Comparison of particle properties in Kerr metric and in rotating coordinates

被引：9

作者：

Grib, Andrey A. ^{[1
,2
]}

Pavlov, Yuri V. ^{[3
,4
]}

机构：

[1] A Friedmann Lab Theoret Phys, St Petersburg, Russia

[2] Herzen Univ, Theoret Phys & Astron Dept, Moika 48, St Petersburg 191186, Russia

[3] Russian Acad Sci, Inst Problems Mech Engn, St Petersburg, Russia

[4] Kazan Fed Univ, NI Lobachevsky Inst Math & Mech, Kazan, Russia

来源：

GENERAL RELATIVITY AND GRAVITATION | 2017年 / 49卷 / 06期

基金：

俄罗斯基础研究基金会;

关键词：

Black holes; Kerr metric; Rotating frames; BLACK-HOLES; ENERGY;

D O I：

10.1007/s10714-017-2238-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Properties of particles in Kerr metric are compared with properties of particles in rotating coordinates in Minkowski space-time. It is shown that particles with negative and zero energies existing in the ergosphere of the rotating black hole also exist in the region out of the static limit in rotating coordinates in Minkowski spacetime. Some similarities like the Penrose process and differences in both cases are analyzed.

引用

页数：20

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