Search for Galactic core-collapse supernovae in a decade of data taken with the IceCube Neutrino Observatory
Creators: name: Abbasi, R.
name: Ackermann, M.
name: Adams, J.
name: Agarwalla, S. K.
name: Aguilar, J. A.
name: Ahlers, M.
name: Alameddine, J. M.
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name: Barwick, S. W.
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name: Butterfield, D.
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name: Chattopadhyay, S.
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name: Coppin, P.
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name: Countryman, S.
name: Cowen, D. F.
name: Dave, P.
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name: DeLaunay, J. J.
name: Delgado, D.
name: Deng, S.
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name: Desai, A.
name: Desiati, P.
name: de Vries, K. D.
name: de Wasseige, G.
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name: Diaz, A.
name: Díaz-Vélez, J. C.
name: Dittmer, M.
name: Domi, A.
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name: Elsässer, D.
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name: Evenson, P. A.
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name: Ishihara, A.
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name: Japaridze, G. S.
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name: Lagunas Gualda, C.
name: Lamoureux, M.
name: Larson, M. J.
name: Latseva, S.
name: Lauber, F.
name: Lazar, J. P.
name: Lee, J. W.
name: Leonard DeHolton, K.
name: Leszczyńska, A.
name: Lincetto, M.
name: Liu, Q. R.
name: Liubarska, M.
name: Lohfink, E.
name: Love, C.
name: Lozano Mariscal, C. J.
name: Lu, L.
name: Lucarelli, F.
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name: Nisa, M. U.
name: Noell, A.
name: Novikov, A.
name: Nowicki, S. C.
name: Pollmann, A. Obertacke
name: O'Dell, V.
name: Oehler, M.
name: Oeyen, B.
name: Olivas, A.
name: Orsoe, R.
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name: O'Sullivan, E.
name: Pandya, H.
name: Park, N.
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name: Paudel, E. N.
name: Paul, L.
name: de los Heros, C. Pérez
name: Peterson, J.
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name: Rodriguez, M. Prado
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name: Przybylski, G. T.
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name: Rack-Helleis, J.
name: Rawlins, K.
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name: Reusch, S.
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name: Robertson, S.
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name: Tosi, D.
name: Trettin, A.
name: Tung, C. F.
name: Turcotte, R.
name: Twagirayezu, J. P.
name: Ty, B.
name: Unland Elorrieta, M. A.
name: Upadhyay, A. K.
name: Upshaw, K.
name: Valtonen-Mattila, N.
name: Vandenbroucke, J.
name: van Eijndhoven, N.
name: Vannerom, D.
name: van Santen, J.
name: Vara, J.
name: Veitch-Michaelis, J.
name: Venugopal, M.
name: Vereecken, M.
name: Verpoest, S.
name: Veske, D.
name: Vijai, A.
name: Walck, C.
name: Weaver, C.
name: Weigel, P.
name: Weindl, A.
name: Weldert, J.
name: Wendt, C.
name: Werthebach, J.
name: Weyrauch, M.
name: Whitehorn, N.
name: Wiebusch, C. H.
name: Willey, N.
name: Williams, D. R.
name: Wolf, A.
name: Wolf, M.
name: Wrede, G.
name: Xu, X. W.
name: Yanez, J. P.
name: Yildizci, E.
name: Yoshida, S.
name: Young, R.
name: Yu, F.
name: Yu, S.
name: Yuan, T.
name: Zhang, Z.
name: Zhelnin, P.
name: IceCube Collaboration
Publisher: name: Deutsches Elektronen-Synchrotron, DESY, Hamburg
Year: 2023
Subjects: neutrino, burst
neutrino, luminosity
mass, solar
neutrino, oscillation
neutrino, production
supernova, luminosity
neutrino, effect
collapse
IceCube
observatory
galaxy
star
black hole
O(10)
energy spectrum
conservation law
cloud

description: The IceCube Neutrino Observatory has been continuously taking data to search for O(0.5-10) s long neutrino bursts since 2007. Even if a Galactic core-collapse supernova is optically obscured or collapses to a black hole instead of exploding, it will be detectable via the O(10) MeV neutrino burst emitted during the collapse. We discuss a search for such events covering the time between April 17, 2008 and December 31, 2019. Considering the average data taking and analysis uptime of 91.7% after all selection cuts, this is equivalent to 10.735 years of continuous data taking. In order to test the most conservative neutrino production scenario, the selection cuts were optimized for a model based on a 8.8 solar mass progenitor collapsing to an O-Ne-Mg core. Conservative assumptions on the effects of neutrino oscillations in the exploding star were made. The final selection cut was set to ensure that the probability to detect such a supernova within the Milky Way exceeds 99%. No such neutrino burst was found in the data after performing a blind analysis. Hence, a 90% C.L. upper limit on the rate of core-collapse supernovae out to distances of ~ 25kpc was determined to be 0.23/yr. For the more distant Magellanic Clouds, only high neutrino luminosity supernovae will be detectable by IceCube, unless external information on the burst time is available. We determined a model-independent limit by parameterizing the dependence on the neutrino luminosity and the energy spectrum.