Search for neutrino-induced cascades with five years of AMANDA data

We report on the search for electromagnetic and hadronic showers ("cascades") produced by a diffuse flux of extraterrestrial neutrinos in the AMANDA neutrino telescope. Data for this analysis were recorded during 1001 days of detector livetime in the years 2000-2004. The observed event rat...

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Veröffentlicht in:Astroparticle physics 2011-01, Vol.34, p.420-430
Hauptverfasser: Abbasi, R., Abdou, Y., Abu-Zayyad, T., Actis, O., Adams, J., Aguilar, J. A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, Mark D., Barwick, S. W., Bay, R., Bazo Alba, J. L., Beattie, K., Beatty, J. J., Bechet, S., Becker, J. K., Becker, K.-H., Benabderrahmane, M. L., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D. Z., Bissok, M., Blaufuss, E., Boersma, D. J., Bohm, C., Böser, S., Botner, O., Bradley, L., Braun, J., Buitink, S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D. F., d'Agostino, M. V., Danninger, M., Davis, J. C., de Clercq, C., Demirörs, L., Depaepe, O., Descamps, F., Desiati, P., de Vries-Uiterweerd, G., Deyoung, T., Díaz-Vélez, J. C., Dreyer, J., Dumm, J. P., Duvoort, M. R., Ehrlich, R., Eisch, J., Ellsworth, R. W., Engdegård, O., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Feusels, T., Filimonov, K., Finley, C., Foerster, M. M., Fox, B. D., Franckowiak, A., Franke, R., Gaisser, T. K., Gallagher, J., Ganugapati, R., Geisler, M., Gerhardt, L., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Goodman, J. A., Grant, D., Griesel, T., Gross, A., Grullon, S., Gunasingha, R. M., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Helbing, K., Herquet, P., Hickford, S., Hill, G. C., Hoffman, K. D., Homeier, A., Hoshina, K., Hubert, D.
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container_title Astroparticle physics
container_volume 34
creator Abbasi, R.
Abdou, Y.
Abu-Zayyad, T.
Actis, O.
Adams, J.
Aguilar, J. A.
Ahlers, M.
Andeen, K.
Auffenberg, J.
Bai, X.
Baker, Mark D.
Barwick, S. W.
Bay, R.
Bazo Alba, J. L.
Beattie, K.
Beatty, J. J.
Bechet, S.
Becker, J. K.
Becker, K.-H.
Benabderrahmane, M. L.
Berdermann, J.
Berghaus, P.
Berley, D.
Bernardini, E.
Bertrand, D.
Besson, D. Z.
Bissok, M.
Blaufuss, E.
Boersma, D. J.
Bohm, C.
Böser, S.
Botner, O.
Bradley, L.
Braun, J.
Buitink, S.
Carson, M.
Chirkin, D.
Christy, B.
Clem, J.
Clevermann, F.
Cohen, S.
Colnard, C.
Cowen, D. F.
d'Agostino, M. V.
Danninger, M.
Davis, J. C.
de Clercq, C.
Demirörs, L.
Depaepe, O.
Descamps, F.
Desiati, P.
de Vries-Uiterweerd, G.
Deyoung, T.
Díaz-Vélez, J. C.
Dreyer, J.
Dumm, J. P.
Duvoort, M. R.
Ehrlich, R.
Eisch, J.
Ellsworth, R. W.
Engdegård, O.
Euler, S.
Evenson, P. A.
Fadiran, O.
Fazely, A. R.
Feusels, T.
Filimonov, K.
Finley, C.
Foerster, M. M.
Fox, B. D.
Franckowiak, A.
Franke, R.
Gaisser, T. K.
Gallagher, J.
Ganugapati, R.
Geisler, M.
Gerhardt, L.
Gladstone, L.
Glüsenkamp, T.
Goldschmidt, A.
Goodman, J. A.
Grant, D.
Griesel, T.
Gross, A.
Grullon, S.
Gunasingha, R. M.
Gurtner, M.
Ha, C.
Hallgren, A.
Halzen, F.
Han, K.
Hanson, K.
Helbing, K.
Herquet, P.
Hickford, S.
Hill, G. C.
Hoffman, K. D.
Homeier, A.
Hoshina, K.
Hubert, D.
description We report on the search for electromagnetic and hadronic showers ("cascades") produced by a diffuse flux of extraterrestrial neutrinos in the AMANDA neutrino telescope. Data for this analysis were recorded during 1001 days of detector livetime in the years 2000-2004. The observed event rates are consistent with the background expectation from atmospheric neutrinos and muons. An upper limit is derived for the diffuse flux of neutrinos of all flavors assuming a flavor ratio of νe:νμ:ντ = 1:1:1 at the detection site. The all-flavor flux of neutrinos with an energy spectrum Φ ∝ E-2 is less than 5.0 × 10-7 GeV s-1 sr-1 cm-2 at a 90% C.L. Here, 90% of the simulated signal would fall within the energy range 40 TeV to 9 PeV. We discuss flux limits in the context of several specific models of extraterrestrial and prompt atmospheric neutrino production.
doi_str_mv 10.1016/J.ASTROPARTPHYS.2010.10.007
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A. ; Ahlers, M. ; Andeen, K. ; Auffenberg, J. ; Bai, X. ; Baker, Mark D. ; Barwick, S. W. ; Bay, R. ; Bazo Alba, J. L. ; Beattie, K. ; Beatty, J. J. ; Bechet, S. ; Becker, J. K. ; Becker, K.-H. ; Benabderrahmane, M. L. ; Berdermann, J. ; Berghaus, P. ; Berley, D. ; Bernardini, E. ; Bertrand, D. ; Besson, D. Z. ; Bissok, M. ; Blaufuss, E. ; Boersma, D. J. ; Bohm, C. ; Böser, S. ; Botner, O. ; Bradley, L. ; Braun, J. ; Buitink, S. ; Carson, M. ; Chirkin, D. ; Christy, B. ; Clem, J. ; Clevermann, F. ; Cohen, S. ; Colnard, C. ; Cowen, D. F. ; d'Agostino, M. V. ; Danninger, M. ; Davis, J. C. ; de Clercq, C. ; Demirörs, L. ; Depaepe, O. ; Descamps, F. ; Desiati, P. ; de Vries-Uiterweerd, G. ; Deyoung, T. ; Díaz-Vélez, J. C. ; Dreyer, J. ; Dumm, J. P. ; Duvoort, M. R. ; Ehrlich, R. ; Eisch, J. ; Ellsworth, R. W. ; Engdegård, O. ; Euler, S. ; Evenson, P. A. ; Fadiran, O. ; Fazely, A. R. ; Feusels, T. ; Filimonov, K. ; Finley, C. ; Foerster, M. M. ; Fox, B. D. ; Franckowiak, A. ; Franke, R. ; Gaisser, T. K. ; Gallagher, J. ; Ganugapati, R. ; Geisler, M. ; Gerhardt, L. ; Gladstone, L. ; Glüsenkamp, T. ; Goldschmidt, A. ; Goodman, J. A. ; Grant, D. ; Griesel, T. ; Gross, A. ; Grullon, S. ; Gunasingha, R. M. ; Gurtner, M. ; Ha, C. ; Hallgren, A. ; Halzen, F. ; Han, K. ; Hanson, K. ; Helbing, K. ; Herquet, P. ; Hickford, S. ; Hill, G. C. ; Hoffman, K. D. ; Homeier, A. ; Hoshina, K. ; Hubert, D.</creator><creatorcontrib>Abbasi, R. ; Abdou, Y. ; Abu-Zayyad, T. ; Actis, O. ; Adams, J. ; Aguilar, J. A. ; Ahlers, M. ; Andeen, K. ; Auffenberg, J. ; Bai, X. ; Baker, Mark D. ; Barwick, S. W. ; Bay, R. ; Bazo Alba, J. L. ; Beattie, K. ; Beatty, J. J. ; Bechet, S. ; Becker, J. K. ; Becker, K.-H. ; Benabderrahmane, M. L. ; Berdermann, J. ; Berghaus, P. ; Berley, D. ; Bernardini, E. ; Bertrand, D. ; Besson, D. Z. ; Bissok, M. ; Blaufuss, E. ; Boersma, D. 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M.</creatorcontrib><creatorcontrib>Gurtner, M.</creatorcontrib><creatorcontrib>Ha, C.</creatorcontrib><creatorcontrib>Hallgren, A.</creatorcontrib><creatorcontrib>Halzen, F.</creatorcontrib><creatorcontrib>Han, K.</creatorcontrib><creatorcontrib>Hanson, K.</creatorcontrib><creatorcontrib>Helbing, K.</creatorcontrib><creatorcontrib>Herquet, P.</creatorcontrib><creatorcontrib>Hickford, S.</creatorcontrib><creatorcontrib>Hill, G. C.</creatorcontrib><creatorcontrib>Hoffman, K. D.</creatorcontrib><creatorcontrib>Homeier, A.</creatorcontrib><creatorcontrib>Hoshina, K.</creatorcontrib><creatorcontrib>Hubert, D.</creatorcontrib><title>Search for neutrino-induced cascades with five years of AMANDA data</title><title>Astroparticle physics</title><description>We report on the search for electromagnetic and hadronic showers ("cascades") produced by a diffuse flux of extraterrestrial neutrinos in the AMANDA neutrino telescope. Data for this analysis were recorded during 1001 days of detector livetime in the years 2000-2004. The observed event rates are consistent with the background expectation from atmospheric neutrinos and muons. An upper limit is derived for the diffuse flux of neutrinos of all flavors assuming a flavor ratio of νe:νμ:ντ = 1:1:1 at the detection site. The all-flavor flux of neutrinos with an energy spectrum Φ ∝ E-2 is less than 5.0 × 10-7 GeV s-1 sr-1 cm-2 at a 90% C.L. Here, 90% of the simulated signal would fall within the energy range 40 TeV to 9 PeV. We discuss flux limits in the context of several specific models of extraterrestrial and prompt atmospheric neutrino production.</description><subject>Astrophysics</subject><subject>Cosmology and Extra-Galactic Astrophysics</subject><subject>High Energy Astrophysical Phenomena</subject><subject>Physics</subject><subject>Sciences of the Universe</subject><issn>0927-6505</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNqVzssKgkAYhuFZFGSHexhoGdo_WorLoQMSnUg3rYYfHXGiVGa06O6T6AZafYv3WXyETBk4DJg_3zk8Ti6nM78k5-gaOy58iwMQ9IgFoRvY_hKWAzI05gbAFuAtLLKKJeq0oHmlaSnbRquyslWZtanMaIomxUwa-lJNR9RT0nfHDa1yyg_8uOY0wwbHpJ_j3cjJb0dktt0kq8gu8C5qrR6o36JCJSK-F6p0a090p8APwX8y7z_9AR9LRbg</recordid><startdate>201101</startdate><enddate>201101</enddate><creator>Abbasi, R.</creator><creator>Abdou, Y.</creator><creator>Abu-Zayyad, T.</creator><creator>Actis, O.</creator><creator>Adams, J.</creator><creator>Aguilar, J. 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M.</creator><creator>Gurtner, M.</creator><creator>Ha, C.</creator><creator>Hallgren, A.</creator><creator>Halzen, F.</creator><creator>Han, K.</creator><creator>Hanson, K.</creator><creator>Helbing, K.</creator><creator>Herquet, P.</creator><creator>Hickford, S.</creator><creator>Hill, G. C.</creator><creator>Hoffman, K. D.</creator><creator>Homeier, A.</creator><creator>Hoshina, K.</creator><creator>Hubert, D.</creator><general>Elsevier</general><scope>1XC</scope><orcidid>https://orcid.org/0000-0003-3108-1141</orcidid><orcidid>https://orcid.org/0000-0003-2636-5000</orcidid><orcidid>https://orcid.org/0000-0001-5634-0766</orcidid><orcidid>https://orcid.org/0000-0002-5481-5040</orcidid><orcidid>https://orcid.org/0000-0003-3108-1141</orcidid></search><sort><creationdate>201101</creationdate><title>Search for neutrino-induced cascades with five years of AMANDA data</title><author>Abbasi, R. ; Abdou, Y. ; Abu-Zayyad, T. ; Actis, O. ; Adams, J. ; Aguilar, J. A. ; Ahlers, M. ; Andeen, K. ; Auffenberg, J. ; Bai, X. ; Baker, Mark D. ; Barwick, S. W. ; Bay, R. ; Bazo Alba, J. L. ; Beattie, K. ; Beatty, J. J. ; Bechet, S. ; Becker, J. K. ; Becker, K.-H. ; Benabderrahmane, M. L. ; Berdermann, J. ; Berghaus, P. ; Berley, D. ; Bernardini, E. ; Bertrand, D. ; Besson, D. Z. ; Bissok, M. ; Blaufuss, E. ; Boersma, D. J. ; Bohm, C. ; Böser, S. ; Botner, O. ; Bradley, L. ; Braun, J. ; Buitink, S. ; Carson, M. ; Chirkin, D. ; Christy, B. ; Clem, J. ; Clevermann, F. ; Cohen, S. ; Colnard, C. ; Cowen, D. F. ; d'Agostino, M. V. ; Danninger, M. ; Davis, J. C. ; de Clercq, C. ; Demirörs, L. ; Depaepe, O. ; Descamps, F. ; Desiati, P. ; de Vries-Uiterweerd, G. ; Deyoung, T. ; Díaz-Vélez, J. C. ; Dreyer, J. ; Dumm, J. P. ; Duvoort, M. R. ; Ehrlich, R. ; Eisch, J. ; Ellsworth, R. W. ; Engdegård, O. ; Euler, S. ; Evenson, P. A. ; Fadiran, O. ; Fazely, A. R. ; Feusels, T. ; Filimonov, K. ; Finley, C. ; Foerster, M. M. ; Fox, B. D. ; Franckowiak, A. ; Franke, R. ; Gaisser, T. K. ; Gallagher, J. ; Ganugapati, R. ; Geisler, M. ; Gerhardt, L. ; Gladstone, L. ; Glüsenkamp, T. ; Goldschmidt, A. ; Goodman, J. A. ; Grant, D. ; Griesel, T. ; Gross, A. ; Grullon, S. ; Gunasingha, R. M. ; Gurtner, M. ; Ha, C. ; Hallgren, A. ; Halzen, F. ; Han, K. ; Hanson, K. ; Helbing, K. ; Herquet, P. ; Hickford, S. ; Hill, G. C. ; Hoffman, K. D. ; Homeier, A. ; Hoshina, K. ; Hubert, D.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-hal_primary_oai_HAL_in2p3_00706906v13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>Astrophysics</topic><topic>Cosmology and Extra-Galactic Astrophysics</topic><topic>High Energy Astrophysical Phenomena</topic><topic>Physics</topic><topic>Sciences of the Universe</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Abbasi, R.</creatorcontrib><creatorcontrib>Abdou, Y.</creatorcontrib><creatorcontrib>Abu-Zayyad, T.</creatorcontrib><creatorcontrib>Actis, O.</creatorcontrib><creatorcontrib>Adams, J.</creatorcontrib><creatorcontrib>Aguilar, J. A.</creatorcontrib><creatorcontrib>Ahlers, M.</creatorcontrib><creatorcontrib>Andeen, K.</creatorcontrib><creatorcontrib>Auffenberg, J.</creatorcontrib><creatorcontrib>Bai, X.</creatorcontrib><creatorcontrib>Baker, Mark D.</creatorcontrib><creatorcontrib>Barwick, S. W.</creatorcontrib><creatorcontrib>Bay, R.</creatorcontrib><creatorcontrib>Bazo Alba, J. L.</creatorcontrib><creatorcontrib>Beattie, K.</creatorcontrib><creatorcontrib>Beatty, J. J.</creatorcontrib><creatorcontrib>Bechet, S.</creatorcontrib><creatorcontrib>Becker, J. K.</creatorcontrib><creatorcontrib>Becker, K.-H.</creatorcontrib><creatorcontrib>Benabderrahmane, M. L.</creatorcontrib><creatorcontrib>Berdermann, J.</creatorcontrib><creatorcontrib>Berghaus, P.</creatorcontrib><creatorcontrib>Berley, D.</creatorcontrib><creatorcontrib>Bernardini, E.</creatorcontrib><creatorcontrib>Bertrand, D.</creatorcontrib><creatorcontrib>Besson, D. Z.</creatorcontrib><creatorcontrib>Bissok, M.</creatorcontrib><creatorcontrib>Blaufuss, E.</creatorcontrib><creatorcontrib>Boersma, D. J.</creatorcontrib><creatorcontrib>Bohm, C.</creatorcontrib><creatorcontrib>Böser, S.</creatorcontrib><creatorcontrib>Botner, O.</creatorcontrib><creatorcontrib>Bradley, L.</creatorcontrib><creatorcontrib>Braun, J.</creatorcontrib><creatorcontrib>Buitink, S.</creatorcontrib><creatorcontrib>Carson, M.</creatorcontrib><creatorcontrib>Chirkin, D.</creatorcontrib><creatorcontrib>Christy, B.</creatorcontrib><creatorcontrib>Clem, J.</creatorcontrib><creatorcontrib>Clevermann, F.</creatorcontrib><creatorcontrib>Cohen, S.</creatorcontrib><creatorcontrib>Colnard, C.</creatorcontrib><creatorcontrib>Cowen, D. F.</creatorcontrib><creatorcontrib>d'Agostino, M. V.</creatorcontrib><creatorcontrib>Danninger, M.</creatorcontrib><creatorcontrib>Davis, J. C.</creatorcontrib><creatorcontrib>de Clercq, C.</creatorcontrib><creatorcontrib>Demirörs, L.</creatorcontrib><creatorcontrib>Depaepe, O.</creatorcontrib><creatorcontrib>Descamps, F.</creatorcontrib><creatorcontrib>Desiati, P.</creatorcontrib><creatorcontrib>de Vries-Uiterweerd, G.</creatorcontrib><creatorcontrib>Deyoung, T.</creatorcontrib><creatorcontrib>Díaz-Vélez, J. C.</creatorcontrib><creatorcontrib>Dreyer, J.</creatorcontrib><creatorcontrib>Dumm, J. P.</creatorcontrib><creatorcontrib>Duvoort, M. R.</creatorcontrib><creatorcontrib>Ehrlich, R.</creatorcontrib><creatorcontrib>Eisch, J.</creatorcontrib><creatorcontrib>Ellsworth, R. W.</creatorcontrib><creatorcontrib>Engdegård, O.</creatorcontrib><creatorcontrib>Euler, S.</creatorcontrib><creatorcontrib>Evenson, P. A.</creatorcontrib><creatorcontrib>Fadiran, O.</creatorcontrib><creatorcontrib>Fazely, A. R.</creatorcontrib><creatorcontrib>Feusels, T.</creatorcontrib><creatorcontrib>Filimonov, K.</creatorcontrib><creatorcontrib>Finley, C.</creatorcontrib><creatorcontrib>Foerster, M. M.</creatorcontrib><creatorcontrib>Fox, B. D.</creatorcontrib><creatorcontrib>Franckowiak, A.</creatorcontrib><creatorcontrib>Franke, R.</creatorcontrib><creatorcontrib>Gaisser, T. K.</creatorcontrib><creatorcontrib>Gallagher, J.</creatorcontrib><creatorcontrib>Ganugapati, R.</creatorcontrib><creatorcontrib>Geisler, M.</creatorcontrib><creatorcontrib>Gerhardt, L.</creatorcontrib><creatorcontrib>Gladstone, L.</creatorcontrib><creatorcontrib>Glüsenkamp, T.</creatorcontrib><creatorcontrib>Goldschmidt, A.</creatorcontrib><creatorcontrib>Goodman, J. A.</creatorcontrib><creatorcontrib>Grant, D.</creatorcontrib><creatorcontrib>Griesel, T.</creatorcontrib><creatorcontrib>Gross, A.</creatorcontrib><creatorcontrib>Grullon, S.</creatorcontrib><creatorcontrib>Gunasingha, R. M.</creatorcontrib><creatorcontrib>Gurtner, M.</creatorcontrib><creatorcontrib>Ha, C.</creatorcontrib><creatorcontrib>Hallgren, A.</creatorcontrib><creatorcontrib>Halzen, F.</creatorcontrib><creatorcontrib>Han, K.</creatorcontrib><creatorcontrib>Hanson, K.</creatorcontrib><creatorcontrib>Helbing, K.</creatorcontrib><creatorcontrib>Herquet, P.</creatorcontrib><creatorcontrib>Hickford, S.</creatorcontrib><creatorcontrib>Hill, G. C.</creatorcontrib><creatorcontrib>Hoffman, K. D.</creatorcontrib><creatorcontrib>Homeier, A.</creatorcontrib><creatorcontrib>Hoshina, K.</creatorcontrib><creatorcontrib>Hubert, D.</creatorcontrib><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Astroparticle physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Abbasi, R.</au><au>Abdou, Y.</au><au>Abu-Zayyad, T.</au><au>Actis, O.</au><au>Adams, J.</au><au>Aguilar, J. A.</au><au>Ahlers, M.</au><au>Andeen, K.</au><au>Auffenberg, J.</au><au>Bai, X.</au><au>Baker, Mark D.</au><au>Barwick, S. W.</au><au>Bay, R.</au><au>Bazo Alba, J. L.</au><au>Beattie, K.</au><au>Beatty, J. J.</au><au>Bechet, S.</au><au>Becker, J. K.</au><au>Becker, K.-H.</au><au>Benabderrahmane, M. L.</au><au>Berdermann, J.</au><au>Berghaus, P.</au><au>Berley, D.</au><au>Bernardini, E.</au><au>Bertrand, D.</au><au>Besson, D. Z.</au><au>Bissok, M.</au><au>Blaufuss, E.</au><au>Boersma, D. J.</au><au>Bohm, C.</au><au>Böser, S.</au><au>Botner, O.</au><au>Bradley, L.</au><au>Braun, J.</au><au>Buitink, S.</au><au>Carson, M.</au><au>Chirkin, D.</au><au>Christy, B.</au><au>Clem, J.</au><au>Clevermann, F.</au><au>Cohen, S.</au><au>Colnard, C.</au><au>Cowen, D. F.</au><au>d'Agostino, M. V.</au><au>Danninger, M.</au><au>Davis, J. C.</au><au>de Clercq, C.</au><au>Demirörs, L.</au><au>Depaepe, O.</au><au>Descamps, F.</au><au>Desiati, P.</au><au>de Vries-Uiterweerd, G.</au><au>Deyoung, T.</au><au>Díaz-Vélez, J. C.</au><au>Dreyer, J.</au><au>Dumm, J. P.</au><au>Duvoort, M. R.</au><au>Ehrlich, R.</au><au>Eisch, J.</au><au>Ellsworth, R. W.</au><au>Engdegård, O.</au><au>Euler, S.</au><au>Evenson, P. A.</au><au>Fadiran, O.</au><au>Fazely, A. R.</au><au>Feusels, T.</au><au>Filimonov, K.</au><au>Finley, C.</au><au>Foerster, M. M.</au><au>Fox, B. D.</au><au>Franckowiak, A.</au><au>Franke, R.</au><au>Gaisser, T. K.</au><au>Gallagher, J.</au><au>Ganugapati, R.</au><au>Geisler, M.</au><au>Gerhardt, L.</au><au>Gladstone, L.</au><au>Glüsenkamp, T.</au><au>Goldschmidt, A.</au><au>Goodman, J. A.</au><au>Grant, D.</au><au>Griesel, T.</au><au>Gross, A.</au><au>Grullon, S.</au><au>Gunasingha, R. M.</au><au>Gurtner, M.</au><au>Ha, C.</au><au>Hallgren, A.</au><au>Halzen, F.</au><au>Han, K.</au><au>Hanson, K.</au><au>Helbing, K.</au><au>Herquet, P.</au><au>Hickford, S.</au><au>Hill, G. C.</au><au>Hoffman, K. D.</au><au>Homeier, A.</au><au>Hoshina, K.</au><au>Hubert, D.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Search for neutrino-induced cascades with five years of AMANDA data</atitle><jtitle>Astroparticle physics</jtitle><date>2011-01</date><risdate>2011</risdate><volume>34</volume><spage>420</spage><epage>430</epage><pages>420-430</pages><issn>0927-6505</issn><abstract>We report on the search for electromagnetic and hadronic showers ("cascades") produced by a diffuse flux of extraterrestrial neutrinos in the AMANDA neutrino telescope. Data for this analysis were recorded during 1001 days of detector livetime in the years 2000-2004. The observed event rates are consistent with the background expectation from atmospheric neutrinos and muons. An upper limit is derived for the diffuse flux of neutrinos of all flavors assuming a flavor ratio of νe:νμ:ντ = 1:1:1 at the detection site. The all-flavor flux of neutrinos with an energy spectrum Φ ∝ E-2 is less than 5.0 × 10-7 GeV s-1 sr-1 cm-2 at a 90% C.L. Here, 90% of the simulated signal would fall within the energy range 40 TeV to 9 PeV. We discuss flux limits in the context of several specific models of extraterrestrial and prompt atmospheric neutrino production.</abstract><pub>Elsevier</pub><doi>10.1016/J.ASTROPARTPHYS.2010.10.007</doi><orcidid>https://orcid.org/0000-0003-3108-1141</orcidid><orcidid>https://orcid.org/0000-0003-2636-5000</orcidid><orcidid>https://orcid.org/0000-0001-5634-0766</orcidid><orcidid>https://orcid.org/0000-0002-5481-5040</orcidid><orcidid>https://orcid.org/0000-0003-3108-1141</orcidid></addata></record>
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source ScienceDirect Journals (5 years ago - present)
subjects Astrophysics
Cosmology and Extra-Galactic Astrophysics
High Energy Astrophysical Phenomena
Physics
Sciences of the Universe
title Search for neutrino-induced cascades with five years of AMANDA data
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