Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

Albert, A.; André, M.; Anghinolfi, M.; Ardid, M.; Aubert, J.J.; Aublin, J.; Avgitas, T.; Baret, B.; Barrios-Martí, J.; Basa, S.; Belhorma, B.; Bertín, V.; Biagi, S.; Bormuth, R.; Bourret, S.; Bouwhuis, M. C.; Brânzaş, H.; Bruijn, R.; Brünner, J.; Busto, J.; Capone, A.; Caramete, L.; Carr, J.; Celli, S.; Moursli, R. Cherkaoui El; Chiarusi, T.; Circella, M.; Coelho, J. A. B.; Coleiro, A.; Coniglione, R.; Costantini, H.; Coyle, P.; Creusot, A.; Dı́az, A.; Deschamps, A.; Bonis, G. De; Distefano, C.; Domi, Alba; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; Bojaddaini, I. El; Khayati, N. El; Elsässer, Dominik; Enzenhöfer, A.; Ettahiri, A.; Fassi, F.; Felis, I.; Fusco, L.; Gay, P.; Giordano, V.; Glotin, Hervé; Grégoire, T.; Ruiz, R. Gracia; Graf, Κ.; Hallmann, S.; Haren, Hans van; Heijboer, A.; Hello, Y.; Hernández-Rey, J. J.; Hößl, J.; Hofestädt, J.; Illuminati, G.; James, C. W.; Jong, M. de; Jongen, M.; Kadler, M.; Kalekin, O.; Kießling, D.; Kouchner, A.; Kreter, M.; Kreykenbohm, I.; Kulikovskiy, V.; Lachaud, C.; Lahmann, R.; Lefèvre, D.; Leonora, E.; Lotze, Martín; Loucatos, S.; Marcelin, M.; Margiotta, A.; Marinelli, A.; Martínez-Mora, J. A.; Mele, R.; Melis, K.; Michael, T.; Migliozzi, P.; Moussa, A.; Navas, S.; Nezri, E.; Organokov, M.; Păvălaş, G. E.; Pellegrino, C.; Perrina, C.; Piattelli, P.; Popa, V.; Pradier, T.; Quinn, L.; Racca, C.; Riccobene, G.; Sánchez-Losa, A.; Saldaña, M.; Salvadori, I.; Samtleben, D. F. E.; Sanguineti, M.; Sapienza, P.; Schüßler, F.; Sieger, C.; Spurio, M.; Stolarczyk, Th.; Taiuti, M.; Tayalati, Y.; Trovato, A.; Turpin, D.; Tönnis, Christoph; Vallage, B.; Elewyck, V. Van; Versari, F.; Vivolo, D.; Vizzoca, A.; Wilms, J.; Zornoza, J. D.; Zúñiga, J.; Aartsen, M. G.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Samarai, I. Al; Altmann, D.; Andeen, K.; Anderson, Tyler; Ansseau, I.; Anton, G.; Argüelles, C.; Auffenberg, J.; Axani, Spencer; Bagherpour, H.; Bai, X.; Barron, J. P.; Barwick, S. W.; Baum, V.; Bay, R.; Tjus, J. Becker; Becker, K.-H.; BenZvi, S.; Berley, D.; Bernardini, E.; Besson, D. Z.; Binder, G.; Bindig, D.; Blaufuss, E.; Blot, Summer; Böhm, C.; Börner, M.; Bos, F.; Bose, D.; Böser, S.; Botner, O.; Bourbeau, Etienne; Bourbeau, J.; Bradascio, Federica; Braun, J.; Brayeur, L.; Brenzke, M.; Bretz, H.-P.; Bron, S.; Brostean-Kaiser, Jannes; Burgman, A.; Carver, T.; Casey, J.; Casier, M.; Cheung, E.; Chirkin, D.; Christov, A.; Clark, K.; Classen, L.; Coenders, S.; Collin, Gabriel; Conrad, J. M.; Cowen, D. F.; Cross, R.; Day, M.; André, J. P. A. M. de; Clercq, C. De; DeLaunay, James; Dembinski, H.-P.; Ridder, S. De; Desiati, P.; Vries, Krijn de; Wasseige, G. de; With, M. de; DeYoung, T.; Díaz–Vélez, Juan Carlos; Lorenzo, V. di; Dujmović, Hrvoje; Dumm, J. P.; Dunkman, M.; Dvorak, Emily; Eberhardt, B.; Ehrhardt, Thomas; Eichmann, B.; Eller, P.; Evenson, P. A.; Fahey, S.; Fazely, A. R.; Felde, J.; Filimonov, K.; Finley, C.; Flis, S.; Franckowiak, A.; Friedman, E.; Fuchs, T.; Gaisser, T. K.; Gallagher, J.; Gerhardt, L.; Ghorbani, K.; Giang, W.; Glauch, Theo; Glüsenkamp, T.; Goldschmidt, A.; González, J. G.; Grant, D.; Griffith, Z.; Haack, Christian; Hallgren, A.; Halzen, F.; Hanson, K.; Hebecker, D.; Heereman, D.; Helbing, K.; Hellauer, R.; Hickford, S.; Hignight, J.; Hoffman, K. D.; Hoffmann, R.; Hokanson-Fasig, B.; Hoshina, K.; Huang, F.; Huber, M. E.; Hultqvist, K.; Hünnefeld, Mirco; In, S.; Ishihara, A.; Jacobi, E.; Japaridze, G. S.; Jeong, Minjin; Jero, K.; Jones, B. J. P.; Kalaczyński, P.; Kang, Woosik; Kappes, A.; Karg, T.; Karle, A.; Katz, U.; Kauer, M.; Keivani, A.; Kelley, J. L.; Kheirandish, Ali; Kim, J.; Kim, M.; Kintscher, T.; Kiryluk, J.; Kittler, T.; Klein, S. R.; Kohnen, G.; Koirala, R.; Kolanoski, H.; Köpke, L.; Kopper, C.; Kopper, S.; Koschinsky, J. P.; Koskinen, D. J.; Kowalski, M.; Krings, K.; Kroll, M.; Krückl, G.; Kunnen, J.; Kunwar, S.; Kurahashi, N.; Kuwabara, T.; Kyriacou, A.; Labare, M.; Lanfranchi, J. L.; Larson, M. J.; Lauber, Frederik Hermann; Lesiak-Bzdak, M.; Leuermann, M.; Liu, Q. R.; Lu, Lu; Lünemann, J.; Luszczak, William; Madsen, J.; Maggi, G.; Mahn, Kendall; Mancina, Sarah; Maruyama, R.; Mase, K.; Maunu, R.; McNally, F.; Meagher, K.; Medici, M.; Meier, Maximilian; Menne, T.; Merino, G.; Meures, T.; Miarecki, S.; Micallef, Jessie; Momenté, G.; Montaruli, T.; Moore, R. W.; Moulai, Marjon; Nahnhauer, R.; Nakarmi, P.; Naumann, Uwe; Neer, G.; Niederhausen, H.; Nowicki, S. C.; Nygren, D. R.; Pollmann, A. Obertacke; Olivas, A.; O’Murchadha, A.; Palczewski, T.; Pandya, Hershal; Pankova, D. V.; Peiffer, P.; Pepper, J. A.; Heros, C. Pérez de los; Pieloth, D.; Pinat, E.; Pranav, D.; Price, P. B.; Przybylski, G. T.; Raab, Christoph; Rädel, L.; Rameez, M.; Rawlins, K.; Rea, Immacolata Carmen; Reimann, R.; Relethford, B.; Relich, M.; Resconi, E.; Rhode, W.; Richman, M.; Robertson, Sally; Rongen, Martin; Rott, C.; Ruhe, T.; Ryckbosch, D.; Rysewyk, D.; Sälzer, T.; Herrera, S. E. Sanchez; Sandrock, A.; Sandroos, J.; Santander, M.; Sarkar, S.; Satalecka, K.; Schlunder, P.; Schmidt, T.; Schneider, A.; Schoenen, S.; Schöneberg, S.; Schumacher, Lisa Johanna; Seckel, D.; Seunarine, S.; Soedingrekso, Jan; Soldin, D.; Song, M.; Spiczak, G. M.; Spiering, Christian; Stachurska, J.; Stamatikos, M.; Stanev, T.; Stasik, A.; Stettner, J.; Steuer, A.; Stezelberger, T.; Stokstad, R. G.; Stößl, A.; Strotjohann, N. L.; Stuttard, T.; Sullivan, G. W.; Sutherland, M.; Taboada, I.; Tatar, J.; Tenholt, F.; Ter–Antonyan, S.; Terliuk, A.; Tešić, G.; Tilav, S.; Toale, P. A.; Tobin, M. N.; Toscano, S.; Tosi, D.; Tselengidou, M.; Tung, Chun Fai; Turcati, A.; Turley, C. F.; Ty, Bunheng; Unger, E.; Usner, M.; Vandenbroucke, J.; Driessche, W. Van; Eijndhoven, N. van; Vanheule, S.; Santen, J. V.; Vehring, M.; Vogel, E.; Vraeghe, M.; Walck, C.; Wallace, A.; Wallraff, M.; Wandler, F. D.; Wandkowsky, N.; Waza, A.; Weaver, C.; Weiss, Matthew J.; Wendt, Chris; Werthebach, Johannes; Westerhoff, S.; Whelan, B. J.; Wiebe, K.; Wiebusch, C. H.; Wille, L.; Williams, Daniel; Wills, L.; Wolf, M.; Wood, J.; Wood, T. R.; Woolsey, E.; Woschnagg, K.; Xu, Dawei; Xu, X. W.; Xu, Yang; Yañez, J. P.; Yodh, G.; Yoshida, Shigeru; Yuan, Tony; Zoll, M.; Aab, A.; Abreu, P.; Aglietta, M.; Albuquerque, I. F. M.; Albury, Justin M.; Allekotte, I.; Almela, A.; Castillo, J.; Álvarez-Muñiz, J.; Anastasi, Gioacchino Alex; Anchordoqui, Luis A.; Andrada, Belén; Andringa, S.; Aramo, C.; Arsene, N.; Asorey, H.; Assis, P.; Ávila, G.; Badescu, A. M.; Bălăceanu, Alexandru; Barbato, Felicia; Luz, Ricardo Jorge Barreira; Beatty, J. J.; Becker, Karl‐Heinz; Bellido, J. A.; Bérat, C.; Bertaina, M.; Bertou, X.; Biermann, P. L.; Biteau, J.; Blaess, S. G.; Blanco, A.; Blažek, Jiří; Bleve, C.; Bohã̌cov́a, M.; Bonifazi, C.; Borodai, N.; Botti, Ana Martina; Brack, J.; Brâncuş, I.M.; Bretz, T.; Bridgeman, A.; Briechle, Florian Lukas; Buchholz, P.; Bueno, A.; Buitink, S.; Buscemi, Mario; Caballero-Mora, K. S.; Caccianiga, Lorenzo; Cancio, A.; Canfora, F.; Caruso, R.; Castellina, A.; Catalani, Fernando; Cataldi, G.; Cazón, L.; Chavez, A. G.; Chinellato, J. A.; Chudoba, J.; Clay, R. W.; Cerutti, Agustín Cobos; Colalillo, R.; Coleman, Alan; Collica, L.; Coluccia, M. R.; Conceição, R.; Consolati, G.; Contreras, F.; Cooper, M. J.; Coutu, S.; Covault, C. E.; Cronin, J.; D’Amico, S.; Daniel, B.; Dasso, S.; Daumiller, K.; Dawson, B. R.; Day, J. A.; Almeida, R. M. de; Jong, S. J. De; Mauro, G. De; Neto, J. R. T. de Mello; Mitri, I. De; Oliveira, Jaime de; Souza, V. de; Debatin, J.; Deligny, O.; Castro, M. L. Díaz; Diogo, F.; Dobrigkeit, C.; D’Olivo, Juan Carlos; Dorosti, Q.; Anjos, Rita Cassia dos; Dova, M. T.; Dundovic, A.; Ebr, Jan; Engel, R.; Erdmann, M.; Erfani, Mostafa; Escobar, C. O.; Espadanal, J.; Etchegoyen, A.; Falcke, H.; Farmer, John; Farrar, Glennys R.; Fauth, A. C.; Fazzini, N.; Feldbusch, Fridtjof; Fenu, Francesco; Fick, B.; Figueira, J. M.; Filipčić, A.; Freire, M. M.; Fujii, Toshihiro; Fuster, Alan; Gaïor, R.; García, Beatriz; Gaté, F.; Gemmeke, H.; Gherghel-Lascu, A.; Ghia, P. L.; Giaccari, U.; Giammarchi, M.; Giller, M.; Głas, D.; Gläser, Christian; Golup, G.; Berisso, M. Gómez; Vitale, Primo F. Gómez; González, Nicolás Martín; Gorgi, A.; Gottowik, Marvin; Grillo, Alfredo; Grubb, Trent D.; Guarino, F.; Guedes, G. P.; Halliday, R.; Hampel, Matías Rolf; Hansen, P.; Harari, D.; Harrison, T. A.; Harvey, Violet M.; Haungs, A.; Hebbeker, T.; Heck, D.; Heimann, P.; Hervé, A. E.; Hill, G. C.; Hojvat, C.; Holt, E.; Homola, P.; Hörandel, J. R.; Horváth, P.; Hrabovský, M.; Huege, T.; Hulsman, J.; Insolia, A.; Isar, P. G.; Jandt, I.; Johnsen, Jeffrey A.; Josebachuili, M.; Jurýšek, Jakub; Kääpä, Alex; Kampert, K. H.; Keilhauer, B.; Kemmerich, N.; Kemp, J.; Kieckhafer, R. M.; Klages, H. O.; Kleifges, M.; Kleinfeller, J.; Krause, R.; Krohm, N.; Kuempel, D.; Mezek, G. Kukec; Kunka, N.; Awad, A. Kuotb; Lago, Bruno L.; LaHurd, D.; Lang, Rodrigo Guedes; Lauscher, M.; Legumina, R.; Oliveira, M. A. Leigui de; Letessier‐Selvon, A.; Lhenry-Yvon, I.; Link, K.; Presti, D. Lo; Lopes, L.; López, R.; Casado, A. López; Lorek, R.; Luce, Quentin; Lucero, A.; Malacari, M.; Mallamaci, M.; Mandat, D.; Mantsch, P.; Mariazzi, Analisa; Maris, Ioana Codrina; Marsella, G.; Martello, D.; Martínez, H.; Bravo, O. Martínez; Meza, J. J. Masías; Mathes, H. J.; Mathys, S.; Matthews, J.; Matthiae, G.; Mayotte, E.; Mazur, Péter; Medina, C.; Medina‐Tanco, G.; Melo, D.; Menshikov, Alexander; Merenda, Kevin-Druis; Michal, Stanislav; Micheletti, M. I.; Middendorf, L.; Miramonti, L.; Mitrica, B.; Mockler, D.; Mollerach, Silvia; Montanet, F.; Morello, C.; Morlino, G.; Mostafá, M.; Müller, Andreas; Müller, G.; Müller, M. A.; Müller, S.; Mussa, R.; Naranjo, I. N.; Nellen, L.; Nguyen, P.; Niculescu-Oglinzanu, M.; Niechciol, Marcus; Niemietz, L.; Niggemann, T.; Nitz, D.; Nosek, D.; Novotný, Vladimír; Nožka, L.; Núñez, Luis A.; Oikonomou, Foteini; Olinto, Angela V.; Palatka, M.; Pallotta, J.; Papenbreer, P.; Parente, G.; Parra, A.; Paul, T.; Pech, M.; Pedreira, F.; Pękala, Jan; Pelayo, R.; Peña-Rodríguez, Jesús; Pereira, L. A. S.; Perlín, M.; Perrone, L.; Peters, C. F. W.; Petrera, S.; Phuntsok, J.; Pierog, T.; Pimenta, M.; Pirronello, V.; Platino, M.; Plum, M.; Poh, J.; Porowski, C.; Prado, R. R.; Privitera, P.; Prouza, M.; Quel, E. J.; Querchfeld, S.; Quinn, S.; Ramos-Pollán, Raúl; Rautenberg, J.; Ravignani, D.; Řídký, J.; Riehn, Felix; Risse, M.; Ristori, P.; Rizi, V.; Carvalho, W. Rodrigues de; Fernandez, G. Rodriguez; Rojo, Juan; Roncoroni, Matías J.; Roth, M.; Roulet, Esteban; Rovero, A. C.; Ruehl, Philip; Saffi, S. J.; Sǎftoiu, A.; Salamida, F.; Salazar, H.; Saleh, A.; Salina, G.; Sánchez, F.; Sánchez-Lucas, P.; Santos, E.; Santos, Eva; Sarazin, F.; Sarmento, R.; Sarmiento-Cano, C.; Sato, R.; Schauer, Markus; Scherini, V.; Schieler, H.; Schimp, Michael; Schmidt, D.; Scholten, Olaf; Schovánek, Petr; Schröder, Frank G.; Schröder, S.; Schulz, Alexander; Schumacher, J.; Sciutto, S. J.; Segreto, A.; Shadkam, A.; Shellard, R. C.; Sigl, Guenter; Silli, Gaia; Šmída, R.; Snow, G. R.; Sommers, P.; Sonntag, S.; Soriano, Jorge F.; Squartini, R.; Stanca, Denis; Stanič, S.; Stasielak, J.; Stassi, P.; Stolpovskiy, M.; Strafella, F.; Streich, Alexander; Suárez, F.; Durán, M. Suarez; Sudholz, T.; Suomijärvi, T.; Supanitsky, A. D.; Šupík, J.; Swain, J.; Szadkowski, Z.; Taboada, A.; Taborda, O. A.; Timmermans, C.; Peixoto, C. J. Todero; Tomankova, L.; Tomé, B.; Elipe, G. 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A.; Amato, A.; Ananyeva, A.; Anderson, S. B.; Anderson, W. G.; Angelova, S. V.; Antier, S.; Appert, S.; Arai, K.; Araya, M. C.; Areeda, J. S.; Arnaud, N.; Arun, K. G.; Ascenzi, S.; Ashton, G.; Ast, M.; Aston, S. M.; Astone, P.; Atallah, D. V.; Aufmuth, P.; Aulbert, C.; AultONeal, K.; Austin, C.; Avila-Alvarez, A.; Babak, S.; Bacon, P.; Bader, M. K. M.; Bae, S.; Baker, P. T.; Baldaccini, F.; Ballardin, G.; Ballmer, S. W.; Banagiri, S.; Barayoga, J. C.; Barclay, S. E.; Barish, B. C.; Barker, D.; Barkett, K.; Barone, F.; Barr, B.; Barsotti, L.; Barsuglia, M.; Bárta, D.; Bartlett, J.; Bartos, I.; Bassiri, R.; Basti, A.; Batch, J. C.; Bawaj, M.; Bayley, J. C.; Bazzan, M.; Bécsy, B.; Beer, C.; Bejger, M.; Belahcene, I.; Bell, A. S.; Berger, B. K.; Bergmann, G.; Bero, J. J.; Berry, C. P. L.; Bersanetti, D.; Bertolini, A.; Betzwieser, J.; Bhagwat, S.; Bhandare, R.; Bilenko, I. A.; Billingsley, G.; Billman, C. R.; Birch, J.; Birney, R.; Birnholtz, O.; Biscans, S.; Biscoveanu, S.; Bisht, A.; Bitossi, M.; Biwer, C.; Bizouard, M. A.; Blackburn, J. K.; Blackman, J.; Blair, C. D.; Blair, D. G.; Blair, R. M.; Bloemen, S.; Böck, O.; Bode, N.; Boër, M.; Bogaert, G.; Bohé, A.; Bondu, F.; Bonilla, E.; Bonnand, R.; Boom, B. A.; Bork, R.; Boschi, V.; Bose, S.; Bossie, K.; Bouffanais, Y.; Bozzi, A.; Bradaschia, C.; Brady, P. R.; Branchesi, M.; Brau, J.; Briant, T.; Brillet, A.; Brinkmann, M.; Brisson, V.; Brockill, P.; Broida, J. E.; Brooks, A. F.; Brown, D. A.; Brown, D. D.; Brunett, S.; Buchanan, C. C.; Buikema, A.; Bulik, T.; Bulten, H. J.; Buonanno, A.; Buskulic, D.; Buy, C.; Byer, R. L.; Cabero, M.; Cadonati, L.; Cagnoli, G.; Cahillane, C.; Bustillo, J. Calderón; Callister, T. A.; Calloni, E.; Camp, J. B.; Canepa, M.; Cañizares, P.; Cannon, K. C.; Cao, H.; Cao, J.; Capano, C. D.; Capocasa, E.; Carbognani, F.; Caride, S.; Carney, M. F.; Díaz, J. Casanueva; Casentini, C.; Caudill, S.; Cavaglià, M.; Cavalier, F.; Cavalieri, R.; Cella, G.; Cepeda, C.; Cerdá–Durán, P.; Cerretani, G.; Cesarini, E.; Chamberlin, S. J.; Chan, M.; Chao, S.; Charlton, P.; Chase, E. A.; Chassande–Mottin, E.; Chatterjee, Debarati; Cheeseboro, B. D.; Chen, H. Y.; Chen, X.; Chen, Y.; Cheng, Hai‐Ping; Chia, H. Y.; Chincarini, A.; Chiummo, A.; Chmiel, T.; Cho, H. S.; Cho, M.; Chow, J. H.; Christensen, N.; Chu, Q.; Chua, Alvin J. K.; Chua, S.; Chung, A. K. W.; Chung, S.; Ciani, G.; Ciolfi, R.; Cirelli, Chiara; Cirone, A.; Clara, F.; Clark, J. A.; Clearwater, P.; Cleva, F.; Cocchieri, C.; Coccia, E.; Cohadon, P.-F.; Cohen, D.; Colla, A.; Collette, Christophe; Cominsky, L.; Constancio, M.; Conti, L.; Cooper, S. J.; Corban, P.; Corbitt, T. R.; Cordero-Carrión, I.; Corley, K. R.; Cornish, N.; Corsi, A.; Cortese, S.; Costa, C. A.; Coughlin, M. W.; Coughlin, S. B.; Coulon, J.-P.; Countryman, S. T.; Couvares, P.; Covas, P. B.; Cowan, E. E.; Coward, D. M.; Cowart, M. J.; Coyne, D. C.; Coyne, R.; Creighton, J. D. E.; Creighton, T. D.; Cripe, J.; Crowder, S. G.; Cullen, T. J.; Cumming, A.; Cunningham, L.; Cuoco, E.; Canton, T. Dal; Dálya, G.; Danilishin, S. L.; D’Antonio, S.; Danzmann, K.; Dasgupta, Arnab; Costa, C. F. Da Silva; Dattilo, V.; Dave, I.; Davier, M.; Davis, D.; Daw, E. J.; Day, B.; De, S.; DeBra, D.; Degallaix, J.; Laurentis, Mariafelicia De; Deléglise, S.; Pozzo, W. Del; Demos, N.; Denker, T.; Dent, T.; Pietri, R. De; Dergachev, V.; Rosa, R. De; DeRosa, R. T.; Rossi, C. De; DeSalvo, R.; Varona, O. de; Devenson, J.; Dhurandhar, S.; Díaz, M. C.; Fiore, L. Di; Giovanni, M. Di; Girolamo, T. Di; Lieto, A. Di; Pace, S. Di; Palma, I. Di; Renzo, F. Di; Doctor, Z.; Dolique, V.; Donovan, F.; Dooley, K. L.; Doravari, S.; Dorrington, I.; Douglas, R.; Álvarez, M. Dovale; Downes, T. P.; Drago, M.; Dreißigacker, C.; Driggers, J. C.; Du, Z.; Ducrot, M.; Dupej, P.; Dwyer, S. E.; Edo, T. B.; Edwards, M. C.; Effler, A.; Eggenstein, H.-B.; Ehrens, P.; Eichholz, J.; Eikenberry, S. S.; Eisenstein, R. A.; Essick, R. C.; Estevez, D.; Etienne, Z. B.; Etzel, T.; Evans, M.; Evans, T. M.; Factourovich, M.; Fafone, V.; Fair, H.; Fairhurst, S.; Fan, X.; Farinon, S.; Farr, B.; Farr, W. M.; Fauchon-Jones, E. J.; Favata, M.; Fays, M.; Fee, Conan J.; Fehrmann, H.; Feicht, J.; Fejer, M. M.; Fernandez-Galiana, A.; Ferrante, I.; Ferreira, E. C.; Ferrini, F.; Fidecaro, F.; Finstad, D.; Fiori, I.; Fiorucci, D.; Fishbach, M.; Fisher, R. P.; Fitz-Axen, M.; Flaminio, R.; Fletcher, M.; Fong, H.; Font, José A.; Forsyth, P. W. F.; Forsyth, S. S.; Fournier, J.-D.; Frasca, S.; Frasconi, F.; Frei, Z.; Freise, A.; Frey, R.; Frey, V.; Fries, E. M.; Fritschel, P.; Frolov, V. V.; Fulda, P.; Fyffe, M.; Gabbard, H. A.; Gadre, B. U.; Gaebel, S. M.; Gair, J. R.; Gammaitoni, L.; Ganija, M. R.; Gaonkar, S. G.; García-Quirós, C.; Garufi, F.; Gateley, B.; Gaudio, S.; Gaur, G.; Gayathri, V.; Gehrels, N.; Gemme, G.; Genin, É.; Gennai, A.; George, D.; George, J.; Gergely, L.; Germain, V.; Ghonge, S.; Ghosh, Abhirup; Ghosh, Archisman; Ghosh, S.; Giaime, J. A.; Giardina, K. D.; Giazotto, A.; Gill, K.; Glover, L.; Goetz, E.; Goetz, R.; Gomes, S.; Goncharov, B.; González, Gabriela; Castro, J. M. Gonzalez; Gopakumar, A.; Gorodetsky, M. L.; Gossan, S. E.; Gosselin, M.; Gouaty, R.; Grado, A.; Graef, C.; Granata, M.; Grant, A.; Gras, S.; Gray, C.; Greco, G.; Green, A. C.; Gretarsson, E. M.; Groot, P.; Grote, H.; Grünewald, S.; Grüning, P.; Guidi, G. M.; Guo, X.; Gupta, Anchal; Gupta, M. K.; Gushwa, K. E.; Gustafson, E. K.; Gustafson, R.; Halim, O.; Hall, B. R.; Hall, E. D.; Hamilton, E. Z.; Hammond, G.; Haney, M.; Hanke, M. M.; Hanks, J.; Hanna, C.; Hannam, M. D.; Hannuksela, O. A.; Hanson, J.; Hardwick, T.; Harms, J.; Harry, G. M.; Harry, I. W.; Hart, M. 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doi:10.3847/2041-8213/aa9aed

Cited by 171 publications

(140 citation statements)

References 60 publications

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“…These windows are consistent with those selected in Albert et al (2017). The expected number of events based on 2976.01 days of SK data, and the number of events that we actually observed, are listed in Table 1 for a ±500-s window and for the following 14-day interval.…”

Section: High-energy Data Samplesupporting

confidence: 67%

“…that the present study is sensitive to neutrinos between 1.6 and 100 GeV, which is not covered in other searches (Albert et al 2017). Our UPMU data may be compared or combined directly with that of other neutrino telescopes.…”

Section: Neutrino Fluence Limitmentioning

confidence: 99%

“…High-energy neutrino signals associated with the merger were also searched for by the Astronomy with a Neutrino Telescope and Abyss Environmental RESearch (ANTARES), IceCube, and Pierre Auger Observatories. It was concluded that no significant neutrino signal was observed (Albert et al 2017).…”

Section: Introductionmentioning

confidence: 99%

See 2 more Smart Citations

Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger

Bronner¹,

Hayato²,

Ikeda³

et al. 2018

ApJL

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We report the results of a neutrino search in Super-Kamiokande (SK) for coincident signals with the first detected gravitational wave (GW) produced by a binary neutron-star merger, GW170817, which was followed by a short gamma-ray burst, GRB170817A, and a kilonova/macronova. We searched for coincident neutrino events in the range from 3.5MeV to ∼100 PeV, in a time window ±500 s around the gravitational wave detection time, as well as during a 14-day period after the detection. No significant neutrino signal was observed for either time window. We calculated 90% confidence level upper limits on the neutrino fluence for GW170817. From the upward-goingmuon events in the energy region above 1.6 GeV, the neutrino fluence limit is -+ 16.0 0.6 0.7 ( -+ 21.3 0.8 1.1 ) cm −2 for muon neutrinos (muon antineutrinos), with an error range of ±5°around the zenith angle of NGC4993, and the energy spectrum is under the assumption of an index of −2. The fluence limit for neutrino energies less than 100MeV, for which the emission mechanism would be different than for higher-energy neutrinos, is also calculated. It is 6.6×10 7 cm −2 for anti-electron neutrinos under the assumption of a Fermi-Dirac spectrum with average energy of 20 MeV.

show abstract

Section: High-energy Data Samplesupporting

confidence: 67%

Section: Neutrino Fluence Limitmentioning

confidence: 99%

See 1 more Smart Citation

Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger

Bronner¹,

Hayato²,

Ikeda³

et al. 2018

ApJL

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show abstract

“…Recent studies have shown that cosmic rays production up to energies near the socalled "ankle" feature in the Galactic cosmic ray spectrum ( 10 18 eV) may be plausible in such merger events [5,6]. Searches for GeV-EeV neutrinos directionally coincident with GW170817 within various time windows, were conducted with ANTARES, IceCube and the Pierre Auger Observatory, but no detections were reported [7]. The non-detection of GW170817 was found to be consistent with the models of neutrino production in binary NS mergers that had been postulated then [8,9].…”

Section: Introductionmentioning

confidence: 99%

High-energy neutrinos from fallback accretion of binary neutron star merger remnants

Guépin

Fang

Kotera

et al. 2020

J. Cosmol. Astropart. Phys.

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Following the coalescence of binary neutron stars, debris from the merger which remains marginally bound to the central compact remnant will fallback at late times, feeding a sustained accretion flow. Unbound winds or a wide-angle jet from this radiatively-inefficient disk may collide with the comparatively slow dense kilonova ejecta released from an earlier phase. Under the assumption that such interaction accelerate cosmic rays to ultra-high energies, we numerically simulate their propagation and interactions through the dynamical ejecta. The hadronuclear and photo-hadronic processes experienced by particles produce isotropic high-energy neutrino fluxes, peaking at times 10 3−4 s, which we calculate for two sets of parameters. A first set is inspired by the observations of GW170817. In the second scenario, which we call optimistic, parameters are chosen so as to optimize the neutrino flux, within the range allowed by observation and theory. We find that single sources can only be detected with IceCube-Gen2 for optimistic scenarios and if located within ∼ 4 Mpc. The cumulative flux could contribute to ∼ 0.5 − 10% of the diffuse flux observed by the IceCube Observatory, depending on the fall-back power and the cosmic ray composition. The neutrino emission powered by fallback is nearly isotropic, and can be used for future correlation studies with gravitational wave signals.

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“…If this bursty scenario is dominant though, one could potentially hope for a correlation between UHECR and GW observations, with one signature of the RS mechanism being that the UHECRs temporally precede the GW (but deflection of the CR particles by magnetic fields may cause them to take a detour, so careful data analysis is needed). So far, efforts had been made to search for photons and neutrinos coincident with GW from a double neutron star merger [72,73], and if BBHs are indeed the sources of UHECRs, two new fronts in multimessenger astronomy may open up, namely the utilization of charged particles as messengers, as well as with BBHs as observation targets.…”

Section: Source Populationmentioning

confidence: 99%

Gravitational slingshots around black holes in a binary

Zhang

2020

Eur. Phys. J. Plus

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The speed gain of a test mass from taking a gravitational slingshot around a celestial object (scattering centre) increases with the latter's speed and compactness (stronger deflection of the mass' trajectory becomes possible without it hitting the surface of the object). The black holes (BHs) in a tight binary (consisting of two black holes; we are not considering X-ray binaries), themselves moving at relativistic speeds, represent optimal scattering centres. Therefore, a sub-population of accreting matter particles, swept up into chaotic orbits around a BH binary, might repeatedly take slingshots and become accelerated to ultra-relativistic speeds (as seen by observers on Earth), ultimately escaping from the binary, as well as the fate of being devoured by a BH. The escaped particles can plausibly be observed on Earth as ultra-high-energy cosmic rays (UHECRs). Investigating such a possibility would require general relativistic slingshot formulae due to the high speeds involved and the close encounters with BHs. We derive them in this paper, and show that the percentage gain per slingshot in a particle's Lorentz factor remains undiminished even as the particle energizes up, thus demonstrating that the slingshot mechanism can in principal accelerate particles to extreme energies.PACS. 9 8.70.Sa -9 5.85.Ry -0 4.70.Bw -0 4.90.+e IntroductionUltra-high energy cosmic rays (UHECRs) [1,2] have garnered tremendous interest since they would suffer less deflection by the galactic and intergalactic magnetic fields, so their paths point roughly back at their sources, potentially helping to identify and elucidate some undoubtedly interesting extremely energetic astrophysical processes, but the nature of which have so far remained an open question. Nevertheless, more recent observations had revealed a wealth of important features in the UHECR spectrum, composition, anisotropy and (lack of) counterparts, that can guide our modelling efforts. For example, the most straightforward top-down approach, where some type of extremely heavy beyond-the-standard-model particle decays into lighter ones whose rest masses add up to only a small fraction of the parent particle's rest mass, is now somewhat disfavoured. Firstly, such processes tend to produce copious amounts of concomitant high energy photons and neutrinos, which are absent observationally [3,4]. Also, composition studies show that there should be large amounts of intermediate mass nuclei at the very highest energies [5,6,7], which would be rather perplexing in the decay picture, as one must wonder why ultra-relativistic nucleons (as decay products) all move in the same direction and remain bound inside a nuclei, instead of simply flying off in all directions.The bottom-up alternative of accelerating initially low energy particles is no less challenging. The macroscopic high energies reaching into hundreds of EeVs means that we need to find an extremely energy-dense environment that can boost the particles to exceptionally high Lorentz factors. Thankfully though, the candidate...

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Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory

Cited by 171 publications

References 60 publications

Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger

Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger

High-energy neutrinos from fallback accretion of binary neutron star merger remnants

Gravitational slingshots around black holes in a binary

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