system for which several observations have been performed the last decades. In contrast to the pre-set distribution of the fast protons along the jet employed in our previous works, in the present paper we simulated it by using a power-law fast proton distribution along the PLUTO hydro-code. This distribution gradually sweeps aside the surrounding winds, during the jet advance through the computational grid. As a first step, in the present work the neutrino energy spectrum is extracted from the model jet, facilitating a range of potential dynamical simulations in currently interesting microquasar jet systems.","url_abs":"http://arxiv.org/abs/1706.03087v1","url_pdf":"http://arxiv.org/pdf/1706.03087v1.pdf","source":{"archive":"pwc-archive (Hugging Face), CC BY-SA 4.0","snapshot":"2025-07-28","licence_url":"https://creativecommons.org/licenses/by-sa/4.0/legalcode","row_kind":"links_only","authors_date_abstract":"arXiv metadata, CC0 1.0 (https://info.arxiv.org/help/license), from the Kaggle arXiv metadata snapshot of 2026-09-12"},"code_links":[{"paper_slug":"neutrino-emission-from-magnetized-micro","repo_url":"https://github.com/teoxxx/neutrino","is_official":0,"mentioned_in_paper":0,"mentioned_in_github":1,"framework":"none","reach":null}],"tasks":[],"methods":[],"datasets_introduced":[],"methods_introduced":[],"results":[],"syntology":{"syntology_url":null,"atlas_url":null,"mcp":null,"developers":"https://syntology.ai/developers"},"arxiv_metadata":null,"syntology_extracted_results":null}