SPIN-3/2 PERTURBATIONS OF THE KERR-NEWMAN SOLUTION

被引：12

作者：

DELCASTILLO, GFT ^{[1
]}

SILVAORTIGOZA, G ^{[1
]}

机构：

[1] INST POLITECN NACL,CTR INVEST & ESTUDIOS AVANZADOS,DEPT FIS,MEXICO CITY 07000,DF,MEXICO

来源：

PHYSICAL REVIEW D | 1992年 / 46卷 / 12期

关键词：

D O I：

10.1103/PhysRevD.46.5395

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The equations for the spin-3/2 perturbations of a rotating charged black hole given by the linearized O(2) extended supergravity model are solved, expressing their complete solution in terms of two Debye potentials that obey the same differential equation. The equation governing the radial parts of the Debye potentials is transformed into a Schrodinger-type equation with a short-range real potential. It is also shown that there exist spin-3/2 perturbations corresponding only to ingoing or only to outgoing waves.

引用

页码：5395 / 5398

页数：4

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