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NSR database version of April 29, 2024.

Search: Author = N.Alam

Found 6 matches.

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2020AL23      Phys.Rev. C 102, 064620 (2020)

N.Alam, G.Chaudhuri, F.Gulminelli

Isospin properties of the pasta phase with an extended statistical model from microscopic energy functionals

NUCLEAR STRUCTURE A=40-200; Z=20, 28, 50, 82; Z/N=0.6-1.25; calculated differences between theoretical and experimental energies per particle. A=6-250; calculated average Z/N and multiplicity of the clusters as a function of their size and density, with and without the Coulomb screening effect. Canonical thermodynamical model (CTM) for nuclear multifragmentation, with inputs from the relativistic mean-field energy density functionals. Relevance to cooling dynamics of proto-neutron stars.

doi: 10.1103/PhysRevC.102.064620
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2018MA58      Phys.Rev. C 98, 035804 (2018)

T.Malik, N.Alam, M.Fortin, C.Providencia, B.K.Agrawal, T.K.Jha, B.Kumar, S.K.Patra

GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability

doi: 10.1103/PhysRevC.98.035804
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2017AL21      Phys.Rev. C 95, 055808 (2017)

N.Alam, H.Pais, C.Providencia, B.K.Agrawal

Warm unstable asymmetric nuclear matter: Critical properties and the density dependence of the symmetry energy

NUCLEAR STRUCTURE ²⁰⁸Pb; calculated binding energy per particle, charge radii, neutron radii, and neutron skin thickness for ²⁰⁸Pb along with the maximum mass of a neutron star and corresponding radius using several relativistic mean-field models.

doi: 10.1103/PhysRevC.95.055808
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2016AL25      Phys.Rev. C 94, 052801 (2016)

N.Alam, B.K.Agrawal, M.Fortin, H.Pais, C.Providencia, Ad.R.Raduta, A.Sulaksono

Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation

doi: 10.1103/PhysRevC.94.052801
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2015AL17      Phys.Rev. C 92, 015804 (2015)

N.Alam, A.Sulaksono, B.K.Agrawal

Diversity of neutron star properties at the fixed neutron-skin thickness of ²⁰⁸Pb

NUCLEAR STRUCTURE ⁴⁸Ca, ¹³²Sn, ²⁰⁸Pb; calculated binding energy, charge and neutron radii, neutron-skin thickness. ²⁰⁸Pb; calculated density dependence of symmetry energy, variations of symmetry energy slope parameter, core-crust transition density and pressure with neutron-skin thickness, mass-radius relationship, plots for the radius of the neutron stars and red shift, tidal polarizability parameter as function of neutron-star mass. Extended relativistic mean-field (RMF) model using different sets of parameters.

doi: 10.1103/PhysRevC.92.015804
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2014AL31      Phys.Rev. C 90, 054317 (2014)

N.Alam, B.K.Agrawal, J.N.De, S.K.Samaddar, G.Colo

Equation of state of nuclear matter from empirical constraints

doi: 10.1103/PhysRevC.90.054317
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