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NSR database version of May 8, 2024.

Search: Author = H.Carr

Found 2 matches.

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2015SC06      Phys.Rev. C 91, 034327 (2015)

N.Schunck, D.Duke, H.Carr

Description of induced nuclear fission with Skyrme energy functionals. II. Finite temperature effects

NUCLEAR REACTIONS 239Pu(n, F), E=thermal to fast; calculated internal and free energy along the least-energy fission pathway across multidimensional potential energy surfaces, inner and outer fission barriers as a function of the excitation energy of the compound nucleus, pairing energy in the ground state and fission isomer, Skyrme interaction energy and between the fission fragments of 240Pu as a function of number of particles in the neck and as function of temperature, direct Coulomb interaction energy in the fission of 240Pu. Local density approximation of density functional theory (DFT) at finite temperature for the description of induced fission.

doi: 10.1103/PhysRevC.91.034327
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2014SC23      Phys.Rev. C 90, 054305 (2014)

N.Schunck, D.Duke, H.Carr, A.Knoll

Description of induced nuclear fission with Skyrme energy functionals: Static potential energy surfaces and fission fragment properties

NUCLEAR REACTIONS 239Pu(n, F)240Pu*, E=slow; calculated potential energy surfaces of 240Pu in (q20, q22), (q20, q40) and (q20, q30) planes, HFB energy along the least-energy fission pathway, variation of the total HFB energy as a function of the hexadecapole moment, total energy as a function of the density of particles in the neck, approximate position of the scission point, variation of the light and heavy fragment proton and neutron numbers as a function of triaxiality, joint contour net (JCN) graphs near the scission, fragment densities, Skyrme interaction energy and Direct Coulomb interaction energy between the fission fragments in 240Pu as a function of the number of particles in the neck. Nuclear density functional theory with Skyrme energy densities within the HFB approach and three parameterization SkM*, UNEDF0 and UNEDF1 using DFT solvers HFODD and HFBTHO.

doi: 10.1103/PhysRevC.90.054305
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