In nuclear astrophysics, Pr 141 is mainly produced by an s process, which has a neutron
magic number (N= 82) leading to its low capture cross section and strongly affecting the s …

Experimental nuclear spectroscopic data are compiled and evaluated for 17 known nuclides
of mass 167 (Sm, Eu, Gd, Tb, Dy, Ho, Er Tm, Yb, Lu, Hf, Ta, W, Re, Os, Ir, Pt), 23 years after …

Abstract Silver indium cadmium (Ag–In–Cd) control rod is widely used in pressurized water
reactor nuclear power plants, and it is continuously consumed in a high neutron flux …

The 74 Se is one of 35 p-nuclei, and 82 Se is a r-process only nucleus, and their (n, γ) cross
sections are vital input parameters for nuclear astrophysics reaction network calculations …

In nuclear astrophysics, the nuclides 151 Eu and 153 Eu are both in the path of the s-
process, and their (n, γ) cross sections are important input parameters for the calculation of …

Er 162 is one of the p nuclei in nuclear astrophysics, and its (n, γ) cross sections are
important input parameters in nuclear astrophysics network calculations. Resonance data …

The neutron capture cross section of 232 Th was measured at the neutron time-of-flight
facility Back-n of China Spallation Neutron Source (CSNS) for the first time. The …

The neutron capture cross sections (n, γ) of bromine were obtained using the time-of-flight
technique at the Back-n facility of the China Spallation Neutron Source. Prompt γ-rays …

Purpose Back-n is a white neutron beamline at China spallation neutron source, which was
established in the year of 2018. It is a powerful facility for nuclear data measurement …

The neutron capture measurement of natural rhenium was performed with the time-of-flight
technique at the Back-n facility of the China Spallation Neutron Source in the energy range …