IceCube sensitivity for low-energy neutrinos from nearby supernovae

This paper describes the response of the IceCube neutrino telescope located at the geographic south pole to outbursts of MeV neutrinos from the core collapse of nearby massive stars. IceCube was completed in December 2010 forming a lattice of 5160 photomultiplier tubes that monitor a volume of ~1 km...

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Main Authors:	Abbasi, R., Abdou, Y., Abu-Zayyad, T., Ackermann, M., Adams, J., Aguilar, J., Ahlers, M., Allen, M., Altmann, D., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S., Baum, V., Bay, R., Bazo Alba, J., Beattie, K., Beatty, J., Bechet, S., Becker, J., Becker, K., Benabderrahmane, M., Benzvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D., Bohm, C., Bose, D., Böser, S., Botner, O., Brown, A., Buitink, S., Caballero-Mora, K., Carson, Michael, Chirkin, D., Christy, B., Clevermann, F., Cohen, S., Colnard, C., Cowen, D., Cruz Silva, A., D'Agostino, M., Danninger, M., Daughhetee, J., Davis, J., De Clercq, C., Degner, T., Demirörs, L., Descamps, F., Desiati, P., De Vries-Uiterweerd, G., Deyoung, T., Díaz-Vélez, J., Dierckxsens, M., Dreyer, J., Dumm, J., Dunkman, M., Eisch, J., Ellsworth, R., Engdegård, O., Euler, S., Evenson, P., Fadiran, O., Fazely, A., Fedynitch, A., Feintzeig, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Fox, B., Franckowiak, A., Franke, R., Gaisser, T., Gallagher, J., Gerhardt, L., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Goodman, J., Góra, D., Grant, D., Griesel, T., Groß, A., Grullon, S.
Format:	Journal Article
Published:	2011
Online Access:	http://hdl.handle.net/20.500.11937/7122

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author	Abbasi, R. Abdou, Y. Abu-Zayyad, T. Ackermann, M. Adams, J. Aguilar, J. Ahlers, M. Allen, M. Altmann, D. Andeen, K. Auffenberg, J. Bai, X. Baker, M. Barwick, S. Baum, V. Bay, R. Bazo Alba, J. Beattie, K. Beatty, J. Bechet, S. Becker, J. Becker, K. Benabderrahmane, M. Benzvi, S. Berdermann, J. Berghaus, P. Berley, D. Bernardini, E. Bertrand, D. Besson, D. Bindig, D. Bissok, M. Blaufuss, E. Blumenthal, J. Boersma, D. Bohm, C. Bose, D. Böser, S. Botner, O. Brown, A. Buitink, S. Caballero-Mora, K. Carson, Michael Chirkin, D. Christy, B. Clevermann, F. Cohen, S. Colnard, C. Cowen, D. Cruz Silva, A. D'Agostino, M. Danninger, M. Daughhetee, J. Davis, J. De Clercq, C. Degner, T. Demirörs, L. Descamps, F. Desiati, P. De Vries-Uiterweerd, G. Deyoung, T. Díaz-Vélez, J. Dierckxsens, M. Dreyer, J. Dumm, J. Dunkman, M. Eisch, J. Ellsworth, R. Engdegård, O. Euler, S. Evenson, P. Fadiran, O. Fazely, A. Fedynitch, A. Feintzeig, J. Feusels, T. Filimonov, K. Finley, C. Fischer-Wasels, T. Fox, B. Franckowiak, A. Franke, R. Gaisser, T. Gallagher, J. Gerhardt, L. Gladstone, L. Glüsenkamp, T. Goldschmidt, A. Goodman, J. Góra, D. Grant, D. Griesel, T. Groß, A. Grullon, S.
author_facet	Abbasi, R. Abdou, Y. Abu-Zayyad, T. Ackermann, M. Adams, J. Aguilar, J. Ahlers, M. Allen, M. Altmann, D. Andeen, K. Auffenberg, J. Bai, X. Baker, M. Barwick, S. Baum, V. Bay, R. Bazo Alba, J. Beattie, K. Beatty, J. Bechet, S. Becker, J. Becker, K. Benabderrahmane, M. Benzvi, S. Berdermann, J. Berghaus, P. Berley, D. Bernardini, E. Bertrand, D. Besson, D. Bindig, D. Bissok, M. Blaufuss, E. Blumenthal, J. Boersma, D. Bohm, C. Bose, D. Böser, S. Botner, O. Brown, A. Buitink, S. Caballero-Mora, K. Carson, Michael Chirkin, D. Christy, B. Clevermann, F. Cohen, S. Colnard, C. Cowen, D. Cruz Silva, A. D'Agostino, M. Danninger, M. Daughhetee, J. Davis, J. De Clercq, C. Degner, T. Demirörs, L. Descamps, F. Desiati, P. De Vries-Uiterweerd, G. Deyoung, T. Díaz-Vélez, J. Dierckxsens, M. Dreyer, J. Dumm, J. Dunkman, M. Eisch, J. Ellsworth, R. Engdegård, O. Euler, S. Evenson, P. Fadiran, O. Fazely, A. Fedynitch, A. Feintzeig, J. Feusels, T. Filimonov, K. Finley, C. Fischer-Wasels, T. Fox, B. Franckowiak, A. Franke, R. Gaisser, T. Gallagher, J. Gerhardt, L. Gladstone, L. Glüsenkamp, T. Goldschmidt, A. Goodman, J. Góra, D. Grant, D. Griesel, T. Groß, A. Grullon, S.
author_sort	Abbasi, R.
building	Curtin Institutional Repository
collection	Online Access
description	This paper describes the response of the IceCube neutrino telescope located at the geographic south pole to outbursts of MeV neutrinos from the core collapse of nearby massive stars. IceCube was completed in December 2010 forming a lattice of 5160 photomultiplier tubes that monitor a volume of ~1 km 3 in the deep Antarctic ice for particle induced photons. The telescope was designed to detect neutrinos with energies greater than 100 GeV. Owing to subfreezing ice temperatures, the photomultiplier dark noise rates are particularly low. Hence IceCube can also detect large numbers of MeV neutrinos by observing a collective rise in all photomultiplier rates on top of the dark noise. With 2 ms timing resolution, IceCube can detect subtle features in the temporal development of the supernova neutrino burst. For a supernova at the galactic center, its sensitivity matches that of a background-free megaton-scale supernova search experiment. The sensitivity decreases to 20 standard deviations at the galactic edge (30 kpc) and 6 standard deviations at the Large Magellanic Cloud (50 kpc). IceCube is sending triggers from potential supernovae to the Supernova Early Warning System. The sensitivity to neutrino properties such as the neutrino hierarchy is discussed, as well as the possibility to © 2011 ESO.
first_indexed	2025-11-14T06:14:46Z
format	Journal Article
id	curtin-20.500.11937-7122
institution	Curtin University Malaysia
institution_category	Local University
last_indexed	2025-11-14T06:14:46Z
publishDate	2011
recordtype	eprints
repository_type	Digital Repository
spelling	curtin-20.500.11937-71222017-09-13T14:40:30Z IceCube sensitivity for low-energy neutrinos from nearby supernovae Abbasi, R. Abdou, Y. Abu-Zayyad, T. Ackermann, M. Adams, J. Aguilar, J. Ahlers, M. Allen, M. Altmann, D. Andeen, K. Auffenberg, J. Bai, X. Baker, M. Barwick, S. Baum, V. Bay, R. Bazo Alba, J. Beattie, K. Beatty, J. Bechet, S. Becker, J. Becker, K. Benabderrahmane, M. Benzvi, S. Berdermann, J. Berghaus, P. Berley, D. Bernardini, E. Bertrand, D. Besson, D. Bindig, D. Bissok, M. Blaufuss, E. Blumenthal, J. Boersma, D. Bohm, C. Bose, D. Böser, S. Botner, O. Brown, A. Buitink, S. Caballero-Mora, K. Carson, Michael Chirkin, D. Christy, B. Clevermann, F. Cohen, S. Colnard, C. Cowen, D. Cruz Silva, A. D'Agostino, M. Danninger, M. Daughhetee, J. Davis, J. De Clercq, C. Degner, T. Demirörs, L. Descamps, F. Desiati, P. De Vries-Uiterweerd, G. Deyoung, T. Díaz-Vélez, J. Dierckxsens, M. Dreyer, J. Dumm, J. Dunkman, M. Eisch, J. Ellsworth, R. Engdegård, O. Euler, S. Evenson, P. Fadiran, O. Fazely, A. Fedynitch, A. Feintzeig, J. Feusels, T. Filimonov, K. Finley, C. Fischer-Wasels, T. Fox, B. Franckowiak, A. Franke, R. Gaisser, T. Gallagher, J. Gerhardt, L. Gladstone, L. Glüsenkamp, T. Goldschmidt, A. Goodman, J. Góra, D. Grant, D. Griesel, T. Groß, A. Grullon, S. This paper describes the response of the IceCube neutrino telescope located at the geographic south pole to outbursts of MeV neutrinos from the core collapse of nearby massive stars. IceCube was completed in December 2010 forming a lattice of 5160 photomultiplier tubes that monitor a volume of ~1 km 3 in the deep Antarctic ice for particle induced photons. The telescope was designed to detect neutrinos with energies greater than 100 GeV. Owing to subfreezing ice temperatures, the photomultiplier dark noise rates are particularly low. Hence IceCube can also detect large numbers of MeV neutrinos by observing a collective rise in all photomultiplier rates on top of the dark noise. With 2 ms timing resolution, IceCube can detect subtle features in the temporal development of the supernova neutrino burst. For a supernova at the galactic center, its sensitivity matches that of a background-free megaton-scale supernova search experiment. The sensitivity decreases to 20 standard deviations at the galactic edge (30 kpc) and 6 standard deviations at the Large Magellanic Cloud (50 kpc). IceCube is sending triggers from potential supernovae to the Supernova Early Warning System. The sensitivity to neutrino properties such as the neutrino hierarchy is discussed, as well as the possibility to © 2011 ESO. 2011 Journal Article http://hdl.handle.net/20.500.11937/7122 10.1051/0004-6361/201117810 fulltext
spellingShingle	Abbasi, R. Abdou, Y. Abu-Zayyad, T. Ackermann, M. Adams, J. Aguilar, J. Ahlers, M. Allen, M. Altmann, D. Andeen, K. Auffenberg, J. Bai, X. Baker, M. Barwick, S. Baum, V. Bay, R. Bazo Alba, J. Beattie, K. Beatty, J. Bechet, S. Becker, J. Becker, K. Benabderrahmane, M. Benzvi, S. Berdermann, J. Berghaus, P. Berley, D. Bernardini, E. Bertrand, D. Besson, D. Bindig, D. Bissok, M. Blaufuss, E. Blumenthal, J. Boersma, D. Bohm, C. Bose, D. Böser, S. Botner, O. Brown, A. Buitink, S. Caballero-Mora, K. Carson, Michael Chirkin, D. Christy, B. Clevermann, F. Cohen, S. Colnard, C. Cowen, D. Cruz Silva, A. D'Agostino, M. Danninger, M. Daughhetee, J. Davis, J. De Clercq, C. Degner, T. Demirörs, L. Descamps, F. Desiati, P. De Vries-Uiterweerd, G. Deyoung, T. Díaz-Vélez, J. Dierckxsens, M. Dreyer, J. Dumm, J. Dunkman, M. Eisch, J. Ellsworth, R. Engdegård, O. Euler, S. Evenson, P. Fadiran, O. Fazely, A. Fedynitch, A. Feintzeig, J. Feusels, T. Filimonov, K. Finley, C. Fischer-Wasels, T. Fox, B. Franckowiak, A. Franke, R. Gaisser, T. Gallagher, J. Gerhardt, L. Gladstone, L. Glüsenkamp, T. Goldschmidt, A. Goodman, J. Góra, D. Grant, D. Griesel, T. Groß, A. Grullon, S. IceCube sensitivity for low-energy neutrinos from nearby supernovae
title	IceCube sensitivity for low-energy neutrinos from nearby supernovae
title_full	IceCube sensitivity for low-energy neutrinos from nearby supernovae
title_fullStr	IceCube sensitivity for low-energy neutrinos from nearby supernovae
title_full_unstemmed	IceCube sensitivity for low-energy neutrinos from nearby supernovae
title_short	IceCube sensitivity for low-energy neutrinos from nearby supernovae
title_sort	icecube sensitivity for low-energy neutrinos from nearby supernovae
url	http://hdl.handle.net/20.500.11937/7122

IceCube sensitivity for low-energy neutrinos from nearby supernovae

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