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Program - Brookhaven National Laboratory

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HF 8 5:45 PM<br />

Beta-delayed Neutron Spectroscopy Using Trapped Ions<br />

R.M. Yee, E.B. Norman, LLNL/UC Berkeley. N.D. Scielzo, S. Padgett, M. Pedretti, LLNL. J.A. Clark,<br />

J.P. Greene, A.F. Levand, A. Perez-Galvan, B.J. Zabransky, ANL. S. Caldwell, G. Savard, M.G.<br />

Sternberg, J. Van Schelt, ANL/U Chicago. D. Lascar, R.E. Segel, ANL/Northwestern University. K.S.<br />

Sharma, U. Manitoba.<br />

Beta-delayed neutron emission is of interest to both the pure and applied nuclear physics communities. For<br />

example, branching ratios are needed to determine how the short-lived neutron-rich isotopes synthesized<br />

in the astrophysical r-process decay back to stability. Also, neutron energy spectra are required for the<br />

design of nuclear reactors. Reliable measurements of delayed neutron properties can be performed with<br />

high precision using a combination of sophisticated ion-trapping techniques and modern radiation-detection<br />

systems. When a radioactive ion decays in the trap, the recoil-daughter nucleus and emitted particles<br />

emerge from the ¡ 1 mm 3 trap volume with minimal scattering and propagate unobstructed through vacuum.<br />

These properties allow the momentum and energy of the emitted neutron to be precisely reconstructed<br />

from the nuclear recoil. Spectroscopy of delayed neutrons can be performed with high efficiency and energy<br />

resolutions approaching 3%. The results from a recent campaign to measure delayed neutron properties of<br />

interest to nuclear reactors and r-process nucleosynthesis will be presented. On-going activities to develop<br />

a dedicated ion trap and detector system to perform new measurements at CARIBU will be discussed. This<br />

work was supported by U.S. DOE under Contracts DE-AC02-06CH11357 (ANL), DE-AC52-07NA27344<br />

(LLNL), and the Department of Homeland Security.<br />

Session IA Plenary Wednesday<br />

Wednesday March 6, 2013<br />

Room: Met East at 8:30 AM<br />

IA 1 8:30 AM<br />

Physics of Neutron Interaction with U-238 Nucleus: New Developments and Challenges<br />

R. Capote<br />

International Atomic Energy Agency, NAPC-Nuclear Data Section<br />

M. Sin<br />

University of Bucharest, Romania<br />

A. Trkov<br />

Jozef Stefan Institute, Slovenia<br />

M.W. Herman<br />

<strong>National</strong> Nuclear Data Center, <strong>Brookhaven</strong> <strong>National</strong> <strong>Laboratory</strong>, USA<br />

The latest release of the EMPIRE-3.1 system (codename Rivoli) is being used in the advanced modeling of<br />

neutron induced reactions on U-238 nucleus aimed at improving our knowledge of the neutron scattering<br />

and prompt fission neutron emission. The reaction model includes - a new rotational-vibrational dispersive<br />

optical model potential couplings the low-lying collective bands of vibrational character observed in eveneven<br />

actinides; - the Engelbretch-Weidenmuller transformation allowing for inclusion of compound-direct<br />

interference effects enhanced by a dispersive treatment of the optical model potential; - a multi-humped<br />

fission barrier with absorption in the secondary well described within the optical model for fission; -<br />

135

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