Results 21 to 30 of about 56,908 (217)

The LIGO Open Science Center [PDF]

open access: yes, 2015
The LIGO Open Science Center (LOSC) fulfills LIGO's commitment to release, archive, and serve LIGO data in a broadly accessible way to the scientific community and to the public, and to provide the information and tools necessary to understand and use ...
Kanner, Jonah   +4 more
core   +3 more sources

Point absorbers in Advanced LIGO [PDF]

open access: yesApplied Optics, 2021
Small, highly absorbing points are randomly present on the surfaces of the main interferometer optics in Advanced LIGO. The resulting nanometer scale thermo-elastic deformations and substrate lenses from these micron-scale absorbers significantly reduce the sensitivity of the interferometer directly though a reduction in the power ...
Aidan F. Brooks   +201 more
openaire   +6 more sources

Simulation tools for future interferometers [PDF]

open access: yes, 2006
For the design and commissioning of the LIGO interferometer, simulation tools have been used explicitly and implicitly. The requirement of the advanced LIGO interferometer is much more demanding than the first generation interferometer.
Barton, M.   +4 more
core   +1 more source

LIGO’s “science reach” [PDF]

open access: yesAIP Conference Proceedings, 2001
Technical discussions of the Laser Interferometer Gravitational Wave Observatory (LIGO) sensitivity often focus on its effective sensitivity to gravitational waves in a given band; nevertheless, the goal of the LIGO Project is to ``do science.'' Exploiting this new observational perspective to explore the Universe is a long-term goal, toward which LIGO'
openaire   +2 more sources

Improving the Sensitivity of Advanced LIGO Using Noise Subtraction [PDF]

open access: yes, 2019
This paper presents an adaptable, parallelizable method for subtracting linearly coupled noise from Advanced LIGO data. We explain the features developed to ensure that the process is robust enough to handle the variability present in Advanced LIGO data.
Davis, D.   +5 more
core   +3 more sources

Prospects for Stochastic Background Searches Using Virgo and LSC Interferometers [PDF]

open access: yes, 2007
We consider the question of cross-correlation measurements using Virgo and the LSC Interferometers (LIGO Livingston, LIGO Hanford, and GEO600) to search for a stochastic gravitational-wave background. We find that inclusion of Virgo into the network will
Cella, Giancarlo   +6 more
core   +8 more sources

Broadband Quantum Enhancement of the LIGO Detectors with Frequency-Dependent Squeezing

open access: yesPhysical Review X, 2023
Quantum noise imposes a fundamental limitation on the sensitivity of interferometric gravitational-wave detectors like LIGO, manifesting as shot noise and quantum radiation pressure noise.
D. Ganapathy   +182 more
doaj   +1 more source

Prospects for detecting gravitational waves at 5 Hz with ground-based detectors [PDF]

open access: yes, 2018
We propose an upgrade to Advanced LIGO (aLIGO), named LIGO-LF, that focuses on improving the sensitivity in the 5-30 Hz low-frequency band, and we explore the upgrade's astrophysical applications.
Barr, Bryan   +18 more
core   +5 more sources

Can we distinguish quark stars from neutron stars with measurements of global properties? [PDF]

open access: yesEPJ Web of Conferences, 2022
The phase state of the dense stellar matter is an exciting topic in the area of nuclear astrophysics. It may be probed by observed properties of neutron stars from, for example, the currently operating satellites (NICER, Neutron star Interior Composition
Li Ang
doaj   +1 more source

Silica suspension and coating developments for Advanced LIGO [PDF]

open access: yes, 2006
The proposed upgrade to the LIGO detectors to form the Advanced LIGO detector system is intended to incorporate a low thermal noise monolithic fused silica final stage test mass suspension based on developments of the GEO 600 suspension design. This will
Acernese F   +41 more
core   +2 more sources

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