1,016 research outputs found

    Neutron--Antineutron Oscillations at the Surface of Nuclei

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    We discuss some aspects of possible neutron--antineutron oscillations in nuclei. The phenomenon occurs mostly at the surface of nuclei, and hence {\sl i)} is not very sensitive to medium corrections and {\sl ii)} makes use of the antinucleon-nucleus interaction in a region probed by experiments at CERN.Comment: Contr. Oak Ridge Workshop on Workshop on Baryon Instability, Latex, 4 pages, comments to [email protected]

    Widths of Ξ\Xi Hypernuclear States

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    The Λ\Lambda and neutron decay widths of Ξ\Xi hypernuclear states, based on calculated \Xi N \to \lala mixing amplitudes, are estimated. The widths which result from using the Nijmegen Model D interaction are sufficiently small, of order 1.5 MeV, that experiments to observe Ξ\Xi hypernuclear states using the (K,K+)(K^-,K^+) reaction may be feasible.Comment: 20 pages, LaTex with one postscript figure in accompanying file, to appear in Progress of Theoretical Physics Supplement No. 11

    Limits on \boldmath n {\bar n} oscillations from nuclear stability

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    The relationship between the lower limit on the nuclear stability lifetime as derived from the non disappearance of `stable` nuclei (Td  5.4 × 1031T_{d}~\gtrsim~5.4~\times~10^{31} yr), and the lower limit thus implied on the oscillation time (τnnˉ)(\tau_{n \bar n}) of a possibly underlying neutron-antineutron oscillation process, is clarified by studying the time evolution of the nuclear decay within a simple model which respects unitarity. The order-of-magnitude result τnnˉ2(Td/Γnˉ)1/2>2×108\tau_{n \bar n} \approx 2 (T_{d}/\Gamma_{\bar n})^{1/2} > 2 \times 10^{8} sec, where Γnˉ\Gamma_{\bar n} is a typical nˉ\bar n nuclear annihilation width, agrees as expected with the limit on τnnˉ\tau_{n \bar n} established by several detailed nuclear physics calculations, but sharply disagreeing by 15 orders of magnitude with a claim published recently in Phys. Rev. CRAP.Comment: 8 pages; this PRC version (accepted for publication, November 4 1999) differs from the original version only by a few minor editorial change

    The influence of strength of hyperon-hyperon interactions on neutron star properties

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    An equation of state of neutron star matter with strange baryons has been obtained. The effects of the strength of hyperon-hyperon interactions on the equations of state constructed for the chosen parameter sets have been analyzed. Numerous neutron star models show that the appearance of hyperons is connected with the increasing density in neutron star interiors. The performed calculations have indicated that the change of the hyperon-hyperon coupling constants affects the chemical composition of a neutron star. The obtained numerical hyperon star models exclude large population of strange baryons in the star interior.Comment: 18 pages, 22 figures, accepted to be published in Journal of Physics G: Nuclear and Particle Physic

    Loosely bound hyperons in the SU(3) Skyrme model

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    Hyperon pairs bound in deuteron like states are obtained within the SU(3) Skyrme model in agreement with general expectations from boson exchange models. The central binding from the flavor symmetry breaking terms increases with the strangeness contents of the interacting baryons whereas the kinetic non-linear σ\sigma-model term fixes the spin and isospin of the bound pair. We give a complete account of the interactions of octet baryons within the product approximation to baryon number B=2B=2 configurations.Comment: 35 pages REVTEX including 2 figs, with 3 further figs available on request from [email protected] or from [email protected] SI-94-TP3S2; STPHY-Th/94-
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