Gravitational radiation in optical geometry applied to super-compact stars

被引：5

作者：

Abramowicz, MA ^{[1
]}

机构：

[1] Chalmers Univ Technol, Inst Theoret Phys, S-41296 Gothenburg, Sweden

来源：

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 1999年 / 311卷 / 3-5期

关键词：

neutron stars; black holes; gravitational radiation;

D O I：

10.1016/S0370-1573(98)00110-0

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Using optical geometry, I derive in a few lines of calculation a simple and accurate formula that describes axial modes of gravitational radiation partially trapped inside a super-compact star. (C) 1999 Elsevier Science B.V. All rights reserved.

引用

页码：325 / 329

页数：5

共 4 条

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ABRAMOWICZ, MA ;

CARTER, B ;

LASOTA, JP .

GENERAL RELATIVITY AND GRAVITATION, 1988, 20 (11) :1173-1183

[2] Gravitational waves from ultracompact stars: the optical geometry view of trapped modes [J].

Abramowicz, MA ;

Andersson, N ;

Bruni, M ;

Ghosh, P ;

Sonego, S .

CLASSICAL AND QUANTUM GRAVITY, 1997, 14 (12) :L189-L194

[3]

ABRAMOWICZ MA, 1998, UNPUB

[4] On the oscillation spectra of ultracompact stars: An extensive survey of gravitational-wave modes [J].

Andersson, N ;

Kojima, Y ;

Kokkotas, KD .

ASTROPHYSICAL JOURNAL, 1996, 462 (02) :855-864

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