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

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Main Authors:	Aguilar, J. A., Allison, P., Beatty, J. J., Bernhoff, H., Besson, D., Bingefors, N., Botner, O., Buitink, S., Carter, K., Clark, B. A., Connolly, A., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Feigl, N., Garcia-Fernandez, D., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Hendricks, B., Hokanson-Fasig, B., Hornhuber, C., Hughes, K., Karle, A., Kelley, J. L., Klein, S. R., Krebs, R., Lahmann, R., Magnuson, M., Meures, T., Meyers, Z. S., Nelles, A., Novikov, A., Oberla, E., Oeyen, B., Pandya, H., Plaisier, I., Pyras, L., Ryckbosch, D., Scholten, O., Seckel, D., Smith, D., Southall, D., Torres, J., Toscano, S., Broeck, D. J. Van Den, van Eijndhoven, N., Vieregg, A. G., Welling, C., Wissel, S., Young, R., Zink, A.
Format:	Preprint
Published:	2020
Subjects:	Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
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_version_	1866913450981064704
author	Aguilar, J. A. Allison, P. Beatty, J. J. Bernhoff, H. Besson, D. Bingefors, N. Botner, O. Buitink, S. Carter, K. Clark, B. A. Connolly, A. Dasgupta, P. de Kockere, S. de Vries, K. D. Deaconu, C. DuVernois, M. A. Feigl, N. Garcia-Fernandez, D. Glaser, C. Hallgren, A. Hallmann, S. Hanson, J. C. Hendricks, B. Hokanson-Fasig, B. Hornhuber, C. Hughes, K. Karle, A. Kelley, J. L. Klein, S. R. Krebs, R. Lahmann, R. Magnuson, M. Meures, T. Meyers, Z. S. Nelles, A. Novikov, A. Oberla, E. Oeyen, B. Pandya, H. Plaisier, I. Pyras, L. Ryckbosch, D. Scholten, O. Seckel, D. Smith, D. Southall, D. Torres, J. Toscano, S. Broeck, D. J. Van Den van Eijndhoven, N. Vieregg, A. G. Welling, C. Wissel, S. Young, R. Zink, A.
author_facet	Aguilar, J. A. Allison, P. Beatty, J. J. Bernhoff, H. Besson, D. Bingefors, N. Botner, O. Buitink, S. Carter, K. Clark, B. A. Connolly, A. Dasgupta, P. de Kockere, S. de Vries, K. D. Deaconu, C. DuVernois, M. A. Feigl, N. Garcia-Fernandez, D. Glaser, C. Hallgren, A. Hallmann, S. Hanson, J. C. Hendricks, B. Hokanson-Fasig, B. Hornhuber, C. Hughes, K. Karle, A. Kelley, J. L. Klein, S. R. Krebs, R. Lahmann, R. Magnuson, M. Meures, T. Meyers, Z. S. Nelles, A. Novikov, A. Oberla, E. Oeyen, B. Pandya, H. Plaisier, I. Pyras, L. Ryckbosch, D. Scholten, O. Seckel, D. Smith, D. Southall, D. Torres, J. Toscano, S. Broeck, D. J. Van Den van Eijndhoven, N. Vieregg, A. G. Welling, C. Wissel, S. Young, R. Zink, A.
contents	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.
format	Preprint
id	arxiv_https___arxiv_org_abs_2010_12279
institution	arXiv
publishDate	2020
record_format	arxiv
spellingShingle	Design and Sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G) Aguilar, J. A. Allison, P. Beatty, J. J. Bernhoff, H. Besson, D. Bingefors, N. Botner, O. Buitink, S. Carter, K. Clark, B. A. Connolly, A. Dasgupta, P. de Kockere, S. de Vries, K. D. Deaconu, C. DuVernois, M. A. Feigl, N. Garcia-Fernandez, D. Glaser, C. Hallgren, A. Hallmann, S. Hanson, J. C. Hendricks, B. Hokanson-Fasig, B. Hornhuber, C. Hughes, K. Karle, A. Kelley, J. L. Klein, S. R. Krebs, R. Lahmann, R. Magnuson, M. Meures, T. Meyers, Z. S. Nelles, A. Novikov, A. Oberla, E. Oeyen, B. Pandya, H. Plaisier, I. Pyras, L. Ryckbosch, D. Scholten, O. Seckel, D. Smith, D. Southall, D. Torres, J. Toscano, S. Broeck, D. J. Van Den van Eijndhoven, N. Vieregg, A. G. Welling, C. Wissel, S. Young, R. Zink, A. Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena 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.
title	Design and Sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G)
topic	Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena
url	https://arxiv.org/abs/2010.12279