Results 11 to 20 of about 381,601 (342)

On combining information from multiple gravitational wave sources [PDF]

open access: yesPhysical Review D, 2019
In the coming years, advanced gravitational wave detectors will observe signals from a large number of compact binary coalescences. The majority of these signals will be relatively weak, making the precision measurement of subtle effects, such as ...
Chatziioannou, Katerina   +2 more
core   +4 more sources

LEGWORK: A Python Package for Computing the Evolution and Detectability of Stellar-origin Gravitational-wave Sources with Space-based Detectors [PDF]

open access: goldJournal of Open Source Software, 2022
We present LEGWORK (LISA Evolution and Gravitational Wave Orbit Kit), an open-source Python package for making predictions about stellar-origin gravitational-wave sources and their detectability in LISA or other space-based gravitational-wave detectors ...
Tom Wagg, Katelyn Breivik, S. E. de Mink
openalex   +3 more sources

Gravitational wave sources: reflections and echoes [PDF]

open access: green, 2017
The recent detection of gravitational waves has generated interest in alternatives to the black hole interpretation of sources. A subset of such alternatives involves a prediction of gravitational wave ‘echoes’. We consider two aspects of possible echoes:
Richard H. Price, Gaurav Khanna
openalex   +3 more sources

Dirty waveforms: multiband harmonic content of gas-embedded gravitational wave sources [PDF]

open access: yes, 2021
We analyse the effect of stochastic torque fluctuations on the orbital evolution and the gravitational wave (GW) emission of gas-embedded sources with intermediate and extreme mass ratios.
L. Zwick   +4 more
semanticscholar   +1 more source

Shouts and Murmurs: Combining Individual Gravitational-wave Sources with the Stochastic Background to Measure the History of Binary Black Hole Mergers [PDF]

open access: yesAstrophysical Journal, 2020
One of the goals of gravitational-wave astronomy is to quantify the evolution of the compact binary merger rate with redshift. The redshift distribution of black hole mergers would offer considerable information about their evolutionary history ...
T. Callister   +3 more
semanticscholar   +1 more source

A Systematic Search of Zwicky Transient Facility Data for Ultracompact Binary LISA-detectable Gravitational-wave Sources [PDF]

open access: yesAstrophysical Journal, 2020
Using photometry collected with the Zwicky Transient Facility, we are conducting an ongoing survey for binary systems with short orbital periods ( with the goal of identifying new gravitational-wave sources detectable by the upcoming Laser Interferometer
K. Burdge   +33 more
semanticscholar   +1 more source

Accurate precision cosmology with redshift unknown gravitational wave sources [PDF]

open access: yes, 2020
Gravitational waves can provide an accurate measurement of the luminosity distance to the source but cannot provide the source redshift unless the degeneracy between mass and redshift can be broken.
S. Mukherjee   +3 more
semanticscholar   +1 more source

Taiji program: Gravitational-wave sources [PDF]

open access: yesInternational Journal of Modern Physics A, 2018
We review potential low-frequency gravitational-wave sources, which are expected to be detected by Taiji, a Chinese space-based gravitational-wave detector, estimate the detection rates of these gravitational-wave sources and present the parameter ...
Zongkuan Guo, R. Cai, Yuan-zhong Zhang
semanticscholar   +1 more source

Enhancing gravitational wave anisotropies with peaked scalar sources [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2022
Gravitational wave (GW) backgrounds of cosmological origin are expected to be nearly isotropic, with small anisotropies resembling those of the cosmic microwave background.
E. Dimastrogiovanni   +3 more
semanticscholar   +1 more source

Search Methods for Continuous Gravitational-Wave Signals from Unknown Sources in the Advanced-Detector Era [PDF]

open access: yesUniverse, 2021
Continuous gravitational waves are long-lasting forms of gravitational radiation produced by persistent quadrupolar variations of matter. Standard expected sources for ground-based interferometric detectors are neutron stars presenting non-axisymmetries ...
R. Tenorio, D. Keitel, A. Sintes
semanticscholar   +1 more source

Home - About - Disclaimer - Privacy