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NSR database version of May 1, 2024.

Search: Author = H.R.Moshfegh

Found 37 matches.

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2024SH05      Phys.Rev. C 109, 025806 (2024)

R.Shafieepour, H.R.Moshfegh, J.Piekarewicz

Correlating isothermal compressibility to nucleon fluctuations in the inner crust of neutron stars

doi: 10.1103/PhysRevC.109.025806
Citations: PlumX Metrics

2023KA16      Nucl.Phys. A1037, 122684 (2023)

R.Karimi, H.R.Moshfegh

Hybrid stars within the framework of the Sigma-Omega-Rho model combined with the MIT and NJL models

doi: 10.1016/j.nuclphysa.2023.122684
Citations: PlumX Metrics

2022NI04      Phys.Rev. C 105, 045809 (2022)

A.Dehghan Niri, H.R.Moshfegh

Number spectra of nonequilibrium neutrinos from neutron stars: Impact of realistic nuclear interactions and free hyperons

doi: 10.1103/PhysRevC.105.045809
Citations: PlumX Metrics

2022SH21      Phys.Rev. C 105, 055809 (2022)

R.Shafieepour, H.R.Moshfegh, J.Piekarewicz

Characterization of the inner edge of the neutron star crust

doi: 10.1103/PhysRevC.105.055809
Citations: PlumX Metrics

2020RA03      Nucl.Phys. A996, 121678 (2020)

H.Rashidi, S.Zaryouni, H.R.Moshfegh

LOCV calculation for nuclear and neutron matter with the Nijmegen potential

doi: 10.1016/j.nuclphysa.2019.121678
Citations: PlumX Metrics

2020SH05      Phys.Rev. C 101, 025807 (2020)

M.Shahrbaf, D.Blaschke, A.G.Grunfeld, H.R.Moshfegh

First-order phase transition from hypernuclear matter to deconfined quark matter obeying new constraints from compact star observations

doi: 10.1103/PhysRevC.101.025807
Citations: PlumX Metrics

2019GO08      Nucl.Phys. A985, 1 (2019)

S.Goudarzi, H.R.Moshfegh

Neutron and nuclear matter properties with chiral three-nucleon forces

doi: 10.1016/j.nuclphysa.2019.02.002
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2019HE02      Phys.Rev. C 99, 024307 (2019)

S.Heidari, S.Zaryouni, H.R.Moshfegh, S.Goudarzi

Role of relativistic effects and three-body forces in nuclear matter properties

doi: 10.1103/PhysRevC.99.024307
Citations: PlumX Metrics

2019SH39      Phys.Rev. C 100, 044314 (2019)

M.Shahrbaf, H.R.Moshfegh, M.Modarres

Equation of state and correlation functions of hypernuclear matter within the lowest order constrained variational method

NUCLEAR STRUCTURE ^6,7He, ⁸Li, ^9,10Be, ⁸⁹Y, ¹³⁹Ba, ²⁰⁸Pb; calculated binding energies of hypernuclei with one hyperon, and for two hyperons for ^6,7He, ⁸Li, ¹⁰Be using Brueckner-Hartree-Fock (BHF) framework for the lowest order constrained variational (LOCV) method. Comparison with experimental data. Discussed effect of baryon density and hyperon density and hyperon-hyperon interaction on the two-body correlation functions.

doi: 10.1103/PhysRevC.100.044314
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2018DE29      Phys.Rev. C 98, 025803 (2018)

A.Dehghan Niri, H.R.Moshfegh, P.Haensel

Role of nuclear correlations and kinematic effects on neutrino emission from the modified Urca processes

doi: 10.1103/PhysRevC.98.025803
Citations: PlumX Metrics

2018GO01      Nucl.Phys. A969, 206 (2018)

S.Goudarzi, H.R.Moshfegh, P.Haensel

The role of three-body forces in nuclear symmetry energy and symmetry free energy

doi: 10.1016/j.nuclphysa.2017.10.007
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2017KH05      Acta Phys.Pol. B48, 661 (2017)

A.Khodaie, A.Dehghan Niri, H.R.Moshfegh, P.Haensel

Emissivity and Mean-free Paths of Neutrinos in Neutron Star Matter via Modified Urca Processes

doi: 10.5506/APhysPolB.48.661
Citations: PlumX Metrics

2016DE13      Phys.Rev. C 93, 045806 (2016)

A.Dehghan Niri, H.R.Moshfegh, P.Haensel

Nuclear correlations and neutrino emissivity from the neutron branch of the modified Urca process

doi: 10.1103/PhysRevC.93.045806
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2015GO10      Phys.Rev. C 91, 054320 (2015); Erratum Phys.Rev. C 96, 049902 (2017)

S.Goudarzi, H.R.Moshfegh

Effects of three-body forces on the maximum mass of neutron stars in the lowest-order constrained variational formalism

doi: 10.1103/PhysRevC.91.054320
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2015GO17      Phys.Rev. C 92, 035806 (2015); Erratum Phys.Rev. C 97, 094904 (2018)

S.Goudarzi, H.R.Moshfegh

Proto-neutron star structure within an extended lowest-order constrained variational method at finite temperature

doi: 10.1103/PhysRevC.92.035806
Citations: PlumX Metrics

2015MO06      Acta Phys.Pol. B46, 419 (2015)

H.R.Moshfegh, S.Goudarzi

Temperature Dependence of Nuclear Symmetry Free Energy

doi: 10.5506/APhysPolB.46.419
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2014ZA02      Phys.Rev. C 89, 014332 (2014)

S.Zaryouni, M.Hassani, H.R.Moshfegh

Thermal properties of nuclear matter in a variational framework with relativistic corrections

doi: 10.1103/PhysRevC.89.014332
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2013GH02      Phys.Rev. C 88, 034601 (2013)

O.N.Ghodsi, H.R.Moshfegh, R.Gharaei

Role of the saturation properties of hot nuclear matter in the proximity formalism

NUCLEAR REACTIONS ⁵⁴Fe, ^58,62Ni, ⁵⁹Co(¹⁶O, X), E(cm)=25-48 MeV; ⁶²Ni(⁴⁰Ca, X), E(cm)=65-110 MeV; ^72,73Ge(³⁷Cl, X), E(cm)=63-77 MeV; ⁵⁸Ni(²⁸Si, X), E(cm)=47-63 MeV; ^62,64Ni(³⁰Si, X), E not given; ⁶⁰Ni(³⁵Cl, X), E not given; calculated barrier heights V_B and positions R_B in fusion reactions, fusion σ(E), diffuseness parameter vs temperature. Equation of state (EoS) extracted from extended Thomas-Fermi model (ETFM) for asymmetric nuclear matter at finite temperature. Comparison with experimental data.

doi: 10.1103/PhysRevC.88.034601
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2013MO02      Eur.Phys.J. A 49, 1 (2013)

H.R.Moshfegh, M.Ghazanfari Mojarrad

Strange baryonic matter in the Thomas-Fermi theory

doi: 10.1140/epja/i2013-13001-4
Citations: PlumX Metrics

2012BA37      Phys.Rev. C 86, 024306 (2012)

M.Baldo, H.R.Moshfegh

Correlations in nuclear matter

doi: 10.1103/PhysRevC.86.024306
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2010MO18      Eur.Phys.J. A 43, 283 (2010)

H.R.Moshfegh, S.Zaryouni

LOCV calculation of nuclear matter with relativistic Hamiltonian

doi: 10.1140/epja/i2010-10907-1
Citations: PlumX Metrics

2010ZA11      Eur.Phys.J. A 45, 69 (2010)

S.Zaryouni, H.R.Moshfegh

A relativistic approach to the equation of state of asymmetric nuclear matter

doi: 10.1140/epja/i2010-10983-1
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2009MO06      Nucl.Phys. A819, 27 (2009)

M.Modarres, T.Pourmirjafari, H.R.Moshfegh

The LOCV nuclear matter calculation and the magnetic susceptibility of neutron matter

doi: 10.1016/j.nuclphysa.2009.01.004
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2009MO15      Acta Phys.Pol. B40, 661 (2009)

H.R.Moshfegh

LOCV Calculations for Neutron Star Properties

2008MO10      Nucl.Phys. A808, 60 (2008)

M.Modarres, A.Rajabi, H.R.Moshfegh

The one-body momentum distribution of nuclear matter at finite temperature

doi: 10.1016/j.nuclphysa.2008.05.013
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2007MO28      Nucl.Phys. A792, 201 (2007)

H.R.Moshfegh, M.Modarres

Thermal properties of asymmetrical nuclear matter with the new charge-dependent Reid potential

doi: 10.1016/j.nuclphysa.2007.04.013
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2007MO36      Phys.Rev. C 76, 064311 (2007)

M.Modarres, A.Rajabi, H.R.Moshfegh

State-dependent calculation of three-body cluster energy for nuclear matter and the validity of the lowest order constrained variational formalism

doi: 10.1103/PhysRevC.76.064311
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2006MO17      Int.J.Mod.Phys. E15, 1127 (2006)

H.R.Moshfegh

Equation of state of hot nuclear and neutron matter: A statistical approach

doi: 10.1142/S0218301306004727
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2005MO06      Nucl.Phys. A749, 130c (2005)

H.R.Moshfegh, M.Modarres

The properties of hot nuclear matter in LOCV formalism

doi: 10.1016/j.nuclphysa.2004.12.021
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2005MO25      Nucl.Phys. A759, 79 (2005)

H.R.Moshfegh, M.Modarres

Asymmetrical nuclear matter calculations with the new charge-dependent Reid potential

doi: 10.1016/j.nuclphysa.2005.04.021
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2005ZA05      Int.J.Mod.Phys. E14, 297 (2005)

S.Zaryouni, H.R.Moshfegh

Relativistic corrections to the nuclear and neutron matter energy in the LOCV framework

doi: 10.1142/S021830130500303X
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2004MO32      Prog.Theor.Phys.(Kyoto) 112, 21 (2004)

M.Modarres, H.R.Moshfegh

Lowest Order Constrained Variational Calculation for Nuclear and Neutron Matter with a New Charge-Dependent Reid Potential

doi: 10.1143/PTP.112.21
Citations: PlumX Metrics

2004ZA05      Nucl.Phys. A734, E108 (2004)

S.Zaryouni, H.R.Moshfegh

Nuclear matter energy with relativistic Hamiltonian in LOCV formalism

doi: 10.1016/j.nuclphysa.2004.03.032
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2002MO04      Prog.Theor.Phys.(Kyoto) 107, 139 (2002)

M.Modarres, H.R.Moshfegh

Δ(1232) Isobar Probability in Frozen and Hot Neutron, Nuclear and β-Stable Matter

NUCLEAR STRUCTURE ³He, ²⁰⁸Pb; calculated Δ probability vs baryon number density. Comparison with data.

doi: 10.1143/PTP.107.139
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2002MO30      Can.J.Phys. 80, 911 (2002)

M.Modarres, H.R.Moshfegh, H.Mariji

Lowest Order Constrained Variational and Local Density Approximation Approach to the Hot Alpha Particle

NUCLEAR STRUCTURE ⁴He; calculated binding energy, free energy, entropy, other thermodynamic quantities. Constrained variational and local density approximation.

doi: 10.1139/p02-041
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2000MO25      Phys.Rev. C62, 044308 (2000)

M.Modarres, H.R.Moshfegh

Lowest-Order Constrained Variational Calculation for β-Stable Matter at Finite Temperature

doi: 10.1103/PhysRevC.62.044308
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1998MO11      J.Phys.(London) G24, 821 (1998)

H.R.Moshfegh, M.Modarres

The Effect of Three-Body Cluster Energy on LOCV Calculation for Hot Nuclear and Neutron Matter

doi: 10.1088/0954-3899/24/4/012
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