19,350 research outputs found

    Structure of super-families

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    At present the study of nuclear interactions induced by cosmic rays is the unique source of information on the nuclear interactions in the energy region above 10 to the 15th power eV. The phenomena in this energy region are observed by air shower arrays or emulsion chambers installed at high mountain. An emulsion chamber is the pile of lead plates and photo-sensitive layers (nuclear emulsion plates and/or X-ray films) used to detect electron showers. High spatial resolution of photographic material used in the emulsion chamber enables the observation of the phenomena in detail, and recent experiments of emulsion chamber with large area are being carried out at high mountain altitudes by several groups in the world

    Effective Theory Approach to the Skyrme model and Application to Pentaquarks

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    The Skyrme model is reconsidered from an effective theory point of view. From the most general chiral Lagrangian up to including terms of order p4p^4, NcN_c and Ī“m2\delta m^2 (Ī“mā‰”msāˆ’m\delta m\equiv m_s-m), new interactions, which have never been considered before, appear upon collective coordinate quantization. We obtain the parameter set best fitted to the observed low-lying baryon masses, by performing the second order perturbative calculations with respect to Ī“m\delta m. We calculate the masses and the decay widths of the other members of (mainly) anti-decuplet pentaquark states. The formula for the decay widths is reconsidered and its baryon mass dependence is clarified.Comment: 65 pages, 1 figure. Revised version:the complete second order perturbative calculations performed and two appendices adde

    Preparation of Neutron-activated Xenon for Liquid Xenon Detector Calibration

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    We report the preparation of neutron-activated xenon for the calibration of liquid xenon (LXe) detectors. Gamma rays from the decay of xenon metastable states, produced by fast neutron activation, were detected and their activities measured in a LXe scintillation detector. Following a five-day activation of natural xenon gas with a Cf-252 (4 x 10^5 n/s) source, the activities of two gamma ray lines at 164 keV and 236 keV, from Xe-131m and Xe-129m metastable states, were measured at about 95 and 130 Bq/kg, respectively. We also observed three additional lines at 35 keV, 100 keV and 275 keV, which decay away within a few days. No long-lifetime activity was observed after the neutron activation.Comment: to be published in NIM A, corrected typos in Table 1 and Fig.6 of the previous versio

    Maximal entanglement of two spinor Bose-Einstein condensates

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    Starting with two weakly-coupled anti-ferromagnetic spinor condensates, we show that by changing the sign of the coefficient of the spin interaction, U2U_{2}, via an optically-induced Feshbach resonance one can create an entangled state consisting of two anti-correlated ferromagnetic condensates. This state is maximally entangled and a generalization of the Bell state from two anti-correlated spin-1/2 particles to two anti-correlated spināˆ’N/2-N/2 atomic samples, where NN is the total number of atoms.Comment: 5 pages, 3 figures, accepted for publication in PR

    Molecular Hydrogen Emission Lines in Far Ultraviolet Spectroscopic Explorer Observations of Mira B

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    We present new Far Ultraviolet Spectroscopic Explorer (FUSE) observations of Mira A's wind-accreting companion star, Mira B. We find that the strongest lines in the FUSE spectrum are H2 lines fluoresced by H I Lyman-alpha. A previously analyzed Hubble Space Telescope (HST) spectrum also shows numerous Lyman-alpha fluoresced H2 lines. The HST lines are all Lyman band lines, while the FUSE H2 lines are mostly Werner band lines, many of them never before identified in an astrophysical spectrum. We combine the FUSE and HST data to refine estimates of the physical properties of the emitting H2 gas. We find that the emission can be reproduced by an H2 layer with a temperature and column density of T=3900 K and log N(H2)=17.1, respectively. Another similarity between the HST and FUSE data, besides the prevalence of H2 emission, is the surprising weakness of the continuum and high temperature emission lines, suggesting that accretion onto Mira B has weakened dramatically. The UV fluxes observed by HST on 1999 August 2 were previously reported to be over an order of magnitude lower than those observed by HST and the International Ultraviolet Explorer (IUE) from 1979--1995. Analysis of the FUSE data reveals that Mira B was still in a similarly low state on 2001 November 22.Comment: 23 pages, 6 figures; AASTEX v5.0 plus EPSF extensions in mkfig.sty; accepted by Ap

    Extremely high energy hadron and gamma-ray families(3). Core structure of the halo of superfamily

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    The study of the core structure seen in the halo of Mini-Andromeda 3(M.A.3), which was observed in the Chacaltaya emulsion chamber, is presented. On the assumption that lateral distribution of darkness of the core is exponential type, i.e., D=D0exp(-R/r0), subtraction of D from halo darkness is performed until the cores are gone. The same quantity on cores obtained by this way are summarized. The analysis is preliminary and is going to be developed

    Meeting in a Polygon by Anonymous Oblivious Robots

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    The Meeting problem for kā‰„2k\geq 2 searchers in a polygon PP (possibly with holes) consists in making the searchers move within PP, according to a distributed algorithm, in such a way that at least two of them eventually come to see each other, regardless of their initial positions. The polygon is initially unknown to the searchers, and its edges obstruct both movement and vision. Depending on the shape of PP, we minimize the number of searchers kk for which the Meeting problem is solvable. Specifically, if PP has a rotational symmetry of order Ļƒ\sigma (where Ļƒ=1\sigma=1 corresponds to no rotational symmetry), we prove that k=Ļƒ+1k=\sigma+1 searchers are sufficient, and the bound is tight. Furthermore, we give an improved algorithm that optimally solves the Meeting problem with k=2k=2 searchers in all polygons whose barycenter is not in a hole (which includes the polygons with no holes). Our algorithms can be implemented in a variety of standard models of mobile robots operating in Look-Compute-Move cycles. For instance, if the searchers have memory but are anonymous, asynchronous, and have no agreement on a coordinate system or a notion of clockwise direction, then our algorithms work even if the initial memory contents of the searchers are arbitrary and possibly misleading. Moreover, oblivious searchers can execute our algorithms as well, encoding information by carefully positioning themselves within the polygon. This code is computable with basic arithmetic operations, and each searcher can geometrically construct its own destination point at each cycle using only a compass. We stress that such memoryless searchers may be located anywhere in the polygon when the execution begins, and hence the information they initially encode is arbitrary. Our algorithms use a self-stabilizing map construction subroutine which is of independent interest.Comment: 37 pages, 9 figure

    Effective range from tetramer dissociation data for cesium atoms

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    The shifts in the four-body recombination peaks, due to an effective range correction to the zero-range model close to the unitary limit, are obtained and used to extract the corresponding effective range of a given atomic system. The approach is applied to an ultracold gas of cesium atoms close to broad Feshbach resonances, where deviations of experimental values from universal model predictions are associated to effective range corrections. The effective range correction is extracted, with a weighted average given by 3.9Ā±0.8RvdW\pm 0.8 R_{vdW}, where RvdWR_{vdW} is the van der Waals length scale; which is consistent with the van der Waals potential tail for the Cs2Cs_2 system. The method can be generally applied to other cold atom experimental setups to determine the contribution of the effective range to the tetramer dissociation position.Comment: A section for two-, three- and four-boson bound state formalism is added, accepted for publication in Phys. Rev.

    Learning to Eat Appreciatively and Thoughtfully (EAT): Connecting with Food through School Gardens

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    Many young people today do not learn to cook, or eat nutritious, regular meals together with their families, or go shopping for produce. Because of this, they do not have the opportunity to develop any real appreciation for food. To make matters worse, many public schools fail to teach students anything at all about the complex environmental and cultural history of food ā€“ how it is produced, preserved, prepared, and distributed. At the same time, schools serve lunches that often lack nutritional value. In this thesis, I argue the importance of giving students the opportunity to connect to food through school gardens and food education programs in schools. First, I trace the history and philosophical origins of school gardens, focusing particularly on the growth of school gardens and relevant literature at the turn of the 20th century and during the two world wars. I then examine the decline and subsequent rise of school gardens during the latter half of the 20th century and analyze two examples of current school gardening and food education programs in the United States: the Edible Schoolyard in Berkeley, California, and the Burlington School Food Project in Burlington, Vermont. Finally, I consider the feasibility of incorporating school gardens and food education into classrooms in Oberlinā€™s schools, and suggest that educating students to be ā€œfood literateā€ is one critical step towards addressing complex problems that we face today, including climate change and obesity
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