Sökning: WFRF:(Marotta P) > Background studies ...
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000 | 13111naa a2203577 4500 | |
001 | oai:DiVA.org:uu-172168 | |
003 | SwePub | |
008 | 120402s2012 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-64442 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-1721682 URI |
024 | 7 | a https://doi.org/10.1016/j.astropartphys.2011.09.0042 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-644422 URI |
040 | a (SwePub)uud (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Abbasi, R.4 aut |
245 | 1 0 | a Background studies for acoustic neutrino detection at the South Pole |
264 | 1 | b Elsevier BV,c 2012 |
338 | a print2 rdacarrier | |
500 | a Publikationen har totalt 263 författare, R. Abbasi et al. | |
520 | a The detection of acoustic signals from ultra-high energy neutrino interactions is a promising method to measure the flux of cosmogenic neutrinos expected on Earth. The energy threshold for this process depends strongly on the absolute noise level in the target material. The South Pole Acoustic Test Setup (SPATS), deployed in the upper part of four boreholes of the IceCube Neutrino Observatory, has monitored the noise in Antarctic ice at the geographic South Pole for more than two years down to 500 m depth. The noise is very stable and Gaussian distributed. Lacking an in situ calibration up to now, laboratory measurements have been used to estimate the absolute noise level in the 10-50 kHz frequency range to be smaller than 20 mPa. Using a threshold trigger, sensors of the South Pole Acoustic Test Setup registered acoustic events in the IceCube detector volume and its vicinity. Acoustic signals from refreezing IceCube holes and from anthropogenic sources have been used to test the localization of acoustic events. An upper limit on the neutrino flux at energies E-v>10(11) GeV is derived from acoustic data taken over eight months. (C) 2011 Elsevier B.V. All rights reserved. | |
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 Acoustic neutrino detection | |
653 | a Absolute noise level | |
653 | a Neutrino flux limit | |
653 | a Physics | |
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773 | 0 | t Astroparticle physicsd : Elsevier BVg 35:6, s. 312-324q 35:6<312-324x 0927-6505x 1873-2852 |
856 | 4 | u https://bib-pubdb1.desy.de/record/95257/files/1103.1216v2.pdf |
856 | 4 | u https://arxiv.org/abs/1103.1216y arXiv:1103.1216 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-172168 |
856 | 4 8 | u https://doi.org/10.1016/j.astropartphys.2011.09.004 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-64442 |
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