stochastic gravitational-wave
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 ...to stochastic backgrounds (near 25 Hz), we predict a total astrophysical ...
12
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 ...
12
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 ...
12
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 ...
12
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 ...
13
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 ...to stochastic backgrounds (near 25 Hz), we predict a total astrophysical ...
12
Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600-1000 Hz
... Data acquired by the LIGO and Virgo interferometers have been analyzed to search for a stochastic background of gravitational waves. This is the first time that data from LIGO and Virgo have been used ...
14
First cross-correlation analysis of interferometric and resonant-bar gravitational-wave data for stochastic backgrounds
... One of the signals targeted by the current genera- tion of ground-based gravitational wave (GW) detectors is a stochastic gravitational-wave background (SGWB) [1, 2, 3]. Such a ...
17
Fundamental Physics in the Era of Gravitational wave Astronomy: The Direct Measurement of Gravitational wave Polarizations and Other Topics
... of gravitational waves: their polarizations, dispersion, speed, and, importantly, energy content are all heavily ...the stochastic gravitational-wave ...by gravitational waves, or rely ...
364
Fundamental Physics Through Gravitational Waves: From No Hair Theorem to Quantum Structures of Black Holes
... reflect gravitational waves, causing echoes that follow the main gravitational waves from binary black hole ...a stochastic gravitational-wave background, which is very substantial if ...
175
Searching for a stochastic background of gravitational waves with the laser interferometer gravitational-wave observatory
... the gravitational-wave spectrum, based on the measurements of the CMB spectrum and pulsar ...the stochastic gravitational- wave background is limited to the LIGO frequency ...the ...
12
Gravitational waves from oscillon preheating
... the stochastic gravita- tional wave background associated with an oscillon-dominated ...radiate gravitational waves, and we show that the flux of gravitational radiation generated between ...
19
Quantum limited measurements in gravitational wave detectors
... The proposed polarisation folded speed meter is illustrated Figure 5.2. This interferometer configuration is based on the advanced Michelson topologies of LIGO, Virgo and KAGRA [9, 11, 12] but with the addition of a ...
226
Data analysis infrastructure for gravitational wave astronomy
... a gravitational wave observatory’s location, orienta tion and sensitivity is ...to gravitational wave sources directly above or below the plane of the two (perpendicular) arms, there is ...
163
Experiments with a laser interferometric gravitational wave antenna
... 136 A Test Mass Testing 139 B Principle of the Optical Phase Detection 144 C Burst and Coalescing Binary Sources 149 C.1 Short Bursts of Gravitational Radiation 149 C.2 Coalescing Compat[r] ...
185
Length Sensing and Control of a Prototype Advanced Interferometric Gravitational Wave Detector
... detect gravitational waves using laser ...interferometric gravitational wave ...of gravitational radiation is a primary goal of the community devoted to the experimental study of ...operating ...
235
A Search for Gravitational Waves from Perturbed Black Hole Ringdowns in LIGO Data
... Once we were satisfied with the tuning of the search the pipeline was applied to the full data set and the search was unblinded. A cumulative histogram of the detection statistic of background events was compared to that ...
221
Topics in Gravitational Physics: Tidal Coupling in Gravitational Wave Searches and Mach’s Principle
... will be at frequencies close to the floor of the LISA noise curve (∼ 3 mHz). LISA will detect the bursts of radiation emitted near periapse throughout the inspiral, but these bursts will not be individually resolvable ...
160
08 Interference.pptx
... Gravitational-wave chirp created from the collision of two neutron stars..[r] ...
81
Noise Cancellation for Gravitational Wave Detectors
... Newtonian gravitational field present a limit to high precision measure- ments, including searches below a few tens of Hz for gravitational waves using laser ...perturbing gravitational field and ...
183