913 research outputs found

    Anomalous population of 10^{10}He states in reactions with 11^{11}Li

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    Structure with the lowest energy observed in the 10^{10}He spectrum populated in the proton knockout reaction with 11^{11}Li beam has a peak at 1.21.51.2-1.5 MeV. This peak is usually interpreted as a resonant 0+0^+ ground state of 10^{10}He. Our theoretical calculations indicate that this peak is likely to be a pileup of 11^-, 0+0^+, and 2+2^+ excitations with very similar shapes. %We predict a very specific nature of the 11^- excitation in 10^{10}He. Moreover, the ``soft'' 11^- excitation appears to be the lowest one in energy. Such an anomalous continuum response is traced to the halo structure of 11^{11}Li providing extreme low energy shift to all the expected continuum excitations. Competitions of the initial state structure (ISS) and the final state interaction (FSI) effects on the spectrum and three-body correlations in 10^{10}He are discussed. Analogous effect of the extreme low-energy shift could also be expected in other cases of 2n2n emitters populated in reactions with halo nuclei. Simplified example of the 10^{10}He spectrum in α\alpha knockout from 14^{14}Be, is given. We also discuss limits on the properties of 9^{9}He stemming from the observed 10^{10}He spectrum.Comment: 10 pages, 13 figure

    Scattering theory with finite-gap backgrounds: Transformation operators and characteristic properties of scattering data

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    We develop direct and inverse scattering theory for Jacobi operators (doubly infinite second order difference operators) with steplike coefficients which are asymptotically close to different finite-gap quasi-periodic coefficients on different sides. We give necessary and sufficient conditions for the scattering data in the case of perturbations with finite second (or higher) moment.Comment: 23 page

    Two-proton radioactivity and three-body decay. V. Improved momentum distributions

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    Nowadays quantum-mechanical theory allows one to reliably calculate the processes of 2p radioactivity (true three-body decays) and the corresponding energy and angular correlations up to distances of the order of 1000 fm. However, the precision of modern experiments has now become sufficient to indicate some deficiency of the predicted theoretical distributions. In this paper we discuss the extrapolation along the classical trajectories as a method to improve the convergence of the theoretical energy and angular correlations at very large distances (of the order of atomic distances), where only the long-range Coulomb forces are still operating. The precision of this approach is demonstrated using the "exactly" solvable semianalytical models with simplified three-body Hamiltonians. It is also demonstrated that for heavy 2p emitters, the 2p decay momentum distributions can be sensitive to the effect of the screening by atomic electrons. We compare theoretical results with available experimental data.Comment: 13 pages, 18 figure

    Scattering Theory for Jacobi Operators with Steplike Quasi-Periodic Background

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    We develop direct and inverse scattering theory for Jacobi operators with steplike quasi-periodic finite-gap background in the same isospectral class. We derive the corresponding Gel'fand-Levitan-Marchenko equation and find minimal scattering data which determine the perturbed operator uniquely. In addition, we show how the transmission coefficients can be reconstructed from the eigenvalues and one of the reflection coefficients.Comment: 14 page

    Azimuthal modulation of the event rate of cosmic ray extensive air showers by the geomagnetic field

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    The Earth's magnetic field effect on the azimuthal distribution of extensive air showers (EAS) of cosmic rays has been evaluated using a bulk of the Yakutsk array data. The uniform azimuthal distribution of the EAS event rate is rejected at the significance level 10^(-14). Amplitude of the first harmonics of observed distribution depends on zenith angle as A1=0.2*sin^2(theta) and is almost independent of the primary energy; the phase coincides with the magnetic meridian. Basing upon the value of measured effect, the correction factor has been derived for the particle density depending on a geomagnetic parameter of a shower.Comment: 4 pages, 3 figures in ps file

    Wildfire propagation modelling

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    Wildfires are a concrete problem with a strong impact on human life, property and the environment, because they cause disruption and are an important source of pollutants. Climate change and the legacy of poor management are responsible for wildfires increasing in occurrence and in extension of the burned area. Wildfires are a challenging task for research, mainly because of their multi-scale and multi-disciplinary nature. Wildfire propagation is studied in the literature by two alternative approaches: the reaction-diffusion equation and the front tracking level-set method. The solution of the reaction-diffusion equation is a smooth function with an infinite domain, while the level-set method generates a sharp function that is not zero inside a compact domain. However, these two approaches can indeed be considered complementary and reconciled. With this purpose we derive a method based on the idea to split the motion of the front into a drifting part and a fluctuating part. This splitting allows specific numerical and physical choices that can improve the models. In particular, the drifting part can be provided by chosen existing method (e.g. one based on the level-set method) and this permits the choice for the best drifting part. The fluctuating part is the result of a comprehensive statistical description of the physics of the system and includes the random effects, e.g., turbulent hot-air transport and fire-spotting. As a consequence, the fluctuating part can have a non-zero mean (for example, due to ember jump lengths), which means that the drifting part does not correspond to the average motion. This last fact distinguishes between the present splitting and the well-known Reynolds decomposition adopted in turbulence studies. Actually, the effective front emerges to be the weighted superposition of drifting fronts according to the probability density function of the fire-line displacement by random effects. The resulting effective process emerges to be governed by an evolution equation of the reaction-diffusion type. In this reconciled approach, the rate of spread of the fire keeps the same key and characterising role that is typical in the level-set approach. Moreover, the model emerges to be suitable for simulating effects due to turbulent convection, such as fire flank and backing fire, the faster fire spread being because of the actions by hot-air pre-heating and by ember landing, and also due to the fire overcoming a fire-break zone, which is a case not resolved by models based on the level-set method. A physical parametrization of fire-spotting is also proposed and numerical simulations are shown.PhD Grant "La Caixa 2014

    THE OPTIMAL PRINCIPLE OF BELLMAN IN THE PROBLEM OF OPTIMAL MEANS DISTRIBUTION BETWEEN ENTERPRISES FOR THE EXPANSION OF PRODUCTION

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    The method of dynamic programming has been considered, which is used in solving multiple problems in economics, on the example of using Bellman’s optimality principle for solving nonlinear programming problems. On a specific numerical example, the features of the solution have been shown in detail with all the calculations. The problem of optimal distribution of funds among enterprises for the expansion of production has been formulated, which would give the maximum total increase in output. The solution of the task has been presented in the case, when the number of enterprises is 3. It has been shown, that the Bellman optimality principle allows you solve applied problems of cost forecasting with obtaining the optimal solution-maximum profit at minimum costs

    From Coulomb excitation cross sections to non-resonant astrophysical rates in three-body systems: 17^{17}Ne case

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    Coulomb and nuclear dissociation of 17^{17}Ne on light and heavy targets are studied theoretically. The dipole E1 strength function is determined in a broad energy range including energies of astrophysical interest. Dependence of the strength function on different parameters of the 17^{17}Ne ground state structure and continuum dynamics is analyzed in a three-body model. The discovered dependence plays an important role for studies of the strength functions for the three-body E1 dissociation and radiative capture. The constraints on the [s2]/[d2][s^2]/[d^2] configuration mixing in 17^{17}Ne and on pp-wave interaction in the 15^{15}O+pp channel are imposed based on experimental data for 17^{17}Ne Coulomb dissociation on heavy target.Comment: 12 pages, 13 figure

    Beauty and standard appearance under globalization

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    This article deals with the perception of normative appearance in the conditions of culture globalization, and raises the question of the relationship between appearance and cultural identity in the context of globalizing processesРассматриваются вопросы восприятия нормативной внешности в условиях глобализации культуры, а также поднимается вопрос о соотношении внешности и культурной идентичности в контексте глобализирующих процессо
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