WU Zhidan, GUO Bing, LI Zhihong, et al. Determination of 15N(n,r)16N astrophysical reaction rate via the (7Li,6Li) reaction[J]. Nuclear techniques, 2014, 37(10): 100512
DOI:
WU Zhidan, GUO Bing, LI Zhihong, et al. Determination of 15N(n,r)16N astrophysical reaction rate via the (7Li,6Li) reaction[J]. Nuclear techniques, 2014, 37(10): 100512 DOI: 10.11889/j.0253-3219.2014.hjs.37.100512.
Determination of 15N(n,r)16N astrophysical reaction rate via the (7Li,6Li) reaction
Background: Chemical properties of projectile residues are important in studying the symmetry energy using isobaric yield ratio (IYR) and isoscaling methods. Purpose: The correlation between chemical properties of intermediate mass residues and reaction systems is to be studied. It is hoped that the symmetry energy information can be extracted more precisely. Methods: In the framework of the grand-canonical ensemble theory
the /T difference between two heave-ion reactions
which was labeled as 21/T
was extracted by using isobaric yield ratio difference (IBD) method. Results: By comparing the 21/T among six different combinations 48Ca+9Be/40Ca+9Be
48Ca+9Be/58Ni+9Be
64Ni+9Be/40Ca+9Be
64Ni+9Be/58Ni+9Be
58Ni+9Be/ 40Ca+9Be
48Ca+9Be/ 64Ni+9Be
it was proved that /T depends on the reaction system. In different reactions
the values of /T were not fixed. When the double neutron-to-proton ratios (N/Z)21=1.17
21/T can be approximately a constant. Conclusion: Symmetry energy can be more reasonable in isoscaling and IBD methods
when double neutron-to-proton ratios (N/Z)21=1.17 between two similar reaction system.Cited