Neutron capture rates of C18

2019 ◽  
Vol 99 (3) ◽  
Author(s):  
M. Dan ◽  
G. Singh ◽  
R. Chatterjee ◽  
Shubhchintak
2021 ◽  
Vol 104 (1) ◽  
Author(s):  
A. V. Voinov ◽  
K. Brandenburg ◽  
C. R. Brune ◽  
R. Giri ◽  
S. M. Grimes ◽  
...  

2018 ◽  
Vol 193 ◽  
pp. 04007
Author(s):  
J. Lerendegui-Marco ◽  
C. Guerrero ◽  
C. Domingo-Pardo ◽  
A. Casanovas ◽  
R. Dressler ◽  
...  

Neutron capture cross sections are among the main inputs for nucleosynthesis network calculations. Although well known for the majority of the stable isotopes, this quantity is still unknown for most of the unstable isotopes of interest. A recent collaboration between ILL, PSI, U. Sevilla and IFIC aims at producing the isotopes of interest at ILL, preparing suitable targets at PSI, and measuring their capture cross sections at facilities such as n_TOF/CERN, LiLiT and the Budapest Research Reactor (BRR). This work is focused on the description of the different beams and techniques and shows some highlights of the preliminary results of the capture measurements on 171Tm, 147Pm and 204Tl, along with the future plans for 79Se and 163Ho.


AIP Advances ◽  
2014 ◽  
Vol 4 (4) ◽  
pp. 041008 ◽  
Author(s):  
R. Surman ◽  
M. Mumpower ◽  
R. Sinclair ◽  
K. L. Jones ◽  
W. R. Hix ◽  
...  

2010 ◽  
Author(s):  
Rene Reifarth ◽  
Michael Heil ◽  
Ralf Plag ◽  
U. Besserer ◽  
A. Couture ◽  
...  

Universe ◽  
2019 ◽  
Vol 5 (1) ◽  
pp. 36
Author(s):  
Bryn Knight ◽  
Liliana Caballero

Neutron captures are likely to occur in the crust of accreting neutron stars (NSs). Their rate depends on the thermodynamic state of neutrons in the crust. At high densities, neutrons are degenerate. We find degeneracy corrections to neutron capture rates off nuclei, using cross sections evaluated with the reaction code TALYS. We numerically integrate the relevant cross sections over the statistical distribution functions of neutrons at thermodynamic conditions present in the NS crust. We compare our results to analytical calculations of these corrections based on a power-law behavior of the cross section. We find that although an analytical integration can simplify the calculation and incorporation of the results for nucleosynthesis networks, there are uncertainties caused by departures of the cross section from the power-law approach at energies close to the neutron chemical potential. These deviations produce non-negligible corrections that can be important in the NS crust.


2011 ◽  
Author(s):  
Matthew Mumpower ◽  
Gail C. Mclaughlin ◽  
Rebecca Surman

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