IceCube Search for High-Energy Neutrinos from Ultra-Luminous Infrared Galaxies
R. Abbasi,M. Ackermann,J. Adams,J. A. Aguilar,M. Ahlers,M. Ahrens,C. Alispach,A. A. Alves,N. M. Amin,R. An,K. Andeen,T. Anderson,G. Anton,C. Arguelles,Y. Ashida,S. Axani,X. Bai,A. Balagopal,A. Barbano,S. W. Barwick,B. Bastian,V. Basu,S. Baur,R. Bay,J. J. Beatty,K. -H. Becker,J. Becker Tjus,C. Bellenghi,S. BenZvi,D. Berley,E. Bernardini,D. Z. Besson,G. Binder,D. Bindig,E. Blaufuss,S. Blot,M. Boddenberg,F. Bontempo,J. Borowka,S. Boser,O. Botner,J. Bottcher,E. Bourbeau,F. Bradascio,J. Braun,S. Bron,J. Brostean-Kaiser,S. Browne,A. Burgman,R. T. Burley,R. S. Busse,M. A. Campana,E. G. Carnie-Bronca,C. Chen,D. Chirkin,K. Choi,B. A. Clark,K. Clark,L. Classen,A. Coleman,G. H. Collin,J. M. Conrad,P. Coppin,P. Correa,D. F. Cowen,R. Cross,C. Dappen,P. Dave,C. De Clercq,J. J. DeLaunay,H. Dembinski,K. Deoskar,S. De Ridder,A. Desai,P. Desiati,K. D. de Vries,G. de Wasseige,M. de With,T. DeYoung,S. Dharani,A. Diaz,J. C. Diaz-Velez,M. Dittmer,H. Dujmovic,M. Dunkman,M. A. DuVernois,E. Dvorak,T. Ehrhardt,P. Eller,R. Engel,H. Erpenbeck,J. Evans,P. A. Evenson,K. L. Fan,A. R. Fazely,S. Fiedlschuster,A. T. Fienberg,K. Filimonov,C. Finley,L. Fischer,D. Fox,A. Franckowiak,E. Friedman,A. Fritz,P. Furst,T. K. Gaisser,J. Gallagher,E. Ganster,A. Garcia,S. Garrappa,L. Gerhardt,A. Ghadimi,C. Glaser,T. Glauch,T. Glusenkamp,A. Goldschmidt,J. G. Gonzalez,S. Goswami,D. Grant,T. Gregoire,S. Griswold,M. Gunduz,C. Gunther,C. Haack,A. Hallgren,R. Halliday,L. Halve,F. Halzen,M. Ha Minh,K. Hanson,J. Hardin,A. A. Harnisch,A. Haungs,S. Hauser,D. Hebecker,K. Helbing,F. Henningsen,E. C. Hettinger,S. Hickford,J. Hignight,C. Hill,G. C. Hill,K. D. Hoffman,R. Hoffmann,T. Hoinka,B. Hokanson-Fasig,K. Hoshina,F. Huang,M. Huber,T. Huber,K. Hultqvist,M. Hunnefeld,R. Hussain,S. In,N. Iovine,A. Ishihara,M. Jansson,G. S. Japaridze,M. Jeong,B. J. P. Jones,D. Kang,W. Kang,X. Kang,A. Kappes,D. Kappesser,T. Karg,M. Karl,A. Karle,U. Katz,M. Kauer,M. Kellermann,J. L. Kelley,A. Kheirandish,K. Kin,T. Kintscher,J. Kiryluk,S. R. Klein,R. Koirala,H. Kolanoski,T. Kontrimas,L. Kopke,C. Kopper,S. Kopper,D. J. Koskinen,P. Koundal,M. Kovacevich,M. Kowalski,T. Kozynets,E. Kun,N. Kurahashi,N. Lad,C. Lagunas Gualda,J. L. Lanfranchi,M. J. Larson,F. Lauber,J. P. Lazar,J. W. Lee,K. Leonard,A. Leszczynska,Y. Li,M. Lincetto,Q. R. Liu,M. Liubarska,E. Lohfink,C. J. Lozano Mariscal,L. Lu,F. Lucarelli,A. Ludwig,W. Luszczak,Y. Lyu,W. Y. Ma,J. Madsen,K. B. M. Mahn,Y. Makino,S. Mancina,I. C. Maris,R. Maruyama,K. Mase,T. McElroy,F. McNally,J. V. Mead,K. Meagher,A. Medina,M. Meier,S. Meighen-Berger,J. Micallef,D. Mockler,T. Montaruli,R. W. Moore,R. Morse,M. Moulai,R. Naab,R. Nagai,U. Naumann,J. Necker,L. V. Nguyen,H. Niederhausen,M. U. Nisa,S. C. Nowicki,D. R. Nygren,A. Obertacke Pollmann,M. Oehler,A. Olivas,E. O'Sullivan,H. Pandya,D. V. Pankova,N. Park,G. K. Parker,E. N. Paudel,L. Paul,C. Perez de los Heros,L. Peters,J. Peterson,S. Philippen,D. Pieloth,S. Pieper,M. Pittermann,A. Pizzuto,M. Plum,Y. Popovych,A. Porcelli,M. Prado Rodriguez,P. B. Price,B. Pries,G. T. Przybylski,C. Raab,A. Raissi,M. Rameez,K. Rawlins,I. C. Rea,A. Rehman,P. Reichherzer,R. Reimann,G. Renzi,E. Resconi,S. Reusch,W. Rhode,M. Richman,B. Riedel,E. J. Roberts,S. Robertson,G. Roellinghoff,M. Rongen,C. Rott,T. Ruhe,D. Ryckbosch,D. Rysewyk Cantu,I. Safa,J. Saffer,S. E. Sanchez Herrera,A. Sandrock,J. Sandroos,M. Santander,S. Sarkar,S. Sarkar,K. Satalecka,M. Scharf,M. Schaufel,H. Schieler,S. Schindler,P. Schlunder,T. Schmidt,A. Schneider,J. Schneider,F. G. Schroder,L. Schumacher,G. Schwefer,S. Sclafani,D. Seckel,S. Seunarine,A. Sharma,S. Shefali,M. Silva,B. Skrzypek,B. Smithers,R. Snihur,J. Soedingrekso,D. Soldin,C. Spannfellner,G. M. Spiczak,C. Spiering,J. Stachurska,M. Stamatikos,T. Stanev,R. Stein,J. Stettner,A. Steuer,T. Stezelberger,T. Sturwald,T. Stuttard,G. W. Sullivan,I. Taboada,F. Tenholt,S. Ter-Antonyan,S. Tilav,F. Tischbein,K. Tollefson,L. Tomankova,C. Tonnis,S. Toscano,D. Tosi,A. Trettin,M. Tselengidou,C. F. Tung,A. Turcati,R. Turcotte,C. F. Turley,J. P. Twagirayezu,B. Ty,M. A. Unland Elorrieta,N. Valtonen-Mattila,J. Vandenbroucke,N. van Eijndhoven,D. Vannerom,J. van Santen,S. Verpoest,M. Vraeghe,C. Walck,T. B. Watson,C. Weaver,P. Weigel,A. Weindl,M. J. Weiss,J. Weldert,C. Wendt,J. Werthebach,M. Weyrauch,N. Whitehorn,C. H. Wiebusch,D. R. Williams,M. Wolf,K. Woschnagg,G. Wrede,J. Wulff,X. W. Xu,Y. Xu,J. P. Yanez,S. Yoshida,S. Yu,T. Yuan,Z. Zhang
37TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2021（2022）
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摘要
With infrared luminosities L-IR >= 10(12)L(circle dot), Ultra-Luminous Infrared Galaxies (ULIRGs) are the most luminous objects in the infrared sky. They are predominantly powered by starburst regions with star-formation rates greater than or similar to 100 M-circle dot yr(-1). ULIRGs can also host an active galactic nucleus (AGN). Both the starburst andAGNenvironments contain plausible hadronic accelerators, making ULIRGs candidate neutrino sources. We present the results of an IceCube stacking analysis searching for high-energy neutrinos from a representative sample of 75 ULIRGs with redshift z <= 0.13. While no significant excess of ULIRG neutrinos is found in 7.5 years of IceCube data, upper limits are reported on the neutrino flux from these 75 ULIRGs as well as an extrapolation for the full ULIRG source population. In addition, constraints are provided on models predicting neutrino emission from ULIRGs.
