Pulsars as probes of gravity and fundamental physics

被引：56

作者：

Kramer, Michael ^{[1
,2
]}

机构：

[1] Max Planck Inst Radioastron, Auf Dem Hugel 69, D-53121 Bonn, Germany

[2] Univ Manchester, Jodrell Bank Ctr Astrophys, Oxford Rd, Manchester M13 9PL, Lancs, England

来源：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2016年 / 25卷 / 14期

基金：

欧洲研究理事会;

关键词：

Pulsars; neutron stars; black holes; gravitational-wave astrophysics; experimental tests of gravitational theories; STRONG-FIELD TESTS; SGR A-ASTERISK; GENERAL-RELATIVITY; BINARY EVOLUTION; SPIN PRECESSION; BLACK-HOLE; DISCOVERY; MASS; EMISSION; SYSTEM;

D O I：

10.1142/S0218271816300299

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Radio-loud neutron stars known as pulsars allow a wide range of experimental tests for fundamental physics, ranging from the study of super-dense matter to tests of General Relativity (GR) and its alternatives. As a result, pulsars provide strong-field tests of gravity, they allow for the direct detection of gravitational waves in a "pulsar timing array" (PTA), and they promise the future study of black hole properties. This contribution gives an overview of the on-going experiments and recent results.

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