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NSR database version of April 27, 2024.

Search: Author = M.D.Schuster

Found 3 matches.

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2016JA03      Phys.Rev. C 94, 011301 (2016)

G.R.Jansen, M.D.Schuster, A.Signoracci, G.Hagen, P.Navratil

Open sd-shell nuclei from first principles

NUCLEAR STRUCTURE ^{18,19,20,21,22,23,24,25,26,27,28,29,30}Ne, ^{20,21,22,23,24,25,26,27,28,29,30}Mg; calculated ground-state energies. ²⁴F, ^{19,20,24,25,26,27}Ne, ^{22,23,24,25,26}Mg; calculated low-spin levels, J, π, B(E2) strengths. Calculations are based on an extension of ab initio coupled-cluster effective interaction (CCEI) method. Comparison with experimental data taken from the ENSDF database.

doi: 10.1103/PhysRevC.94.011301
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2015SC12      Phys.Rev. C 92, 014320 (2015)

M.D.Schuster, S.Quaglioni, C.W.Johnson, E.D.Jurgenson, P.Navratil

Operator evolution for ab initio electric dipole transitions of ⁴He

NUCLEAR REACTIONS ⁴He(γ, X), E>26 MeV; calculated total photoabsorption cross section, total dipole strength through renormalized matrix elements obtained in the framework of similarity renormalization (SRG) group method with NN+3N interactions. Comparison with experimental data.

NUCLEAR STRUCTURE ⁴He; calculated ground-state energy, point-proton root-mean-square radius, total dipole strength, and electric dipole polarizability using NN+3N Hamiltonians. The ab initio no-core shell-model calculations. Comparison with experimental results.

doi: 10.1103/PhysRevC.92.014320
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2014SC08      Phys.Rev. C 90, 011301 (2014)

M.D.Schuster, S.Quaglioni, C.W.Johnson, E.D.Jurgenson, P.Navratil

Operator evolution for ab initio theory of light nuclei

NUCLEAR STRUCTURE ³H; calculated rms radius as a function of SRG evolution parameter. ⁴He; calculated ground-state energy, rms radius, and total strength of dipole transition, renormalization percent as a function of range of Gaussian operator. The ab initio calculations using similarity renormalization group (SRG). SRG-evolved operators in the two- and three-body spaces. Importance of three-body contribution at long range.

doi: 10.1103/PhysRevC.90.011301
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