The Radio Neutrino Observatory Greenland (RNO-G)

Rno-g,; Aguilar, J. A.; Allison, P.; Beatty, J. J.; Bernhoff, Hans; Besson, D.; Bingefors, N.; Botner, O.; Bouma, Sjoerd; Buitink, S.; Carter, Katie; Cataldo, Maddalena; Clark, Brian; Curtis-Ginsberg, Zachary; Connolly, A.; Dasgupta, P.; Kockere, Simon De; Vries, Krijn de; Deaconu, C.; DuVernois, Michael; Gläser, Christian; Hallgren, A.; Hallmann, S.; Hanson, Jordan C.; Hendricks, B. Clifford; Hokanson-Fasig, B.; Hornhuber, C.; Hughes, K.; Karle, A.; Kelley, J. L.; Klein, S. R.; Krebs, Ryan; Lahmann, R.; Latif, Uzair Abdul; Magnuson, Mitchell; Meures, T.; Meyers, Zachary S.; Mulrey, Katharine; Nelles, A.; Novikov, Alexander; Oberla, E.; Oeyen, Bob; Pandya, Hershal; Plaisier, Ilse; Pyras, Lilly; Ryckbosch, D.; Scholten, Olaf; Seckel, D.; Smith, Daniel A.; Southall, Daniel; Torres, Jorge; Toscano, S.; Tosi, D.; Broeck, Dieder Van den; Eijndhoven, N. van; Vieregg, A. G.; Wissel, Stephanie; Young, Robert D.; Zink, A.

doi:10.22323/1.395.0001

Cited by 3 publications

(6 citation statements)

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“…This field is mature enough to be rapidly growing with new planned experimental setups [92][93][94][95][96][97][98], but at the same time, there are still aspects that require further development, such as exploring other mechanisms leading to coherent pulses like transition radiation [99,100], or the full development of dedicated interferometric approaches [101] that are likely to provide new opportunities for the future.…”

Section: Progress In the Radio Technique And (The Role Of) Simulation...mentioning

confidence: 99%

Progress in the Simulation and Modelling of Coherent Radio Pulses from Ultra High-Energy Cosmic Particles

Álvarez-Muñiz

Zas

2022

Universe

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In the last decade, many experiments have been planned, designed or constructed to detect Ultra High Energy showers produced by cosmic rays or neutrinos using the radio technique. This technique consists in detecting short radio pulses emitted by the showers. When the detected wavelengths are longer than typical shower length scales, the pulses are coherent. Radio emission can be simulated by adding up the contributions of all the particle showers in a coherent way. The first program to use this approach was based on an algorithm developed more than thirty years ago and referred to as “ZHS”. Since then, much progress has been obtained using the ZHS algorithm with different simulation programs to investigate pulses from showers in dense homogeneous media and the atmosphere, applying it to different experimental initiatives, and developing extensions to address different emission mechanisms or special circumstances. We here review this work, primarily led by the authors in collaboration with other scientists, illustrating the connections between different articles, and giving a pedagogical approach to most of the work.

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Section: Progress In the Radio Technique And (The Role Of) Simulation...mentioning

confidence: 99%

Progress in the Simulation and Modelling of Coherent Radio Pulses from Ultra High-Energy Cosmic Particles

Álvarez-Muñiz

Zas

2022

Universe

View full text Add to dashboard Cite

show abstract

“…Right: KM3NeT Detection Unit Line Fit position reconstruction with top-view for each line with respect to their position on the sea bed [28]. which hides the track in noise which can be removed in the analysis [6].…”

Section: Discussionmentioning

confidence: 99%

“…With RNO-G (Radio Neutrino Observatory Greenland) the first large scale implementation of a radio neutrino array is currently being deployed at Summit Station in its first season. 35 stations are planned and fully-funded [6]. The radio in-ice techniques targets neutrino energies above 10 PeV.…”

Section: New Players Under Constructionmentioning

confidence: 99%

“…Figure 1: Attenuation length vs. wavelength from the simultaneous multi-wavelength fit of all available STRAW data. Measurements from various other neutrino telescope sites are shown shown as well [4][5][6]. Also the results from a study of attenuation lengths in the clearest ocean waters are shown for comparison [7].…”

Section: P R E L I M I N a R Ymentioning

confidence: 99%

“…Rapporteur ncy of this analysis compared to the most recent ARA Station 2 e ciency, scaled to e blue curve is the e ciency on neutrinos in the deep region; the red curve assumes os are recoverable, a conservative estimate that causes a 21% loss in e ciency over is e cient on events with low SNR that the traditional ARA trigger is not sensitive for the deep region was set to 57 degrees, a conservative boundary from at a depth of 20 m below the surface. This was chosen to avoid impacting h are expected to penetrate to 20 m maximally [6]. le is the ratio of the correlation within 10 m of the surface and the global This also strongly correlates with surface events in the 10% sample.…”

Section: Pos(icrc2021)048mentioning

confidence: 99%

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