31 research outputs found

    Triton photodisintegration in three-dimensional approach

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    Two- and three- particles photodisintegration of the triton is investigated in a three-dimensional (3D) Faddeev approach. For this purpose the Jacobi momentum vectors for three particles system and spin-isospin quantum numbers of the individual nucleons are considered. Based on this picture the three-nucleon Faddeev integral equations with the two-nucleon interaction are formulated without employing the partial wave decomposition. The single nucleon current as well as π\pi- and ρ\rho- like exchange currents are used in an appropriate form to be employed in 3D approach. The exchange currents are derived from AV18 NN force. The two-body t-matrix, Deuteron and Triton wave functions are calculated in the 3D approach by using AV18 potential. Benchmarks are presented to compare the total cross section for the two- and three- particles photodisintegration in the range of Eγ<30MeVE_{\gamma}<30 MeV. The 3D Faddeev approach shows promising results

    Photodisintegration of the triton with realistic potentials

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    The process γ+tn+d\gamma + t \to n + d is treated by means of three-body integral equations employing in their kernel the W-Matrix representation of the subsystem amplitudes. As compared to the plane wave (Born) approximation the full solution of the integral equations, which takes into account the final state interaction, shows at low energies a 24% enhancement. The calculations are based on the semirealistic Malfliet-Tjon and the realistic Paris and Bonn B potentials. For comparison with earlier calculations we also present results for the Yamaguchi potential. In the low-energy region a remarkable potential dependence is observed, which vanishes at higher energies.Comment: 16 pages REVTeX, 8 postscript figures included, uses epsfig.st

    Photonuclear Reactions of Three-Nucleon Systems

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    We discuss the available data for the differential and the total cross section for the photodisintegration of 3^3He and 3^3H and the corresponding inverse reactions below Eγ=100E_\gamma = 100 MeV by comparing with our calculations using realistic NNNN interactions. The theoretical results agree within the errorbars with the data for the total cross sections. Excellent agreement is achieved for the angular distribution in case of 3^3He, whereas for 3^3H a discrepancy between theory and experiment is found.Comment: 11 pages (twocolumn), 12 postscript figures included, uses psfig, RevTe

    Energieverteilung und Ausbeute der Photo-?-Teilchen aus Al, Ar, Se und Ag

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    The Reaction4He(?p) T

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    Zum Kernphotoeffekt am Ar40 und Ar38

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    The (γ,p)-reaction in some light and medium weight nuclei

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    Energy Distributions of Photoprotons from Y 89

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