8 research outputs found

    Brueckner Rearrangement Effects in Λ5^5_\LambdaHe and ΛΛ6^6_{\Lambda\Lambda}He

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    Rearrangement effects in light hypernuclei are investigated in the framework of the Brueckner theory. We can estimate without detailed numerical calculations that the energy of the α\alpha-core is reduced by more than 2.5 MeV when the Λ\Lambda adheres to 4^4He to form Λ5^5_\LambdaHe. Similar assessment of rearrangement contributions is essential to deduce the strength of ΛΛ\Lambda\Lambda interaction from experimentally observed ΔBΛΛ\Delta B_{\Lambda\Lambda}. The recently observed experimental value of ∼\sim 1 MeV for the ΔBΛΛ\Delta B_{\Lambda\Lambda} of \hll suggests that the matrix element of in \hll is around -2 MeV.Comment: 7 pages, to appear in Phys. Rev.

    Structure of neutron-rich Λ\Lambda hypernuclei

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    Properties of light neutron-rich Λ\Lambda hypernuclei (Λ16^{16}_{\Lambda}C, Λ12^{12}_{\Lambda}Be, and Λ11^{11}_{\Lambda}Li) are calculated within the Skyrme-Hartree-Fock approach. Interplay between hypernuclear interaction features and properties of these hypernuclei is studied. Response of weakly bound neutron states to hyperon addition depends generally on core distortion by hyperon, and it is essentially different for the different states. This response is especially sensitive to details of the ΛN{\Lambda}N interaction for 1p1/21p_{1/2} states. Implications of the nuclear spin-orbit potential and nuclear incompressibility in the neutron-rich system properties are inferred. Dependence of the Λ\Lambda binding energies in hypernuclei on ZZ at fixed AA is discussed

    Exotic hypernuclear systems and heavy ion collisions

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    We discuss perspectives in hypernuclear studies opened by their integration with heavy ion physics. Particularly, neutron–rich Λ hypernuclei and double–Λ hypernucleican be produced, which are hardly attainable by traditional reactions and can enrich our knowledge on hadronic interactions

    Structure of neutron-rich Λ hypernuclei

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    Structures of S = −2 hypernuclei predicted by the ESC04 model

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