The ORNL Deuterated Spectroscopic Array — ODeSA

M. Febbraro, R. Toomey, S. D. Pain, K. A. Chipps, B. Becker, R. J. Newby, Z. Meisel, T. N. Massey, C. R. Brune, Q. Liu, R. J. deBoer, K. T. Macon, A. Boeltzig, J. O'Neill, M. S. Smith, M. Wiescher, D. Soltesz, I. Sultana, K. Brandenburg, S. SubediS. Paneru, T. Danley, Y. Alberty-Jones

Research output: Contribution to journalArticlepeer-review

9 Scopus citations

Abstract

An array consisting of 12 deuterated organic liquid scintillator detectors for fast-neutron spectroscopy was designed and built at Oak Ridge National Laboratory (ORNL). This versatile array is designed for measurements with low reaction yields, such as those performed with rare isotope beams, as well as at high current DC facilities used for underground nuclear astrophysics research. Because some measurements also offer limited, or no, additional timing information, the ORNL Deuterated Spectroscopic Array (ODeSA) was optimized to utilize spectrum unfolding to extract neutron energy spectra. This array was characterized for n/γ pulse shape discrimination, light response, resolution, and intrinsic efficiency by using the neutron time-of-flight tunnel at the Edwards Accelerator Laboratory at Ohio University. Results and future plans are discussed.

Funding

We gratefully thank the staff of the Ohio University Edwards Accelerator Laboratory for their assistance with experimental setup and operation of the accelerator. We would like to also thank Dr. Bildstein and Dr. Wang for providing their respective data sets. This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-AC05-00OR22725 and DE-FG02-88ER40387. Also, the National Nuclear Security Administration, United States of America under the Stewardship Science Academic Alliances program through DOE Cooperative Agreement No. DE-NA0002132, DE-NA0002905, and DE-NA00383, and National Science Foundation, United States of America grants PHY-1404218, and NSF-PHY-1812316. AB, RJD, KTM and MW acknowledge support by the National Science Foundation, United States of America through Grant No. Phys-1713857, and the Joint Institute for Nuclear Astrophysics, United States of America through Grant No. Phys-0822648 and PHY-1430152 (JINA Center for the Evolution of the Elements). We gratefully thank the staff of the Ohio University Edwards Accelerator Laboratory for their assistance with experimental setup and operation of the accelerator. We would like to also thank Dr. Bildstein and Dr. Wang for providing their respective data sets. This material is based upon work supported by the U.S. Department of Energy , Office of Science, Office of Nuclear Physics, under Award Number DE-AC05-00OR22725 and DE-FG02-88ER40387 . Also, the National Nuclear Security Administration, United States of America under the Stewardship Science Academic Alliances program through DOE Cooperative Agreement No. DE-NA0002132 , DE-NA0002905 , and DE-NA00383 , and National Science Foundation, United States of America grants PHY-1404218 , and NSF-PHY-1812316 . AB, RJD, KTM and MW acknowledge support by the National Science Foundation, United States of America through Grant No. Phys-1713857 , and the Joint Institute for Nuclear Astrophysics, United States of America through Grant No. Phys-0822648 and PHY-1430152 (JINA Center for the Evolution of the Elements).

Keywords

  • Deuterated scintillators
  • Neutron detection
  • Pulse shape discrimination
  • Radioactive Ion Beams
  • Spectrum unfolding

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