Upgrading gSeaGen: from MeV to PeV neutrinos
A. Garcia Soto, C. Distefano, P. Kalaczy\'nski (for the KM3NeT, Collaboration)
TL;DR
This paper presents an upgraded gSeaGen framework capable of simulating neutrino interactions across a broad energy spectrum from MeV to PeV, including new features for tau neutrino and lepton propagation relevant for next-generation neutrino telescopes.
Contribution
The upgraded gSeaGen now simulates neutrino interactions from MeV to PeV energies and includes new lepton propagation features for PeV tau neutrinos, enhancing its applicability.
Findings
Effective simulation of neutrino interactions from MeV to EeV energies.
New capabilities for tau neutrino and charged lepton propagation.
Application to KM3NeT detector simulations.
Abstract
The gSeaGen framework has been upgraded to simulate events detectable in neutrino telescopes induced by neutrino or cosmic ray interactions. The new version is well-suited to generate neutrino interactions at energies from a few MeV to EeV, profiting from the latest GENIE extensions to lower and higher energies. In addition, a brand new functionality to propagate leptons from CORSIKA air showers has been developed. Novel features of gSeaGen will be presented, related to simulation of PeV tau neutrinos and charged lepton propagation, using the KM3NeT detectors as physics case.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.