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Program - Brookhaven National Laboratory

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of the setup. One option explored is to use PPAC’s (Parallel Plate Avalanche Detectors) which works very<br />

well for detecting fission fragments but requires more consideration for detecting protons and other deeply<br />

penetrating particles.<br />

[1] U. Tippawan et al., Phys. Rev. C 79, 064611 (2009). [2] R. Bevliacqua et al., Nucl. Instr. Meth. Phys.<br />

Res., A 646 100 (2011). [3] X. Ledoux et al., AIP Conf. Proc. 1412, 55 (2011).<br />

DB 7 5:30 PM<br />

Dipole Strength in Xenon Isotopes<br />

R. Massarczyk, R. Schwengner, A.R. Junghans<br />

Institute for Radiation Physics, Helmholtz-Zentrum Dresden-Rossendorf, 01314 Dresden, Germany<br />

The low-lying dipole strength in medium mass nuclei, which are known as typical fission products, was<br />

investigated in systematic studies using the photon-scattering facility at the electron accelerator of the<br />

Helmholtz-Zentrum Dresden-Rossendorf, Germany [1]. It has been shown, that the experimental strength<br />

found in (γ, γ) studies compared with phenomenological approximations used in statistical model calculations<br />

can have direct consequences for neutron capture cross sections [2] and the resulting deexcitation<br />

spectrum [3]. To investigate if the nuclear deformation has an influence on the dipole strength [4], especially<br />

in the energy region below the neutron-separation energy, we studied the photo-absorption cross<br />

sections of different isotopes in the xenon chain. Additional measurements at the HIγS facility at the Duke<br />

University, USA, allowed us to distinguish between electric and magnetic dipole strength. We will present<br />

experimental results from photon scattering experiments on the gaseous targets 124,128,134 Xe. These will<br />

be compared with results of experiments from other nuclei in the mass region around the closed neutron<br />

shell N = 82 [5,6,7]. The experiments are supported by Deutsche Forschungsgemeinschaft, Project No.<br />

SCHW883/1-1, the German BMBF project TRAKULA and the EURATOM FP7 project ERINDA.<br />

[1] R. Schwengner NIM A 555 211-219 (2005) [2] M. Beard et al. PRC 85, 065808 (2012) [3] G. Schramm<br />

et al. PRC 85, 014311 (2012) [4] A.R. Junghans et al. PLB 670 200-204 (2008) [5] R. Massarczyk et al.<br />

PRC 86, 014319 (2012) [6] A. Makinaga et al. PRC 82, 024314 (2010) [7] A. Tonchev et al. PRL 104,<br />

072501 (2010)<br />

DB 8 5:45 PM<br />

Absolute Cross Sections for Proton Induced Reactions on 147,149 Sm Below Coulomb Barrier<br />

A. Gheorghe, D. Filipescu, T. Glodariu, C. Mihai, D. Bucurescu, M. Ivascu, I. Cata-Danil, L. Stroe, D.<br />

Deleanu, D. G. Ghita, R. Lica, N. Marginean, R. Marginean, A. Negret, T. Sava, S. Toma, and N. V.<br />

Zamfir<br />

Horia Hulubei <strong>National</strong> Institute of Physics and Nuclear Engineering - IFIN HH<br />

M. Sin, O. Sima<br />

Nuclear Physics Department, University of Bucharest, Bucharest, Romania<br />

G. Cata-Danil<br />

Physics Department, University Politehnica of Bucharest, Bucharest, Romania<br />

The optical model parameters for charged particles (proton - alpha) are key ingredients in reaction cross<br />

sections evaluations widely used to calculate astrophysical reaction rates.These cross sections data may<br />

also be important to the extension of the nuclear data bases required by the development of the future<br />

generations of nuclear reactors. At incident energies below the Coulomb barrier, the predictions of different<br />

optical model parameterizations are tested against experimental cross sections for the (p,gamma) and (p,n)<br />

60

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