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Gravitational radiation: The theoretical aspect

 

作者: S.W. Hawking,  

 

期刊: Contemporary Physics  (Taylor Available online 1972)
卷期: Volume 13, issue 3  

页码: 273-282

 

ISSN:0010-7514

 

年代: 1972

 

DOI:10.1080/00107517208205681

 

出版商: Taylor & Francis Group

 

数据来源: Taylor

 

摘要:

The Theory of Relativity requires that theie should be a gravitational analogue to electromagnetic radiation. It is impossible to generate measurable quantities in the laboratory but recent observations indicate that there may be a tremendous flux coming from the centre of our galaxy. Collisions between gravita-tionally collapsed objects (black holes) seem to be the only mechanism which could produce this amount of radiation.

 

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