Cosmic implications of the 12C(n,y)13C reaction: a nuclear astrophysical perspective

被引：0

作者：

Saha, Soumya ^{[1
,2
]}

机构：

[1] Bidhan Chandra Coll, Dept Phys, 31 GT Rd East, Rishra 712248, Hooghly, India

[2] Univ Calcutta, Dept Phys, 92 Acharya Prafulla Chandra Rd, Kolkata 700009, India

来源：

CHINESE PHYSICS C | 2024年 / 48卷 / 02期

关键词：

reaction cross section; R-matrix; reaction rates; spectroscopic factors; NEUTRON-CAPTURE; C-12(N; GAMMA)C-13; REACTION;

D O I：

10.1088/1674-1137/ad102a

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

We conducted a comprehensive study of the neutron capture cross section of within the relevant as C-12 trophysical energy range. Through rigorous R-matrix analysis, we determined the Maxwellian-averaged cross section to be 11.98 +/- 0.25 mu b at kT = 30 keV. This result is approximately four times higher than the thermal neutron capture cross section estimated in earlier studies assuming the law. The implications of our findings extend to the (1)/ (v) region of inhomogeneous Big-Bang models in nuclear astrophysics, where understanding the behaviour of neutron capture cross sections plays a crucial role in elucidating the intricate processes that shaped the early universe.

引用

页数：4

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