RARITA-SCHWINGER FIELDS IN THE KERR GEOMETRY

被引：19

作者：

DELCASTILLO, GFT ^{[1
]}

SILVAORTIGOZA, G ^{[1
]}

机构：

[1] UNIV AUTONOMA PUEBLA,ESCUELA CIENCIAS FIS MATEMAT,PUEBLA 72570,MEXICO

来源：

PHYSICAL REVIEW D | 1990年 / 42卷 / 12期

关键词：

D O I：

10.1103/PhysRevD.42.4082

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The spin-3/2 perturbations of a rotating black hole are analyzed in the framework of linearized supergravity, expressing the complete solution of the Rarita-Schwinger equation in terms of a Debye potential. The equation governing the Debye potential is separated and the radial equation is transformed into a Schrodinger-type equation with a short-range potential from which the reflection and transmission coefficients can be calculated.

引用

页码：4082 / 4086

页数：5

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