Perturbation theory of nuclear matter with a microscopic effective interaction
Abstract
Here, an updated and improved version of the effective interaction based on the Argonne-Urbana nuclear Hamiltonian, derived using the formalism of correlated basis functions and the cluster expansion technique, is employed to obtain a number of properties of cold nuclear matter at arbitrary neutron excess within the formalism of many-body perturbation theory. The numerical results, including the ground-state energy per nucleon, the symmetry energy, the pressure, the compressibility, and the single-particle spectrum, are discussed in the context of the available empirical information, obtained from measured nuclear properties and heavy-ion collisions.
- Authors:
-
- "Sapienza" Univ. di Roma, Rome (Italy)
- Argonne National Lab. (ANL), Argonne, IL (United States)
- Publication Date:
- Research Org.:
- Argonne National Laboratory (ANL), Argonne, IL (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP)
- OSTI Identifier:
- 1422397
- Alternate Identifier(s):
- OSTI ID: 1406393
- Grant/Contract Number:
- AC02-06CH11357
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review C
- Additional Journal Information:
- Journal Volume: 96; Journal Issue: 5; Journal ID: ISSN 2469-9985
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS
Citation Formats
Benhar, Omar, and Lovato, Alessandro. Perturbation theory of nuclear matter with a microscopic effective interaction. United States: N. p., 2017.
Web. doi:10.1103/PhysRevC.96.054301.
Benhar, Omar, & Lovato, Alessandro. Perturbation theory of nuclear matter with a microscopic effective interaction. United States. https://doi.org/10.1103/PhysRevC.96.054301
Benhar, Omar, and Lovato, Alessandro. Wed .
"Perturbation theory of nuclear matter with a microscopic effective interaction". United States. https://doi.org/10.1103/PhysRevC.96.054301. https://www.osti.gov/servlets/purl/1422397.
@article{osti_1422397,
title = {Perturbation theory of nuclear matter with a microscopic effective interaction},
author = {Benhar, Omar and Lovato, Alessandro},
abstractNote = {Here, an updated and improved version of the effective interaction based on the Argonne-Urbana nuclear Hamiltonian, derived using the formalism of correlated basis functions and the cluster expansion technique, is employed to obtain a number of properties of cold nuclear matter at arbitrary neutron excess within the formalism of many-body perturbation theory. The numerical results, including the ground-state energy per nucleon, the symmetry energy, the pressure, the compressibility, and the single-particle spectrum, are discussed in the context of the available empirical information, obtained from measured nuclear properties and heavy-ion collisions.},
doi = {10.1103/PhysRevC.96.054301},
journal = {Physical Review C},
number = 5,
volume = 96,
place = {United States},
year = {Wed Nov 01 00:00:00 EDT 2017},
month = {Wed Nov 01 00:00:00 EDT 2017}
}
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Works referencing / citing this record:
Cooling Timescale for Protoneutron Stars and Properties of Nuclear Matter: Effective Mass and Symmetry Energy at High Densities
journal, June 2019
- Nakazato, Ken’ichiro; Suzuki, Hideyuki
- The Astrophysical Journal, Vol. 878, Issue 1
Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities
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- Nakazato, Ken'ichiro; Suzuki, Hideyuki
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