[PDF] Top 20 Search for gravitational waves from intermediate mass binary black holes
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Search for gravitational waves from intermediate mass binary black holes
... ringdown. Gravitational waves from the inspiral stage are quasiperi- odic ‘‘chirp’’ signals of increasing frequency and amplitude which are well described by analytical post- Newtonian (PN) models ... See full document
13
Search for gravitational waves from binary black hole inspiral, merger, and ringdown in LIGO-Virgo data from 2009-2010
... The gravitational-wave strain data from the detectors contain a larger number of transient noise events (glitches) with high amplitude than would occur in colored Gaussian ...to gravitational ... See full document
15
Search for gravitational waves from binary black hole inspirals in LIGO data
... of gravitational waves observed during our search or on the coalescence rate of BBH in the Universe than it was for the BNS search in the S2 data ...our search, we did calculate an ... See full document
17
Search for gravitational waves from binary inspirals in S3 and S4 LIGO data
... signal from such an event unlikely, though possible, with the current generation of gravitational-wave ...of binary black hole (BBH) or black hole/neutron star binaries, but they are ... See full document
12
Search for gravitational waves from low mass binary coalescences in the first year of LIGO's S5 data
... the search was that no plausible gravitational-wave signals were observed above the ...to gravitational waves from com- pact binary coalescences and are preparing for the first ... See full document
14
Search for gravitational waves from galactic and extra-galactic binary neutron stars
... a search for gravitational waves from binary neutron star systems, using data from the science run conducted early in ...These waves are expected to be emitted at fre- ... See full document
22
A Search for Gravitational Waves from Perturbed Black Hole Ringdowns in LIGO Data
... detect gravitational waves at threshold of 5.5. We are a long way from being able to claim a detection of gravitational wave ringdown from co-located detectors however requiring two ... See full document
221
Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO's fifth science run
... Interferometer Gravitational-wave Observatory (LIGO) reached design sensitivity and began a two-year period of observations (known as the fifth science run, or S5) which concluded in October 2007 ...of ... See full document
8
Search for gravitational waves from primordial black hole binary coalescences in the galactic halo
... this search by introducing an artificial time offset t 17 s to the trig- gers coming from the Livingston detector relative to the Hanford ...output from a search if no signals are present in ... See full document
8
Search for gravitational waves from binary black hole inspiral, merger, and ringdown
... two black holes has proven to be remarkably ...colliding black holes [32] to compute the gravitational- wave signal from the last orbits, merger, and ringdown of a ... See full document
20
Observation of Gravitational Waves from a Binary Black Hole Merger
... Both detectors were in steady state operation for several hours around GW150914. All performance measures, in particular their average sensitivity and transient noise behavior, were typical of the full analysis period ... See full document
16
Observation of gravitational waves from a binary black hole merger
... Both detectors were in steady state operation for several hours around GW150914. All performance measures, in particular their average sensitivity and transient noise behavior, were typical of the full analysis period ... See full document
16
Fundamental Physics Through Gravitational Waves: From No Hair Theorem to Quantum Structures of Black Holes
... of black holes and search for exotic, compact ...to black holes, but can also produce a sequence of distinct pulses resembling the initial ...Schwarzschild black hole into the ... See full document
175
GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence.
... the gravitational-wave candidate GW151226 was identified within 70 s by an online matched-filter search ...online search at a rate of approximately 1 per 1000 ... See full document
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GW151226 : observation of gravitational waves from a 22-solar-mass binary black hole coalescence
... the gravitational-wave candidate GW151226 was identified within 70 s by an online matched-filter search ...online search at a rate of approximately 1 per 1000 ... See full document
14
Search for gravitational wave ringdowns from perturbed black holes in LIGO S4 data
... perturbed black hole will settle to a stationary configuration by the emission of gravitational ...a black hole binary, following their inspiral and subsequent ...to search for this ... See full document
9
Event horizons, gravitational waves and astrophysical kicks in black-hole spacetimes
... topologies from the mergers of multiple black holes (BHs) (see [243] for a possible example), and very few that have shown event horizons of any form (see [243, ...obtained from the AHs (us- ... See full document
252
GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
... test mass suspension wires, control noise, the 50 Hz mains line and harmonics, and scattered light driven by seismic ...comes from shot noise of the main interferometer beam, with smaller contributions ... See full document
16
Formation of Galaxies in the Context of Gravitational Waves and Primordial Black Holes
... Gravitational waves may be produced extensively during the initial phase of ga- laxy formation in the early ...massive black holes at the center of galaxies at redshifts corresponding to the ... See full document
11
GW150914 : implications for the stochastic gravitational-wave background from binary black holes
... this search at the 2σ level will correspond to Ω GW ∼ 10 −9 at 25 Hz with the full- sensitivity network of the Advanced LIGO and Advanced Virgo ...stochastic search alone will not be able to distinguish ... See full document
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