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WFRF:(Pohl Annika)
 

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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00003904naa a2200553 4500
001oai:DiVA.org:uu-87508
003SwePub
008081219s2007 | |||||||||||000 ||eng|
009oai:DiVA.org:lnu-1566
0247 a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-875082 URI
0247 a https://doi.org/10.1086/5185962 DOI
0247 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 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
1001 a Achterberg, A.u Department of Physics and Astronomy, Utrecht University4 aut
2451 0a Search for neutrino-induced cascades from gamma-ray bursts with AMANDA
264 1b 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 7a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng
650 7a NATURVETENSKAPx Fysikx Subatomär fysik0 (SwePub)103012 hsv//swe
650 7a 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
7001 a Botner, Olga,d 1953-u Uppsala universitet,Högenergifysik,high energy physics4 aut
7001 a Bouchta, Adamu Uppsala universitet,Högenergifysik4 aut
7001 a Davour, Annau Uppsala universitet,Högenergifysik4 aut
7001 a Hallgren, Allanu Uppsala universitet,Högenergifysik4 aut0 (Swepub:uu)allahall
7001 a Lundberg, Johanu Uppsala universitet,Högenergifysik4 aut
7001 a Perez de los Heros, Carlosu Uppsala universitet,Högenergifysik4 aut0 (Swepub:uu)capedlhe
7001 a Pohl, Annika C.u Uppsala universitet,Högenergifysik4 aut
7001 a Zornoza, J. D.4 aut
7001 a IceCube Collaboration, -4 aut
7001 a Pohl, Arvidu Högskolan i Kalmar,Naturvetenskapliga institutionen4 aut0 (Swepub:lnu)tpoar
7102 a Department of Physics and Astronomy, Utrecht Universityb Högenergifysik4 org
7730 t Astrophysical Journald : American Astronomical Societyg 664:1, s. 397-410q 664:1<397-410x 0004-637Xx 1538-4357
8564 u https://bib-pubdb1.desy.de/record/82860/files/search.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-87508
8564 8u https://doi.org/10.1086/518596
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-1566

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