12 research outputs found

    Eta and eta-prime meson production in the reaction pn -> dM near threshold

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    The two-step model with pi-, rho- and omega- exchanges taken into account is applied to investigate the reactions pn -> d eta and pn -> d eta-prime. The existing experimental data on the reaction pn -> d eta are analysed and predictions for the cross section of the reaction pn -> d eta-prime are presented. It is found that pi- as well as rho exchange yield significant contributions in both reactions. The effect of the final state interaction is also studied.Comment: 15 pages, 4 figure

    Incoherent Photoproduction of η\eta-mesons from the Deuteron near Threshold

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    Incoherent photoproduction of the η\eta-meson on the deuteron is studied for photon energies from threshold to 800 MeV. The dominant contribution, the γ\gammaN-η\etaN amplitude, is described within an isobar model. The final state interaction derived from the CD-Bonn potential is included and found to be important for the description of the production cross section close to threshold. Possible effects from the ηN\eta N final state interaction are discussed.Comment: 11 pages, revtex, including 6 figure

    Eta Meson Production in NN Collisions

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    Eta meson production in both proton-proton and proton-neutron collisions is investigated within a relativistic meson exchange model of hadronic interactions. It is found that the available cross section data can be described equally well by either the vector or pseudoscalar meson exchange mechanism for exciting the S_{11}(1535) resonance. It is shown that the analyzing power data can potentially be very useful in distinguishing these two scenarios for the excitaion of the S_{11}(1535) resonance.Comment: Revtex, 35 pages, 8 figure

    Near-threshold ω\omega and ϕ\phi meson productions in pppp collisions

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    Using a relativistic effective Lagrangian at the hadronic level, near-threshold ω\omega and ϕ\phi meson productions in proton proton (pppp) collisions, ppppω/ϕp p \to p p \omega/\phi, are studied within the distorted wave Born approximation. Both initial and final state pppp interactions are included. In addition to total cross section data, both ω\omega and ϕ\phi angular distribution data are used to constrain further the model parameters. For the ppppωp p \to p p \omega reaction we consider two different possibilities: with and without the inclusion of nucleon resonances. The nucleon resonances are included in a way to be consistent with the πpωn\pi^- p \to \omega n reaction. It is shown that the inclusion of nucleon resonances can describe the data better overall than without their inclusion. However, the SATURNE data in the range of excess energies Q<31Q < 31 MeV are still underestimated by about a factor of two. As for the ppppϕp p \to p p \phi reaction it is found that the presently limited available data from DISTO can be reproduced by four sets of values for the vector and tensor ϕNN\phi NN coupling constants. Further measurements of the energy dependence of the total cross section near threshold energies should help to constrain better the ϕNN\phi NN coupling constant.Comment: Latex, 37 pages, 13 figures (14 EPS-figure files), text modified, version to appear in Phys. ReV.

    K− 3He and K− 4He interactions at low energies

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    Using the multiple scattering approach (MSA) in the fixed center approximation we calculated the K− 4He and K− 3He scattering lengths. The K− 4He scattering length is also analyzed in the optical potential model. Within the MSA the K− 3He final state interaction factor was also calculated. It is found that the K− 3He mass spectrum for the pd → 3HeK+ K− reaction is expected to be influenced by the K− 3He FSI effect

    Inclusive pentaquark and strange baryons production in hadron beam experiments at high energy

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    Determination of the <mml:math altimg="si1.gif" overflow="scroll" xmlns:xocs="http://www.elsevier.com/xml/xocs/dtd" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ja="http://www.elsevier.com/xml/ja/dtd" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:cals="http://www.elsevier.com/xml/common/cals/dtd"><mml:msup><mml:mover accent="true"><mml:mi>K</mml:mi><mml:mo>¯</mml:mo></mml:mover><mml:mn>0</mml:mn></mml:msup><mml:mi>d</mml:mi></mml:math> scattering length from the reaction <mml:math altimg="si2.gif" overflow="scroll" xmlns:xocs="http://www.elsevier.com/xml/xocs/dtd" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ja="http://www.elsevier.com/xml/ja/dtd" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:cals="http://www.elsevier.com/xml/common/cals/dtd"><mml:mi>p</mml:mi><mml:mi>p</mml:mi><mml:mo>→</mml:mo><mml:mi>d</mml:mi><mml:msup><mml:mover accent="true"><mml:mi>K</mml:mi><mml:mo>¯</mml:mo></mml:mover><mml:mn>0</mml:mn></mml:msup><mml:msup><mml:mi>K</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:math>

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