The Stochastic Gravitational Wave Background
Polarization-Based Tests of Gravity with the Stochastic Gravitational-Wave Background
... of gravitational waves with Advanced LIGO and Advanced Virgo offers novel oppor- tunities to test general relativity in strong-field, highly dynamical ...of gravitational-wave ...tensor ...
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Search for Tensor, Vector, and Scalar Polarizations in the Stochastic Gravitational Wave Background
... of gravitational waves with Advanced LIGO and Advanced Virgo has enabled novel tests of general relativity, including direct study of the polarization of gravitational ...tensor ...
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A Search for Tensor, Vector, and Scalar Polarizations in the Stochastic Gravitational-Wave Background
... of gravitational waves with Advanced LIGO and Advanced Virgo has enabled novel tests of general relativity, including direct study of the polarization of gravitational ...tensor ...
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GW150914 : implications for the stochastic gravitational-wave background from binary black holes
... the gravitational wave transient GW150914, from the inspiral and merger of two black holes with masses ≳30M ⊙ , suggests a population of binary black holes with relatively high ...the stochastic ...
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GW170817: Implications for the Stochastic Gravitational Wave Background from Compact Binary Coalescences
... of gravitational waves from the coalescence of two neutron ...astrophysical stochastic gravitational-wave ...astrophysical background relative to previous ...to stochastic ...
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GW170817 : Implications for the stochastic gravitational-wave background from compact binary coalescences
... of gravitational waves from the coalescence of two neutron ...astrophysical stochastic gravitational-wave ...astrophysical background relative to previous ...to stochastic ...
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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences
... of gravitational waves from the coalescence of two neutron ...astrophysical stochastic gravitational-wave ...astrophysical background relative to previous ...to stochastic ...
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Upper Limits on the Stochastic Gravitational Wave Background from Advanced LIGO's First Observing Run
... a stochastic gravitational-wave ...the stochastic background from unresolved compact binary coalescences is expected to be particularly ...isotropic stochastic ...
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Upper limits on the stochastic gravitational-wave background from Advanced LIGO’s first observing run
... a stochastic gravitational-wave ...the stochastic background from unresolved compact binary coalescences is expected to be particularly ...isotropic stochastic ...
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Noise-marginalized optimal statistic: A robust hybrid frequentist-Bayesian statistic for the stochastic gravitational-wave background in pulsar timing arrays
... Long-wavelength gravitational waves (GWs) with frequencies of 10 −9 –10 −7 Hz can be observed with pulsar timing arrays (PTAs) composed of millisecond pulsars (MSPs) ...isotropic stochastic ...
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Limits on anisotropy in the nanohertz stochastic gravitational-wave background
... the gravitational wave background (GWB) from this population is anisotropic, rendering existing analyses ...nanohertz stochastic GWB from circular, inspiral-driven SMBHBs using the 2015 ...
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Limits on Anisotropy in the Nanohertz Stochastic Gravitational Wave Background
... nanohertz stochastic gravitational-wave back- ground (SGWB) by looking for correlated deviations in the pulse times of arrival (TOAs) of multiple radio millisec- ond pulsars distributed across the ...
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Stochastic gravitational-wave background from spin loss of black holes
... spin-down gravitational-wave back- ground is observationally relevant: (i) at least a moderate fraction of the spin energy of black holes are lost over time, (ii) at least a moderate fraction of the energy ...
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GW170817 : Implications for the stochastic gravitational-wave background from compact binary coalescences
... the stochastic background is dominated by unresolvable sources, the energy-density spectra in ...astrophysical background given the inferred rate and mass distribution indicate that removing sources ...
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GW150914: Implications for the Stochastic Gravitational-Wave Background from Binary Black Holes
... Relative to the Fiducial model, the LowMass model shows a greater energy density at all frequencies, partic- ularly at high frequencies due to the signals from lower- mass binaries. This model indicates that if there is ...
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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences
... such as star formation rate, metallicity evolution and de- lay times. However, we have verified that variations on our assumptions are contained within the Poisson band shown in Fig. 1, consistent with the detailed study ...
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European Pulsar Timing Array Limits On An Isotropic Stochastic Gravitational-Wave Background
... the background we obtain a limit of A = ...the background, but obtain limits on the correlated power spectrum at a series of discrete frequencies, and show that our sen- sitivity is greatest at a frequency ...
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Sensitivity to a Frequency-Dependent Circular Polarization in an Isotropic Stochastic Gravitational Wave Background
... Most gravitational wave observatories, such as LIGO, LISA, and PTAs, effectively have only three masses which, as a result, are necessarily ...space-based gravitational wave observatories such ...
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European Pulsar Timing Array limits on an isotropic stochastic gravitational-wave background
... the background we obtain a limit of A = ...the background, but obtain limits on the correlated power spectrum at a series of discrete frequencies, and show that our sen- sitivity is greatest at a frequency ...
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Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s First Observing Run
... the background predictions due to BBH coalescences using data from ...BBH background, as this provides the most promising candidate for first detecting the ...
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