Program - Brookhaven National Laboratory
Program - Brookhaven National Laboratory
Program - Brookhaven National Laboratory
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purity of the sources. A brief summary of the latest results of the measurements using a new segmented<br />
total absorption spectrometer, the faced challenges depending of the particular nuclei as well as new developments<br />
of the techniques of analysis will be discussed. The impact of the measurements on summation<br />
calculations of the decay heat in reactors and in nuclear structure will be addressed [2,3,4]. Future plans<br />
and the development of a new modular TAS detector (DTAS) for the DEcay SPECtroscopy (DESPEC)<br />
experiment at FAIR will also be presented.<br />
[1] A. Algora et al., Phys. Rev. Letts. 105 (2010) 202501 [2] A. Petrovici private communication [3] K-L.<br />
Kratz, private communication [4] A. Sonzogni, private communication<br />
DD 2 4:00 PM<br />
First Results from the Modular Total Absorption Spectrometer at the HRIBF (ORNL,<br />
Oak Ridge)*<br />
M. Karny, Faculty of Physics, University of Warsaw, Warsaw, Poland; ORNL, Oak Ridge, USA; ORAU,<br />
Oak Ridge, USA. A. Fijalkowska, Faculty of Physics, University of Warsaw, Warsaw, Poland; University<br />
of Tennessee, Knoxville, USA. K.P. Rykaczewski, ORNL, Oak Ridge, USA. M. Wolińska-Cichocka,<br />
ORNL, Oak Ridge, USA; ORAU, Oak Ridge, USA. B.C. Rasco, Louisiana State University, Baton<br />
Rouge, USA. C.J. Gross, ORNL, Oak Ridge, USA. R.K. Grzywacz, University of Tennessee, Knoxville,<br />
USA; ORNL, Oak Ridge, USA. L. Cartegni, University of Tennessee, Knoxville, USA. R. Goans, ORNL,<br />
Oak Ridge, USA. K.C. Goetz, University of Tennessee, Knoxville, USA. J. W. Johnson, ORNL, Oak<br />
Ridge, USA. J.H. Hamilton, Dept. of Physics and Astronomy, Vanderbilt University, Nashville, USA. C.<br />
Jost, ORAU, Oak Ridge, USA. M. Madurga, University of Tennessee, Knoxville, USA. K. Miernik,<br />
Faculty of Physics, University of Warsaw, Warsaw, Poland; ORNL, Oak Ridge, USA. D. Miller,<br />
University of Tennessee, Knoxville, USA. S.W. Padgett, University of Tennessee, Knoxville, USA. S.V.<br />
Paulauskas, University of Tennessee, Knoxville, USA. A.V. Ramayya, Dept. of Physics and Astronomy,<br />
Vanderbilt University, Nashville, USA. M. Al-Shudifat, University of Tennessee, Knoxville, USA. E.<br />
Spejewski, ORAU, Oak Ridge, USA. D. Stracener, ORNL, Oak Ridge, USA. E. Zganjar, Louisiana State<br />
University, Baton Rouge, USA.<br />
Total Absorption Spectrometers (TAS) capable of detecting most of the gamma transitions occurring during<br />
the decay process are perfect tools for establishing a true beta feeding pattern. TAS-aided experiments are<br />
particularly important for neutron-rich nuclei, where the beta strength is highly distributed over many final<br />
states. Knowledge of the correct beta feeding pattern is important for the analysis of the structure of parent<br />
and daughter activities as well as for the determination of the decay heat released by fission products during<br />
nuclear fuel cycle. The Modular Total Absorption Spectrometer (MTAS) has been recently constructed<br />
at the Holifield Radioactive Ion Beam Facility (HRIBF) at Oak Ridge <strong>National</strong> <strong>Laboratory</strong>. It consists of<br />
19 NaI(Tl) hexagonal shape modules, with a full energy gamma ray efficiency approaching 90% around<br />
300 keV [1]. The decays of over twenty 238 U fission products have been studied with MTAS during the<br />
first online experiment at the HRIBF. Already online data for some isotopes show significant discrepancy<br />
between the observed beta feeding and the corresponding database values. In this contribution the first<br />
results for nuclei with mass ranging from 86 to 90, including 86,87 Br, 89,90 Kr, will be presented. The impact<br />
of this new data on the decay heat calculation will be discussed as well. ∗ This work was supported by the<br />
U.S. Department of Energy Office of Nuclear Physics.<br />
[1] M. Wolińska-Cichocka et al., ”Modular total Absorption Spectrometer at HRIBF”, this conference<br />
DD 3 4:20 PM<br />
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