| 1. |
- Abbasi, R, et al.
(författare)
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Determination of the atmospheric neutrino flux and searches for new physics with AMANDA-II
- 2009
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Ingår i: Physical Review D. - 1550-7998 .- 1550-2368. ; 79, s. 102005-
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Tidskriftsartikel (refereegranskat)abstract
- The AMANDA-II detector, operating since 2000 in the deep ice at the geographic South Pole, has accumulated a large sample of atmospheric muon neutrinos in the 100 GeV to 10 TeV energy range. The zenith angle and energy distribution of these events can be used to search for various phenomenological signatures of quantum gravity in the neutrino sector, such as violation of Lorentz invariance or quantum decoherence. Analyzing a set of 5511 candidate neutrino events collected during 1387 days of livetime from 2000 to 2006, we find no evidence for such effects and set upper limits on violation of Lorentz invariance and quantum decoherence parameters using a maximum likelihood method. Given the absence of evidence for new flavor-changing physics, we use the same methodology to determine the conventional atmospheric muon neutrino flux above 100 GeV.
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| 2. |
- Abbasi, R, et al.
(författare)
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FIRST NEUTRINO POINT-SOURCE RESULTS FROM THE 22 STRING ICECUBE DETECTOR
- 2009
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Ingår i: Astrophysical Journal Letters. - 2041-8205. ; 701, s. L47-L51
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Tidskriftsartikel (refereegranskat)abstract
- We present new results of searches for neutrino point sources in the northern sky, using data recorded in 2007-2008 with 22 strings of the IceCube detector (approximately one-fourth of the planned total) and 275.7 days of live time. The final sample of 5114 neutrino candidate events agrees well with the expected background of atmospheric muon neutrinos and a small component of atmospheric muons. No evidence of a point source is found, with the most significant excess of events in the sky at 2.2 sigma after accounting for all trials. The average upper limit over the northern sky for point sources of muon-neutrinos with E-2 spectrum is E-2 Phi(v mu) < 1.4 x 10(-11) TeV cm(-2) s(-1), in the energy range from 3 TeV to 3 PeV, improving the previous best average upper limit by the AMANDA-II detector by a factor of 2.
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| 3. |
- Abbasi, R, et al.
(författare)
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Limits on a Muon Flux from Neutralino Annihilations in the Sun with the IceCube 22-String Detector
- 2009
-
Ingår i: Physical Review Letters. - 0031-9007 .- 1079-7114. ; 102:20, s. 201302-
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Tidskriftsartikel (refereegranskat)abstract
- A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the IceCube 22-string neutrino detector using data collected in 104.3 days of live time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured neutralinos in the Sun and converted to limits on the weakly interacting massive particle (WIMP) proton cross sections for WIMP masses in the range 250-5000 GeV. These results are the most stringent limits to date on neutralino annihilation in the Sun.
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| 4. |
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| 5. |
- Nord, Stefan, 1980-, et al.
(författare)
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The RimP protein is important for maturation of the 30S ribosomal subunit
- 2009
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Ingår i: Journal of Molecular Biology. - : Elsevier BV. - 0022-2836 .- 1089-8638. ; 386:3, s. 742-753
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Tidskriftsartikel (refereegranskat)abstract
- The in vivo assembly of ribosomal subunits requires assistance by auxiliary proteins that are not part of mature ribosomes. More such assembly proteins have been identified for the assembly of the 50S than for the 30S ribosomal subunit. Here, we show that the RimP protein (formerly YhbC or P15a) is important for the maturation of the 30S subunit. A rimP deletion (DeltarimP135) mutant in Escherichia coli showed a temperature-sensitive growth phenotype as demonstrated by a 1.2-, 1.5-, and 2.5-fold lower growth rate at 30, 37, and 44 degrees C, respectively, compared to a wild-type strain. The mutant had a reduced amount of 70S ribosomes engaged in translation and showed a corresponding increase in the amount of free ribosomal subunits. In addition, the mutant showed a lower ratio of free 30S to 50S subunits as well as an accumulation of immature 16S rRNA compared to a wild-type strain, indicating a deficiency in the maturation of the 30S subunit. All of these effects were more pronounced at higher temperatures. RimP was found to be associated with free 30S subunits but not with free 50S subunits or with 70S ribosomes. The slow growth of the rimP deletion mutant was not suppressed by increased expression of any other known 30S maturation factor.
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