دورية أكاديمية

Searching for High-energy Neutrino Emission from Galaxy Clusters with IceCube

التفاصيل البيبلوغرافية
العنوان: Searching for High-energy Neutrino Emission from Galaxy Clusters with IceCube
المؤلفون: Abbasi, R., Ackermann, Markus, Anderson, T., Friedman, E., Fritz, A., Fürst, P., Gaisser, T. K., Gallagher, J., Ganster, E., Garcia, A., Garrappa, Simone, Gerhardt, L., Ghadimi, A., Anton, G., Glaser, C., Glauch, T., Glüsenkamp, T., Goehlke, N., Gonzalez, J. G., Goswami, S., Grant, D., Grégoire, T., Griswold, S., Günther, C., Argüelles, C., Gutjahr, P., Haack, C., Hallgren, A., Halliday, R., Halve, L., Halzen, F., Hamdaoui, H., Ha Minh, M., Hanson, K., Hardin, J., Ashida, Y., Harnisch, A. A., Hatch, P., Haungs, A., Helbing, K., Hellrung, J., Henningsen, F., Hettinger, E. C., Heuermann, L., Hickford, S., Hignight, J., Athanasiadou, Sofia, Hill, C., Hill, G. C., Hoffman, K. D., Hoshina, K., Hou, W., Huber, M., Huber, T., Hultqvist, K., Hünnefeld, M., Hussain, R., Axani, S., Hymon, K., In, S., Iovine, N., Ishihara, A., Jansson, M., Japaridze, G. S., Jeong, M., Jin, M., Jones, B. J. P., Kang, D., Bai, X., Kang, W., Kang, X., Kappes, A., Kappesser, D., Kardum, L., Karg, T., Karl, M., Karle, A., Katz, U., Kauer, M., Balagopal V., A., Kelley, J. L., Kheirandish, A., Kin, K., Kiryluk, J., Klein, S. R., Kochocki, A., Koirala, R., Kolanoski, H., Kontrimas, T., Köpke, L., Baricevic, M., Kopper, C., Kopper, S., Koskinen, D. J., Koundal, P., Kovacevich, M., Kowalski, M., Kozynets, T., Krupczak, E., Kun, E., Kurahashi, N., Barwick, S. W., Lad, Neha Navnitkumar, Gualda, C. Lagunas, Larson, M. J., Lauber, F., Lazar, J. P., Lee, J. W., Leonard, K., Leszczyńska, A., Lincetto, M., Liu, Q. R., Adams, J., Basu, V., Liubarska, M., Lohfink, E., Mariscal, C. J. Lozano, Lu, L., Lucarelli, F., Ludwig, A., Luszczak, W., Lyu, Y., Ma, Wing Yan, Madsen, J., Bay, R., Mahn, K. B. M., Makino, Y., Mancina, S., Sainte, W. Marie, Mariş, I. C., Martinez-Soler, I., Maruyama, R., McCarthy, S., McElroy, T., McNally, F., Beatty, J. J., Mead, J. V., Meagher, K., Mechbal, Sarah, Medina, A., Meier, M., Meighen-Berger, S., Merckx, Y., Micallef, J., Mockler, D., Montaruli, T., Becker, K.-H., Moore, R. W., Morse, R., Moulai, M., Mukherjee, T., Naab, Richard, Nagai, R., Naumann, U., Necker, Jannis David, Nguyen, L. V., Nguy, Becker Tjus, J., Niederhausen, H., Nisa, M. U., Nowicki, S. C., Obertacke Pollmann, A., Oehler, M., Oeyen, B., Olivas, A., Osborn, J., O'Sullivan, E., Pandya, H., Beise, J., Pankova, D. V., Park, N., Parker, G. K., Paudel, E. N., Paul, L., Pérez de los Heros, C., Peters, L., Peterson, J., Philippen, S., Pieper, S., Bellenghi, C., Pizzuto, A., Plum, M., Popovych, Y., Porcelli, A., Rodriguez, M. Prado, Pries, B., Przybylski, G. T., Raab, C., Rack-Helleis, J., Raissi, A., Benda, S., Rameez, M., Rawlins, K., Rea, I. C., Rechav, Z., Rehman, A., Reichherzer, P., Renzi, G., Resconi, E., Reusch, Simeon, Rhode, W., BenZvi, S., Richman, M., Riedel, B., Roberts, E. J., Robertson, S., Roellinghoff, G., Rongen, M., Rott, C., Ruhe, T., Ryckbosch, D., Cantu, D. Rysewyk, Berley, D., Safa, I., Saffer, J., Salazar-Gallegos, D., Sampathkumar, P., Herrera, S. E. Sanchez, Sandrock, A., Santander, M., Sarkar, S., Satalecka, K., Schaufel, M., Aguilar, J. A., Bernardini, E., Schieler, H., Schindler, S., Schmidt, T., Schneider, A., Schneider, J., Schröder, F. G., Schumacher, L., Schwefer, G., Sclafani, S., Seckel, D., Besson, D. Z., Seunarine, S., Sharma, A., Shefali, S., Shimizu, N., Silva, M., Skrzypek, B., Smithers, B., Snihur, R., Soedingrekso, J., Sogaard, A., Binder, G., Soldin, D., Spannfellner, C., Spiczak, G. M., Spiering, Christian, Stamatikos, M., Stanev, T., Stein, Robert, Stettner, J., Stezelberger, T., Stürwald, T., Bindig, D., Stuttard, T., Sullivan, G. W., Taboada, I., Ter-Antonyan, S., Thompson, W. G., Thwaites, J., Tilav, S., Tollefson, K., Tönnis, C., Toscano, S., Blaufuss, E., Tosi, D., Trettin, Alexander, Tselengidou, M., Tung, C. F., Turcati, A., Turcotte, R., Twagirayezu, J. P., Ty, B., Unland Elorrieta, M. A., Unland Elorrieta, M., Blot, Summer, Upshaw, K., Valtonen-Mattila, N., Vandenbroucke, J., van Eijndhoven, N., Vannerom, D., Santen, Jakob van, Veitch-Michaelis, J., Verpoest, S., Walck, C., Wang, W., Bontempo, F., Watson, T. B., Weaver, C., Weigel, P., Weindl, A., Weldert, J., Wendt, C., Werthebach, J., Weyrauch, M., Whitehorn, N., Wiebusch, C. H., Book, J. Y., Willey, N., Williams, D. R., Wolf, M., Wrede, G., Wulff, J., Xu, X. W., Yanez, J. P., Yildizci, E., Yoshida, S., Yu, S., Borowka, J., Yuan, T., Zhang, Z., Zhelnin, P., IceCube Collaboration, Böser, S., Ahlers, M., Botner, O., Böttcher, J., Bourbeau, E., Bradascio, Federica, Braun, J., Brinson, B., Bron, S., Brostean-Kaiser, Jannes, Burley, R. T., Busse, R. S., Ahrens, M., Campana, M. A., Carnie-Bronca, E. G., Chen, C., Chen, Z., Chirkin, D., Choi, K., Clark, B. A., Clark, K., Classen, L., Coleman, A., Alameddine, J. M., Collin, G. H., Connolly, A., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dappen, C., Dave, P., De Clercq, C., Alves, A. A., DeLaunay, J. J., Delgado López, D., Dembinski, H., Deoskar, K., Desai, A., Desiati, P., de Vries, K. D., de Wasseige, G., DeYoung, T., Diaz, A., Amin, N. M., Díaz-Vélez, J. C., Dittmer, M., Dujmovic, H., DuVernois, M. A., Ehrhardt, T., Eller, P., Engel, R., Erpenbeck, H., Evans, J., Evenson, P. A., Andeen, K., Fan, K. L., Fazely, A. R., Fedynitch, A., Feigl, N., Fiedlschuster, S., Fienberg, A. T., Finley, C., Fischer, Leander, Fox, D., Franckowiak, A.
المصدر: The astrophysical journal / 2 938(2), L11 (2022). doi:10.3847/2041-8213/ac966b
بيانات النشر: Univ.
سنة النشر: 2022
المجموعة: DESY Publication Database (PUBDB)
مصطلحات موضوعية: info:eu-repo/classification/ddc/520, galaxy: cluster, neutrino: flux, neutrino: secondary, IceCube, stacking, muon, gamma ray, acceleration, observatory, redshift, gas, site, tracks, UHE, accretion, cosmic radiation, Planck, TeV
جغرافية الموضوع: DE
الوصف: Galaxy clusters have the potential to accelerate cosmic rays (CRs) to ultrahigh energies via accretion shocks or embedded CR acceleration sites. The CRs with energies below the Hillas condition will be confined within the cluster and eventually interact with the intracluster medium gas to produce secondary neutrinos and gamma rays. Using 9.5 yr of muon neutrino track events from the IceCube Neutrino Observatory, we report the results of a stacking analysis of 1094 galaxy clusters with masses ≳10$^{14}$ M $_{⊙}$ and redshifts between 0.01 and ∼1 detected by the Planck mission via the Sunyaev–Zel’dovich effect. We find no evidence for significant neutrino emission and report upper limits on the cumulative unresolved neutrino flux from massive galaxy clusters after accounting for the completeness of the catalog up to a redshift of 2, assuming three different weighting scenarios for the stacking and three different power-law spectra. Weighting the sources according to mass and distance, we set upper limits at a 90% confidence level that constrain the flux of neutrinos from massive galaxy clusters (≳10$^{14}$ M $_{⊙}$) to be no more than 4.6% of the diffuse IceCube observations at 100 TeV, assuming an unbroken E $^{−2.5}$ power-law spectrum.
نوع الوثيقة: article in journal/newspaper
اللغة: English
العلاقة: info:eu-repo/semantics/altIdentifier/wos/WOS:000868883400001; info:eu-repo/semantics/altIdentifier/issn/1538-4357; info:eu-repo/semantics/altIdentifier/issn/2041-8205; info:eu-repo/semantics/altIdentifier/issn/2041-8213; info:eu-repo/semantics/altIdentifier/issn/0004-637X; info:eu-repo/semantics/altIdentifier/arxiv/arXiv:2206.02054; https://bib-pubdb1.desy.de/record/491411Test; https://bib-pubdb1.desy.de/search?p=id:%22PUBDB-2023-00135%22Test
الإتاحة: https://doi.org/10.3847/2041-8213/ac966bTest
https://doi.org/10.3204/PUBDB-2023-00135Test
https://bib-pubdb1.desy.de/record/491411Test
https://bib-pubdb1.desy.de/search?p=id:%22PUBDB-2023-00135%22Test
حقوق: info:eu-repo/semantics/openAccess
رقم الانضمام: edsbas.76D0DDF6
قاعدة البيانات: BASE