Design and sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G)

Design and sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G)
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DOI:
10.1088/1748-0221/16/03/p03025
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发表时间:
2020-10
影响因子:
1.3
通讯作者:
J. Aguilar;P. Allison;J. Beatty;H. Bernhoff;D. Besson;N. Bingefors;O. Botner;S. Buitink;K. Carter;B. Clark;A. Connolly;P. Dasgupta;S. D. Kockere;K. D. Vries;C. Deaconu;M. DuVernois;N. Feigl;D. García-Fernández;C. Glaser;A. Hallgren;S. Hallmann;J. Hanson;B. Hendricks;B. Hokanson-Fasig;C. Hornhuber;K. Hughes;A. Karle;J. Kelley;S. Klein;R. Krebs;R. Lahmann;M. Magnuson;T. Meures;Z. Meyers;A. Nelles;A. Novikov;E. Oberla;B. Oeyen;H. Pandya;I. Plaisier;L. Pyras;D. Ryckbosch;O. Scholten;D. Seckel;D. Smith;D. Southall;J. Torres;S. Toscano;D. V. D. Broeck-D.-V.-D.-Broeck-2131955910;N. Eijndhoven;A. Vieregg;C. Welling;S. Wissel;R. Young;A. Zink
J. Aguilar;P. Allison;J. Beatty;H. Bernhoff;D. Besson;N. Bingefors;O. Botner;S. Buitink;K. Carter;B. Clark;A. Connolly;P. Dasgupta;S. D. Kockere;K. D. Vries;C. Deaconu;M. DuVernois;N. Feigl;D. García-Fernández;C. Glaser;A. Hallgren;S. Hallmann;J. Hanson;B. Hendricks;B. Hokanson-Fasig;C. Hornhuber;K. Hughes;A. Karle;J. Kelley;S. Klein;R. Krebs;R. Lahmann;M. Magnuson;T. Meures;Z. Meyers;A. Nelles;A. Novikov;E. Oberla;B. Oeyen;H. Pandya;I. Plaisier;L. Pyras;D. Ryckbosch;O. Scholten;D. Seckel;D. Smith;D. Southall;J. Torres;S. Toscano;D. V. D. Broeck-D.-V.-D.-Broeck-2131955910;N. Eijndhoven;A. Vieregg;C. Welling;S. Wissel;R. Young;A. Zink
中科院分区:
工程技术4区
文献类型:
--
作者:
J. Aguilar;P. Allison;J. Beatty;H. Bernhoff;D. Besson;N. Bingefors;O. Botner;S. Buitink;K. Carter;B. Clark;A. Connolly;P. Dasgupta;S. D. Kockere;K. D. Vries;C. Deaconu;M. DuVernois;N. Feigl;D. García-Fernández;C. Glaser;A. Hallgren;S. Hallmann;J. Hanson;B. Hendricks;B. Hokanson-Fasig;C. Hornhuber;K. Hughes;A. Karle;J. Kelley;S. Klein;R. Krebs;R. Lahmann;M. Magnuson;T. Meures;Z. Meyers;A. Nelles;A. Novikov;E. Oberla;B. Oeyen;H. Pandya;I. Plaisier;L. Pyras;D. Ryckbosch;O. Scholten;D. Seckel;D. Smith;D. Southall;J. Torres;S. Toscano;D. V. D. Broeck-D.-V.-D.-Broeck-2131955910;N. Eijndhoven;A. Vieregg;C. Welling;S. Wissel;R. Young;A. Zink

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本文介绍了格陵兰射电中微子观测站(RNO-G)的设计,并讨论了它的科学前景。RNO-G使用一系列无线电传感器,试图通过利用冰中中微子诱导级联的Askaryan效应来测量10 PeV以上的中微子。我们讨论的实验考虑,驱动RNO-G的设计,目前的第一次测量的硬件,部署和讨论的仪器的投影灵敏度。RNO-G将是第一个用于冰中中微子信号的生产规模无线电探测器。
This article presents the design of the Radio Neutrino Observatory Greenland (RNO-G) and discusses its scientific prospects. Using an array of radio sensors, RNO-G seeks to measure neutrinos above 10 PeV by exploiting the Askaryan effect in neutrino-induced cascades in ice. We discuss the experimental considerations that drive the design of RNO-G, present first measurements of the hardware that is to be deployed and discuss the projected sensitivity of the instrument. RNO-G will be the first production-scale radio detector for in-ice neutrino signals.