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Abstract
NuRadioMC is a Monte Carlo framework designed to simulate ultra-high energy neutrino detectors that rely on the radio detection method. This method exploits the radio emission generated in the electromagnetic component of a particle shower following a neutrino interaction. NuRadioMC simulates everything from the neutrino interaction in a medium, the subsequent Askaryan radio emission, the propagation of the radio signal to the detector and finally the detector response. NuRadioMC is designed as a modern, modular Python-based framework, combining flexibility in detector design with user-friendliness. It includes a state-of-the-art event generator, an improved modelling of the radio emission, a revisited approach to signal propagation and increased flexibility and precision in the detector simulation. This paper focuses on the implemented physics processes and their implications for detector design. A variety of models and parameterizations for the radio emission of neutrino-induced showers are compared and reviewed. Comprehensive examples are used to discuss the capabilities of the code and different aspects of instrumental design decisions.
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1 University of California, Department of Physics and Astronomy, Irvine, USA (GRID:grid.266093.8) (ISNI:0000 0001 0668 7243)
2 DESY, Zeuthen, Germany (GRID:grid.7683.a) (ISNI:0000 0004 0492 0453); Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erlangen, Germany (GRID:grid.5330.5) (ISNI:0000 0001 2107 3311)
3 Universidade de Santiago de Compostela, IGFAE, Depto. de Física de Partículas, Santiago de Compostela, Spain (GRID:grid.11794.3a) (ISNI:0000000109410645)
4 University of Kansas, Department of Physics and Astronomy, Lawrence, USA (GRID:grid.266515.3) (ISNI:0000 0001 2106 0692)
5 The Ohio State University, Department of Physics and Center for Cosmology and Astroparticle Physics, Columbus, USA (GRID:grid.261331.4) (ISNI:0000 0001 2285 7943)
6 University of Chicago, Kavli Institute for Cosmological Physics, Chicago, USA (GRID:grid.170205.1) (ISNI:0000 0004 1936 7822)
7 Vrije Universiteit Brussels, Brussels, Belgium (GRID:grid.8767.e) (ISNI:0000 0001 2290 8069)
8 Whittier College, Department of Physics, Whittier, USA (GRID:grid.422678.d) (ISNI:0000 0000 8790 5830)
9 University of Wisconsin, Department of Physics and Wisconsin IceCube Particle Astrophysics Center, Madison, USA (GRID:grid.28803.31) (ISNI:0000 0001 0701 8607)
10 University of California, Department of Physics and Astronomy, Irvine, USA (GRID:grid.266093.8) (ISNI:0000 0001 0668 7243); Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen Centre for Astroparticle Physics, Erlangen, Germany (GRID:grid.5330.5) (ISNI:0000 0001 2107 3311)
11 University of California, Department of Electrical Engineering and Computer Science, Irvine, USA (GRID:grid.266093.8) (ISNI:0000 0001 0668 7243)
12 University of Delaware, Department of Physics and Astronomy, Bartol Research Institute, Newark, USA (GRID:grid.33489.35) (ISNI:0000 0001 0454 4791)
13 Otterbein University, Westerville, USA (GRID:grid.261485.c) (ISNI:0000 0001 2235 8896)
14 Université Libre, Brussels, Belgium (GRID:grid.4989.c) (ISNI:0000 0001 2348 0746)
15 Vrije Universiteit Brussels, Brussels, Belgium (GRID:grid.8767.e) (ISNI:0000 0001 2290 8069); Max-Planck Institute for Radio Astronomy, Bonn, Germany (GRID:grid.450267.2)
16 California Polytechnic State University, Physics Department, San Luis Obispo, USA (GRID:grid.253547.2) (ISNI:000000012222461X)