The upgraded summing NaI(Tl) (SuN++) absorption spectrometer

Simulations of astrophysical processes require a plethora of nuclear physics input. In particular, models of neutron-capture nucleosynthesis like the s, i, and r processes require β-decay information and experimentally constrained neutron-capture reaction rates. Past experiments with the 4π Summing NaI(Tl) (SuN) total absorption spectrometer have provided these physics quantities. Here, we outline an upgrade of SuN to SuN++, where 20 new segments (12 NaI(Tl) and 8 CeBr3) have been integrated into the pre-existing SuN total absorption spectrometer to provide increased energy and time resolution in β-decay experiments. The details of the newly upgraded SuN++ total absorption spectrometer are discussed with results from the commissioning experiment at the Facility for Rare Isotope Beams (FRIB) utilizing a 70Cu beam.

Authors

Publication Details

Journal
Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment
Published
2025-08-15
DOI
https://doi.org/10.1016/j.nima.2025.170930
Citations
1
Primary Topic
Nuclear physics research studies
Type
article
Field-Weighted Citation Impact
1.87

Funders

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The upgraded summing NaI(Tl) (SuN++) absorption spectrometer

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Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment
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article

The upgraded summing NaI(Tl) (SuN++) absorption spectrometer

A. Tsantiri, G. Owens-Fryar, Matthew R. Mumpower, T. H. Ogunbeku, Scott E. Campbell, R. Jain, N. D. Gamage, Xiangcheng Chen, D. P. Scriven, A. A. Doetsch, H. Arora, B. Greaves, M.K. Smith, M. Wiedeking, R.J. Coleman, A. C. Hartley, Howard C. Berg, E. Good, A. Richard, R. Ringle, Johan Emil Linnestad Larsson, M. J. Mogannam, Chris M. Ireland, C. Sumithrarachchi, D. L. Bleuel, T. Gaballah, R. S. Lubna, A. Spyrou, S. N. Liddick, B. P. Crider, F.M. Maier, E. K. Ronning, S. Uthayakumaar, C. Izzo, P. A. DeYoung, A. Sweet, J. M. Berkman, H. Erington, John C. Huffman, Kyle Taft, K. Bosmpotinis
article en
1 citations

Abstract

Simulations of astrophysical processes require a plethora of nuclear physics input. In particular, models of neutron-capture nucleosynthesis like the s, i, and r processes require β-decay information and experimentally constrained neutron-capture reaction rates. Past experiments with the 4π Summing NaI(Tl) (SuN) total absorption spectrometer have provided these physics quantities. Here, we outline an upgrade of SuN to SuN++, where 20 new segments (12 NaI(Tl) and 8 CeBr3) have been integrated into the pre-existing SuN total absorption spectrometer to provide increased energy and time resolution in β-decay experiments. The details of the newly upgraded SuN++ total absorption spectrometer are discussed with results from the commissioning experiment at the Facility for Rare Isotope Beams (FRIB) utilizing a 70Cu beam.

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated EquipmentVol. 1082
National Science Foundation, U.S. Department of Energy, Murray State University, Canada Foundation for Innovation, Office of Science, National Nuclear Security Administration, Natural Sciences and Engineering Research Council of Canada, Office of Defense Nuclear Nonproliferation, Nuclear Physics, Laboratory Directed Research and Development, Lawrence Livermore National Laboratory
Affordable and clean energy
Openalex Percentile: Top 12%
Nuclear physics research studies
1.87
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