NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = H.Wibowo Found 7 matches. 2022CA19 Phys.Lett. B 833, 137374 (2022) J.Carter, L.M.Donaldson, H.Fujita, Y.Fujita, M.Jingo, C.O.Kureba, M.B.Latif, E.Litvinova, F.Nemulodi, P.von Neumann-Cosel, R.Neveling, P.Papakonstantinou, P.Papka, L.Pellegri, V.Yu.Ponomarev, A.Richter, R.Roth, E.Sideras-Haddad, F.D.Smit, J.A.Swartz, A.Tamii, R.Trippel, I.T.Usman, H.Wibowo Damping of the isovector giant dipole resonance in 40, 48Ca NUCLEAR REACTIONS 40,48Ca(p, p'), E=200 MeV; measured reaction products; deduced σ(θ, E), Coulomb σ, contributions from the IsoScalar Giant Monopole Resonance (ISGMR) and the ISGQR lying under the IsoVector Giant Dipole Resonance (IVGDR). Comparison with calculations in the framework of RPA and beyond-RPA in a relativistic approach based on an effective meson-exchange interaction, with the UCOM effective interaction. The Separated Sector Cyclotron (SSC) at the iThemba Laboratory for Accelerator Based Sciences (iThemba LABS), Cape Town, South Africa.
doi: 10.1016/j.physletb.2022.137374
2022HL01 Phys.Rev. C 106, 024319 (2022) M.Q.Hlatshwayo, Y.Zhang, H.Wibowo, R.LaRose, D.Lacroix, E.Litvinova Simulating excited states of the Lipkin model on a quantum computer
doi: 10.1103/PhysRevC.106.024319
2022WI03 Phys.Rev. C 106, 044304 (2022) Nuclear shell structure in a finite-temperature relativistic framework NUCLEAR STRUCTURE 68,70,72,74,76,78Ni; calculated single-particle states at zero and finite temperature up to 4 MeV, dominant fragments of the single-particle states and their spectroscopic factors, temperature evolution of the neutron and proton states, temperature dependence of the quadrupole and octupole phonon strength distributions, temperature-dependent nucleon effective mass, symmetry energy coefficient temperature dependence. Relativistic mean-field calculations taking into account the particle-vibration coupling (RMF+PVC).
doi: 10.1103/PhysRevC.106.044304
2020WI10 Phys.Rev. C 102, 054321 (2020) H.Wibowo, E.Litvinova, Y.Zhang, P.Finelli Temperature evolution of the nuclear shell structure and the dynamical nucleon effective mass NUCLEAR STRUCTURE 56Fe, 68Ni; calculated single-particle states, and dominant fragments of the single-particle states at zero and finite temperatures in the RMF approximation, temperature evolution of the neutron pairing gap and the neutron and proton single-quasiparticle states around the Fermi surface, neutron and proton dynamical effective masses. 56Ni; calculated temperature evolution of the nucleon dynamical effective mass. Single fermion Dyson equation with the dynamical kernel of the particle-vibration-coupling (PVC) using the grand canonical potential with the meson-nucleon covariant energy density functional. Possible relevance to astrophysical modeling of various stages of stellar evolution.
doi: 10.1103/PhysRevC.102.054321
2019LI59 Eur.Phys.J. A 55, 223 (2019) Nuclear response in a finite-temperature relativistic framework
doi: 10.1140/epja/i2019-12771-9
2019WI09 Phys.Rev. C 100, 024307 (2019) Nuclear dipole response in the finite-temperature relativistic time-blocking approximation NUCLEAR STRUCTURE 48Ca, 68Ni, 100,120,132Sn; calculated temperature dependence of the isovector giant electric dipole (IV GDR) response, strength functions widths, contributions of neutron and proton configurations using finite-temperature relativistic time-blocking approximation method.
doi: 10.1103/PhysRevC.100.024307
2018LI41 Phys.Rev.Lett. 121, 082501 (2018) Finite-Temperature Relativistic Nuclear Field Theory: An Application to the Dipole Response NUCLEAR STRUCTURE 48Ca, 100,120,132Sn; calculated temperature dependence of dipole spectra in the even-even nuclei, giant dipole resonance width, the low-energy dipole strength distribution. Thermal (imaginary-time) Green's function formalism.
doi: 10.1103/PhysRevLett.121.082501
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