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Featured researches published by E. Osnes.


Physics Reports | 1995

Realistic effective interactions for nuclear systems

M. Hjorth-Jensen; T.T.S. Kuo; E. Osnes

Abstract A review of perturbative many-body descriptions of several nuclear systems is presented in this report. Examples of systems considered are symmetric and asymmetric nuclear matter and finite nuclei with few valence particles. Our many-body description starts with the most recent meson-exchange potential models for the nucleon-nucleon interaction, an interaction which in turn is used in our perturbative schemes to evaluate the effective interaction for finite nuclei and infinite nuclear matter. A unified perturbative approach based on time-dependent perturbation theory is elaborated. For finite nuclei we present new results for the effective interaction and the energy spectra in the mass areas of oxygen, calcium and tin.


Physical Review Letters | 1994

ASYMMETRIC NUCLEAR MATTER AND NEUTRON STAR PROPERTIES

L. Engvik; M. Hjorth-Jensen; E. Osnes; G. Bao; Ostgaard E

We calculate properties of neutron stars such as mass and radius using a relativistic Dirac-Brueckner-Hartree-Fock approach. Modern meson-exchange potential models are used to evaluate the [ital G] matrix for asymmetric nuclear matter. For pure neutron matter we find the maximum mass to be [ital M][sub max][approx]2.4[ital M][sub [circle dot]] for a radius [ital R][approx]12 km, whereas with a proton fraction of 30% we find [ital M][sub max][approx]2.1[ital M][sub [circle dot]] for a radius [ital R][approx]10.5 km, close to the experimental values. The implications are discussed.


Physical Review Letters | 1996

SUPERFLUIDITY IN BETA -STABLE NEUTRON STAR MATTER

Øystein Elgarøy; L. Engvik; M. Hjorth-Jensen; E. Osnes

In this work we present results for pairing gaps in


The Astrophysical Journal | 1996

Asymmetric Nuclear Matter and Neutron Star Properties

L. Engvik; E. Osnes; M. Hjorth-Jensen; G. Bao; Ostgaard E

\beta


Progress in Particle and Nuclear Physics | 2004

Effective interactions and the nuclear shell-model

D. J. Dean; T. Engeland; M. Hjorth-Jensen; Maxim Kartamyshev; E. Osnes

--stable neutron star matter with electrons and muons using a relativistic Dirac--Brueckner--Hartree--Fock approach, starting with modern meson--exchange models for the nucleon--nucleon interaction. Results are given for superconducting


Nuclear Physics | 1996

Model-space approach to 1S0 neutron and proton pairing in neutron star matter with the Bonn meson-exchange potentials

Øystein Elgarøy; L. Engvik; M. Hjorth-Jensen; E. Osnes

^1S_0


Nuclear Physics | 1975

On the recoil term in the particle-rotor model☆

E. Osnes; J. Rekstad; O.K. Gjøtterud

protons and


Nuclear Physics | 1996

Triplet pairing of neutrons in β-stable neutron star matter

Øystein Elgarøy; L. Engvik; M. Hjorth-Jensen; E. Osnes

^3P_2


Annals of Physics | 1981

A simple method for evaluating Goldstone diagrams in an angular momentum coupled representation

T.T.S. Kuo; J Shurpin; K.C Tam; E. Osnes; Paul J. Ellis

and


Annals of Physics | 1992

Folded-diagram effective interactions with the Bonn meson-exchange potential model

M. Hjorth-Jensen; E. Osnes; H. Müther

^1D_2

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T.T.S. Kuo

Stony Brook University

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D. J. Dean

Oak Ridge National Laboratory

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