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NSR database version of May 6, 2024.

Search: Author = E.Yuksel

Found 22 matches.

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2024KA02      Phys.Rev. C 109, 014314 (2024)

A.Kaur, E.Yuksel, N.Paar

Electric dipole transitions in the relativistic quasiparticle random-phase approximation at finite temperature

doi: 10.1103/PhysRevC.109.014314
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2024KA04      Phys.Rev. C 109, 024305 (2024)

A.Kaur, E.Yuksel, N.Paar

Finite-temperature effects in magnetic dipole transitions

doi: 10.1103/PhysRevC.109.024305
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2024PA14      Nuovo Cim. C 47, 50 (2024)

N.Paar, E.Yuksel

Nuclear energy density functionals constrained by collective nuclear excitations and parity violating electron scattering experiments

NUCLEAR STRUCTURE 48Ca, 208Pb; calculated dipole polarizability using nuclear energy density functionals (EDF) and a novel relativistic EDF DD-PCX based on point coupling interaction, adjusted using not only the ground state properties of nuclei but also the properties of isoscalar giant monopole resonance and the dipole polarizability in 208Pb; deduced weak-charge form factors extracted from the CREX and PREX-II experiments to optimize the relativistic density-dependent point coupling EDFs.

doi: 10.1393/ncc/i2024-24050-y
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2024RA05      Phys.Rev. C 109, 014318 (2024)

A.Ravlic, E.Yuksel, T.Niksic, N.Paar

Global properties of nuclei at finite-temperature within the covariant energy density functional theory

doi: 10.1103/PhysRevC.109.014318
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2023RA22      Phys.Rev. C 108, 054305 (2023)

A.Ravlic, E.Yuksel, T.Niksic, N.Paar

Influence of the symmetry energy on the nuclear binding energies and the neutron drip line position

doi: 10.1103/PhysRevC.108.054305
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2023YU01      Phys.Lett. B 836, 137622 (2023)

E.Yuksel, N.Paar

Implications of parity-violating electron scattering experiments on 48Ca (CREX) and 208Pb (PREX-II) for nuclear energy density functionals

NUCLEAR STRUCTURE 48Ca, 208Pb; analyzed available data; deduced implications of CREX and PREX-II data on nuclear matter symmetry energy and isovector properties of finite nuclei: neutron skin thickness and dipole polarizability.

doi: 10.1016/j.physletb.2022.137622
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2022YU07      Phys.Rev. C 106, 054309 (2022)

E.Yuksel, F.Mercier, J.-P.Ebran, E.Khan

Clustering in nuclei at finite temperature

NUCLEAR STRUCTURE 20,32Ne; calculated deformation parameter, pairing gap, entropy, total intrinsic density and excitation energy as a function of temperature, proton, neutron and α localization densities, proton and nuetron isoscalar and isovector densities. Finite temperature relativistic Hartree-Bogoliubov (FT-RHB) method with the relativistic density-dependent meson-nucleon coupling functional DD-ME2.

doi: 10.1103/PhysRevC.106.054309
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2021RA26      Phys.Rev. C 104, 054318 (2021)

A.Ravlic, E.Yuksel, Y.F.Niu, N.Paar

Evolution of β-decay half-lives in stellar environments

RADIOACTIVITY 52,54,56,58,60Ti, 62,64,66,68,70Fe, 120,122,124,126,128Cd, 130,132,134,136,138Sn(β-); Z=8-82, N=12-184; calculated β-decay half-lives of even-even nuclei as a function of temperature and density, Gamow-Teller strength as a function of temperature. Relativistic nuclear energy density functional framework with D3C* parametrization, and finite-temperature proton-neutron relativistic quasiparticle random-phase approximation (FT-PNRQRPA). Relevance to initial stages of the r-process or other astrophysical processes such as rp-process, dense thermonuclear explosions, and supernovae simulations.

doi: 10.1103/PhysRevC.104.054318
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2021YU02      Int.J.Mod.Phys. E30, 2150017 (2021)

E.Yuksel, D.Soydaner, H.Bahtiyar

Nuclear binding energy predictions using neural networks: Application of the multilayer perceptron

NUCLEAR STRUCTURE Z<120; calculated binding energies using the Multilayer Perceptron (MLP). Comparison with available data.

doi: 10.1142/S0218301321500178
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2021YU03      Nucl.Phys. A1014, 122238 (2021)

E.Yuksel

Temperature dependence of nuclear properties: A systematic study along the isotopic and isotonic chains of nuclei

NUCLEAR STRUCTURE Z=20, 28, 50, 82; calculated the neutron pairing gap values, internal excitation energies, entropy, two-neutron separation energies, and neutron skin thickness with increasing temperature using the finite temperature Hartree-Fock-Bogoliubov (FT-HFB) calculations are performed using the Skyrme-type SkM* functional and mixed-type pairing interaction.

doi: 10.1016/j.nuclphysa.2021.122238
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2020RA29      Phys.Rev. C 102, 065804 (2020)

A.Ravlic, E.Yuksel, Y.F.Niu, G.Colo, E.Khan, N.Paar

Stellar electron-capture rates based on finite-temperature relativistic quasiparticle random-phase approximation

NUCLEAR REACTIONS 44Ti, 56Fe(e-, ν), E<30 MeV; calculated electron capture cross sections in stellar environment for the 0+, 0-, 1+, 1-, 2+ and 2- multipoles, B(GT+) transition strength distributions; concluded that for the complete description of electron capture, both pairing and temperature effects must be considered. Nuclear ground-state properties calculated using finite-temperature Hartree BCS theory (FT-HBCS), and nuclear excitations in the charge exchange channel using finite-temperature proton-neutron relativistic QRPA (FT-PNRQRPA), with relativistic energy density functional (DD-ME2) in both cases.

doi: 10.1103/PhysRevC.102.065804
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2020YU03      Phys.Rev. C 101, 044305 (2020)

E.Yuksel, N.Paar, G.Colo, E.Khan, Y.F.Niu

Gamow-Teller excitations at finite temperature: Competition between pairing and temperature effects

NUCLEAR STRUCTURE 42Ca, 46Ti, 118Sn; calculated B(GT-), centroid energies of Gamow-Teller (GT) resonances, summed B(GT-), quasiparticle configuration of low-lying GT- states as function of temperature. Relativistic and nonrelativistic finite temperature proton-neutron quasiparticle RPA (FT-PNQRPA) with Skyrme-type functional SkM*, and meson-exchange interaction DD-ME2. Comparison with experimental data. Relevance to universal modeling of the weak-interaction processes in stellar environments, such as electron capture, β decays, and neutrino-nucleus reactions.

doi: 10.1103/PhysRevC.101.044305
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2019YU02      Phys.Rev. C 99, 034318 (2019)

E.Yuksel, T.Marketin, N.Paar

Optimizing the relativistic energy density functional with nuclear ground state and collective excitation properties

NUCLEAR STRUCTURE 36,38,40,42,44,46,48,50,52,54,56Ca, 54,56,58,60,62,64,66,68,70,72Ni, 100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132,134Sn, 190,192,194,196,198,200,202,204,206,208,210,212,214Pb, 90Zr; calculated binding energies using DD-PCX, DD-PC1, and DD-ME2 interactions, charge radii. 90Zr, 120Sn, 208Pb; calculated isoscalar GMR energies. 48Ca, 68Ni, 208Pb, 112,116,118,120,122,124Sn; calculated dipole polarizabilities using RHB+(Q)RPA with DD-PCX, DD-PC1, and DD-ME2 interactions. 208Pb; calculated neutron skin thickness. Relativistic energy density functional with DD-PCX interaction, based on the RHB plus (Q)RPA, supplemented with the covariance analysis. Comparison with experimental data.

doi: 10.1103/PhysRevC.99.034318
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2019YU06      Eur.Phys.J. A 55, 230 (2019)

E.Yuksel, G.Colo, E.Khan, Y.F.Niu

Nuclear excitations within microscopic EDF approaches: Pairing and temperature effects on the dipole response

doi: 10.1140/epja/i2019-12918-8
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2018YU03      Phys.Rev. C 97, 064308 (2018)

E.Yuksel, G.Colo, E.Khan, Y.F.Niu

Low-energy quadrupole states in neutron-rich tin nuclei

NUCLEAR STRUCTURE 116,118,120,122,124,126,128,130,132,134Sn; calculated mean value of the neutron pairing gap of even-A 116Sn to 130Sn isotopes, proton and neutron single-particle energies of even-A 116Sn to 132Sn, quasiparticle energies and occupation probabilities of neutron states around the Fermi level in 116,120,124,128Sn, energies and B(E2) of first 2+ states, running energy weighted sum of 120Sn, isoscalar quadrupole strengths in even-A 116Sn to 132Sn, reduced transition probabilities of the isoscalar quadrupole responses in 116,120,124,128Sn, quasiparticle contributions to the first 2+ and low-energy states in 120,124,128Sn, proton and neutron transition densities for first 2+, low-energy peak, and GQR region states of 116,120,124,128Sn. Fully self-consistent quasiparticle random phase approximation (QRPA) with Skyrme-type energy density functionals SGII, SLy5 and SkM*. Comparison with experimental values.

doi: 10.1103/PhysRevC.97.064308
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2018YU04      Turk.J.Phys. 42, 613 (2018)

E.Yuksel

Gamow-Teller strength in 56Fe nucleus at finite temperatures

NUCLEAR STRUCTURE 56Fe; calculated Gamow-Teller strength distribution, occupation probabilities for neutrons as a function of temperature around the Fermi level, major low-energy states for GT excitations. Skyrme-type SkM* interaction.

doi: 10.3906/fiz-1804-17
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2017YU03      Phys.Rev. C 96, 024303 (2017)

E.Yuksel, G.Colo, E.Khan, Y.F.Niu, K.Bozkurt

Multipole excitations in hot nuclei within the finite temperature quasiparticle random phase approximation framework

NUCLEAR STRUCTURE 68Ni, 120,122Sn; calculated isovector dipole and isoscalar quadrupole strength functions as function of temperature within the fully self-consistent finite temperature quasiparticle random phase approximation framework, based on the Skyrme-type SLy5 energy density functional. Comparison with available experimental data.

doi: 10.1103/PhysRevC.96.024303
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2014YU04      Phys.Rev. C 89, 064322 (2014)

E.Yuksel, N.Van Giai, E.Khan, K.Bozkurt

Effects of the tensor force on the ground state and first 2+ states of the magic 54Ca nucleus

NUCLEAR STRUCTURE 54Ca, 56Ti, 58Cr, 60Fe; calculated single-particle spectra, occupation probabilities for the neutron states in N=34 isotones. 42,44,46,48,50,52,54Ca; calculated energies and B(E2) of first 2+ states with and without the inclusion of tensor force in the mean-field; deduced magic nature of 52,54Ca isotopes. Importance of the tensor force on the shell evolution of p-f shell nuclei. Hartree-Fock-Bogoliubov (HFB) and Hartree-Fock (HF)+BCS methods using Skyrme-type SLy5, SLy5+T, and T44 interactions. Comparison with experimental data.

doi: 10.1103/PhysRevC.89.064322
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2014YU06      Eur.Phys.J. A 50, 160 (2014)

E.Yuksel, E.Khan, K.Bozkurt, G.Colo

Effect of temperature on the effective mass and the neutron skin of nuclei

NUCLEAR STRUCTURE 112,120Sn; calculated neutron pairing gap vs temperature, proton and neutron radii vs temperature, partial density of states using finite-temperature Hartree-Fock-BCS with zero-range Skyrme forces. 100,102,104,106,108,110,112,114,116,118,120Sn; calculated neutron skin vs neutron number using finite-temperature Hartree-Fock-BCS with zero-range Skyrme forces. 120Sn; calculated neutron levels, J, nucleon effective mass vs temperature and critical temperature, neutron and proton densities vs radius and temperature using different Skyrme interactions.

doi: 10.1140/epja/i2014-14160-4
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2013YU05      Eur.Phys.J. A 49, 124 (2013)

E.Yuksel, E.Khan, K.Bozkurt

The soft Giant Monopole Resonance as a probe of the spin-orbit splitting

NUCLEAR STRUCTURE 100,132Sn, 208Pb; calculated isoscalar monopole strength distribution using Skyrme HF plus RPA model.

doi: 10.1140/epja/i2013-13124-6
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2012YU01      Nucl.Phys. A877, 35 (2012)

E.Yuksel, E.Khan, K.Bozkurt

Analysis of the neutron and proton contributions to the pygmy dipole mode in doubly magic nuclei

NUCLEAR STRUCTURE 16,24O, 40,48,70Ca, 56,68,78Ni, 100,132Sn, 208Pb; calculated GDR, Pygmy dipole strength distribution using self-consistent HF+RPA with Skyrme interactions. Comparison with data.

doi: 10.1016/j.nuclphysa.2012.01.006
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2011YU03      Int.J.Mod.Phys. E20, 2143 (2011)

E.Yuksel, K.Bozkurt

Tensor effects in pygmy dipole excitation

NUCLEAR STRUCTURE 68Ni, 124Sn; calculated Pigmy and Giant Dipole Resonance strength functions, QRPA transition densities. HFB theory with QRPA.

doi: 10.1142/S0218301311020216
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