538 research outputs found

    This feels familiar

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    This is a book about in-betweenness. It’s an examination of how we identify people and objects, the categories we use to do so, and those that don’t fit squarely into one or the other. It considers the grey areas of identity--race, gender, species, function, living, inanimate. It slips and slides through the ambiguous and indefinite, forever moving, always simultaneously being “both,” “all,” “neither,” and “none.

    Multi-cluster dynamics in Λ13C^{13}_\Lambda{\rm C} and analogy to clustering in 12C^{12}{\rm C}

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    We investigate structure of Λ13C^{13}_\Lambda{\rm C} and discuss the difference and similarity between the structures of 12C^{12}{\rm C} and Λ13C^{13}_\Lambda{\rm C} by answering the questions if the linear-chain and gaslike cluster states, which are proposed to appear in 12C^{12}{\rm C}, survives, or new structure states appear or not. We introduce a microscopic cluster model called, Hyper-Tohsaki-Horiuchi-Schuck-R\"opke (H-THSR) wave function, which is an extended version of the THSR wave function so as to describe Λ\Lambda hypernuclei. We obtained two bound states and two resonance (quasi-bound) states for Jπ=0+J^\pi=0^+ in Λ13C^{13}_\Lambda{\rm C}, corresponding to the four 0+0^+ states in 12C^{12}{\rm C}. However, the inversion of level ordering between the spectra of 12C^{12}{\rm C} and Λ13C^{13}_\Lambda{\rm C}, i.e. that the 03+0_3^+ and 04+0_4^+ states in Λ13C^{13}_\Lambda{\rm C} correspond to the 04+0_4^+ and 03+0_3^+ states in 12C^{12}{\rm C}, respectively, is shown to occur. The additional Λ\Lambda particle reduces sizes of the 02+0_2^+ and 03+0_3^+ states in Λ13C^{13}_\Lambda{\rm C} very much, but the shrinkage of the 04+0_4^+ state is only a half of the other states. In conclusion, the Hoyle state becomes quite a compact object with Λ9Be+α{^{9}_\Lambda{\rm Be}}+\alpha configuration in Λ13C^{13}_\Lambda{\rm C} and is no more gaslike state composed of the 3α3\alpha clusters. Instead, the 04+0_4^+ state in Λ13C^{13}_\Lambda{\rm C}, coming from the 12C(03+)^{12}{\rm C}(0_3^+) state, appears as a gaslike state composed of α+α+Λ5He\alpha+\alpha+^{5}_\Lambda{\rm He} configuration, i.e. the Hoyle analog state. A linear-chain state in a Λ\Lambda hypernucleus is for the first time predicted to exist as the 03+0_3^+ state in Λ13C^{13}_\Lambda{\rm C} with more shrunk arrangement of the 3α3\alpha clusters along zz-axis than the 3α3\alpha linear-chain configuration realized in the 12C(04+)^{12}{\rm C}(0_4^+) state.Comment: 9 pages, 6 figures, figures rearranged, accepted for publication in PL

    Imaginary-time method for radiative capture reaction rate

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    We propose a new computational method for astrophysical reaction rate of radiative capture process. In the method, an evolution of a wave function is calculated along the imaginary-time axis which is identified as the inverse temperature. It enables direct evaluation of reaction rate as a function of temperature without solving any scattering problem. The method is tested for two-body radiative capture reaction, 16O(α,γ)20Ne{^{16}{\rm O}}(\alpha,\gamma){^{20}{\rm Ne}}, showing that it gives identical results to that calculated by the ordinary procedure. The new method will be suited for calculation of triple-alpha radiative capture rate for which an explicit construction of the scattering solution is difficult.Comment: 8 pages, 7 figure

    Analysis of previous microscopic calculations for second 0+0^+ state in 12^{12}C in terms of 3-alpha particle Bose-condensed state

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    The wave function of the second 0+0^+ state of 12^{12}C which was obtained long time ago by solving the microscopic 3α\alpha problem is shown to be almost completely equivalent to the wave function of the 3α\alpha condensed state which has been proposed recently by the present authors. This equivalence of the wave functions is shown to hold in two cases where different effective two-nucleon forces are adopted. This finding gives strong support for interpreting the second 0+0^+ state of 12^{12}C which is the key state for the synthesis of 12^{12}C in stars ('Hoyle' state), and which is one of the typical mysterious 0+0^+ states in light nuclei, as a gas-like structure of three α\alpha particles, Bose-condensed into an identical s-wave function.Comment: revtex, 5 pages, 2 figures, submitted to Phys. Rev.

    Fluctuations for the Ginzburg-Landau ϕ\nabla \phi Interface Model on a Bounded Domain

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    We study the massless field on Dn=D1nZ2D_n = D \cap \tfrac{1}{n} \Z^2, where DR2D \subseteq \R^2 is a bounded domain with smooth boundary, with Hamiltonian \CH(h) = \sum_{x \sim y} \CV(h(x) - h(y)). The interaction \CV is assumed to be symmetric and uniformly convex. This is a general model for a (2+1)(2+1)-dimensional effective interface where hh represents the height. We take our boundary conditions to be a continuous perturbation of a macroscopic tilt: h(x)=nxu+f(x)h(x) = n x \cdot u + f(x) for xDnx \in \partial D_n, uR2u \in \R^2, and f ⁣:R2Rf \colon \R^2 \to \R continuous. We prove that the fluctuations of linear functionals of h(x)h(x) about the tilt converge in the limit to a Gaussian free field on DD, the standard Gaussian with respect to the weighted Dirichlet inner product (f,g)β=Diβiifiigi(f,g)_\nabla^\beta = \int_D \sum_i \beta_i \partial_i f_i \partial_i g_i for some explicit β=β(u)\beta = \beta(u). In a subsequent article, we will employ the tools developed here to resolve a conjecture of Sheffield that the zero contour lines of hh are asymptotically described by SLE(4)SLE(4), a conformally invariant random curve.Comment: 58 page

    Determination of Pinning Parameters in Flux Creep-Flow Model for E-J characteristics of High Temperature Superconductors by using Differential Evolution

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    The pinning parameters such as strength of pinning force, temperature dependence of pinning force and so on using in flux creep-flow model to explain electric field vs current density (E-J) characteristics were determined by Differential Evolution (DE). DE is one of the methods in Evolutionary Computation (EC) to find an optimization of a problem. First, a model data of E-J characteristics in which the pinning parameters were given was prepared, and it was confirmed that DE can find the given pinning parameters from the model data. Then, DE and mesh method were used to determine the pinning parameters in experimental E-J characteristics of GdBa2CuO7-δ high temperature superconductor. In mesh method, the all combinations of pinning parameters with constant interval for each parameter are calculated, and best set of pinning parameters is selected. It was found that DE shows better performance than mesh method in terms of calculation time and accuracy for determining pinning parameters

    Nuclear Alpha-Particle Condensates

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    The α\alpha-particle condensate in nuclei is a novel state described by a product state of α\alpha's, all with their c.o.m. in the lowest 0S orbit. We demonstrate that a typical α\alpha-particle condensate is the Hoyle state (Ex=7.65E_{x}=7.65 MeV, 02+0^+_2 state in 12^{12}C), which plays a crucial role for the synthesis of 12^{12}C in the universe. The influence of antisymmentrization in the Hoyle state on the bosonic character of the α\alpha particle is discussed in detail. It is shown to be weak. The bosonic aspects in the Hoyle state, therefore, are predominant. It is conjectured that α\alpha-particle condensate states also exist in heavier nαn\alpha nuclei, like 16^{16}O, 20^{20}Ne, etc. For instance the 06+0^+_6 state of 16^{16}O at Ex=15.1E_{x}=15.1 MeV is identified from a theoretical analysis as being a strong candidate of a 4α4\alpha condensate. The calculated small width (34 keV) of 06+0^+_6, consistent with data, lends credit to the existence of heavier Hoyle-analogue states. In non-self-conjugated nuclei such as 11^{11}B and 13^{13}C, we discuss candidates for the product states of clusters, composed of α\alpha's, triton's, and neutrons etc. The relationship of α\alpha-particle condensation in finite nuclei to quartetting in symmetric nuclear matter is investigated with the help of an in-medium modified four-nucleon equation. A nonlinear order parameter equation for quartet condensation is derived and solved for α\alpha particle condensation in infinite nuclear matter. The strong qualitative difference with the pairing case is pointed out.Comment: 71 pages, 41 figures, review article, to be published in "Cluster in Nuclei (Lecture Notes in Physics) - Vol.2 -", ed. by C. Beck, (Springer-Verlag, Berlin, 2011
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