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Title: Three-body force effect on {sup 3}P F{sub 2} neutron superfluidity in neutron matter, neutron star matter, and neutron stars

Abstract

We investigate the effect of microscopic three-body forces on the {sup 3}P F{sub 2} neutron superfluidity in neutron matter, {beta}-stable neutron star matter, and neutron stars by using the BCS theory and the Brueckner-Hartree-Fock approach. We adopt the Argonne V18 potential supplemented with a microscopic three-body force as the realistic nucleon-nucleon interaction. We have concentrated on studying the three-body force effect on the {sup 3}P F{sub 2} neutron pairing gap. It is found that the three-body force effect considerably enhances the {sup 3}P F{sub 2} neutron superfluidity in neutron star matter and neutron stars.

Authors:
;  [1];  [2];  [3]
  1. Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000 (China)
  2. Department of Physics and Astrophysics, Catania University, Via Santa Sofia 64, I-95123 (Italy)
  3. INFN Sezione di Catania, I-95123 Catania (Italy)
Publication Date:
OSTI Identifier:
21192070
Resource Type:
Journal Article
Journal Name:
Physical Review. C, Nuclear Physics
Additional Journal Information:
Journal Volume: 78; Journal Issue: 1; Other Information: DOI: 10.1103/PhysRevC.78.015805; (c) 2008 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0556-2813
Country of Publication:
United States
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS; BCS THEORY; HARTREE-FOCK METHOD; NEUTRON STARS; NEUTRONS; NUCLEAR MATTER; NUCLEON-NUCLEON INTERACTIONS; SUPERFLUIDITY; THREE-BODY PROBLEM

Citation Formats

Zuo, W, Cui, C X, Lombardo, U, and Schulze, H -J. Three-body force effect on {sup 3}P F{sub 2} neutron superfluidity in neutron matter, neutron star matter, and neutron stars. United States: N. p., 2008. Web. doi:10.1103/PHYSREVC.78.015805.
Zuo, W, Cui, C X, Lombardo, U, & Schulze, H -J. Three-body force effect on {sup 3}P F{sub 2} neutron superfluidity in neutron matter, neutron star matter, and neutron stars. United States. https://doi.org/10.1103/PHYSREVC.78.015805
Zuo, W, Cui, C X, Lombardo, U, and Schulze, H -J. 2008. "Three-body force effect on {sup 3}P F{sub 2} neutron superfluidity in neutron matter, neutron star matter, and neutron stars". United States. https://doi.org/10.1103/PHYSREVC.78.015805.
@article{osti_21192070,
title = {Three-body force effect on {sup 3}P F{sub 2} neutron superfluidity in neutron matter, neutron star matter, and neutron stars},
author = {Zuo, W and Cui, C X and Lombardo, U and Schulze, H -J},
abstractNote = {We investigate the effect of microscopic three-body forces on the {sup 3}P F{sub 2} neutron superfluidity in neutron matter, {beta}-stable neutron star matter, and neutron stars by using the BCS theory and the Brueckner-Hartree-Fock approach. We adopt the Argonne V18 potential supplemented with a microscopic three-body force as the realistic nucleon-nucleon interaction. We have concentrated on studying the three-body force effect on the {sup 3}P F{sub 2} neutron pairing gap. It is found that the three-body force effect considerably enhances the {sup 3}P F{sub 2} neutron superfluidity in neutron star matter and neutron stars.},
doi = {10.1103/PHYSREVC.78.015805},
url = {https://www.osti.gov/biblio/21192070}, journal = {Physical Review. C, Nuclear Physics},
issn = {0556-2813},
number = 1,
volume = 78,
place = {United States},
year = {Tue Jul 15 00:00:00 EDT 2008},
month = {Tue Jul 15 00:00:00 EDT 2008}
}