Orbit-space sensitivity of two-step reaction gamma-ray spectroscopy

Abstract We calculate the orbit-space sensitivity of two-step reaction gamma-ray spectroscopy diagnostics in toroidally symmetric magnetic equilibria, using the reaction between alpha particles and beryllium-9 as an example. To reduce the computational cost, we use analytical solutions obtained by neglecting the velocity of the thermal beryllium. The sensitivity is quantified by weight functions, which we calculate in the alpha-particle orbit space of energy, maximum major radius and pitch at that maximum major radius. Each alpha-particle guiding-center orbit leads to a characteristic gamma-ray spectrum depending on the line-of-sight geometry. We highlight the geometry dependence by repeating the calculation for three different cases, observing significant changes in the sensitivity patterns. Weight functions also allow one to quickly compute forward model problems if spectra from many distribution functions are to be calculated and compared with experimental measurements.

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Publication Details

Journal
Nuclear Fusion
Published
2025-09-01
DOI
https://doi.org/10.1088/1741-4326/ae013d
Citations
2
Primary Topic
Nuclear Physics and Applications
Type
article
Field-Weighted Citation Impact
3.77

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Orbit-space sensitivity of two-step reaction gamma-ray spectroscopy

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Orbit-space sensitivity of two-step reaction gamma-ray spectroscopy

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article en
2 citations

Abstract

Abstract We calculate the orbit-space sensitivity of two-step reaction gamma-ray spectroscopy diagnostics in toroidally symmetric magnetic equilibria, using the reaction between alpha particles and beryllium-9 as an example. To reduce the computational cost, we use analytical solutions obtained by neglecting the velocity of the thermal beryllium. The sensitivity is quantified by weight functions, which we calculate in the alpha-particle orbit space of energy, maximum major radius and pitch at that maximum major radius. Each alpha-particle guiding-center orbit leads to a characteristic gamma-ray spectrum depending on the line-of-sight geometry. We highlight the geometry dependence by repeating the calculation for three different cases, observing significant changes in the sensitivity patterns. Weight functions also allow one to quickly compute forward model problems if spectra from many distribution functions are to be calculated and compared with experimental measurements.

Nuclear FusionVol. 65(11)
Uppsala University (SE), University of Helsinki (FI), Helsinki Institute of Physics (FI), Culham Centre for Fusion Energy (GB), Finland University (FI), Czech Academy of Sciences, Institute of Plasma Physics (CZ), Max Planck Institute for Plasma Physics - Greifswald (DE), 358 (Finland) (FI), Laboratoire de Physique des Plasmas (FR), Oak Ridge Institute for Science and Education, University of Milano-Bicocca (IT), VTT Technical Research Centre of Finland (FI), Technical University of Denmark (DK)
EUROfusion, Academy of Finland
Openalex Percentile: Top 6%
Nuclear Physics and Applications
3.77
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