Activation cross section measurement of the 14N(p,gamma)15O astrophysical key reaction

TL;DR

This study measures the total 14N(p,gamma)15O cross section using a novel activation method over a wide energy range, providing data crucial for accurate astrophysical reaction rate extrapolations.

Contribution

It introduces a new activation-based experimental approach to measure the 14N(p,gamma)15O cross section, complementing existing data and improving the reliability of astrophysical models.

Findings

Measured cross section between 550 keV and 1400 keV with 10% uncertainty.

Found agreement with recent data when including weak transitions.

Provides data to better constrain low-energy extrapolations for astrophysics.

Abstract

14N(p,gamma)15O is one of the key reactions of nuclear astrophysics playing a role in various stellar processes and influencing energy generation of stars, stellar evolution and nucleosynthesis. For a reliable reaction rate calculation the low energy cross section of 14N(p,gamma)15O must be known with high accuracy. Owing to the unmeasurable low cross sections, theoretical calculations are unavoidable. High precision experimental cross section data are needed in a wide energy range in order to provide the necessary basis for low energy extrapolations. In the present work the total 14N(p,gamma)15O cross section was measured with a method complementary to the available data sets. The cross section was measured with activation, based on the detection of the annihilation radiation following the beta+ decay of the reaction product 15O. This method, which provides directly the astrophysically important total cross section, was never used for the 14N(p,gamma)15O cross section measurement in the studied energy range. The non-resonant cross section was measured between 550 keV and 1400 keV center-of-mass energies with total uncertainty of about 10%. The results were compared with literature data using an R-matrix analysis. It is found that the cross sections measured in this work are in acceptable agreement with the two recent measurements only if the weak transitions - not measured in those works - are included. The present data set, being largely independent from the other available data, can be used to constrain the extrapolated cross sections to astrophysical energies and helps to make the astrophysical model calculations more reliable.