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利用电磁频谱观测对强场引力的探测与测试

Probes and Tests of Strong-Field Gravity with Observations in the Electromagnetic Spectrum.

作者信息

Psaltis Dimitrios

机构信息

Physics and Astronomy Departments, University of Arizona, Tucson, AZ 85721 USA.

出版信息

Living Rev Relativ. 2008;11(1):9. doi: 10.12942/lrr-2008-9. Epub 2008 Nov 18.

DOI:10.12942/lrr-2008-9
PMID:28163608
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC5253923/
Abstract

Neutron stars and black holes are the astrophysical systems with the strongest gravitational fields in the universe. In this article, I review the prospect of using observations of such compact objects to probe some of the most intriguing general relativistic predictions in the strong-field regime: the absence of stable circular orbits near a compact object and the presence of event horizons around black-hole singularities. I discuss the need for a theoretical framework, within which future experiments will provide detailed, quantitative tests of gravity theories. Finally, I summarize the constraints imposed by current observations of neutron stars on potential deviations from general relativity.

摘要

中子星和黑洞是宇宙中具有最强引力场的天体物理系统。在本文中，我回顾了利用对此类致密天体的观测来探究强场 regime 中一些最引人入胜的广义相对论预测的前景：致密天体附近不存在稳定的圆形轨道以及黑洞奇点周围存在事件视界。我讨论了对理论框架的需求，在该框架内未来的实验将对引力理论进行详细的定量测试。最后，我总结了当前中子星观测对与广义相对论潜在偏差所施加的限制。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c17d/5253923/f5c068bb3f0b/41114_2016_9_Fig19.jpg
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