Secondary lepton production, propagation, and interactions

dc.contributor.affiliationUniversidade de Santiago de Compostela. Instituto Galego de Física de Altas Enerxías (IGFAE)
dc.contributor.affiliationUniversidade de Santiago de Compostela. Departamento de Física de Partículas
dc.contributor.authorCummings, Austin
dc.contributor.authorKrebs, Ryan
dc.contributor.authorWissel, Stephanie
dc.contributor.authorÁlvarez Muñiz, Jaime
dc.contributor.authorCarvalho, Washington Rodrigues De
dc.contributor.authorRomero-Wolf, Andrés
dc.contributor.authorSchoorlemmer, Harm
dc.contributor.authorZas Arregui, Enrique
dc.date.accessioned2025-09-18T08:11:45Z
dc.date.available2025-09-18T08:11:45Z
dc.date.issued2025-01-08
dc.description.abstractCharged current interactions of neutrinos inside the Earth can result in secondary muons and τ-leptons which are detectable by several existing and planned neutrino experiments through a wide variety of event topologies. Consideration of such events can improve detector performance and provide unique signatures which help with event reconstruction. In this work, we describe NuLeptonSim, a propagation tool for neutrinos and charged leptons that builds on the fast NuTauSim framework. NuLeptonSim considers energy losses of charged leptons, modeled both continuously for performance or stochastically for accuracy, as well as interaction models for all flavors of neutrinos, including the Glashow resonance. We demonstrate the results from including these effects on the Earth emergence probability of various charged leptons from different flavors of primary neutrino and their corresponding energy distributions. We find that the emergence probability of muons can be higher than that of taus for energies below 100 PeV, whether from a primary muon or τ neutrino, and that the Glashow resonance contributes to a surplus of emerging leptons near the resonant energy.
dc.description.peerreviewedSI
dc.description.sponsorshipFunded by SCOAP3.
dc.identifier.citationCummings, A., Krebs, R., Wissel, S., Alvarez-Muñiz, J., Carvalho, W. R., Romero-Wolf, A., Schoorlemmer, H., Zas, E. (2025). Secondary lepton production, propagation, and interactions. Physical Review D, 111(2). https://doi.org/10.1103/PhysRevD.111.023012
dc.identifier.doi10.1103/PhysRevD.111.023012
dc.identifier.issn2470-0010
dc.identifier.urihttps://hdl.handle.net/10347/42852
dc.issue.number2
dc.journal.titlePhysical Review D (particles, fields, gravitation, and cosmology) (PRD)
dc.language.isoeng
dc.page.final14
dc.page.initial1
dc.publisherAmerican Physical Society
dc.relation.publisherversionhttps://doi.org/10.1103/PhysRevD.111.023012
dc.rightsPublished by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.
dc.rightsAttribution 4.0 International
dc.rights.accessRightsopen access
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectCosmic rays & astroparticles
dc.subjectExtrasolar neutrino astronomy
dc.subjectNeutrino interactions
dc.titleSecondary lepton production, propagation, and interactions
dc.typejournal article
dc.type.hasVersionVoR
dc.volume.number111
dspace.entity.typePublication
relation.isAuthorOfPublicationea5dad89-ecc2-4557-88b3-7644ef0d63d1
relation.isAuthorOfPublication53dcfe79-4e34-4c0f-8b04-6d43f424b090
relation.isAuthorOfPublication.latestForDiscoveryea5dad89-ecc2-4557-88b3-7644ef0d63d1

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