We analyze the 115In 8-decay energy spectrum through the spectral moment method (SMM), previously introduced in the context of 113Cd 8 decay. The spectral moments mu n are defined as averaged nth powers of the 8 particle energy, characterizing the spectrum normalization (n = 0) and shape (n 1) above a given threshold. For 115In, we consider three independent datasets characterized by different thresholds. We also consider three nuclear model calculations with two free parameters: the ratio of axial-vector to vector couplings, r = gA/gV, and the small vector-like relativistic nuclear matrix element (NME), s = s-NME. By using the most recent of the three datasets, we show that the first few spectral moments can determine (r, s) values in good agreement with those obtained by full-fledged experimental fits. We then work out the SMM results for the other datasets. We find that, although gA quenching is generally favored, the preferred quenching factors may differ considerably depending on the chosen experimental data and nuclear models. We discuss various issues affecting both the overall normalization and the low-energy behavior of the measured and computed spectra, and their joint effects on the experimentally quoted half-life values. Furthermore, 115In 8-decay data at the lowest possible energy threshold appear to be crucial to clarify these issues.
Analysis of in 115 β decay through the spectral moment method
Lisi E.;
2024-01-01
Abstract
We analyze the 115In 8-decay energy spectrum through the spectral moment method (SMM), previously introduced in the context of 113Cd 8 decay. The spectral moments mu n are defined as averaged nth powers of the 8 particle energy, characterizing the spectrum normalization (n = 0) and shape (n 1) above a given threshold. For 115In, we consider three independent datasets characterized by different thresholds. We also consider three nuclear model calculations with two free parameters: the ratio of axial-vector to vector couplings, r = gA/gV, and the small vector-like relativistic nuclear matrix element (NME), s = s-NME. By using the most recent of the three datasets, we show that the first few spectral moments can determine (r, s) values in good agreement with those obtained by full-fledged experimental fits. We then work out the SMM results for the other datasets. We find that, although gA quenching is generally favored, the preferred quenching factors may differ considerably depending on the chosen experimental data and nuclear models. We discuss various issues affecting both the overall normalization and the low-energy behavior of the measured and computed spectra, and their joint effects on the experimentally quoted half-life values. Furthermore, 115In 8-decay data at the lowest possible energy threshold appear to be crucial to clarify these issues.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.