Sökning: onr:"swepub:oai:DiVA.org:uu-87508" > Search for neutrino...
Fältnamn | Indikatorer | Metadata |
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000 | 03904naa a2200553 4500 | |
001 | oai:DiVA.org:uu-87508 | |
003 | SwePub | |
008 | 081219s2007 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:lnu-1566 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-875082 URI |
024 | 7 | a https://doi.org/10.1086/5185962 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-15662 URI |
040 | a (SwePub)uud (SwePub)lnu | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Achterberg, A.u Department of Physics and Astronomy, Utrecht University4 aut |
245 | 1 0 | a Search for neutrino-induced cascades from gamma-ray bursts with AMANDA |
264 | 1 | b American Astronomical Society,c 2007 |
338 | a print2 rdacarrier | |
520 | a Using the neutrino telescope AMANDA-II, we have conducted two analyses searching for neutrino-induced cascades from gamma-ray bursts. No evidence of astrophysical neutrinos was found, and limits are presented for several models. We also present neutrino effective areas which allow the calculation of limits for any neutrino production model. The first analysis looked for a statistical excess of events within a sliding window of 1 or 100 s (for short and long burst classes, respectively) during the years 2001-2003. The resulting upper limit on the diffuse flux normalization times E2 for the Waxman-Bahcall model at 1 PeV is 1.6×10-6 GeV cm-2 s-1 sr-1 (a factor of 120 above the theoretical prediction). For this search 90% of the neutrinos would fall in the energy range 50 TeV to 7 PeV. The second analysis looked for neutrino-induced cascades in coincidence with 73 bursts detected by BATSE in the year 2000. The resulting upper limit on the diffuse flux normalization times E2, also at 1 PeV, is 1.5×10-6 GeV cm-2 s-1 sr-1 (a factor of 110 above the theoretical prediction) for the same energy range. The neutrino-induced cascade channel is complementary to the up-going muon channel. We comment on its advantages for searches of neutrinos from GRBs and its future use with IceCube. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysikx Subatomär fysik0 (SwePub)103012 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Subatomic Physics0 (SwePub)103012 hsv//eng |
653 | a Gamma Rays: Bursts | |
653 | a Neutrinos | |
653 | a Telescopes | |
653 | a Physics | |
653 | a Fysik | |
653 | a Astroparticle physics | |
653 | a Astroparticle Physics | |
700 | 1 | a Botner, Olga,d 1953-u Uppsala universitet,Högenergifysik,high energy physics4 aut |
700 | 1 | a Bouchta, Adamu Uppsala universitet,Högenergifysik4 aut |
700 | 1 | a Davour, Annau Uppsala universitet,Högenergifysik4 aut |
700 | 1 | a Hallgren, Allanu Uppsala universitet,Högenergifysik4 aut0 (Swepub:uu)allahall |
700 | 1 | a Lundberg, Johanu Uppsala universitet,Högenergifysik4 aut |
700 | 1 | a Perez de los Heros, Carlosu Uppsala universitet,Högenergifysik4 aut0 (Swepub:uu)capedlhe |
700 | 1 | a Pohl, Annika C.u Uppsala universitet,Högenergifysik4 aut |
700 | 1 | a Zornoza, J. D.4 aut |
700 | 1 | a IceCube Collaboration, -4 aut |
700 | 1 | a Pohl, Arvidu Högskolan i Kalmar,Naturvetenskapliga institutionen4 aut0 (Swepub:lnu)tpoar |
710 | 2 | a Department of Physics and Astronomy, Utrecht Universityb Högenergifysik4 org |
773 | 0 | t Astrophysical Journald : American Astronomical Societyg 664:1, s. 397-410q 664:1<397-410x 0004-637Xx 1538-4357 |
856 | 4 | u https://bib-pubdb1.desy.de/record/82860/files/search.pdf |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-87508 |
856 | 4 8 | u https://doi.org/10.1086/518596 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-1566 |
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