Search for neutrino emission from cores of active galactic nuclei

Abbasi, Rasha; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alameddine, Jean-Marco; Alispach, Cyril Martin; Alves, A. A.; Amin, Najia Moureen Binte; Andeen, K.; Anderson, Tyler; Anton, Gisela; Argüelles, C.; Ashida, Yosuke; Axani, Spencer; Bai, X.; A., Balagopal V.,; Barbano, Anastasia Maria; Barwick, S. W.; Bastian, Benjamin; Basu, Vedant; Baur, S.; Bay, R.; Beatty, J. J.; Becker, Karl‐Heinz; Tjus, Julia Becker; Bellenghi, Chiara; BenZvi, S.; Berley, D.; Bernardini, E.; Besson, D.; Binder, G.; Bindig, D.; Blaufuss, E.; Blot, Summer; Boddenberg, Matthias; Bontempo, Federico; Borowka, Jürgen; Böser, S.; Botner, O.; Böttcher, Jakob; Bourbeau, Etienne; Bradascio, Federica; Braun, J.; Brinson, Bennett; Bron, S.; Brostean-Kaiser, Jannes; Browne, Sally-Ann; Burgman, A.; Burley, Ryan; Busse, Raffaela; Campana, Michael; Carnie-Bronca, Erin; Chen, C.; Chen, Z.; Chirkin, D.; Choi, Ki‐Young; Clark, Brian; Clark, K.; Classen, L.; Coleman, Alan; Collin, Gabriel; Conrad, J. M.; Coppin, Paul; Correa, Pablo; Cowen, D. F.; Cross, R.; Dappen, Christian; Dave, Pranav; Clercq, C. De; DeLaunay, James; López, D. Delgado; Dembinski, H.-P.; Deoskar, Kunal; Desai, Abhishek; Desiati, P.; Vries, Krijn de; Wasseige, Gwenhaël de; With, M. de; DeYoung, T.; Dı́az, A.; Díaz–Vélez, Juan Carlos; Dittmer, Markus; Dujmović, Hrvoje; Dunkman, M.; DuVernois, Michael; Dvorak, Emily; Ehrhardt, Thomas; Eller, P.; Engel, R.; Erpenbeck, Hannah; Evans, John; Evenson, P. A.; Fan, Kwok Lung; Fazely, A. R.; Fedynitch, Anatoli; Feigl, Nora; Fiedlschuster, Sebastian; Fienberg, Aaron; Filimonov, K.; Finley, C.; Fischer, Leander; Fox, D. B.; Franckowiak, A.; Friedman, E.; Fritz, A.; Fürst, Philipp; Gaisser, T. K.; Gallagher, J.; Ganster, Erik; García, Alfonso; Garrappa, S.; Gerhardt, L.; Ghadimi, Ava; Gläser, Christian; Glauch, Theo; Glüsenkamp, T.; González, J. G.; Goswami, Sreetama; Grant, D.; Grégoire, T.; Griswold, Spencer; Günther, C.; Gutjahr, Pascal; Haack, Christian; Hallgren, A.; Halliday, R.; Halve, L.; Halzen, F.; Minh, Martin Ha; Hanson, K.; Hardin, John; Harnisch, Alexander; Haungs, A.; Hebecker, D.; Helbing, K.; Henningsen, Felix; Hettinger, Emma C.; Hickford, S.; Hignight, J.; Hill, Colton; Hill, G. C.; Hoffman, K. D.; Hoffmann, R.; Hokanson-Fasig, B.; Hoshina, K.; Huang, F.; Huber, Matthías; Huber, Thomas; Hultqvist, K.; Hünnefeld, Mirco; Hussain, Raamis; Hymon, Karolin; In, S.; Iovine, N.; Ishihara, A.; Jansson, Matti; Japaridze, G. S.; Jeong, Minjin; Jin, M.; Jones, B. J. P.; Kang, D.; Kang, Woosik; Kang, X.; Kappes, A.; Kappesser, David; Kardum, Leonora; Karg, T.; Karl, Martina; Karle, A.; Katz, U.; Kauer, M.; Kellermann, Moritz; Kelley, J. L.; Kheirandish, Ali; Kin, Ken'ichi; Kintscher, T.; Kiryluk, J.; Klein, S. R.; Koirala, R.; Kolanoski, H.; Kontrimas, Tomas; Köpke, L.; Kopper, C.; Kopper, S.; Koskinen, D. J.; Koundal, Paras; Kovacevich, Michael; Kowalski, M.; Kozynets, Tetiana; Kun, Emma; Kurahashi, N.; Lad, Nisha Nareshbhai; Gualda, Cristina Lagunas; Lanfranchi, J. L.; Larson, M. J.; Lauber, Frederik Hermann; Lazar, Jeffrey; Lee, J. W.; Leonard, K.; Leszczyńska, Agnieszka; Li, Y.; Lincetto, Massimiliano; Liu, Q. R.; Liubarska, Maria; Lohfink, Elisa; Mariscal, Cristian Jesús Lozano; Lu, Lina; Lucarelli, F.; Ludwig, Andrew; Luszczak, William; Lyu, Y.; Ma, W. Y.; Madsen, J.; Mahn, Kendall; Makino, Yuya; Mancina, Sarah; Maris, Ioana Codrina; Martinez-Soler, Ivan; Maruyama, R.; Mase, K.; McElroy, Thomas; McNally, F.; Mead, James Vincent; Meagher, K.; Mechbal, Sarah; Medina, Andrés; Meier, Maximilian; Meighen-Berger, Stephan; Micallef, Jessie; Mockler, D.; Montaruli, T.; Moore, R. W.; Morse, R.; Moulai, Marjon; Naab, Richard; Nagai, Ryo; Naumann, Uwe; Necker, Jannis; Nguyen, Le Viet; Niederhausen, H.; Nisa, Mehr; Nowicki, S. C.; Pollmann, A. Obertacke; Oehler, Marie; Oeyen, Bob; Olivas, A.; O’Sullivan, Erin; Pandya, Hershal; Pankova, D. V.; Park, N.; Parker, Grant; Paudel, Ek Narayan; Paul, Larissa; Heros, C. Pérez de los; Peters, Lilly; Peterson, Josh; Philippen, Saskia; Pieper, Sarah; Pittermann, Martin; Pizzuto, A.; Plum, M.; Popovych, Yuriy; Porcelli, A.; Rodriguez, Maria Prado; Price, P. B.; Pries, Brandom; Przybylski, G. T.; Raab, Christoph; Raissi, Amirreza; Rameez, M.; Rawlins, K.; Rea, Immacolata Carmen; Rehman, Abdul; Reichherzer, Patrick; Reimann, R.; Renzi, Giovanni; Resconi, E.; Reusch, Simeon; Rhode, W.; Richman, M.; Riedel, Benedikt; Roberts, E. J.; Robertson, Sally; Roellinghoff, Gerrit; Rongen, Martin; Rott, C.; Ruhe, T.; Ryckbosch, D.; Cantu, Devyn Rysewyk; Safa, Ibrahim; Saffer, Julian; Herrera, S. E. Sanchez; Sandrock, Alexander; Sandroos, J.; Santander, M.; Sarkar, Sourav; Satalecka, K.; Schaufel, Merlin; Schieler, H.; Schindler, Sebastian; Schmidt, T.; Schneider, A.; Schneider, Judith; Schröder, Frank G.; Schumacher, Lisa Johanna; Schwefer, Georg; Sclafani, S.; Seckel, D.; Seunarine, S.; Sharma, Ankur; Shefali, S.; Silva, M.; Skrzypek, Barbara; Smithers, B.; Snihur, R.; Soedingrekso, Jan; Soldin, D.; Spannfellner, Christian; Spiczak, G. M.; Spiering, C.; Stachurska, J.; Stamatikos, M.; Stanev, T.; Stein, R.; Stettner, J.; Steuer, A.; Stezelberger, T.; Stürwald, Timo; Stuttard, Thomas; Sullivan, G. W.; Taboada, I.; Ter–Antonyan, S.; Tilav, S.; Tischbein, Franziska; Tollefson, K.; Tönnis, Christoph; Toscano, S.; Tosi, D.; Trettin, Alexander; Tselengidou, M.; Tung, Chunfai; Turcati, A.; Turcotte, Roxanne; Turley, C. F.; Twagirayezu, Jean Pierre; Ty, Bunheng; Elorrieta, M. A. Unland; Valtonen-Mattila, Nora; Vandenbroucke, J.; Eijndhoven, N. van; Vannerom, D.; Santen, J. V.; Verpoest, Stef; Walck, C.; Watson, Timothyblake; Weaver, Ch.; Weigel, Philip; Weindl, A.; Weiss, Matthew J.; Weldert, Jan; Wendt, C.; Werthebach, Johannes; Weyrauch, Mark; Whitehorn, N.; Wiebusch, Christopher; Williams, D. R.; Wolf, M.; Woschnagg, K.; Wrede, Gerrit; Wulff, Johan; Xu, X. W.; Yañez, J. P.; Yoshida, Shigeru; Yu, Shiqi; Yuan, Tianlu; Zhang, Z.; Zhelnin, Pavel

doi:10.1103/physrevd.106.022005

Cited by 22 publications

(9 citation statements)

References 69 publications

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“…This scrambling method is well established and preserves the structure in energy and decl. (see, e.g., Braun et al 2008;Abbasi et al 2022aAbbasi et al , 2022bAbbasi et al , 2022c.…”

Section: Analysis Methodsmentioning

confidence: 99%

Constraining High-energy Neutrino Emission from Supernovae with IceCube

Abbasi

Ackermann

Adams

et al. 2023

ApJL

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Core-collapse supernovae are a promising potential high-energy neutrino source class. We test for correlation between seven years of IceCube neutrino data and a catalog containing more than 1000 core-collapse supernovae of types IIn and IIP and a sample of stripped-envelope supernovae. We search both for neutrino emission from individual supernovae as well as for combined emission from the whole supernova sample, through a stacking analysis. No significant spatial or temporal correlation of neutrinos with the cataloged supernovae was found. All scenarios were tested against the background expectation and together yield an overall p-value of 93%; therefore, they show consistency with the background only. The derived upper limits on the total energy emitted in neutrinos are 1.7 × 1048 erg for stripped-envelope supernovae, 2.8 × 1048 erg for type IIP, and 1.3 × 1049 erg for type IIn SNe, the latter disfavoring models with optimistic assumptions for neutrino production in interacting supernovae. We conclude that stripped-envelope supernovae and supernovae of type IIn do not contribute more than 14.6% and 33.9%, respectively, to the diffuse neutrino flux in the energy range of about [ 103–105] GeV, assuming that the neutrino energy spectrum follows a power-law with an index of −2.5. Under the same assumption, we can only constrain the contribution of type IIP SNe to no more than 59.9%. Thus, core-collapse supernovae of types IIn and stripped-envelope supernovae can both be ruled out as the dominant source of the diffuse neutrino flux under the given assumptions.

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“…This scrambling method is well established and preserves the structure in energy and decl. (see, e.g., Braun et al 2008;Abbasi et al 2022aAbbasi et al , 2022bAbbasi et al , 2022c.…”

Section: Analysis Methodsmentioning

confidence: 99%

Constraining High-energy Neutrino Emission from Supernovae with IceCube

Abbasi

Ackermann

Adams

et al. 2023

ApJL

Self Cite

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“…[36]). In addition, a correlation analysis between neutrino emission and a large sample of active galaxies finds that the IceCube data are compatible with a predominant production of extragalactic neutrinos in this population [37]. Interestingly, a related transient phenomenon, the tidal disruption of stars in the gravitational field of otherwise quiet supermassive black holes that lead to the formation of temporary accretion disks, have also been linked to the emission of high-energy neutrinos [38,39].…”

Section: (D) Astrophysical Observationsmentioning

confidence: 88%

Searches for beyond-standard-model physics with astroparticle physics instruments

Ackermann,

Helbing

2023

Phil. Trans. R. Soc. A.

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Many instruments for astroparticle physics are primarily geared towards multi-messenger astrophysics, to study the origin of cosmic rays and to understand high-energy astrophysical processes. Since these instruments observe the Universe at extreme energies and in kinematic ranges not accessible at accelerators these experiments provide also unique and complementary opportunities to search for particles and physics beyond the standard model of particle physics. In particular, the reach of IceCube, Fermi and KATRIN to search for and constrain Dark Matter, Axions, heavy Big Bang relics, sterile neutrinos and Lorentz invariance violation will be discussed. The contents of this article are based on material presented at the Humboldt–Kolleg ‘Clues to a mysterious Universe—exploring the interface of particle, gravity and quantum physics’ in June 2022. This article is part of the theme issue ‘The particle-gravity frontier’.

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“…The contributions of known source populations to the total cosmic neutrino flux detected by IceCube, constrained through stacking analyses 209,210 , are the following: prompt phase of GRBs (< 1%) 196 , blazars (< 17%) 211 , non-jetted TDEs (< 26%) and jetted TDEs (< 1%) 212 , ultraluminous infrared galaxies (< 10%) 213 , Galactic sources (< 14%) 214 , SNe IIn (< 55.2%), SNe IIP (< 79.6%) and SNe Ibc (< 28.6%) 195 , microquasars (< 7.3%) 193 , galaxy clusters out to redshift 2 (<5%) 215 , and radio galaxies (< 30%) 216 . Recently, a 2.6σ excess of neutrinos from the directions of non-jetted AGN weighted by their soft X-ray flux has been reported 217 . If this is a genuine signal, it implies that 27% to 100% of neutrinos at 100 TeV come from non-jetted AGN.…”

Section: Constraints On Source Populationsmentioning

confidence: 99%

High-energy neutrino transients and the future of multi-messenger astronomy

Guépin¹,

Kotera²,

Oikonomou³

2022

Preprint

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The recent discovery of high-energy astrophysical neutrinos and first hints of coincident electromagnetic and neutrino emission herald the beginning of the era of multi-messenger astronomy. Due to their high power, transient sources are expected to supply a significant fraction of the observed energetic astroparticles, through enhanced particle acceleration and interactions. Here, we review theoretical expectations of neutrino emission from transient astrophysical sources and the current and upcoming experimental landscape, highlighting the most promising channels for discovery and specifying their detectability.

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Search for neutrino emission from cores of active galactic nuclei

Cited by 22 publications

References 69 publications

Constraining High-energy Neutrino Emission from Supernovae with IceCube

Constraining High-energy Neutrino Emission from Supernovae with IceCube

Searches for beyond-standard-model physics with astroparticle physics instruments

High-energy neutrino transients and the future of multi-messenger astronomy

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