Venters TM, Reno MH, Krizmanic JF, Olinto AV, Adams JH, Aloisio R, Anchordoqui LA, Anzalone A, Bagheri M, Barghini D, Battisti M, Bergman DR, Bertaina ME, Bertone PF, Bisconti F, Bustamante M, Cafagna F, Caruso R, Casolino M, Černý K, Christl MJ, Cummings AL, De Mitri I, Diesing R, Engel R, Eser J, Fang K, Fenu F, Filippatos G, Gazda E, Guepin C, Haungs A, Hays EA, Judd EG, Klimov PA, Kungel V, Kuznetsov E, Mackovjak , Mandát D, Marcelli L, McEnery J, Medina-Tanco G, Merenda KD, Meyer SS, Mitchell JW, Miyamoto H, Nachtman JM, Neronov A, Oikonomou F, Onel Y, Osteria G, Otte AN, Parizot E, Paul T, Pech M, Perkins JS, Picozza P, Piotrowski LW, Plebaniak Z, Prévôt G, Reardon P, Ricci M, Romero Matamala OF, Sarazin F, Schovánek P, Scotti V, Shinozaki K, Soriano JF, Stecker F, Takizawa Y, Ulrich R, Unger M, Wiencke L, Winn D, Young RM, Zotov MY, Abdellaoui G, Abe S, Allard D, Alonso G, Arnone E, Asano K, Attallah R, Attoui H, Ave Pernas M, Baláz J, Bakiri M, Bartocci S, Bayer J, Beldjilali B, Belenguer T, Belkhalfa N, Bellotti R, Belov AA, Benmessai K, Biermann PL, Blaksley C, Blanc N, Blin-Bondil S, Bobik P, Bogomilov M, Bolmgren K, Bozzo E, Briz S, Bruno A, Caballero KS, Cambié G, Campana D, Capdevielle JN, Capel F, Caramete A, Caramete L, Carlson P, Cassardo C, Castellina A, Catalano O, Cellino A, Chikawa M, Chiritoi G, Colalillo R, Conti L, Cotto G, Crawford HJ, Cremonini R, Creusot A, de Castro Gónzalez A, de la Taille C, del Peral L, Diaz Damian A, Dinaucourt P, Djakonow A, Djemil T, Ebersoldt A, Ebisuzaki T, Fernández-González S, Ferrarese S, Finch WI, Fornaro C, Fouka M, Franceschi A, Franchini S, Fuglesang C, Fujii T, Fukushima M, Galeotti P, García-Ortega E, Gardiol D, Garipov GK, Gascón E, Genci J, Golzio A, González Alvarado C, Gorodetzky P, Green A, Guarino F, Guzmán A, Hachisu Y, Hernández Carretero J, Hulett L, Ikeda D, Inoue N, Inoue S, Isgrò F, Itow Y, Jammer T, Jeong S, Joven E, Jochum J, Kajino F, Kajino T, Kalli S, Kaneko I, Karadzhov Y, Kasztelan M, Katahira K, Kawai K, Kawasaki Y, Kedadra A, Khales H, Khrenov BA, Kim JS, Kim SW, Kleifges M, Kolev D, Kreykenbohm I, Królik K, Kurihara Y, Kusenko A, Lahmar H, Lakhdari F, Licandro J, López Campano L, López Martínez F, Mahdi M, Manfrin M, Marcos JL, Marszał W, Martín Y, Martinez O, Mase K, Matev R, Matthews JN, Mebarki N, Menshikov GA, Merino A, Mese M, Meseguer J, Mimouni J, Mizumoto Y, Monaco A, Morales de los Ríos JA, Mastafa M, Nagataki S, Naitamor S, Napolitano T, Nomoto JK, Nonaka T, Ogawa T, Ogio S, Ohmori H, Pagliaro A, Painter W, Panasyuk MI, Panico B, Park IH, Pastircak B, Pérez-Grande I, Perfetto F, Peter T, Pindado S, Piraino S, Pollini ZA, Popescu EM, Prevete R, Prieto H, Przybylak M, Puehlhofer G, Putis M, Reyes M, Rodríguez Frías MD, Ronga F, Sabau MD, Saccá G, Sáez Cano G, Sagawa H, Sahnoune Z, Saito A, Sakaki N, Salazar H, Sanchez Balanzar JC, Sánchez JL, Santangelo A, Sanz-Andrés A, Sanz Palomino M, Saprykin OA, Sato M, Scagliola A, Schanz T, Schieler H, Serra M, Sharakin SA, Shimizu HM, Sotgiu A, Stan I, Strharský I, Sugiyama N, Supanitsky D, Suzuki M, Szabelski J, Tajima N, Tajima T, Takahashi Y, Takeda M, Talai MC, Tameda Y, Tenzer C, Thomas SB, Tibolla O, Tkachev LG, Tomida T, Tone N, Toscano S, Traïche M, Tsunesada Y, Tsuno K, Turriziani S, Uchihori Y, Vaduvescu O, Valdés-Galicia JF, Vallania P, Valore L, Vankova-Kirilova G, Vigorito C, Villaseñor L, Vlcek B, von Ballmoos P, Vrabel M, Wada S, Watanabe J, Watts J, Weigand Muñoz R, Weindl A, Wille M, Wilms J, Yamamoto T, Yang J, Yano H, Yashin IV, Yonetoku D, Yoshida S, Zgura IS, Zuccaro Marchi A (2022)
Publication Type: Conference contribution
Publication year: 2022
Publisher: Sissa Medialab Srl
Book Volume: 395
Conference Proceedings Title: Proceedings of Science
Event location: Virtual, Berlin, DEU
Cosmic-ray accelerators capable of reaching ultra-high energies are expected to also produce very-high energy neutrinos via hadronic interactions within the source or its surrounding environment. Many of the candidate astrophysical source classes are either transient in nature or exhibit flaring activity. Using the Earth as a neutrino converter, suborbital and space-based optical Cherenkov detectors, such as POEMMA and EUSO-SPB2, will be able to detect upward-moving extensive air showers induced by decaying tau-leptons generated from cosmic tau neutrinos with energies ∼ 10 PeV and above. Both EUSO-SPB2 and POEMMA will be able to quickly repoint, enabling rapid response to astrophysical transient events. We calculate the transient sensitivity and sky coverage for both EUSO-SPB2 and POEMMA, accounting for constraints imposed by the Sun and the Moon on the observation time. We also calculate both detectors' neutrino horizons for a variety of modeled astrophysical neutrino fluences. We find that both EUSO-SPB2 and POEMMA will achieve transient sensitivities at the level of modeled neutrino fluences for nearby sources. We conclude with a discussion of the prospects of each mission detecting at least one transient event for various modeled astrophysical neutrino sources.
APA:
Venters, T.M., Reno, M.H., Krizmanic, J.F., Olinto, A.V., Adams, J.H., Aloisio, R.,... Zuccaro Marchi, A. (2022). Neutrino Target-of-Opportunity Observations with Space-based and Suborbital Optical Cherenkov Detectors. In Proceedings of Science. Virtual, Berlin, DEU: Sissa Medialab Srl.
MLA:
Venters, Tonia M., et al. "Neutrino Target-of-Opportunity Observations with Space-based and Suborbital Optical Cherenkov Detectors." Proceedings of the 37th International Cosmic Ray Conference, ICRC 2021, Virtual, Berlin, DEU Sissa Medialab Srl, 2022.
BibTeX: Download