Search: WFRF:(Wikstrom M) > Search for relativi...
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000 | 12855naa a2203517 4500 | |
001 | oai:DiVA.org:uu-133739 | |
003 | SwePub | |
008 | 101115s2010 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-47316 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-1337392 URI |
024 | 7 | a https://doi.org/10.1140/epjc/s10052-010-1411-62 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-473162 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 Search for relativistic magnetic monopoles with the AMANDA-II neutrino telescope |
264 | c 2010-08-28 | |
264 | 1 | b Springer Science and Business Media LLC,c 2010 |
338 | a print2 rdacarrier | |
500 | a Publikationen har totalt 259 författare, R. Abbasi et al. | |
520 | a We present the search for Cherenkov signatures from relativistic magnetic monopoles in data taken with the AMANDA-II detector, a neutrino telescope deployed in the Antarctic ice cap at the Geographic South Pole. The non-observation of a monopole signal in data collected during the year 2000 improves present experimental limits on the flux of relativistic magnetic monopoles: Our flux limit varies between 3.8x10(-17) cm(-2) s(-1) sr(-1) (for monopoles moving at the vacuum speed of light) and 8.8x10(-16) cm(-2) s(-1) sr(-1) (for monopoles moving at a speed beta=v/c=0.76, just above the Cherenkov threshold in ice). These limits apply to monopoles that are energetic enough to penetrate the Earth and enter the detector from below the horizon. The limit obtained for monopoles reaching the detector from above the horizon is less stringent by roughly an order of magnitude, due to the much larger background from down-going atmospheric muons. This looser limit is however valid for a larger class of magnetic monopoles, since the monopoles are not required to pass through the Earth. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 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 High energy astrophysics | |
653 | a Högenergiastrofysik | |
653 | a Astroparticle physics | |
653 | a fysik | |
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710 | 2 | a Stockholms universitetb Fysikum4 org |
773 | 0 | t European Physical Journal Cd : Springer Science and Business Media LLCg 69:3-4, s. 361-378q 69:3-4<361-378x 1434-6044x 1434-6052 |
856 | 4 | u https://link.springer.com/content/pdf/10.1140%2Fepjc%2Fs10052-010-1411-6.pdf |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-133739 |
856 | 4 8 | u https://doi.org/10.1140/epjc/s10052-010-1411-6 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-47316 |
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