NSR Query Results
Output year order : Descending NSR database version of May 2, 2024. Search: Author = G.H.Bordbar Found 19 matches. 2022MO01 Nucl.Phys. A1017, 122339 (2022) Nuclear matter calculations with the phenomenological three-nucleon interaction
doi: 10.1016/j.nuclphysa.2021.122339
2022MO04 Nucl.Phys. A1017, 122339 (2022) Nuclear matter calculations with the phenomenological three-nucleon interaction
doi: 10.1016/j.nuclphysa.2021.122339
2020KA14 Eur.Phys.J. A 56, 2 (2020) F.Kayanikhoo, K.Naficy, G.H.Bordbar Influence of strong magnetic field on the structure properties of strange quark stars
doi: 10.1140/epja/s10050-019-00004-y
2017RE03 Eur.Phys.J. A 53, 43 (2017) Hot magnetized nuclear matter: Thermodynamic and saturation properties
doi: 10.1140/epja/i2017-12236-3
2016BO27 Rom.J.Phys. 61, 413 (2016) Calculation of Nuclear Matter in the Presence of Strong Magnetic Field Using LOCV Technique
2016RE11 Eur.Phys.J. A 52, 132 (2016) Saturation properties of nuclear matter in the presence of strong magnetic field
doi: 10.1140/epja/i2016-16132-0
2015BO14 Rom.J.Phys. 60, 1010 (2015) G.H.Bordbar, R.Feridoonnezhad, M.Taghizade Asymmetry Energy of Nuclear Matter: Temperature and Density Dependence, and Validity of Semi-Empirical Formula
2011BO11 Phys.Rev. C 83, 044310 (2011) G.H.Bordbar, Z.Rezaei, A.Montakhab Investigation of the field-induced ferromagnetic phase transition in spin-polarized neutron matter: A lowest order constrained variational approach
doi: 10.1103/PhysRevC.83.044310
2010BI08 Phys.Rev. C 82, 034309 (2010) M.Bigdeli, G.H.Bordbar, A.Poostforush Finite-temperature calculations for spin-polarized asymmetric nuclear matter with the lowest order constrained variational method
doi: 10.1103/PhysRevC.82.034309
2009BI06 Phys.Rev. C 80, 034310 (2009) M.Bigdeli, G.H.Bordbar, Z.Rezaei Temperature dependence of magnetic susceptibility of nuclear matter: Lowest order constrained variational calculations
doi: 10.1103/PhysRevC.80.034310
2008BO06 Phys.Rev. C 77, 015805 (2008) Spin polarized asymmetric nuclear matter and neutron star matter within the lowest order constrained variational method
doi: 10.1103/PhysRevC.77.015805
2008BO33 Phys.Rev. C 78, 054315 (2008) Lowest order constrained variational calculation of polarized neutron matter at finite temperature
doi: 10.1103/PhysRevC.78.054315
2007BO14 Phys.Rev. C 75, 045804 (2007) Polarized neutron matter: A lowest order constrained variational approach
doi: 10.1103/PhysRevC.75.045804
2007BO35 Phys.Rev. C 76, 035803 (2007) Lowest order constrained variational calculation of polarized nuclear matter with the modern AV18 potential
doi: 10.1103/PhysRevC.76.035803
2004BO17 Int.J.Theor.Phys. 43, 399 (2004) Isospin Symmetry Breaking Effects on the Properties of Asymmetrical Nuclear Matter and β-Stable Matter
doi: 10.1023/B:IJTP.0000028872.40417.47
2001BO48 Int.J.Theor.Phys. 40, 1671 (2001) Equation of State of Newborn Neutron Star Matter with Untrapped Neutrinos
doi: 10.1023/A:1011654424207
1998BO03 Phys.Rev. C57, 714 (1998) Lowest Order Constrained Variational Calculation for Asymmetrical Nuclear Matter with the New Argonne Potential
doi: 10.1103/PhysRevC.57.714
1998MO28 Phys.Rev. C58, 2781 (1998) Incompressibility of Hot Asymmetrical Nuclear Matter: Lowest order constrained variational approach
doi: 10.1103/PhysRevC.58.2781
1997BO35 J.Phys.(London) G23, 1631 (1997) LOCV Calculation of Nuclear Matter with Phenomenological Two-Nucleon Interaction Operators
doi: 10.1088/0954-3899/23/11/011
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