The Extended Nuclear Matter Model with Smooth Transition Surface
Solar and Stellar Astrophysics
2009-03-26 v1
Abstract
The existence of electric fields close to their critical value has been proved for massive cores of up to nucleons using a proton distribution of constant density and a sharp step function at its boundary. We explore the modifications of this effect by considering a smoother density profile with a proton distribution fulfilling a Woods--Saxon dependence. The occurrence of a critical field has been confirmed. We discuss how the location of the maximum of the electric field as well as its magnitude is modified by the smoother distribution.
Cite
@article{arxiv.0903.4282,
title = {The Extended Nuclear Matter Model with Smooth Transition Surface},
author = {Jorge A. Rueda H. and B. Patricelli and M. Rotondo and R. Ruffini and S-S. Xue},
journal= {arXiv preprint arXiv:0903.4282},
year = {2009}
}
Comments
To appear in the Proceedings of The 3rd Stueckelberg Workshop on Relativistic Field Theories