The Extended Nuclear Matter Model with Smooth Transition Surface

dc.creatorH., Jorge A. Rueda
dc.creatorPatricelli, B.
dc.creatorRotondo, M.
dc.creatorRuffini, R.
dc.creatorXue, S-S.
dc.date2009-03-25
dc.date.accessioned2026-07-07T12:56:24Z
dc.date.available2026-07-07T12:56:24Z
dc.descriptionThe 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.descriptionTo appear in the Proceedings of The 3rd Stueckelberg Workshop on Relativistic Field Theories
dc.identifierhttps://arxiv.org/abs/0903.4282
dc.identifierhttp://arxiv.org/abs/0903.4282
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/224570
dc.subjectSolar and Stellar Astrophysics
dc.titleThe Extended Nuclear Matter Model with Smooth Transition Surface
dc.typetext

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