TY - JOUR
T1 - νSpaceSim
T2 - 37th International Cosmic Ray Conference, ICRC 2021
AU - the νSpaceSim Collaboration
AU - Krizmanic, John F.
AU - Wissel, Stephanie
AU - Akaike, Yosui
AU - Anchordoqui, Luis
AU - Bergman, Douglas
AU - Buckland, Isaac
AU - Cummings, Austin
AU - Eser, Johannes
AU - Guépin, Claire
AU - Mackovjak, Simon
AU - Olinto, Angela
AU - Paul, Thomas
AU - Patel, Sameer
AU - Reustle, Alex
AU - Romero-Wolf, Andrew
AU - Reno, Mary Hall
AU - Sarazin, Fred
AU - Venters, Tonia
AU - Wiencke, Lawrence
N1 - Publisher Copyright:
© Copyright owned by the author(s).
PY - 2022/3/18
Y1 - 2022/3/18
N2 - νSpaceSim is a comprehensive end-to-end simulation package to model the optical and radio signals from extensive air showers (EAS) induced by cosmic neutrino interactions. The development has initially focused on modeling the upward-moving EASs sourced from tau neutrino interactions within the Earth that employs a new modeling package, nuPyProp. νSpaceSim is designed to model all aspects of the processes that lead to the neutrino-induced EAS signals, including the modeling of the neutrino interactions inside the Earth, propagating the leptons into the atmosphere, modeling the tau-lepton decays, forming composite EAS, generating the air optical Cherenkov and radio signals, modeling their propagation through the atmosphere, including using a MERRA-2 database driven application to generate cloud maps, and modeling detector responses. νSpaceSim uses a vectorized Python implementation of a sampled library approach to efficiently simulate neutrino-induced and background signals at a specific orbit or balloon altitude. A detector response module, based on user-inputted response parameters, subsequently is used to record the events and determine acceptance. The framework will allow for the calculation of the sky coverage and the pointing requirements needed for target-of-opportunity (ToO) follow-up observations of transients, as well as the assessment of the effects of dark-sky airglow and UHECR backgrounds. νSpaceSim will provide an efficient and practical cosmic neutrino EAS signal generation modeling package to aid in the development of future sub-orbital and space-based experiments. In this paper, the νSpaceSim framework, physics modeling, and the cosmic neutrino measurement capabilities of the current β-version are discussed with an example experimental configuration are presented as well as a discussion of additional features currently under development.
AB - νSpaceSim is a comprehensive end-to-end simulation package to model the optical and radio signals from extensive air showers (EAS) induced by cosmic neutrino interactions. The development has initially focused on modeling the upward-moving EASs sourced from tau neutrino interactions within the Earth that employs a new modeling package, nuPyProp. νSpaceSim is designed to model all aspects of the processes that lead to the neutrino-induced EAS signals, including the modeling of the neutrino interactions inside the Earth, propagating the leptons into the atmosphere, modeling the tau-lepton decays, forming composite EAS, generating the air optical Cherenkov and radio signals, modeling their propagation through the atmosphere, including using a MERRA-2 database driven application to generate cloud maps, and modeling detector responses. νSpaceSim uses a vectorized Python implementation of a sampled library approach to efficiently simulate neutrino-induced and background signals at a specific orbit or balloon altitude. A detector response module, based on user-inputted response parameters, subsequently is used to record the events and determine acceptance. The framework will allow for the calculation of the sky coverage and the pointing requirements needed for target-of-opportunity (ToO) follow-up observations of transients, as well as the assessment of the effects of dark-sky airglow and UHECR backgrounds. νSpaceSim will provide an efficient and practical cosmic neutrino EAS signal generation modeling package to aid in the development of future sub-orbital and space-based experiments. In this paper, the νSpaceSim framework, physics modeling, and the cosmic neutrino measurement capabilities of the current β-version are discussed with an example experimental configuration are presented as well as a discussion of additional features currently under development.
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M3 - Conference article
AN - SCOPUS:85145357770
SN - 1824-8039
VL - 395
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 1205
Y2 - 12 July 2021 through 23 July 2021
ER -