1948
DOI: 10.1103/physrev.74.898
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On the Life of Self-Quenching Counters

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Cited by 18 publications
(10 citation statements)
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“…Therefore, to insure a stable operation, monatomic gases are usually mixed with few percents of polyatomic gases such as CH 4 , N 2 , CO 2 and Iso-C 4 H 10 called quenching gases [6]. The addition of polyatomic gases can reduce the counter lifetime because of the decomposition of the polyatomic molecules leading to a modification of the gas composition [9]. However, this problem can be overcome by using gas flow counters.…”
Section: Introductionmentioning
confidence: 99%
“…Therefore, to insure a stable operation, monatomic gases are usually mixed with few percents of polyatomic gases such as CH 4 , N 2 , CO 2 and Iso-C 4 H 10 called quenching gases [6]. The addition of polyatomic gases can reduce the counter lifetime because of the decomposition of the polyatomic molecules leading to a modification of the gas composition [9]. However, this problem can be overcome by using gas flow counters.…”
Section: Introductionmentioning
confidence: 99%
“…Firstly, the best fit point lies in the region which is excluded by the atmospheric neutrino data [12]. Secondly, while the disfavored region at 3σ CL almost coincides with the one by the atmospheric neutrino data [12], the significance of the standard case (ε ee = ε eτ = 0) compared with the best fit point is only 0.07σ CL. Therefore, we conclude that it is not worth introducing this scenario to explain the MINOS anomaly.…”
Section: (Iii) Non-standard Interactions In Propagation With E τ Commentioning
confidence: 56%
“…The disfavored region [11] obtained from the MINOS data [1]. The region above the diagonal straight lines is excluded because of the atmospheric neutrino data [12]. The contours are drawn to exaggerate its significance.…”
Section: (I) Non-standard Interactions In Propagation With µ τ Compomentioning
confidence: 99%
“…Neutrino non-standard interactions (NSI) were originally proposed [1] as a mechanism to produce neutrino flavour conversion in matter and considered as a possible explanation for the solar and atmospheric neutrino deficits [1,2,3,4,5,6,7,8,9]. Although it is now clear that such NSI cannot fully account for the observed neutrino flavour conversion, the increasing sensitivity of neutrino oscillation experiments to sub-leading effects has triggered a new interest in them and their interference with neutrino oscillations at present (e.g., K2K, MINOS, OPERA [10,11,12,13,14,15,16,17]) and future (e.g., SuperBeams, βBeams or Neutrino Factories [18,19,20,21,22,23,24,25,26,27,28,29,30]) facilities. In particular, the determination of the leptonic mixing angle θ 13 could be severely affected by degeneracies with the non-standard parameters [31,32,33].…”
Section: Introductionmentioning
confidence: 99%
“…Consequently, the non-standard coupling strength ε f f eµ was neglected in a large number of studies (see for example Refs. [12,13,14,15,16,29,40,41,42,43,44]). However, as we will show, when gauge invariance is imposed, only naturalness arguments can be invoked.…”
Section: Introductionmentioning
confidence: 99%