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Simulation and Optimisation for the Radar Echo Telescope for Cosmic Rays
dc.contributor.author | Stanley, R.S. | |
dc.contributor.author | De Kockere, S. | |
dc.contributor.author | Allison, P. | |
dc.contributor.author | Beatty, J. | |
dc.contributor.author | Besson, D. | |
dc.contributor.author | Connolly, A. | |
dc.contributor.author | Dasgupta, P. | |
dc.contributor.author | Deaconu, C. | |
dc.contributor.author | de Vries, K. | |
dc.contributor.author | Frikken, D. | |
dc.contributor.author | Hast, C. | |
dc.contributor.author | Huesca Santiago, E. | |
dc.contributor.author | Kuo, C.Y. | |
dc.contributor.author | Latif, U.A. | |
dc.contributor.author | Lukic, V. | |
dc.contributor.author | Meures, T. | |
dc.contributor.author | Mulrey, K. | |
dc.contributor.author | Nam, J. | |
dc.contributor.author | Nozdrina, A. | |
dc.contributor.author | Oberla, E. | |
dc.contributor.author | Prohira, S. | |
dc.contributor.author | Ralston, John P. | |
dc.contributor.author | Sbrocco, C. | |
dc.contributor.author | Torres, J. | |
dc.contributor.author | Toscano, S. | |
dc.contributor.author | Van den Broeck, D. | |
dc.contributor.author | van Eijndhoven, N. | |
dc.contributor.author | Wissel, S. | |
dc.date.accessioned | 2023-07-31T21:07:31Z | |
dc.date.available | 2023-07-31T21:07:31Z | |
dc.date.issued | 2022-03-18 | |
dc.identifier.citation | R.S. Stanley et al. Simulation and Optimisation for the Radar Echo Telescope for Cosmic Rays. 37th International Cosmic Ray Conference (ICRC 2021). July 12th – 23rd, 2021. Online – Berlin, Germany | en_US |
dc.identifier.uri | https://hdl.handle.net/1808/34682 | |
dc.description.abstract | The SLAC T-576 beam test experiment showed the feasibility of the radar detection technique to probe high-energy particle cascades in dense media. Corresponding particle-level simulations indicate that the radar method has very promising sensitivity to probe the > PeV cosmic neutrino flux. As such, it is crucial to demonstrate the in-situ feasibility of the radar echo method, which is the main goal of the current RET-CR experiment. Although the final goal of the Radar Echo Telescope is to detect cosmic neutrinos, we seek a proof of principle using cosmic-ray air showers penetrating the (high-altitude) Antarctic ice sheet.When an UHECR particle cascade propagates into a high-elevation ice sheet, it produces a dense in-ice cascade of charged particles which can reflect incoming radio waves. Using a surface cosmic-ray detector, the energy and direction of the UHECR can be reconstructed, and as such this constitutes a nearly ideal in-situ test beam to provide the proof of principle for the radar echo technique. RET-CR will consist of a transmitter array, receiver antennas and a surface scintillator plate array.Here we present the simulation efforts for RET-CR performed to optimise the surface array layout and triggering system, which affords an estimate of the expected event rate. | en_US |
dc.publisher | Sissa Medialab | en_US |
dc.rights | © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). | en_US |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/ | en_US |
dc.title | Simulation and Optimisation for the Radar Echo Telescope for Cosmic Rays | en_US |
dc.type | Article | en_US |
kusw.kuauthor | Ralston, John P. | |
kusw.kudepartment | Physics & Astronomy | en_US |
dc.identifier.doi | 10.22323/1.395.0416 | en_US |
kusw.oaversion | Scholarly/refereed, publisher version | en_US |
kusw.oapolicy | This item meets KU Open Access policy criteria. | en_US |
dc.rights.accessrights | openAccess | en_US |