23,212 research outputs found

    Magnetic and axial-vector transitions of the baryon antidecuplet

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    We report the recent results of the magnetic transitions and axial-vector transitions of the baryon antidecuplet within the framework of the chiral quark-soliton model. The dynamical model parameters are fixed by experimental data for the magnetic moments of the baryon octet, for the hyperon semileptonic decay constants, and for the singlet axial-vector constant. The transition magnetic moments ÎŒÎ›ÎŁ\mu_{\Lambda\Sigma} and ÎŒNΔ\mu_{N\Delta} are well reproduced and other octet-decuplet and octet-antidecuplet transitions are predicted. In particular, the present calculation of ÎŒÎŁÎŁâˆ—\mu_{\Sigma\Sigma^*} is found to be below the upper bound 0.82ÎŒN0.82\mu_N that the SELEX collaboration measured very recently. The results explains consistently the recent findings of a new N∗N^* resonance from the GRAAL and Tohoku LNS group. We also obtain the transition axial-vector constants for the Θ+→KN\Theta^+\to KN from which the decay width of the Θ+\Theta^{+} pentaquark baryon is determined as a function of the pion-nucleon sigma term ÎŁÏ€N\Sigma_{\pi N}. We investigate the dependence of the decay width of the Θ+\Theta^{+} on the gA(0)g_{A}^{(0)}, with the gA(0)g_{A}^{(0)} varied within the range of the experimental uncertainty. We show that a small decay width of the Θ+→KN\Theta^{+}\to KN, i.e. ΓΘKN≀1\Gamma_{\Theta KN} \leq 1 MeV, is compatible with the values of all known semileptonic decays with the generally accepted value of gA(0)≈0.3g_{A}^{(0)} \approx 0.3 for the proton.Comment: 8 pages, 5 figures, Talk given at the Yukawa International Seminar (YKIS) 2006, "New frontiers in QCD", Kyoto, Japan, 20 Nov. - 8 Dec. 200

    Pion form factors with improved infrared factorization

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    We calculate electromagnetic pion form factors with an analytic model for αs(Q2)\alpha_{\rm s}(Q^2) which is infrared (IR) finite without invoking a ``freezing'' hypothesis. We show that for the asymptotic pion distribution amplitude, Fπ0γ∗γF_{\pi ^{0}\gamma ^{*}\gamma} agrees well with the data, whereas the IR-enhanced hard contribution to FπF_{\pi} and the soft (nonfactorizing) part can jointly account for the data.Comment: 12 pages; 3 figures as PS files (1 figure added); modified text; added references. To appear in Phys. Lett.

    Production of the pentaquark Θ+\Theta^+ in npnp scattering

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    We study np→ΛΘ+np\to \Lambda\Theta^{+} and np→Σ0Θ+np\to \Sigma^{0}\Theta^{+} processes for both of the positive and negative parities of the Θ+\Theta^{+}. Employing the effective chiral Lagrangians for the KNYKNY and K∗NYK^*NY interactions, we calculate differential cross sections as well as total cross sections for the np→Σ0Θ+np\to \Sigma^0 \Theta^+ and np→ΛΘ+np\to \Lambda\Theta^+ reactions. The total cross sections for the positive-parity Θ+\Theta^+ turn out to be approximately ten times larger than those for the negative parity Θ+\Theta^+ in the range of the CM energy sth≀s≀3.5GeV\sqrt{s}_{\rm th}\le \sqrt{s}\le 3.5 {\rm GeV}. The results are rather sensitive to the mechanism of KK exchanges in the tt -- channel.Comment: 9 pages and 11 figure

    Magnetic moments of exotic pentaquark baryons

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    In this talk, we present our recent investigation on the magnetic moments of the exotic pentaquark states, based on the chiral quark-soliton model, all relevant intrinsic parameters being fixed by using empirical data.Comment: 5 pages, 1 figure, a talk presented at the 10th International Conference on Baryons (Baryons04), Palaiseau, October 25-29, 200

    Cug2 is essential for normal mitotic control and CNS development in zebrafish.

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    Background: We recently identified a novel oncogene, Cancer-upregulated gene 2 (CUG2), which is essential for kinetochore formation and promotes tumorigenesis in mammalian cells. However, the in vivo function of CUG2 has not been studied in animal models. Results: To study the function of CUG2 in vivo, we isolated a zebrafish homologue that is expressed specifically in the proliferating cells of the central nervous system (CNS). Morpholino-mediated knockdown of cug2 resulted in apoptosis throughout the CNS and the development of neurodegenerative phenotypes. In addition, cug2-deficient embryos contained mitotically arrested cells displaying abnormal spindle formation and chromosome misalignment in the neural plate. Conclusions: Therefore, our findings suggest that Cug2 is required for normal mitosis during early neurogenesis and has functions in neuronal cell maintenance, thus demonstrating that the cug2 deficient embryos may provide a model system for human neurodegenerative disorders

    The Effect of the Random Magnetic Field Component on the Parker Instability

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    The Parker instability is considered to play important roles in the evolution of the interstellar medium. Most studies on the development of the instability so far have been based on an initial equilibrium system with a uniform magnetic field. However, the Galactic magnetic field possesses a random component in addition to the mean uniform component, with comparable strength of the two components. Parker and Jokipii have recently suggested that the random component can suppress the growth of small wavelength perturbations. Here, we extend their analysis by including gas pressure which was ignored in their work, and study the stabilizing effect of the random component in the interstellar gas with finite pressure. Following Parker and Jokipii, the magnetic field is modeled as a mean azimuthal component, B(z)B(z), plus a random radial component, Ï”(z)B(z)\epsilon(z) B(z), where Ï”(z)\epsilon(z) is a random function of height from the equatorial plane. We show that for the observationally suggested values of 1/2^{1/2}, the tension due to the random component becomes important, so that the growth of the instability is either significantly reduced or completely suppressed. When the instability still works, the radial wavenumber of the most unstable mode is found to be zero. That is, the instability is reduced to be effectively two-dimensional. We discuss briefly the implications of our finding.Comment: 10 pages including 2 figures, to appear in The Astrophysical Journal Letter
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