Energy of the 9.17 MeV excited state of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow /><mml:mrow><mml:mn>14</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">N</mml:mi></mml:math>

Barker, P.H.; Scott, A.

doi:10.1103/physrevc.64.064305

Cited by 5 publications

(2 citation statements)

References 7 publications

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“…Excited states in 14 N were studied in a number of experiments. In most of the cases, the 13 C(p, γ) reaction was used [79][80][81][82][83][84], but also the 9 Be( 7 Li,2nγ) [85], the 12 C( 3 He,p) [86], and the 13 C(p, n) reactions [87] were explored.…”

Section: Experimental Data About 14 Nmentioning

confidence: 99%

Renewed Interest in Spectroscopy of the Lightest Doubly-Odd N = Z Nuclei

Kuşoğlu,

Balabanski

2023

QuBS

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The existing experimental data for the γ decay of the stable N=Z doubly-odd nuclei and the β decay of the corresponding isospin multiplets is reviewed. The structure of the lightest nuclei with masses A≤14 is used to test and constrain ab initio nuclear theories. Most of the data were obtained in the second half of the last century and, in some cases, lack the needed precision for comparison with theoretical calculations. Recent spectroscopic studies in the lightest doubly-odd N = Z nuclei are discussed, as well as open problems related to the understanding of their structures and ideas for future experiments.

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Section: Experimental Data About 14 Nmentioning

confidence: 99%

Renewed Interest in Spectroscopy of the Lightest Doubly-Odd N = Z Nuclei

Kuşoğlu,

Balabanski

2023

QuBS

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“…[6] The measurement of the resonance parameters for the 13 C(p, γ) 14 N reaction at E x = 9.17 MeV have been observed by several investigators, in which they have obtained the resonant energy and the total width. [3,7] The thick target yield of the 9.17-MeV gamma ray has been measured by Seagrave and Hanna, [5,8] using a Geiger-Muller counter and NaI detector, respectively. However, in the former, no correction has been made for the branch to other levels, while doubts were raised about the efficiency of the NaI detector for the 9.17-MeV γrays in the latter research.…”

Section: Introductionmentioning

confidence: 99%

New measurement of thick target yield for narrow resonance at E x = 9.17 MeV in the ¹³C( p , γ )¹⁴N reaction*

Dang¹,

Liu²,

Fu³

et al. 2019

Chinese Phys. B

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High energy γ-rays can be used in many fields, such as nuclear waste transmutation, flash photographics, and astrophysics. The 13C( p , γ )14N resonance reaction was used to generate high energy and mono-energetic γ-rays in this work. The thick-target yield of the 9.17-MeV γ-ray from the resonance in this reaction was determined to be (4.7±0.4) × 10 − 9 γ /proton, which was measured by a HPGe detector. Meanwhile, the angular distribution of 9.17-MeV γ-ray was also determined. The absolute efficiency of HPGe detector was calibrated using 56Co and 152Eu sources with known radioactive activities and calculated by GEANT4 simulation.

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