NUMERICAL IMPLEMENTATION OF A PERTURBATION-THEORY UP TO THE 3RD ORDER FOR ROTATING POLYTROPIC STARS - APPLICATION TO A SOLAR MODEL

被引：6

作者：

GEROYANNIS, VS ^{[1
]}

VALVI, FN ^{[1
]}

机构：

[1] UNIV PATRAS,DEPT MATH,PATRAS,GREECE

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1986年 / 123卷 / 02期

关键词：

D O I：

10.1007/BF00653948

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：273 / 295

页数：23

共 50 条

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[38] FORMULAS FROM 1ST-ORDER, 2ND-ORDER, AND 3RD-ORDER PERTURBATION-THEORY FOR ATOMS WITH ONE VALENCE ELECTRON
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GUO, DS
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[39] CONVERGENCE STUDIES OF THE EFFECTIVE VALENCE SHELL HAMILTONIAN FOR CORRELATION ENERGIES OF THE FLUORINE ATOM AND ITS IONS USING 3RD ORDER QUASIDEGENERATE MANY-BODY PERTURBATION-THEORY
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[40] NUMERICAL-SOLUTION OF THE SINGULAR PERTURBATION 3RD BOUNDARY-PROBLEM FOR THE GENERAL EQUATION OF THE 2ND-ORDER
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