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Stochastic backgrounds of gravitational waves
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We review the motivations for the search of stochastic backgrounds of gravitational waves and we compare the experimental sensitivities that can be reached in the near future with the existing bounds and with the theoretical predictions.
Forward citations
Cited by 4 Pith papers
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Residual Galactic binary foreground in LISA stochastic gravitational-wave background inference: source power concentration and spectral degeneracy
Residual Galactic binaries left after catalog-matched recovery inflate the LISA flat-SGWB amplitude uncertainty by 13.6% when their amplitude is marginalized, and would bias it by ~120σ if omitted.
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Constraints on High-Frequency Gravitational Waves from Graviton-Photon Conversion in the M87 Galaxy
Graviton–photon conversion in M87's magnetic field sets h_c and Ωgw h² limits 1–5 orders of magnitude tighter than Milky Way-based bounds across 10^10–10^27 Hz.
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The MeerKAT Pulsar Timing Array: The first search for gravitational waves with the MeerKAT radio telescope
The first MeerKAT PTA search reports Hellings-Downs correlations at about 3.4 sigma under some noise models, but the significance vanishes under slightly different assumptions, leaving the data ambiguous.
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The MeerKAT Pulsar Timing Array: The $4.5$-year data release and the noise and stochastic signals of the millisecond pulsar population
The MeerKAT PTA data release finds a common red noise signal with amplitude log10 A = -14.25 to -14.28, larger than other PTAs, and provides detailed noise models for 83 pulsars.
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