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

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arxiv 2010.12279 v5 pith:AVGW6KPC submitted 2020-10-23 astro-ph.IM astro-ph.HE

J. A. Aguilar , P. Allison , J. J. Beatty , H. Bernhoff , D. Besson , N. Bingefors , O. Botner , S. Buitink
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K. Carter B. A. Clark A. Connolly P. Dasgupta S. de Kockere K. D. de Vries C. Deaconu M. A. DuVernois N. Feigl D. Garcia-Fernandez C. Glaser A. Hallgren S. Hallmann J. C. Hanson B. Hendricks B. Hokanson-Fasig C. Hornhuber K. Hughes A. Karle J. L. Kelley S. R. Klein R. Krebs R. Lahmann M. Magnuson T. Meures Z. S. 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. J. Van Den Broeck N. van Eijndhoven A. G. Vieregg C. Welling S. Wissel R. Young A. Zink
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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.

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