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Open AccessJournal ArticleDOI

Screening effects in superfluid nuclear and neutron matter within Brueckner theory

L. G. Cao, +2 more
- 01 Dec 2006 - 
- Vol. 74, Iss: 6, pp 064301
TLDR
In this paper, the effects of medium polarization on pairing in neutron and nuclear matter were studied and the screening potential was calculated in the RPA limit, suitably renormalized to cure the low density mechanical instability of nuclear matter.
Abstract
Effects of medium polarization are studied for ${}^{1}{S}_{0}$ pairing in neutron and nuclear matter. The screening potential is calculated in the RPA limit, suitably renormalized to cure the low density mechanical instability of nuclear matter. The self-energy corrections are consistently included resulting in a strong depletion of the Fermi surface. All medium effects are calculated based on the Brueckner theory. The ${}^{1}{S}_{0}$ gap is determined from the generalized gap equation. The self-energy corrections always lead to a quenching of the gap, which is enhanced by the screening effect of the pairing potential in neutron matter, whereas it is almost completely compensated by the antiscreening effect in nuclear matter.

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Citations
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Physics of Neutron Star Crusts

TL;DR: This review summarizes the progress, which has been achieved over the last few years, in modeling neutron star crusts, both at the microscopic and macroscopic levels.
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Nuclear Energy Density Optimization

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The BCS–BEC crossover: From ultra-cold Fermi gases to nuclear systems

TL;DR: In this article, the authors focus on the BCS-BEC crossover in ultra-cold Fermi gases and nuclear matter, and discuss the mean field treatment of the superfluid phase, both for homogeneous and inhomogeneous systems.
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The BCS-BEC crossover: From ultra-cold Fermi gases to nuclear systems

TL;DR: The BCS-BEC crossover has recently been realized experimentally, and essentially in all of its aspects, with ultra-cold Fermi gases and nuclear matter as mentioned in this paper.
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Neutron Matter from Low to High Density

TL;DR: In this paper, the authors review the behavior of very low density neutron matter, which forms a strongly paired superfluid and is thus similar to cold Fermi atoms, although at energy scales that differ by many orders of magnitude.
References
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Book

The Nuclear Many-body Problem

TL;DR: In this paper, the Hartree-Fock method pairing correlations and superfluid nuclei was used to restore broken symmetries in the generator coordinate method of the generator-coordinate method.
Book

Theory Of Interacting Fermi Systems

TL;DR: In this article, a detailed exposition of field theoretical methods as applied to zero temperature Fermi liquids is provided, with special attention paid to the concept of quasiparticles.
BookDOI

Nuclear methods and the nuclear equation of state

TL;DR: The Brueckner-Bethe-Goldstone expansion, R. Dickoff Dirac-Bruecker approach for finite nuclei, H. Muether long range correlations, T. Kuo non-nucleonic degrees of freedom, L.S. Lombardo astrophysical applications, I. Bombaci EOS at finite temperature, M. Baldo superfluidity, U.T.
Book ChapterDOI

Superfluidity in Neutron Star Matter

TL;DR: In fact, during more than two decades of neutron-star physics the presence of neutron and proton superfluid phases has been invoked to explain the dynamical and thermal evolution of a neutron star as discussed by the authors.
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