MARES: A macroscopic model for the Radar Echo Telescope Contribution to ICRC 2023

RET collaboration

MARES: A macroscopic model for the Radar Echo Telescope Contribution to ICRC 2023

RET collaboration

Physics

Research output: Contribution to journal › Conference article › peer-review

Abstract

Upon interaction in a dense medium like polar ice, a high-energy neutrino will deposit its energy abruptly, producing a short-lived electron plasma. The Radar Echo Telescope (RET) collaboration aims to utilize the radar technique to probe this plasma and, thus, detect neutrinos in the PeV to EeV energy range. This work presents the Macroscopic Approach to the Radar Echo Scatter (MARES) model. MARES is based on a macroscopic, semi-analytical approach and includes all the known relevant physics that will affect the radar signal. Here we show how MARES is used to investigate the effect that the ice temperature, via the free electron lifetime, might have on the radar scatter signal.

Original language	English (US)
Article number	1087
Journal	Proceedings of Science
Volume	444
State	Published - Sep 27 2024
Event	38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japan Duration: Jul 26 2023 → Aug 3 2023

All Science Journal Classification (ASJC) codes

General

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@article{4852eb6f7a22410787daef7bbacfb8d3,

title = "MARES: A macroscopic model for the Radar Echo Telescope Contribution to ICRC 2023",

abstract = "Upon interaction in a dense medium like polar ice, a high-energy neutrino will deposit its energy abruptly, producing a short-lived electron plasma. The Radar Echo Telescope (RET) collaboration aims to utilize the radar technique to probe this plasma and, thus, detect neutrinos in the PeV to EeV energy range. This work presents the Macroscopic Approach to the Radar Echo Scatter (MARES) model. MARES is based on a macroscopic, semi-analytical approach and includes all the known relevant physics that will affect the radar signal. Here we show how MARES is used to investigate the effect that the ice temperature, via the free electron lifetime, might have on the radar scatter signal.",

author = "\{RET collaboration\} and \{Huesca Santiago\}, Enrique and \{de Vries\}, Krijn and P. Allison and J. Beatty and D. Besson and A. Connolly and A. Cummings and C. Deaconu and \{De Kockere\}, S. and \{de Vries\}, \{K. D.\} and D. Frikken and C. Hast and \{Huesca Santiago\}, E. and Kuo, \{C. Y.\} and A. Kyriacou and Latif, \{U. A.\} and V. Lukic and K. Mulrey and J. Nam and K. Nivedita and A. Nozdrina and E. Oberla and S. Prohira and Ralston, \{J. P.\} and Seikh, \{M. F.H.\} and Stanley, \{R. S.\} and S. Toscano and \{Van den Broeck\}, D. and \{van Eijndhoven\}, N. and S. Wissel",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons.; 38th International Cosmic Ray Conference, ICRC 2023 ; Conference date: 26-07-2023 Through 03-08-2023",

year = "2024",

month = sep,

day = "27",

language = "English (US)",

volume = "444",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

TY - JOUR

T1 - MARES

T2 - 38th International Cosmic Ray Conference, ICRC 2023

AU - RET collaboration

AU - Huesca Santiago, Enrique

AU - de Vries, Krijn

AU - Allison, P.

AU - Beatty, J.

AU - Besson, D.

AU - Connolly, A.

AU - Cummings, A.

AU - Deaconu, C.

AU - De Kockere, S.

AU - de Vries, K. D.

AU - Frikken, D.

AU - Hast, C.

AU - Huesca Santiago, E.

AU - Kuo, C. Y.

AU - Kyriacou, A.

AU - Latif, U. A.

AU - Lukic, V.

AU - Mulrey, K.

AU - Nam, J.

AU - Nivedita, K.

AU - Nozdrina, A.

AU - Oberla, E.

AU - Prohira, S.

AU - Ralston, J. P.

AU - Seikh, M. F.H.

AU - Stanley, R. S.

AU - Toscano, S.

AU - Van den Broeck, D.

AU - van Eijndhoven, N.

AU - Wissel, S.

PY - 2024/9/27

Y1 - 2024/9/27

N2 - Upon interaction in a dense medium like polar ice, a high-energy neutrino will deposit its energy abruptly, producing a short-lived electron plasma. The Radar Echo Telescope (RET) collaboration aims to utilize the radar technique to probe this plasma and, thus, detect neutrinos in the PeV to EeV energy range. This work presents the Macroscopic Approach to the Radar Echo Scatter (MARES) model. MARES is based on a macroscopic, semi-analytical approach and includes all the known relevant physics that will affect the radar signal. Here we show how MARES is used to investigate the effect that the ice temperature, via the free electron lifetime, might have on the radar scatter signal.

AB - Upon interaction in a dense medium like polar ice, a high-energy neutrino will deposit its energy abruptly, producing a short-lived electron plasma. The Radar Echo Telescope (RET) collaboration aims to utilize the radar technique to probe this plasma and, thus, detect neutrinos in the PeV to EeV energy range. This work presents the Macroscopic Approach to the Radar Echo Scatter (MARES) model. MARES is based on a macroscopic, semi-analytical approach and includes all the known relevant physics that will affect the radar signal. Here we show how MARES is used to investigate the effect that the ice temperature, via the free electron lifetime, might have on the radar scatter signal.

UR - https://www.scopus.com/pages/publications/85212286935

UR - https://www.scopus.com/inward/citedby.url?scp=85212286935&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:85212286935

SN - 1824-8039

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 1087

Y2 - 26 July 2023 through 3 August 2023

ER -

MARES: A macroscopic model for the Radar Echo Telescope Contribution to ICRC 2023

Abstract

All Science Journal Classification (ASJC) codes

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