6533b7d3fe1ef96bd125ffa9

RESEARCH PRODUCT

Upgrading gSeaGen: from MeV to PeV neutrinos

C. DistefanoP. KalaczyńskiA. Garcia Soto

subject

PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Neutrino detectorHigh Energy Physics::ExperimentNeutrinoInstrumentationMathematical Physics

description

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.

https://doi.org/10.1088/1748-0221/16/09/c09008