NSR Query Results


Output year order : Descending
Format : Normal

NSR database version of May 9, 2024.

Search: Author = S.Gmuca

Found 10 matches.

Back to query form



2007MA74      Phys.Atomic Nuclei 70, 1611 (2007)

L.Majling, S.Gmuca

What can we learn about baryon-baryon interaction from hypernuclei 6ΛH and 8ΛH?

NUCLEAR STRUCTURE 4,6,8H; calculated level energies, J, π for Λ hypernuclei.

doi: 10.1134/S1063778807090190
Citations: PlumX Metrics


2004BU24      Phys.Rev. C 70, 054309 (2004)

J.K.Bunta, S.Gmuca

Hyperons in a relativistic mean-field approach to asymmetric nuclear matter

doi: 10.1103/PhysRevC.70.054309
Citations: PlumX Metrics


2004GM01      Nucl.Phys. A734, 172 (2004)

S.Gmuca, J.K.Bunta

Nuclear Symmetry Energy Constraints for RMF Calculations of Superheavy Nuclei

NUCLEAR STRUCTURE Fm, No, Rf, Sg, Hs; A=244-268; calculated binding energies, symmetry energy effects.

doi: 10.1016/j.nuclphysa.2004.01.027
Citations: PlumX Metrics


2004GM02      Acta Phys.Hung.N.S. 19, 155 (2004)

S.Gmuca

Superheavy Nuclei in the RMF Framework

NUCLEAR STRUCTURE 244,246,248,250,252,254Fm, 250,252,254,256,258,260,262No, 254,256,258,260,262,264Rf, 258,260,262,264,266Sg, 264,266,268Hs; calculated relative binding energies. 248,250,252,254,256,258,260,262,264,266,268No, 252,254,256,258,260,262,264,266,268,270Rf, 256,258,260,262,264,266,268,270,272,274Sg, 262,264,266,268,270,272,274,276,278,280Hs; calculated Qα. Relativistic mean-field approach.

doi: 10.1556/APH.19.2004.1-2.24
Citations: PlumX Metrics


2003BU19      Phys.Rev. C 68, 054318 (2003)

J.K.Bunta, S.Gmuca

Asymmetric nuclear matter in the relativistic mean-field approach with vector cross interaction

doi: 10.1103/PhysRevC.68.054318
Citations: PlumX Metrics


2001LE22      Acta Phys.Slovaca 51, 201 (2001)

J.Leja, S.Gmuca

Relativistic Mean-Field Study of Even-Even Oxygen Isotopes

NUCLEAR STRUCTURE 12,14,16,18,20,22,24,26,28O; calculated binding energies, single-particle levels. 26,28O deduced particle stability. Relativistic mean-field theory, several parameterizations compared.


1997GM01      Acta Phys.Hung.N.S. 6, 99 (1997)

S.Gmuca

Halo Nuclei Studied by Relativistic Mean-Field Approach

NUCLEAR STRUCTURE 7,9,10,11,12,14Be; calculated matter radii; deduced halo nuclei properties. Relativistic mean field approach. Comparison with data.


1992GM01      Nucl.Phys. A547, 447 (1992)

S.Gmuca

Finite-Nuclei Calculations Based on Relativistic Mean-Field Effective Interactions

NUCLEAR STRUCTURE 16O, 40Ca; calculated proton, neutron levels, charge radius, binding energy per nucleon.

doi: 10.1016/0375-9474(92)90032-F
Citations: PlumX Metrics


1991GM02      J.Phys.(London) G17, 1115 (1991)

S.Gmuca

Relativistic Mean-Field Fit to Microscopic Results in Nuclear Matter

NUCLEAR STRUCTURE 16O; calculated binding energy per particle, proton, neutron single particle energies, rms radius, charge distribution. Relativistic mean field approximation.

doi: 10.1088/0954-3899/17/7/010
Citations: PlumX Metrics


1983RI12      J.Phys.(London) G9, 1537 (1983)

I.Ribansky, S.Gmuca

Neutron Activation Cross Sections for Ti Isotopes at 14.8 MeV

NUCLEAR REACTIONS 46,47,48,50Ti(n, p), 47,48,49Ti(n, np), 50Ti(n, α), E=14.8 MeV; measured 47,48,50Sc, 47Ca, 46,46mSc production σ. Activation technique. Natural, enriched samples, Ge(Li) detector, preequilibrium, equilibrium models.

doi: 10.1088/0305-4616/9/12/014
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset30660.


Back to query form