方法证据记录
Pulsar Timing Array
A pulsar timing array uses multiple millisecond pulsars as a distributed network of gravitational wave detectors across the galaxy. Proposed theoretically by Stephen Detweiler in 1979, this method exploits the extraordinary timing precision of pulsars to detect the subtle spacetime distortions caused by gravitational waves. In 2023, the first evidence for a stochastic background of gravitational waves was announced using pulsar timing arrays.
源记录
引文逐字复制自方法源记录。这些引文不代表任何层级的验证。
Pulsar Timing Array for Gravitational Wave Detection
分类方法记录 · process-pipeline / astronomy
- Sazhin, M. V. (1978). Opportunities for detecting ultralong gravitational waves. Soviet Astronomy, 22, 36-38. · URL
- Detweiler, S. (1979). Pulsar timing and its application for detection of gravitational waves. Astrophysical Journal, 234, 1100-1104. · URL
- Arzoumanian, Z., et al. (2023). The NANOGrav 12.5 Year Data Release. Astrophysical Journal Letters, 951(1), L8. · URL
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