16,635 research outputs found

    The Hidden Costs: A Case Study for Sustainable Development Studies

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    Large lepton mixing and supernova 1987A

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    We reconsider the impact of νˉe↔νˉμ,τ\bar\nu_e \leftrightarrow \bar\nu_{\mu,\tau} neutrino oscillations on the observed νˉe\bar\nu_e signal of supernova SN 1987A. Performing a maximum-likelihood analysis using as fit parameters the released binding energy \Eb and the average neutrino energy \Ee, we find as previous analyses that νˉe↔νˉμ,τ\bar\nu_e \leftrightarrow \bar\nu_{\mu,\tau} oscillations with large mixing angles have lower best-fit values for \Ee than small-mixing angle (SMA) oscillations. Moreover, the inferred value of \Ee is already in the SMA case lower than those found in simulations. This apparent conflict has been interpreted as evidence against the large mixing oscillation solutions to the solar neutrino problem. In order to quantify the degree to which the experimental data favour the SMA over the large mixing solutions we use their likelihood ratios as well as a Kolmogorov-Smirnov test. We find within the range of SN parameters predicted by simulations regions in which the LMA-MSW solution is either only marginally disfavoured or favoured compared to the SMA-MSW solution. We conclude therefore that the LMA-MSW solution is not in conflict with the current understanding of SN physics. In contrast, the vacuum oscillation and the LOW solutions to the solar neutrino problem can be excluded at the 4σ4\sigma level for most of the SN parameter ranges found in simulations. Only a marginal region with low values of \Ee, and \Eb is left over, in which these oscillation solutions can be reconciled with the neutrino signal of SN 1987A.Comment: 23 pages, 20 figures, v2: brief comments adde

    Scattering of accelerated wave packets

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    Wave-packet scattering from a stationary potential is significantly modified when the wave-packet is subject to an external time-dependent force during the interaction. In the semiclassical limit, wave--packet motion is simply described by Newtonian equations and the external force can, for example, cancel the potential force making a potential barrier transparent. Here we consider wave-packet scattering from reflectionless potentials, where in general the potential becomes reflective when probed by an accelerated wave-packet. In the particular case of the recently-introduced class of complex Kramers-Kronig potentials we show that a broad class of time dependent forces can be applied without inducing any scattering, while there is a breakdown of the reflectionless property when there is a broadband distribution of initial particle momentum, involving both positive and negative components.Comment: 13 pages, 4 figures, to appear in Phys. Rev.
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