The effective relativistic quantum field theory for nuclear matter with many-body forces revisited
Author:
Affiliation:
1. Physics Department, Instituto de Física; Universidade Federal do Rio Grande do Sul-UFRGS; Porto Alegre Rio Grande do Sul Brazil
2. Physics Department; Universidade Federal do Pampa-UNIPAMPA; Caçapava do Sul Rio Grande do Sul Brazil
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1002/asna.201913588/fullpdf
Reference7 articles.
1. A two-solar-mass neutron star measured using Shapiro delay
2. An effective field theory for neutron stars with many-body forces, strong ∑-repulsion, andK-and $\bar K^0$ condensation
3. Saturation of nuclear matter and roles of many-body forces: nuclear matter in neutron stars probed by nucleus—nucleus scattering
4. Recent Progress in Quantum Hadrodynamics
5. Influence of theσ−ωmeson interaction on neutron star matter
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