par Aguilar Sanchez, Juan Antonio 
;Dasgupta, Paramita ;Korntheuer, Michaël ;Schlüter, Felix ;Toscano, Simona ; [et al.]
Référence (26 July 2023 through 3 August 2023: Nagoya), 38th International Cosmic Ray Conference, ICRC 2023, Pos proceedings of science (444), 1485
Publication Publié, 2024-03-01
;Dasgupta, Paramita ;Korntheuer, Michaël ;Schlüter, Felix ;Toscano, Simona ; [et al.]Référence (26 July 2023 through 3 August 2023: Nagoya), 38th International Cosmic Ray Conference, ICRC 2023, Pos proceedings of science (444), 1485
Publication Publié, 2024-03-01
Publication dans des actes
| Résumé : | The Radio Neutrino Observatory in Greenland (RNO-G) is the only ultrahigh energy (UHE, ?30 PeV) neutrino monitor of the Northern sky and will soon be the world’s most sensitive high-uptime detector of UHE neutrinos. Because of this, RNO-G represents an important piece of the multimessenger landscape over the next decade. In this talk, we will highlight RNO-G’s multimessenger capabilities and its potential to provide key information in the search for the most extreme astrophysical accelerators. In particular, we will highlight opportunities enabled by RNO-G’s unique field-of-view, its potential to constrain the sources of UHE cosmic rays, and its complementarity with IceCube at lower energies. |
