Time-domain Implementation of the Optimal Cross-Correlation Statistic for Stochastic Gravitational-Wave Background Searches in Pulsar Timing Data
- Phys.Rev.D 91 (2015) 4, 044048
- Published: Feb 27, 2015
- 1410.8256 [astro-ph.IM]
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Supermassive black hole binaries, cosmic strings, relic gravitational waves from inflation, and first-order phase transitions in the early Universe are expected to contribute to a stochastic background of gravitational waves in the
- 12 pages, 3 figures, submitted to Physical Review D
- 04.30.-w
- 04.80.Nn
- background: stochastic
- gravitational radiation: background
- gravitational radiation: stochastic
- pulsar
- black hole: binary
- cosmic string
- gravitational radiation: primordial
- critical phenomena
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