RELATIVISTIC RING MODELS

被引：2

作者：

Ujevic, Maximiliano ^{[1
]}

Letelier, Patricio S. ^{[2
]}

Vogt, Daniel ^{[2
]}

机构：

[1] Univ Fed ABC, Ctr Ciencias Nat & Humanas, BR-09210170 Sao Paulo, Brazil

[2] Univ Estadual Campinas, Inst Matemat Estat & Comp Cient, Dept Matemat Aplicada, BR-13081970 Campinas, SP, Brazil

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2011年 / 20卷 / 12期

基金：

巴西圣保罗研究基金会;

关键词：

General relativity; rings; stability; DENSITY-POTENTIAL PAIRS; SUPERPOSED WEYL FIELDS; FLAT RINGS; GALAXIES; STABILITY; DISKS;

D O I：

10.1142/S0218271811020305

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Relativistic thick ring models are constructed using previously found analytical Newtonian potential-density pairs for flat rings and toroidal structures obtained from Kuzmin-Toomre family of disks. In particular, we present systems with one ring, two rings and a disk with a ring. Also, the circular velocity of a test particle and its stability when performing circular orbits are presented in all these models. In general, we find that regions of non-stability appear between the rings when they become thinner.

引用

页码：2291 / 2304

页数：14

共 28 条

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