BUNTING IDENTITY AND MAZUR IDENTITY FOR NON-LINEAR ELLIPTIC-SYSTEMS INCLUDING THE BLACK-HOLE EQUILIBRIUM PROBLEM

被引：38

作者：

CARTER, B

机构：

来源：

关键词：

D O I：

10.1007/BF01215910

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

引用

页码：563 / 591

页数：29

共 30 条

[1]

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[2]

BUNTING G, 1981, UNPUB 2ND P AUSTR MA

CARTER, B .

[4] AXISYMMETRIC BLACK HOLE HAS ONLY 2 DEGREES OF FREEDOM [J].

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[5]

Carter B., 1979, GENERAL RELATIVITY

[6]

CARTER B, 1985, LECTURE NOTES PHYSIC, V223, P72

[7]

CARTER B, 1973, BLACK HOLDS

[8]

CARTER B, 1979, NATO ADV STUDY I S B, V44

DEVEGA, HJ .

[10] MORE ABOUT NON-LINEAR SIGMA-MODELS ON SYMMETRIC-SPACES [J].

EICHENHERR, H ;

FORGER, M .