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arxiv: 1608.07378 · v2 · submitted 2016-08-26 · 🌌 astro-ph.HE

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Ultrahigh-energy neutrino follow-up of Gravitational Wave events GW150914 and GW151226 with the Pierre Auger Observatory

The Pierre Auger Collaboration: A. Aab , P. Abreu , M. Aglietta , I. Al Samarai , I.F.M. Albuquerque , I. Allekotte , A. Almela , J. Alvarez Castillo
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J. Alvarez-Mu\~niz M. Ambrosio G.A. Anastasi L. Anchordoqui B. Andrada S. Andringa C. Aramo F. Arqueros N. Arsene H. Asorey P. Assis J. Aublin G. Avila A.M. Badescu A. Balaceanu R.J. Barreira Luz C. Baus J.J. Beatty K.H. Becker J.A. Bellido C. Berat M.E. Bertaina X. Bertou P.L. Biermann P. Billoir J. Biteau S.G. Blaess A. Blanco J. Blazek C. Bleve M. Boh\'a\v{c}ov\'a D. Boncioli C. Bonifazi N. Borodai A.M. Botti J. Brack I. Brancus T. Bretz A. Bridgeman F.L. Briechle P. Buchholz A. Bueno S. Buitink M. Buscemi K.S. Caballero-Mora L. Caccianiga A. Cancio F. Canfora L. Caramete R. Caruso A. Castellina G. Cataldi L. Cazon R. Cester A.G. Chavez J.A. Chinellato J. Chudoba R.W. Clay R. Colalillo A. Coleman L. Collica M.R. Coluccia R. Concei\c{c}\~ao F. Contreras M.J. Cooper S. Coutu C.E. Covault J. Cronin S. D'Amico B. Daniel S. Dasso K. Daumiller B.R. Dawson R.M. de Almeida S.J. De Jong G. De Mauro J.R.T. de Mello Neto I. De Mitri J. de Oliveira V. de Souza J. Debatin O. Deligny C. Di Giulio A. Di Matteo M.L. D\'iaz Castro F. Diogo C. Dobrigkeit J.C. D'Olivo A. Dorofeev R.C. dos Anjos M.T. Dova A. Dundovic J. Ebr R. Engel M. Erdmann M. Erfani C.O. Escobar J. Espadanal A. Etchegoyen H. Falcke K. Fang G. Farrar A.C. Fauth N. Fazzini B. Fick J.M. Figueira A. Filip\v{c}i\v{c} O. Fratu M.M. Freire T. Fujii A. Fuster R. Gaior B. Garc\'ia D. Garcia-Pinto F. Gat\'e H. Gemmeke A. Gherghel-Lascu P.L. Ghia U. Giaccari M. Giammarchi M. Giller D. G{\l}as C. Glaser H. Glass G. Golup M. G\'omez Berisso P.F. G\'omez Vitale N. Gonz\'alez B. Gookin A. Gorgi P. Gorham P. Gouffon A.F. Grillo T.D. Grubb F. Guarino G.P. Guedes M.R. Hampel P. Hansen D. Harari T.A. Harrison J.L. Harton Q. Hasankiadeh A. Haungs T. Hebbeker D. Heck P. Heimann A.E. Herve G.C. Hill C. Hojvat E. Holt P. Homola J.R. H\"orandel P. Horvath M. Hrabovsk\'y T. Huege J. Hulsman A. Insolia P.G. Isar I. Jandt S. Jansen J.A. Johnsen M. Josebachuili A. K\"a\"ap\"a O. Kambeitz K.H. Kampert P. Kasper I. Katkov B. Keilhauer E. Kemp J. Kemp R.M. Kieckhafer H.O. Klages M. Kleifges J. Kleinfeller R. Krause N. Krohm D. Kuempel G. Kukec Mezek N. Kunka A. Kuotb Awad D. LaHurd M. Lauscher P. Lebrun R. Legumina M.A. Leigui de Oliveira A. Letessier-Selvon I. Lhenry-Yvon K. Link L. Lopes R. L\'opez A. L\'opez Casado Q. Luce A. Lucero M. Malacari M. Mallamaci D. Mandat P. Mantsch A.G. Mariazzi I.C. Mari\c{s} G. Marsella D. Martello H. Martinez O. Mart\'inez Bravo J.J. Mas\'ias Meza H.J. Mathes S. Mathys J. Matthews J.A.J. Matthews G. Matthiae E. Mayotte P.O. Mazur C. Medina G. Medina-Tanco D. Melo A. Menshikov S. Messina M.I. Micheletti L. Middendorf I.A. Minaya L. Miramonti B. Mitrica D. Mockler L. Molina-Bueno S. Mollerach F. Montanet C. Morello M. Mostaf\'a G. M\"uller M.A. Muller S. M\"uller I. Naranjo L. Nellen J. Neuser P.H. Nguyen M. Niculescu-Oglinzanu M. Niechciol L. Niemietz T. Niggemann D. Nitz D. Nosek V. Novotny H. No\v{z}ka L.A. N\'u\~nez L. Ochilo F. Oikonomou A. Olinto D. Pakk Selmi-Dei M. Palatka J. Pallotta P. Papenbreer G. Parente A. Parra T. Paul M. Pech F. Pedreira J. P\k{e}kala R. Pelayo J. Pe\~na-Rodriguez L. A. S. Pereira L. Perrone C. Peters S. Petrera J. Phuntsok R. Piegaia T. Pierog P. Pieroni M. Pimenta V. Pirronello M. Platino M. Plum C. Porowski R.R. Prado P. Privitera M. Prouza E.J. Quel S. Querchfeld S. Quinn R. Ramos-Pollan J. Rautenberg D. Ravignani D. Reinert B. Revenu J. Ridky M. Risse P. Ristori V. Rizi W. Rodrigues de Carvalho G. Rodriguez Fernandez J. Rodriguez Rojo D. Rogozin M. Roth E. Roulet A.C. Rovero S.J. Saffi A. Saftoiu H. Salazar A. Saleh F. Salesa Greus G. Salina J.D. Sanabria Gomez F. S\'anchez P. Sanchez-Lucas E.M. Santos E. Santos F. Sarazin B. Sarkar R. Sarmento C.A. Sarmiento R. Sato M. Schauer V. Scherini H. Schieler M. Schimp D. Schmidt O. Scholten P. Schov\'anek F.G. Schr\"oder A. Schulz J. Schulz J. Schumacher S.J. Sciutto A. Segreto M. Settimo A. Shadkam R.C. Shellard G. Sigl G. Silli O. Sima A. \'Smia{\l}kowski R. \v{S}m\'ida G.R. Snow P. Sommers S. Sonntag J. Sorokin R. Squartini D. Stanca S. Stani\v{c} J. Stasielak P. Stassi F. Strafella F. Suarez M. Suarez Dur\'an T. Sudholz T. Suomij\"arvi A.D. Supanitsky J. Swain Z. Szadkowski A. Taboada O.A. Taborda A. Tapia V.M. Theodoro C. Timmermans C.J. Todero Peixoto L. Tomankova B. Tom\'e G. Torralba Elipe D. Torres Machado M. Torri P. Travnicek M. Trini R. Ulrich M. Unger M. Urban J.F. Vald\'es Galicia I. Vali\~no L. Valore G. van Aar P. van Bodegom A.M. van den Berg A. van Vliet E. Varela B. Vargas C\'ardenas G. Varner J.R. V\'azquez R.A. V\'azquez D. Veberi\v{c} I.D. Vergara Quispe V. Verzi J. Vicha L. Villase\~nor S. Vorobiov H. Wahlberg O. Wainberg D. Walz A.A. Watson M. Weber A. Weindl L. Wiencke H. Wilczy\'nski T. Winchen D. Wittkowski B. Wundheiler S. Wykes L. Yang D. Yelos A. Yushkov E. Zas D. Zavrtanik M. Zavrtanik A. Zepeda B. Zimmermann M. Ziolkowski Z. Zong F. Zuccarello
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keywords neutrinosgw150914augereventsgw151226searchblackenergy
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On September 14, 2015 the Advanced LIGO detectors observed their first gravitational-wave (GW) transient GW150914. This was followed by a second GW event observed on December 26, 2015. Both events were inferred to have arisen from the merger of black holes in binary systems. Such a system may emit neutrinos if there are magnetic fields and disk debris remaining from the formation of the two black holes. With the surface detector array of the Pierre Auger Observatory we can search for neutrinos with energy above 100 PeV from point-like sources across the sky with equatorial declination from about -65 deg. to +60 deg., and in particular from a fraction of the 90% confidence-level (CL) inferred positions in the sky of GW150914 and GW151226. A targeted search for highly-inclined extensive air showers, produced either by interactions of downward-going neutrinos of all flavors in the atmosphere or by the decays of tau leptons originating from tau-neutrino interactions in the Earth's crust (Earth-skimming neutrinos), yielded no candidates in the Auger data collected within $\pm 500$ s around or 1 day after the coordinated universal time (UTC) of GW150914 and GW151226, as well as in the same search periods relative to the UTC time of the GW candidate event LVT151012. From the non-observation we constrain the amount of energy radiated in ultrahigh-energy neutrinos from such remarkable events.

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