R. Hannaske

Nuclear deformation and neutron excess as competing effects for dipole strength in the pygmy region.

The electromagnetic dipole strength below the neutron-separation energy has been studied for the xenon isotopes with mass numbers A=124, 128, 132, and 134 in nuclear resonance fluorescence experiments using the γELBE bremsstrahlung facility at Helmholtz-Zentrum Dresden-Rossendorf and the HIγS facility at Triangle Universities Nuclear Laboratory Durham. The systematic study gained new information about the influence of the neutron excess as well as of nuclear deformation on the strength in the region of the pygmy dipole resonance. The results are compared with those obtained for the chain of molybdenum isotopes and with predictions of a random-phase approximation in a deformed basis. It turned out that the effect of nuclear deformation plays a minor role compared with the one caused by neutron excess. A global parametrization of the strength in terms of neutron and proton numbers allowed us to derive a formula capable of predicting the summed E1 strengths in the pygmy region for a wide mass range of nuclides.

Resonance strengths in the 14N(p,gamma)15O and 15N(p,alpha gamma)12C reactions

The 14N(p, \gamma)15O reaction is the slowest reaction of the carbon-nitrogen-oxygen cycle of hydrogen burning in stars. As a consequence, it determines the rate of the cycle. The 15N(p, \alpha \gamma)12C reaction is frequently used in inverse kinematics for hydrogen depth profiling in materials. The 14N(p, \gamma)15O and 15N(p, \alpha \gamma)12C reactions have been studied simultaneously, using titanium nitride targets of natural isotopic composition and a proton beam. The strengths of the resonances at Ep = 1058 keV in 14N(p, \gamma)15O and at Ep = 897 and 430 keV in 15N(p, \alpha \gamma)12C have been determined with improved precision, relative to the well-known resonance at Ep = 278 keV in 14N(p, \gamma)15O. The new recommended values are \omega \gamma = 0.353

Neutron total cross section measurements of gold and tantalum at the nELBE photoneutron source

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Measurement of the photodissociation of the deuteron at energies relevant to Big Bang nucleosynthesis

0.018, 362

EXPERIMENTS WITH NEUTRONS AND PHOTONS AT ELBE

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The resonance triplet at E_alpha = 4.5 MeV in the 40Ca(alpha,gamma)44Ti reaction

20, and 21.9

Resonance triplet atEα=4.5 MeV in the40Ca(α,γ)44Ti reaction

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Pygmy dipole strength in 86 Kr and systematics of N = 50 isotones

1.0 eV for their respective strengths. In addition, the branching ratios for the decay of the Ep = 1058 keV resonance in 14N(p, \gamma)15O have been redetermined. The data reported here should facilitate future studies of off-resonant capture in the 14N(p, \gamma)15O reaction that are needed for an improved R-matrix extrapolation of the cross section. In addition, the data on the 430 keV resonance in 15N(p, \alpha \gamma)12C may be useful for hydrogen depth profiling.

Electromagnetic dipole strength of 136Ba below the neutron separation energy

Neutron total cross sections of 197Au and natTa have been measured at the nELBE photoneutron source in the energy range 0.1–10MeV with a statistical uncertainty of up to 2% and a total systematic uncertainty of 1%. This facility is optimized for the fast neutron energy range and combines an excellent time structure of the neutron pulses (electron bunch width 5ps) with a short flight path of 7m. Because of the low instantaneous neutron flux transmission measurements of neutron total cross sections are possible, that exhibit very different beam and background conditions than found at other neutron sources.

Inelastic scattering of fast neutrons from excited states in 56Fe

The photodissociation of the deuteron is a key reaction in Big Bang nucleosynthesis, but is only sparsely measured in the relevant energy range. To determine the cross section of the d(γ,n)p reaction we used pulsed bremsstrahlung and measured the time-of-flight of the neutrons. In this article, we describe how the efficiency of the neutron detectors was experimentally determined and how the modification of the neutron spectrum by parts of the experimental setup was simulated and corrected.