Eccentric Black Hole Gravitational-wave Capture Sources in Galactic Nuclei: Distribution of Binary Parameters [PDF]
Astrophysical Journal, 2017 Mergers of binary black holes on eccentric orbits are among the targets for second-generation ground-based gravitational-wave detectors. These sources may commonly form in galactic nuclei due to gravitational-wave emission during close flyby events of ...
L. Gondán +3 more
semanticscholar +1 more source
Machine Learning for the Characterization of Gravitational Wave Data
, 2021 The low-latency characterization of detector noise is a crucial step in the detection of gravitational waves. In particular, a rapid classification and identification of transient noise sources, usually referred to as glitches, is very important when ...
Elena Cuoco +3 more
core +1 more source
GRB 211211A-like Events and How Gravitational Waves May Tell Their Origins
The Astrophysical Journal Letters, 2023 GRB 211211A is a rare burst with a genuinely long duration, yet its prominent kilonova association provides compelling evidence that this peculiar burst was the result of a compact binary merger.
Yi-Han Iris Yin +7 more
doaj +1 more source
Gravitational wave emission from the CMB and other thermal fields
Physics Letters B, 2021 We calculate the gravitational wave power density emitted by quantum thermal sources. As particular cases, we calculate the emission of gravitational waves from the cosmic microwave background and from stellar sources.
Petar Simidzija +2 more
doaj +1 more source
Black hole binaries in galactic nuclei and gravitational wave sources [PDF]
, 2015 Stellar black hole (BH) binaries are one of the most promising gravitational wave (GW) sources for GW detection by the ground-based detectors. Nuclear star clusters (NCs) located at the centre of galaxies are known to harbour massive black holes (MBHs ...
Jongsuk Hong, Hyung-Mok Lee
semanticscholar +1 more source
Gravitational Waves, Sources, and Detectors
, 2001 82 pages, 9 figures, lecture notes from 1999, not posted to ArXiV at the time because they exceeded the article/figure size ...
Schutz, B., Ricci, F.
openaire +3 more sources
Black hole mergers from globular clusters observable by LISA II. Resolved eccentric sources and the gravitational wave background [PDF]
Monthly notices of the Royal Astronomical Society, 2018 In paper I of this series we showed that a large percentage of the binary black hole (BBH) mergers that form through dynamical interactions in globular clusters will have significant eccentricity in the ~10^{-3}-10^{-1} Hz LISA band.
D. D’Orazio, J. Samsing
semanticscholar +1 more source
Space gravitational wave antenna DECIGO and B-DECIGO
The Sixteenth Marcel Grossmann Meeting, 2023 DECIGO is a future Japanese gravitational wave detector in space, designed to enhance gravitational wave astronomy. Operating within a frequency range of 0.1 Hz to 10 Hz, DECIGO plays a vital role in detecting gravitational wave signals from various ...
S. Kawamura
semanticscholar +1 more source
All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run [PDF]
, 2021 This paper presents the results of a search for generic short-duration gravitational-wave transients in data from the third observing run of Advanced LIGO and Advanced Virgo.
Talbot, C. J. +9 more
core
Gravitational Wave signals from Various Sources
, 2022 Simulated Binary Black Hole (BBH) merger gravitational wave signals from various ...
Li, Xiyuan
core +1 more source