Response of test masses to gravitational waves in the local Lorentz gauge
M Rakhmanov - Physical Review D—Particles, Fields, Gravitation, and …, 2005 - APS
The local Lorentz gauge represents a natural coordinate frame for an observer to analyze
the effect of gravitational waves on detectors, and has been widely used to describe the …
the effect of gravitational waves on detectors, and has been widely used to describe the …
Characterization of the LIGO 4 km Fabry–Perot cavities via their high-frequency dynamic responses to length and laser frequency variations
Recent measurements at the LIGO Hanford Observatory have confirmed the predicted high-
frequency dynamic response of km scale Fabry–Perot cavities to length and laser frequency …
frequency dynamic response of km scale Fabry–Perot cavities to length and laser frequency …
Optical sensitivities of current gravitational wave observatories at higher kHz, MHz and GHz frequencies
R Schnabel, M Korobko - arXiv preprint arXiv:2409.03019, 2024 - arxiv.org
GEO 600, Kagra, LIGO, and Virgo were built to observe gravitational waves at frequencies in
the audio band, where the highest event rates combined with the largest signal to noise …
the audio band, where the highest event rates combined with the largest signal to noise …
[PDF][PDF] Response of LIGO to gravitational waves at high frequencies and in the vicinity of the FSR (37.5 kHz)
M Rakhmanov - LIGO Document LIGO-T060237, 2005 - dcc.ligo.org
A laser interferometer defines its own coordinate system so that the x and y axes run along
the two interferometer arms and the origin is at the beam-splitter. In general, these …
the two interferometer arms and the origin is at the beam-splitter. In general, these …
[图书][B] Search for a high frequency stochastic background of gravitational waves
S Giampanis - 2008 - search.proquest.com
Over the past decades significant efforts have been made worldwide in the search for
gravitational waves. Ground-based interferometry, primarily with the LIGO detectors, has …
gravitational waves. Ground-based interferometry, primarily with the LIGO detectors, has …
[图书][B] Characterization of the high frequency response of LASER interferometer gravitational wave detectors
WE Butler - 2004 - search.proquest.com
This thesis describes a search for a stochastic background of gravitational waves at high
frequency, 37.52 kHz. At this frequency the separation between the available instruments …
frequency, 37.52 kHz. At this frequency the separation between the available instruments …
Motion of photons in a background of gravitational wave
Z Chang, CG Huang, ZC Zhao - arXiv preprint arXiv:1612.06939, 2016 - arxiv.org
The photon motion in a Michelson interferometer is re-analyzed in both geometrical optics
and wave optics. The classical paths of the photons in the background of gravitational wave …
and wave optics. The classical paths of the photons in the background of gravitational wave …