方法证据记录
Gravitational Wave Matched Filtering
Matched filtering is a signal processing technique used to detect gravitational waves by correlating detector data with theoretical waveform templates. When two massive objects (black holes, neutron stars) merge, they emit gravitational waves that pass through Earth, producing tiny distortions in laser interferometers like LIGO and Virgo. Matched filtering, formalized by Harry Nyquist, optimally extracts these signals from noise, enabling the detection of mergers billions of light-years away.
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。
Gravitational Wave Signal Detection via Matched Filtering
分类方法记录 · process-pipeline / applied-physics
- Abbott, B. P., et al. (2016). Observation of Gravitational Waves from a Binary Black Hole Merger. Physical Review Letters, 116(6), 061102. · DOI 10.1103/PhysRevLett.116.061102
- Weedman, D. (2010). Statistics of Matched Filtering and Bayes Theorem Applied to Gravitational Wave Data Analysis. Classical and Quantum Gravity, 10(9), S211. · URL
- Allen, B., Anderson, W. G., Brady, P. R., Brown, D. A., & Creighton, J. D. (2012). FINDCHIRP: An Algorithm for Detection of Gravitational Waves from Inspiraling Compact Binaries. Physical Review D, 85(12), 122006. · DOI 10.1103/PhysRevD.85.122006
精选声明
声明已持久化到证据分类账中，每个声明都有自己的评估。
尚无精选声明
当分类账中没有声明时，此视图不会自行创建声明评估。
相关方法
从方法图中生成，显示为机器建议的关系 — 不推断任何证据声明。