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NSR database version of April 27, 2024.

Search: Author = C.Constantinou

Found 9 matches.

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2022FA05      Phys.Rev. C 105, 054301 (2022)

P.J.Fasano, C.Constantinou, M.A.Caprio, P.Maris, J.P.Vary

Natural orbitals for the ab initio no-core configuration interaction approach

NUCLEAR STRUCTURE ^3,6He; calculated ground-state energy, point-proton and point-neutron rms radii, radial wave functions. Improved accuracy of the ab initio no-core configuration interaction (NCCI) calculations by implementing the basis of natural orbitals in the NCCI framework. Comparison to experimental data.

doi: 10.1103/PhysRevC.105.054301
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2019LA04      Eur.Phys.J. A 55, 10 (2019)

S.Lalit, M.A.A.Mamun, C.Constantinou, M.Prakash

Dense matter equation of state for neutron star mergers

doi: 10.1140/epja/i2019-12670-1
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2019SC15      Phys.Rev. C 100, 025803 (2019)

A.S.Schneider, C.Constantinou, B.Muccioli, M.Prakash

Akmal-Pandharipande-Ravenhall equation of state for simulations of supernovae, neutron stars, and binary mergers

doi: 10.1103/PhysRevC.100.025803
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2018AL26      Phys.Rev. C 97, 064324 (2018)

M.A.Al Mamun, C.Constantinou, M.Prakash

Pairing properties from random distributions of single-particle energy levels

NUCLEAR STRUCTURE ⁵⁷Co, ¹²⁶Sn, ¹⁹⁷Pt; calculated neutron single-particle energy levels from HFB and HF+BCS using the SkO energy density functional with full pairing, pairing gap vs temperature for 500 sets of randomly generated single-particle levels, pairing phase transitions from HF+BCS, pairing gap vs temperature and projection of the total angular momentum. ¹⁹⁷Pt; calculated temperature dependence of most probable and average pairing gap for protons and neutrons, proton and neutron excitation energies and specific heats at constant volume. Constant spacing (CS) model with BCS formalism. Comparison with results from random spacing (RS) model calculations.

doi: 10.1103/PhysRevC.97.064324
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2017CO06      Phys.Rev. C 95, 055802 (2017)

C.Constantinou, M.Prakash

Enforcing causality in nonrelativistic equations of state at finite temperature

doi: 10.1103/PhysRevC.95.055802
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2015CO14      Phys.Rev. C 92, 025801 (2015)

C.Constantinou, B.Muccioli, M.Prakash, J.M.Lattimer

Thermal properties of hot and dense matter with finite range interactions

doi: 10.1103/PhysRevC.92.025801
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2014CO11      Phys.Rev. C 89, 065802 (2014)

C.Constantinou, B.Muccioli, M.Prakash, J.M.Lattimer

Thermal properties of supernova matter: The bulk homogeneous phase

doi: 10.1103/PhysRevC.89.065802
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2012CA13      Phys.Rev. C 85, 034324 (2012)

M.A.Caprio, F.Q.Luo, K.Cai, V.Hellemans, Ch.Constantinou

Generalized seniority for the shell model with realistic interactions

NUCLEAR STRUCTURE ^{41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59}Ca; calculated levels, J, π, orbital occupations, quadrupole moments, B(E2), magnetic moment. Comparison between seniority (ν=1-3) model space and full shell-model space.

doi: 10.1103/PhysRevC.85.034324
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2012CA30      J.Phys.(London) G39, 105108 (2012)

M.A.Caprio, F.Q.Luo, K.Cai, Ch.Constantinou, V.Hellemans

Generalized seniority with realistic interactions in open-shell nuclei

NUCLEAR STRUCTURE ^{40,42,44,46,48,50,52,54,56,58,60}Ca, ^{42,44,46,48,50,52,54,56,58,60,62}Ti, ^{44,46,48,50,52,54,56,58,60,62,64}Cr; calculated energy levels, J, π, electric quadrupole and dipole magnetic moments. Shell model calculations, FPD6 and GXPF1 interactions, comparison with available data.

doi: 10.1088/0954-3899/39/10/105108
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