Introduction
“How were the elements from iron to uranium made?” This is a highly fascinating question and has been listed in “Connecting Quarks with the Cosmos: Eleven Science Questions for the New Century” [1]. Rapid neutron capture processes (r-process) are responsible for producing approximately half of these heavy elements [3, 2] and represent the only mechanism for synthesizing elements heavier than bismuth [4]. One of the key challenges in studying the r-process is obtaining precise nuclear physics inputs, such as nuclear masses, β-decay half-lives, neutron-capture cross-sections, and fission rates [5]. β-decay, the primary decay mode for most nuclei, plays a crucial role in determining the timescale of the r-process. Predictions indicate that there are 9035 bound nuclides with proton numbers between 8 and 120 [6]. However, only approximately 3,000 nuclides have been observed experimentally [7]. In particular, for nuclei far from the β-stability line—those most relevant to the r-process—current experimental data remain limited. Theoretical calculations not only guide experimental observations but also provide explanations for existing experiments, thereby advancing a deeper understanding of the essence of matter and the laws of nature. Nevertheless, providing a precise description of the β-decay half-lives of nuclei remains a significant challenge owing to the non-perturbative nature of nuclear forces and the complexity of quantum many-body problems.
Theoretical studies on β-decay half-lives can be broadly classified into empirical formulas, gross theories, and microscopic theories. The empirical formula is particularly suitable for fitting experimental data and calculating β-decay half-lives on a large scale [9, 8]. Compared to empirical formulas, gross theory can handle more complex situations and offers broader applicability [10-13]. Microscopic theories include the shell model [14-18] and the quasiparticle random phase approximation (QRPA) model [19-29]. The shell model provides reliable predictions for β-decay half-lives, particularly for nuclei in the light nuclear region and near magic numbers. However, shell model calculations become increasingly challenging as the number of valence nucleons increases. QRPA, on the other hand, is widely used to calculate the β-decay properties of the majority of nuclei on the nuclear chart, with the exception of some light nuclei. When experimental data is unavailable, researchers frequently rely on QRPA predictions based on the finite-range droplet model (FRDM + QRPA) [30-33] to provide essential inputs for r-process simulations.
In recent years, with rapid advancements in artificial intelligence, machine learning has provided researchers with novel approaches. The application of machine learning in the field of nuclear physics has become increasingly prominent [34], with applications spanning various areas, including nuclear mass predictions [35-41], investigations of charge radii [42-47], predictions of the distribution of fission fragment yields [48, 49], studies of giant dipole resonances [50, 51], explorations of excited states [52, 53], and other relevant topics [54-63].
The use of machine learning to study β-decay half-lives has also garnered significant attention in recent years, with predictive accuracy continually improving [64-68]. Recent studies demonstrated that machine learning predictions for β-decay half-lives deviate from experimental values by only 2.24 times for nuclei with half-lives shorter than 106 seconds [67]. In this study, we propose a novel application of neural networks to identify nuclei exhibiting deviations from systematic behavior in β-decay half-lives. For these nuclei, machine learning fails to accurately describe the β-decay half-lives. Furthermore, theoretical models such as FRDM+QRPA [32, 33], relativistic Hartree-Bogoliubov + quasiparticle random phase approximation (RHB+QRPA) [26], gross theory based on the WS4 mass model (WS4+GT) [13], and Skyrme-Hartree-Fock-Bogoliubov with the finite amplitude method (SHFB+FAM) [69] also encounter difficulties in describing these specific nuclei. After predicting β-decay half-lives and selecting these anomalous nuclei based on deviations between experimental values and neural network predictions, we analyzed the challenges faced by the neural network in describing these nuclei and explored the potential underlying physics.
Neural network model
In this study, the neural network employed (Z, N, Qβ) as inputs to predict β-decay half-lives and identify abnormal nuclei based on deviations between experimental values and neural network predictions. Here, Z, N, and Qβ represent the proton number, neutron number, and β-decay energy, respectively. The Qβ values were calculated using nuclear masses obtained from the Bayesian Machine Learning (BML) model [37], which achieves a root mean square error (RMSE) of only 84 keV compared to experimental values. The neural network output corresponds to the logarithm of the β-decay half-life (
A total of 1,072 nuclei from the NUBASE2020 database [7] were selected based on the following criteria:
In this study, a double-hidden-layer neural network was used, which is described by the following formula:
After calculating the output value y for each input, the loss function Loss is determined as follows:
Results and discussion
Figure 1 presents the RMSE values for the predictions of the ANN1 and ANN2 models across various half-life ranges. To facilitate a clearer comparison between ANN1 and ANN2, the RMSE values for ANN1, excluding the abnormal nuclei, are also shown. The results indicate that in most cases, the performance differences between the two neural networks on both the training and validation sets are minimal, suggesting that neither model suffers from overfitting. Furthermore, Figure 1 demonstrates that the predictive accuracy of the neural network generally improves as nuclear half-lives decrease, except for nuclei with half-lives in the ranges of 10-2~10-1 to 10-3~10-2 s. For a clearer comparison of the ANN1 and ANN2 predictions, the RMSE values for ANN1, with abnormal nuclei excluded, are presented. Notably, ANN1, when the selected 70 abnormal nuclei are excluded, achieves prediction accuracy comparable to that of ANN2. This consistency suggests that the selected abnormal nuclei exhibit behavior distinct from that of other nuclei.
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Figure 2 illustrates typical abnormal nuclei identified by the neural networks. The predicted β-decay half-lives for nuclei in isotopic chains exhibit a generally smooth decrease as they move further from the β-stability line, consistent with experimental data. To improve predictions of β-decay half-lives, additional physical parameters were introduced alongside the inputs (Z, N, Qβ). These included the odd-even information
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For these nuclei, the predictions from the machine learning models exhibited significant discrepancies when compared with the experimental data. However, accurately describing these isotopes remains a challenge even when employing other theoretical models. For the Al isotopes, the FRDM+QRPA model can accurately predict the β-decay half-lives of 31Al and 32Al but shows a significant deviation in predicting the β-decay half-lives of 33Al to 36Al compared to the experimental data. On the other hand, RHB+QRPA offers more accurate predictions for the β-decay half-lives of 34Al to 36Al but shows notable discrepancies when predicting the β-decay half-lives of other nuclei in the isotopic chain. Both models fail to reproduce the observed trend of anomalous increases in β-decay half-lives from 32Al to 36Al. For the Co isotopes, RHB+QRPA provides better predictions for the β-decay half-life of 70Co when compared to the neural network, although, for other nuclei in this isotopic chain, its predictive accuracy is lower than that of the neural networks. The FRDM+QRPA model shows better agreement with the experimental data for nuclei lighter than 66Co compared to the neural networks; however, for nuclei heavier than 67Co, its predictions are less accurate than those of the neural networks. Moreover, predicting the β-decay half-life of 70Co using FRDM+QRPA remains particularly challenging. Both models also struggle to reliably predict the β-decay half-lives of all the nuclei in the Co isotopes. For the other isotopes selected in Fig. 2, neither the FRDM+QRPA nor the RHB+QRPA models are able to accurately reproduce the β-decay half-lives of the abnormal nuclei or their neighboring nuclei.
In Fig. 3, the extrapolation results of two models are presented, accompanied by the 1σ (68% confidence interval) error bands. From Fig. 3, for nuclei with measured half-lives, the error bands of the neural network are small, indicating good agreement with the experimental data. For the nuclei selected by the neural network based on deviations between the experimental values and the predictions, both neural network models provide consistent results. Benefiting from training on an abnormal dataset, ANN1 achieved slightly improved predictive performance. However, neither model can precisely describe these abnormal nuclei. For nuclei without experimental values, ANN1 exhibits larger error bands. For all nuclei, the RMS between the means/upper bound/lower bound of ANN1 and ANN2 were 0.115, 0.196, and 0.162 orders of magnitude, respectively, which are very close, with the predictions of ANN1 being slightly shorter than those of ANN2 in some cases.
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Figure 4 compares the β-decay half-lives of isotones predicted by ANN2 and other theoretical models. For nuclei with experimental data, the predictions of the neural network show better agreement with the experimental results than those of other theoretical models. For the selected dataset of 1072 nuclei, the RMSE between the predictions of ANN1 and the experimental values was 0.437, while the FRDM+QRPA model shows an RMSE of 0.806. Since the predictions of RHB+QRPA for some of the 1072 nuclei were stable, the RMSE for RHB+QRPA predictions for nuclei with half-lives shorter than 106s was 1.025 for a subset of 920 nuclei. Compared to these theoretical models, the neural network demonstrates higher predictive accuracy for β-decay half-lives. The neural network predicts shorter half-lives than those predicted by other theoretical models in the neutron-rich region of N=50 isotones. However, in the neutron-rich regions of N=82 and 126 isotones, the predictions from the neural network align more closely with those from the other theoretical models, showing less disagreement.
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Figure 5 shows the logarithmic differences between the β-decay half-lives predicted by ANN1 and the experimental values from NUBASE2020 for the 1072 nuclei selected in the dataset. The figure indicates that nuclei with significant deviations between the predictions of ANN1 and experimental values are concentrated near the β-stability line. For most nuclei (75.2%), the deviation between the predictions of ANN1 and the experimental values was within 0.4 orders of magnitude. Among the 1072 β-decay half-lives, 548 (51.1%) were overestimated, and 524 (48.9%) were underestimated by ANN1. ANN1 exhibited alternating blocks of overestimation and underestimation in predicting the β-decay half-lives of the nuclei, accompanied by a certain degree of randomness. Neural networks tend to underestimate the β-decay half-life of nuclei with magic numbers. For nuclei with magic numbers of protons or neutrons, 52 (58.4%) were underestimated, and 37 (41.6%) were overestimated by ANN1. This suggests that the greater stability of magic nuclei presents additional challenges for neural networks in predicting their β-decay half-lives.
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In Fig. 6, a concise analysis is provided to explain why the neural network faces challenges in predicting certain nuclei. For 52Ca, both the predictions from the WS4 model and the experimental values reveal a significant Δ2n value (Δ2n = S2n(Z,N) - S2n(Z,N+2), where S2n is the two-neutron separation energy), indicating the presence of shell effects. A recent study also identified N = 32 as a new magicity [74]. However, our neural network model does not incorporate this information, which leads to reduced predictive accuracy for nuclei in this region. For 112Zr, the experimental half-life measurements have relatively large uncertainties, resulting in different outcomes depending on how the error bars are treated. For instance, NUBASE2020 reports a half-life of 43 ± 21 ms using symmetric error bars, while the original measurement of the β-decay half-life for this nucleus was
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The selected nuclei are listed in Table 1 along with their experimental half-lives and predictions from ANN1 and ANN2. The abnormal nuclei include 32 odd-odd nuclei, 26 odd-A nuclei, and 12 even-even nuclei. Owing to the presence of unpaired nucleons in odd nuclei, these exhibit complex energy-level structures, vibrational modes, and other properties, making theoretical descriptions more challenging. While neural networks outperform traditional nuclear models in their representation capabilities, their performance is somewhat worse when dealing with odd nuclei compared to even nuclei. This highlights the vital role of physics in enhancing the performance of machine learning algorithms.
Z | N | Z | N | ||||||
---|---|---|---|---|---|---|---|---|---|
9 | 13 | 0.626 | -0.094 | -0.467 | 33 | 48 | 1.522 | 2.272 | 2.384 |
9 | 15 | -0.416 | -1.200 | -1.379 | 35 | 45 | 3.063 | 4.390 | 4.757 |
10 | 16 | -0.706 | -0.193 | 0.063 | 35 | 50 | 2.241 | 3.269 | 3.242 |
10 | 17 | -1.510 | -1.132 | -1.105 | 40 | 57 | 4.780 | 2.983 | 2.936 |
10 | 18 | -1.726 | -1.198 | -1.127 | 40 | 58 | 1.487 | 2.460 | 2.387 |
11 | 13 | 4.731 | 1.972 | 1.446 | 40 | 72 | -1.367 | -1.713 | -1.687 |
11 | 16 | -0.521 | -0.042 | 0.040 | 41 | 57 | 0.456 | 1.456 | 1.699 |
11 | 17 | -1.480 | -1.121 | -1.122 | 41 | 58 | 1.176 | 1.964 | 2.390 |
12 | 18 | -0.499 | 0.051 | 0.445 | 42 | 63 | 1.560 | 0.820 | 0.752 |
12 | 20 | -1.095 | -0.743 | -0.565 | 43 | 57 | 1.189 | 2.036 | 2.407 |
12 | 21 | -1.036 | -1.472 | -1.338 | 43 | 61 | 3.041 | 1.261 | 0.922 |
13 | 18 | -0.191 | 0.388 | 0.690 | 43 | 66 | -0.043 | 0.432 | 0.388 |
13 | 19 | -1.487 | -0.686 | -0.458 | 45 | 64 | 1.907 | 2.655 | 2.857 |
13 | 20 | -1.382 | -0.758 | -0.517 | 45 | 65 | 0.525 | 1.411 | 1.153 |
13 | 23 | -1.046 | -1.509 | -1.502 | 45 | 66 | 1.041 | 1.819 | 1.871 |
14 | 20 | 0.442 | 1.075 | 1.508 | 47 | 65 | 4.052 | 2.101 | 1.386 |
15 | 19 | 1.094 | 2.117 | 2.145 | 47 | 67 | 0.663 | 1.507 | 0.982 |
19 | 35 | -2.000 | -1.543 | -1.508 | 47 | 69 | 2.361 | 1.090 | 0.861 |
20 | 29 | 2.719 | 1.678 | 1.537 | 50 | 75 | 5.920 | 4.046 | 3.512 |
20 | 32 | 0.663 | 0.060 | 0.000 | 51 | 83 | -0.171 | 0.439 | 0.544 |
20 | 36 | -1.959 | -1.593 | -1.555 | 52 | 77 | 3.621 | 5.005 | 5.330 |
21 | 35 | -1.585 | -1.101 | -1.058 | 53 | 75 | 3.207 | 5.067 | 5.702 |
23 | 33 | -0.666 | -0.140 | 0.132 | 59 | 85 | 3.016 | 4.331 | 4.721 |
25 | 37 | -1.036 | -0.649 | -0.473 | 75 | 119 | 0.699 | 1.315 | 1.420 |
26 | 35 | 2.555 | 1.461 | 1.399 | 77 | 119 | 1.716 | 2.451 | 2.769 |
26 | 46 | -1.770 | -1.414 | -1.373 | 77 | 121 | 0.940 | 1.761 | 1.982 |
26 | 48 | -2.301 | -1.727 | -1.671 | 77 | 122 | 0.845 | 1.742 | 1.914 |
27 | 37 | -0.523 | 0.335 | 0.640 | 78 | 124 | 5.200 | 2.528 | 2.509 |
27 | 38 | 0.064 | 0.704 | 0.757 | 79 | 123 | 1.453 | 2.338 | 2.618 |
27 | 39 | -0.712 | -0.176 | 0.082 | 79 | 124 | 1.778 | 2.509 | 2.642 |
27 | 43 | -0.294 | -0.737 | -0.658 | 81 | 125 | 2.402 | 3.485 | 3.697 |
28 | 37 | 3.957 | 2.658 | 2.211 | 81 | 126 | 2.457 | 3.525 | 3.648 |
29 | 39 | 1.490 | 2.287 | 2.436 | 87 | 146 | -0.046 | 1.115 | 1.128 |
32 | 45 | 4.606 | 2.889 | 2.754 | 91 | 148 | 3.812 | 2.348 | 2.151 |
33 | 47 | 1.182 | 2.168 | 2.505 | 94 | 153 | 5.293 | 2.939 | 2.625 |
Summary and Outlook
In this study, a neural network was employed to predict β-decay half-lives and to identify nuclei whose β-decay half-lives deviated from systematic patterns, based on the differences between experimental values and the neural network predictions. After excluding these anomalous data points, the models were retrained. Both neural network models exhibited similar
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