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The Simulation of the Sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan Radiation from Cosmogenic Neutrinos Interacting in the Antarctic Ice

التفاصيل البيبلوغرافية
العنوان: The Simulation of the Sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan Radiation from Cosmogenic Neutrinos Interacting in the Antarctic Ice
المؤلفون: Tsung-Che Liu, David Saltzberg, O. Banerjee, A. Romero-Wolf, S. H. Wang, M. S. Sutherland, Keith Bechtol, Abigail G. Vieregg, L. Batten, R. J. Nichol, Brian Rauch, Po-Hsun Chen, D. Seckel, Luca Macchiarulo, P. F. Dowkontt, R. Hupe, B. Strutt, C. C. Chen, Cosmin Deaconu, Chun Hsiung Chen, S. Y. Lin, J. J. Beatty, Eric Oberla, K. M. Liewer, D. Z. Besson, J. Stockham, G. S. Varner, P. Cao, B. Rotter, S. Matsuno, Harm Schoorlemmer, Amy Connolly, Stephanie Wissel, Berkeley Hill, Jiwoo Nam, C. Miki, K. Hughes, Katharine Mulrey, V. Bugaev, Andrew Ludwig, Alexander Novikov, M. H. Israel, J. W. H. Gordon, J. W. Russell, L. Cremonesi, J. Shiao, W. R. Binns, J. J. Huang, B. Dailey, J. M. Robert, Konstantin Belov, S. Stafford, Patrick Allison, B. D. Fox, M. Stockham, J. Stuhr, K. McBride, Peter Gorham, J. M. Clem, S. Prohira
بيانات النشر: arXiv, 2019.
سنة النشر: 2019
مصطلحات موضوعية: Physics, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Monte Carlo method, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Geophysics, Radiation, 01 natural sciences, 7. Clean energy, 030218 nuclear medicine & medical imaging, 03 medical and health sciences, 0302 clinical medicine, 0103 physical sciences, Parametrization (atmospheric modeling), Sensitivity (control systems), Transient (oscillation), Antenna (radio), Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation, Instrumentation and Methods for Astrophysics (astro-ph.IM), Mathematical Physics, Radio detection, Physics::Atmospheric and Oceanic Physics
الوصف: A Monte Carlo simulation program for the radio detection of Ultra High Energy (UHE) neutrino interactions in the Antarctic ice as viewed by the Antarctic Impulsive Transient Antenna (ANITA) is described in this article. The program, icemc, provides an input spectrum of UHE neutrinos, the parametrization of the Askaryan radiation generated by their interaction in the ice, and the propagation of the radiation through ice and air to a simulated model of the third and fourth ANITA flights. This paper provides an overview of the icemc simulation, descriptions of the physics models used and of the ANITA electronics processing chain, data/simulation comparisons to validate the predicted performance, and a summary of the impact of published results.
DOI: 10.48550/arxiv.1903.11043
URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f0cf89ce4e6242cdea0198a1b7dd750d
حقوق: OPEN
رقم الأكسشن: edsair.doi.dedup.....f0cf89ce4e6242cdea0198a1b7dd750d
قاعدة البيانات: OpenAIRE
الوصف
DOI:10.48550/arxiv.1903.11043