The Extended Nuclear Matter Model with Smooth Transition Surface
| dc.creator | H., Jorge A. Rueda | |
| dc.creator | Patricelli, B. | |
| dc.creator | Rotondo, M. | |
| dc.creator | Ruffini, R. | |
| dc.creator | Xue, S-S. | |
| dc.date | 2009-03-25 | |
| dc.date.accessioned | 2026-07-07T12:56:24Z | |
| dc.date.available | 2026-07-07T12:56:24Z | |
| dc.description | The existence of electric fields close to their critical value $E_c=\frac{m_e^2 c^3}{e \hbar}$ has been proved for massive cores of $10^7$ up to $10^{57}$ 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. | |
| dc.description | To appear in the Proceedings of The 3rd Stueckelberg Workshop on Relativistic Field Theories | |
| dc.identifier | https://arxiv.org/abs/0903.4282 | |
| dc.identifier | http://arxiv.org/abs/0903.4282 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/224570 | |
| dc.subject | Solar and Stellar Astrophysics | |
| dc.title | The Extended Nuclear Matter Model with Smooth Transition Surface | |
| dc.type | text |