Výsledky vyhledávání - "Moore, Blake P."

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Constraining Gravity with Eccentric Gravitational Waves: Projected Upper Bounds and Model Selection

Gravitational waves allow us to test general relativity in the highly dynamical regime. While current observations have been consistent with waves emitted by quasi-circular binaries, eccentric binaries may also produce detectable signals in the near

Externí odkaz: http://arxiv.org/abs/2002.05775

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Data Analysis Implications of Moderately Eccentric Gravitational Waves

Autor: Moore, Blake, Yunes, Nicolás

While the expectation is that the majority of gravitational wave events observable by ground-based detectors will be emitted by compact binaries in quasi-circular orbits, the growing number of detections suggests the possibility of detecting waves fr

Externí odkaz: http://arxiv.org/abs/1910.01680

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A 3PN Fourier Domain Waveform for Non-Spinning Binaries with Moderate Eccentricity

Autor: Moore, Blake, Yunes, Nicolás

While current gravitational wave observations with ground based detectors have been consistent with compact binaries in quasi-circular orbits, eccentric binaries may be detectable by ground-based and space-based instruments in the near future. Eccent

Externí odkaz: http://arxiv.org/abs/1903.05203

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A Fourier Domain Waveform for Non-Spinning Binaries with Arbitrary Eccentricity

Autor: Moore, Blake, Robson, Travis, Loutrel, Nicholas, Yunes, Nicolas

Although the gravitational waves observed by advanced LIGO and Virgo are consistent with compact binaries in a quasi-circular inspiral prior to coalescence, eccentric inspirals are also expected to occur in Nature. Due to their complexity, we current

Externí odkaz: http://arxiv.org/abs/1807.07163

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Gravitational-wave phasing for low-eccentricity inspiralling compact binaries to 3PN order

Autor: Moore, Blake, Favata, Marc, Arun, K. G., Mishra, Chandra Kant

Publikováno v: Phys. Rev. D 93, 124061 (2016)

[abridged] Although gravitational radiation causes inspiralling compact binaries to circularize, a variety of astrophysical scenarios suggest that binaries might have small but nonnegligible orbital eccentricities when they enter the low-frequency ba

Externí odkaz: http://arxiv.org/abs/1605.00304

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