Gravitational wave detectors

被引：37

作者：

Aufmuth, P ^{[1
]}

Danzmann, K ^{[1
]}

机构：

[1] Leibniz Univ Hannover, Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany

来源：

NEW JOURNAL OF PHYSICS | 2005年 / 7卷

关键词：

D O I：

10.1088/1367-2630/7/1/202

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The existence of gravitational radiation is a prediction of Einstein's general theory of relativity. Gravitational waves are perturbations in the curvature of spacetime caused by accelerated masses. Since the 1960s gravitational wave detectors have been built and constantly improved. The present-day generation of resonant mass antennas and laser interferometers has reached the necessary sensitivity to detect gravitational waves from sources in the Milky Way. Within a few years, the next generation of detectors will open the field of gravitational wave astronomy.

引用

页数：15

共 51 条

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