NSR Query Results


Output year order : Descending
Format : Normal

NSR database version of April 24, 2024.

Search: Author = H.Dussan

Found 5 matches.

Back to query form



2016DI12      Phys.Rev. C 94, 025802 (2016); Pub.Note Phys.Rev. C 94, 029901 (2016)

D.Ding, A.Rios, H.Dussan, W.H.Dickhoff, S.J.Witte, A.Carbone, A.Polls

Pairing in high-density neutron matter including short- and long-range correlations

doi: 10.1103/PhysRevC.94.025802
Citations: PlumX Metrics


2014DU15      Phys.Rev. C 90, 061603 (2014)

H.Dussan, M.H.Mahzoon, R.J.Charity, W.H.Dickhoff, A.Polls

Elastic nucleon-nucleus scattering as a direct probe of correlations beyond the independent-particle model

NUCLEAR REACTIONS 40Ca(p, p), (n, n), E<200 MeV; analyzed scattering and structure data using the full nonlocal treatment of the dispersive optical model (DOM). Discussed application for inverse kinematics reactions.

doi: 10.1103/PhysRevC.90.061603
Citations: PlumX Metrics


2014MA18      Phys.Rev.Lett. 112, 162503 (2014)

M.H.Mahzoon, R.J.Charity, W.H.Dickhoff, H.Dussan, S.J.Waldecker

Forging the Link between Nuclear Reactions and Nuclear Structure

NUCLEAR REACTIONS 40Ca(n, n), (p, p), E<200 MeV; calculated σ, σ(θ), spectral strength. Comparison with experimental data.

doi: 10.1103/PhysRevLett.112.162503
Citations: PlumX Metrics


2011DU21      Phys.Rev. C 84, 044319 (2011)

H.Dussan, S.J.Waldecker, W.H.Dickhoff, H.Muther, A.Polls

Microscopic self-energy of 40Ca from the charge-dependent Bonn potential

NUCLEAR STRUCTURE 40Ca; calculated spectral functions, single-particle levels, spectroscopic factors, natural orbits; comparison of microscopic CD Bonn Self-Energy and Dispersive Optical Model fit. 40Ca(n, n), E=0-100 MeV; calculated total and differential cross sections. Comparison with experimental data; analyzed non-locality of the imaginary part of the CD Bonn Self-energy.

doi: 10.1103/PhysRevC.84.044319
Citations: PlumX Metrics


2008HO06      Phys.Rev. C 77, 045807 (2008)

C.J.Horowitz, H.Dussan, D.K.Berry

Fusion of neutron-rich oxygen isotopes in the crust of accreting neutron stars

NUCLEAR REACTIONS 24O(24O, X);28Ne(28Ne, X), E=1, 1.5, 2, 3, 4, 6, 8; calculated astrophysical S-factor, reaction rates. O, Ne, Ti, Se; radial distribution functions, screening potentials, thermonuclear fusion reaction rates.

doi: 10.1103/PhysRevC.77.045807
Citations: PlumX Metrics


Back to query form