Equation of state of nuclear matter from empirical constraints

N. Alam, B. K. Agrawal, J. N. De, S. K. Samaddar, and G. Colò
Phys. Rev. C 90, 054317 – Published 14 November 2014

Abstract

From empirically determined values of some of the characteristic constants associated with homogeneous nuclear matter at saturation and subsaturation densities, within the framework of a Skyrme-inspired energy density functional, we construct an equation of state (EoS) of nuclear matter. This EoS is then used to predict values of density slope parameters of symmetry energy L(ρ), isoscalar incompressibility K(ρ), and a few related quantities. The close consonance of our predicted values with the currently available ones for the density dependence of symmetry energy and incompressibility gleaned from diverse approaches offers the possibility that our method may help in settling their values in tighter bounds. Extrapolation of our EoS at supranormal densities shows that it is in good harmony with the one extracted from experimental data.

  • Figure
  • Figure
  • Figure
  • Figure
  • Received 16 April 2014
  • Revised 14 October 2014

DOI:https://doi.org/10.1103/PhysRevC.90.054317

©2014 American Physical Society

Authors & Affiliations

N. Alam, B. K. Agrawal, J. N. De, and S. K. Samaddar

  • Saha Institute of Nuclear Physics, 1/AF Bidhannagar, Kolkata 700064, India

G. Colò

  • Dipartimento di Fisica, Università degli Studi di Milano, via Celoria 16, I-20133 Milano, Italy and INFN, sezione di Milano, via Celoria 16, I-20133 Milano, Italy

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 90, Iss. 5 — November 2014

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review C

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×