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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