115 research outputs found

    Neutrino conversions in random magnetic fields and Μ~e\tilde{\nu}_e from the Sun

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    The magnetic field in the convective zone of the Sun has a random small-scale component with the r.m.s. value substantially exceeding the strength of a regular large-scale field. For two Majorana neutrino flavors ×\times two helicities in the presence of a neutrino transition magnetic moment and nonzero neutrino mixing we analyze the displacement of the allowed (Δm2−sin⁥22Ξ\Delta m^2- \sin^22\theta)-parameter region reconciled for the SuperKamiokande(SK) and radiochemical (GALLEX, SAGE, Homestake) experiments in dependence on the r.m.s. magnetic field value bb, or more precisely, on a value ÎŒb\mu b assuming the transition magnetic moment ÎŒ=10−11ÎŒB\mu = 10^{-11}\mu_B. In contrast to RSFP in regular magnetic fields we find an effective production of electron antineutrinos in the Sun even for small neutrino mixing through cascade conversions ÎœeL→ΜΌL→Μ~eR\nu_{eL}\to \nu_{\mu L}\to \tilde{\nu}_{eR}, ÎœeL→ΜΌR→Μ~eR\nu_{eL}\to \nu_{\mu R}\to \tilde{\nu}_{eR} in a random magnetic field that would be a signature of the Majorana nature of neutrino if Îœ~eR\tilde{\nu}_{eR} will be registered. Basing on the present SK bound on electron antineutrinos we have also found an excluded area in the same Δm2, sin⁥22Ξ\Delta m^2,~\sin^22\theta-plane and revealed a strong sensitivity to the random magnetic field correlation length L0L_0.Comment: LaTex 36 pages including 14 PostScript figure

    Nonlinear Waves in Bose-Einstein Condensates: Physical Relevance and Mathematical Techniques

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    The aim of the present review is to introduce the reader to some of the physical notions and of the mathematical methods that are relevant to the study of nonlinear waves in Bose-Einstein Condensates (BECs). Upon introducing the general framework, we discuss the prototypical models that are relevant to this setting for different dimensions and different potentials confining the atoms. We analyze some of the model properties and explore their typical wave solutions (plane wave solutions, bright, dark, gap solitons, as well as vortices). We then offer a collection of mathematical methods that can be used to understand the existence, stability and dynamics of nonlinear waves in such BECs, either directly or starting from different types of limits (e.g., the linear or the nonlinear limit, or the discrete limit of the corresponding equation). Finally, we consider some special topics involving more recent developments, and experimental setups in which there is still considerable need for developing mathematical as well as computational tools.Comment: 69 pages, 10 figures, to appear in Nonlinearity, 2008. V2: new references added, fixed typo
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