학술논문

All-Sky Search for Transient Astrophysical Neutrino Emission with 10 Years of IceCube Cascade Events
Document Type
Working Paper
Author
Abbasi, R.Ackermann, M.Adams, J.Agarwalla, S. K.Aguilar, J. A.Ahlers, M.Alameddine, J. M.Amin, N. M.Andeen, K.Anton, G.Argüelles, C.Ashida, Y.Athanasiadou, S.Ausborm, L.Axani, S. N.Bai, X.V., A. BalagopalBaricevic, M.Barwick, S. W.Basu, V.Bay, R.Beatty, J. J.Tjus, J. BeckerBeise, J.Bellenghi, C.Benning, C.BenZvi, S.Berley, D.Bernardini, E.Besson, D. Z.Blaufuss, E.Blot, S.Bontempo, F.Book, J. Y.Meneguolo, C. BoscoloBöser, S.Botner, O.Böttcher, J.Braun, J.Brinson, B.Brostean-Kaiser, J.Brusa, L.Burley, R. T.Busse, R. S.Butterfield, D.Campana, M. A.Carloni, K.Carnie-Bronca, E. G.Chattopadhyay, S.Chau, N.Chen, C.Chen, Z.Chirkin, D.Choi, S.Clark, B. A.Coleman, A.Collin, G. H.Connolly, A.Conrad, J. M.Coppin, P.Correa, P.Cowen, D. F.Dave, P.De Clercq, C.DeLaunay, J. J.Delgado, D.Deng, S.Deoskar, K.Desai, A.Desiati, P.de Vries, K. D.de Wasseige, G.DeYoung, T.Diaz, A.Díaz-Vélez, J. C.Dittmer, M.Domi, A.Dujmovic, H.DuVernois, M. A.Ehrhardt, T.Eimer, A.Eller, P.Ellinger, E.Mentawi, S. ElElsässer, D.Engel, R.Erpenbeck, H.Evans, J.Evenson, P. A.Fan, K. L.Fang, K.Farrag, K.Fazely, A. R.Fedynitch, A.Feigl, N.Fiedlschuster, S.Finley, C.Fischer, L.Fox, D.Franckowiak, A.Fürst, P.Gallagher, J.Ganster, E.Garcia, A.Gerhardt, L.Ghadimi, A.Glaser, C.Glauch, T.Glüsenkamp, T.Gonzalez, J. G.Grant, D.Gray, S. J.Gries, O.Griffin, S.Griswold, S.Groth, K. M.Günther, C.Gutjahr, P.Ha, C.Haack, C.Hallgren, A.Halliday, R.Halve, L.Halzen, F.Hamdaoui, H.Minh, M. HaHandt, M.Hanson, K.Hardin, J.Harnisch, A. A.Hatch, P.Haungs, A.Häußler, J.Helbing, K.Hellrung, J.Hermannsgabner, J.Heuermann, L.Heyer, N.Hickford, S.Hidvegi, A.Hill, C.Hill, G. C.Hoffman, K. D.Hori, S.Hoshina, K.Hou, W.Huber, T.Hultqvist, K.Hünnefeld, M.Hussain, R.Hymon, K.In, S.Ishihara, A.Jacquart, M.Janik, O.Jansson, M.Japaridze, G. S.Jeong, M.Jin, M.Jones, B. J. P.Kamp, N.Kang, D.Kang, W.Kang, X.Kappes, A.Kappesser, D.Kardum, L.Karg, T.Karl, M.Karle, A.Katil, A.Katz, U.Kauer, M.Kelley, J. L.Zathul, A. KhateeKheirandish, A.Kiryluk, J.Klein, S. R.Kochocki, A.Koirala, R.Kolanoski, H.Kontrimas, T.Köpke, L.Kopper, C.Koskinen, D. J.Koundal, P.Kovacevich, M.Kowalski, M.Kozynets, T.Krishnamoorthi, J.Kruiswijk, K.Krupczak, E.Kumar, A.Kun, E.Kurahashi, N.Lad, N.Gualda, C. LagunasLamoureux, M.Larson, M. J.Latseva, S.Lauber, F.Lazar, J. P.Lee, J. W.DeHolton, K. LeonardLeszczyńska, A.Lincetto, M.Liu, Y.Liubarska, M.Lohfink, E.Love, C.Mariscal, C. J. LozanoLu, L.Lucarelli, F.Luszczak, W.Lyu, Y.Madsen, J.Magnus, E.Mahn, K. B. M.Makino, Y.Manao, E.Mancina, S.Sainte, W. MarieMariş, I. C.Marka, S.Marka, Z.Marsee, M.Martinez-Soler, I.Maruyama, R.Mayhew, F.McElroy, T.McNally, F.Mead, J. V.Meagher, K.Mechbal, S.Medina, A.Meier, M.Merckx, Y.Merten, L.Micallef, J.Mitchell, J.Montaruli, T.Moore, R. W.Morii, Y.Morse, R.Moulai, M.Mukherjee, T.Naab, R.Nagai, R.Nakos, M.Naumann, U.Necker, J.Negi, A.Neumann, M.Niederhausen, H.Nisa, M. U.Noell, A.Novikov, A.Nowicki, S. C.Pollmann, A. ObertackeO'Dell, V.Oeyen, B.Olivas, A.Orsoe, R.Osborn, J.O'Sullivan, E.Pandya, H.Park, N.Parker, G. K.Paudel, E. N.Paul, L.Heros, C. Pérez de losPeterson, J.Philippen, S.Pizzuto, A.Plum, M.Pontén, A.Popovych, Y.Rodriguez, M. PradoPries, B.Procter-Murphy, R.Przybylski, G. T.Raab, C.Rack-Helleis, J.Rawlins, K.Rechav, Z.Rehman, A.Reichherzer, P.Resconi, E.Reusch, S.Rhode, W.Riedel, B.Rifaie, A.Roberts, E. J.Robertson, S.Rodan, S.Roellinghoff, G.Rongen, M.Rosted, A.Rott, C.Ruhe, T.Ruohan, L.Ryckbosch, D.Safa, I.Saffer, J.Salazar-Gallegos, D.Sampathkumar, P.Herrera, S. E. SanchezSandrock, A.Santander, M.Sarkar, S.Savelberg, J.Savina, P.Schaufel, M.Schieler, H.Schindler, S.Schlickmann, L.Schlüter, B.Schlüter, F.Schmeisser, N.Schmidt, T.Schneider, J.Schröder, F. G.Schumacher, L.Sclafani, S.Seckel, D.Seikh, M.Seunarine, S.Shah, R.Shefali, S.Shimizu, N.Silva, M.Skrzypek, B.Smithers, B.Snihur, R.Soedingrekso, J.Søgaard, A.Soldin, D.Soldin, P.Sommani, G.Spannfellner, C.Spiczak, G. M.Spiering, C.Stamatikos, M.Stanev, T.Stezelberger, T.Stürwald, T.Stuttard, T.Sullivan, G. W.Taboada, I.Ter-Antonyan, S.Thiesmeyer, M.Thompson, W. G.Thwaites, J.Tilav, S.Tollefson, K.Tönnis, C.Toscano, S.Tosi, D.Trettin, A.Tung, C. F.Turcotte, R.Twagirayezu, J. P.Elorrieta, M. A. UnlandUpadhyay, A. K.Upshaw, K.Vaidyanathan, A.Valtonen-Mattila, N.Vandenbroucke, J.van Eijndhoven, N.Vannerom, D.van Santen, J.Vara, J.Veitch-Michaelis, J.Venugopal, M.Vereecken, M.Verpoest, S.Veske, D.Vijai, A.Walck, C.Wang, Y.Weaver, C.Weigel, P.Weindl, A.Weldert, J.Wen, A. Y.Wendt, C.Werthebach, J.Weyrauch, M.Whitehorn, N.Wiebusch, C. H.Williams, D. R.Witthaus, L.Wolf, A.Wolf, M.Wrede, G.Xu, X. W.Yanez, J. P.Yildizci, E.Yoshida, S.Young, R.Yu, S.Yuan, T.Zhang, Z.Zhelnin, P.Zilberman, P.Zimmerman, M.
Source
Subject
Astrophysics - High Energy Astrophysical Phenomena
High Energy Physics - Experiment
Language
Abstract
We present the results of a time-dependent search for neutrino flares in data collected by IceCube between May 2011 and 2021. This data set contains cascade-like events originating from charged-current electron neutrino and tau neutrino interactions and all-flavor neutral-current interactions. IceCube's previous all-sky searches for neutrino flares used data sets consisting of track-like events originating from charged-current muon neutrino interactions. The cascade data sets are statistically independent of the track data sets and provide a new opportunity to observe the transient all-sky landscape. This search uses the spatial, temporal, and energy information of the cascade-like events to conduct searches for the most statistically significant neutrino flares in the northern and southern skies. No statistically significant time-dependent neutrino emission was observed. For the most statistically significant location in the northern sky, $p_\mathrm{global} =$ 0.71, and in the southern sky, $p_\mathrm{global} =$ 0.51. These results are compatible with the background hypothesis. Assuming an E$^{-2.53}$ spectrum from the diffuse astrophysical neutrino flux as measured with cascades, these results are used to calculate upper limits at the 90\% confidence level on neutrino flares of varying duration and constrain the contribution of these flares to the diffuse astrophysical neutrino flux. These constraints are independent of a specified class of astrophysical objects and show that multiple unresolved transient sources may contribute to the diffuse astrophysical neutrino flux.
Comment: Submitted to The Astrophysical Journal