Skip to main content
We gratefully acknowledge support from the Simons Foundation, member institutions, and all contributors. Donate
arXiv logo
Cornell University Logo

Nuclear Theory

arXiv:nucl-th/0012014 (nucl-th)
[Submitted on 5 Dec 2000]

Title:Microscopic Theory of the Nuclear Equation of State and Neutron Star Structure

Authors:Marcello Baldo, Fiorella Burgio (Istituto Nazionale di Fisica Nucleare, Sezione di Catania, Italy)
View PDF
Abstract: The Bethe-Brueckner-Goldstone many-body theory of the Nuclear Equation of State is reviewed in some details. In the theory, one performs an expansion in terms of the Brueckner two-body scattering matrix and an ordering of the corresponding many-body diagrams according to the number of their hole-lines. Recent results are reported, both for symmetric and for pure neutron matter, based on realistic two-nucleon interactions. It is shown that there is strong evidence of convergence in the expansion. Once three-body forces are introduced, the phenomenological saturation point is reproduced and the theory is applied to the study of neutron star properties. One finds that in the interior of neutron stars the onset of hyperons strongly softens the Nuclear Equation of State. As a consequence, the maximum mass of neutron stars turns out to be at the lower limit of the present phenomenological observation.
Comments: 30 pages, 21 postscript figures included. Lecture presented at the workshop on "Physics of Neutron Stars Interior" held at the European Center for Theoretical Nuclear Physics, June 2000, Trento, Italy. To be published in Lecture Notes in Physics, eds. D. Blaschke, N. K. Glendenning and A. Sedrakian (Springer, 2001)
Subjects: Nuclear Theory (nucl-th); Astrophysics (astro-ph)
Cite as: arXiv:nucl-th/0012014
  (or arXiv:nucl-th/0012014v1 for this version)
  https://doi.org/10.48550/arXiv.nucl-th/0012014
Journal reference: Lect.Notes Phys. 578 (2001) 1-29

Submission history

From: [view email]
[v1] Tue, 5 Dec 2000 13:34:47 UTC (137 KB)
Full-text links:

Access Paper:

  • View PDF
  • TeX Source
  • Other Formats
view license
Current browse context:
nucl-th
< prev   |   next >
new | recent | 2000-12

References & Citations

export BibTeX citation

Bookmark

BibSonomy logo Reddit logo

Bibliographic and Citation Tools

Bibliographic Explorer (What is the Explorer?)
Connected Papers (What is Connected Papers?)
Litmaps (What is Litmaps?)
scite Smart Citations (What are Smart Citations?)

Code, Data and Media Associated with this Article

alphaXiv (What is alphaXiv?)
CatalyzeX Code Finder for Papers (What is CatalyzeX?)
DagsHub (What is DagsHub?)
Gotit.pub (What is GotitPub?)
Hugging Face (What is Huggingface?)
Papers with Code (What is Papers with Code?)
ScienceCast (What is ScienceCast?)

Demos

Replicate (What is Replicate?)
Hugging Face Spaces (What is Spaces?)
TXYZ.AI (What is TXYZ.AI?)

Recommenders and Search Tools

Influence Flower (What are Influence Flowers?)
CORE Recommender (What is CORE?)

arXivLabs: experimental projects with community collaborators

arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website.

Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them.

Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.

Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?)