Determination of gamma-ray widths in $^{15}$N using nuclear resonance fluorescence
T. Sz\"ucs, D. Bemmerer, A. Caciolli, Zs. F\"ul\"op, R. Massarczyk, C., Michelagnoli, T. P. Reinhardt, R. Schwengner, M. P. Tak\'acs, C. A. Ur, A., Wagner, and L. Wagner

TL;DR
This study measured gamma-ray widths of $^{15}$N levels using nuclear resonance fluorescence, providing more precise data to improve understanding of nuclear properties relevant to astrophysics and nuclear physics.
Contribution
The paper presents new, highly precise measurements of $^{15}$N gamma-ray widths using NRF, updating and improving upon the limited data from previous studies and the 1991 compilation.
Findings
Gamma and proton widths consistent with literature
Improved precision in gamma-ray width measurements
Measured photon scattering cross sections for multiple levels
Abstract
The stable nucleus N is the mirror of O, the bottleneck in the hydrogen burning CNO cycle. Most of the N level widths below the proton emission threshold are known from just one nuclear resonance fluorescence (NRF) measurement, with limited precision in some cases. A recent experiment with the AGATA demonstrator array determined level lifetimes using the Doppler Shift Attenuation Method (DSAM) in O. As a reference and for testing the method, level lifetimes in N have also been determined in the same experiment. The latest compilation of N level properties dates back to 1991. The limited precision in some cases in the compilation calls for a new measurement in order to enable a comparison to the AGATA demonstrator data. The widths of several N levels have been studied with the NRF method. The solid nitrogen compounds enriched in N…
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