financially supported by Ministry of Science and Higher Education of the Russian Federation(Grant No.FENU-2023-0013)。
The high entropy alloys(HEAs)are the newly developed high-performance materials that have gained significant importance in defence,nuclear and aerospace sector due to their superior mechanical properties,heat resistan...
This work was supported by the National Natural Science Foundation of China(Nos.U1832182,11875328,11761161001,and U2032137);the Natural Science Foundation of Guangdong Province,China(Nos.18zxxt65 and 2022A1515011184);the Science and Technology Development Fund,Macao SAR(Grant No.008/2017/AFJ);the Macao Young Scholars Program of China(No.AM201907);the China Postdoctoral Science Foundation(Nos.2016LH0045 and 2017M621573);the Fundamental Research Funds for the Central Universities(Nos.22qntd3101 and 2021qntd28).
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.Promptγ-rays originating from neutron-induced capture ...
supported by the Japan Society for the Promotion of Science(JSPS)KAKENHI(Nos.18K11399 and 19H01097);the Telecommunications Advancement Foundation.
Systems containing multiple graphics-processing-unit(GPU)clusters are difficult to use for real-time electroholography when using only a single spatial light modulator because the transfer of the computer-generated ho...
This research is co-supported by National Key R&D Program of China(No.2017YFC1500402);National Natural Science Foundation of China(Nos.41874063 and U1939203);Shanghai Sheshan National Geophysical Observatory(No.2020K02)。
Earthquake detection and location are essential in earthquake studies,which generally consists of two main classes:waveform-based and pick-based methods.To evaluate the ability of two different methods,a graphicsproce...
In recent years,a large number of experimental data have been obtained from the measurement of the stable nuclear neutron capture cross section,which has been applied to the calculation of the neutron synthesis networ...
The 13C(, n)16O reaction is the key neutron source reaction for the main s-process nucleosynthesis[1]. Theimportant energy range (Gamow window) for the 13C( , n)16O reaction during the s-process spans from 140 to230 k...
supported by the National Natural Science Foundation of China (Grant Nos. 11021504, 11175258, 11275068 and 11175001);the Major State Basic Research Development Program of China (Grant No.2013CB834406)
The heavy elements in the Universe are formed during the s- and r-processes mainly in AGB stars and supernovae, respectively. Simulation of s- and r-nucleosynthesis critically depends on the neutron capture and weak d...
performed under the auspices of the U.S.Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344;support by the National Science Foundation(NSF)under Grant No.DMS-0724560,Grant No.EAR-0838541,and Grant No.EAR-0941666;the Department of Energy(DOE)under Grant No.DE-EE0002764.
Lattice-Boltzmann methods are versatile numerical modeling techniques capable of reproducing a wide variety of fluid-mechanical behavior.These methods are well suited to parallel implementation,particularly on the sin...
Supported by National Natural Science Foundation of China (11021504, 11175258, 11275068, 11175001)
The heavy elements in the universe are formed during the s- and r-processes mainly in AGB stars and supernovae, respectively. Simulation of s- and r-nucleosynthesis critically depends on the neutron capture and weak d...
supported by National Basic Research Program of China (No.2007CB815003);National Natural Science Foundation of China(Nos.10705053,11021504,10720101076,10735100 and 10975193)
The 13^C(a, n)160 reaction is believed to be the main neutron source reaction for the s-process in asymptotic giant branch (AGB) stars. The astrophysical S-factors of this reaction have been determined based on an...