Results 1 to 10 of about 1,615 (134)

A high load torsion pendulum of trifilar suspension magnetic damper for inertial sensor test [PDF]

open access: yesScientific Reports
Space-based gravitational waves (GW) detection requires the residual noise spectral density of the inertial sensors to reach $$10^{-15}\textrm{m}\cdot \textrm{s}^{-2}\cdot \textrm{Hz}^{-1/2}$$ from 0.1 mHz to 1Hz.
Hongfan Liu   +7 more
doaj   +2 more sources

Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA

open access: yesLiving Reviews in Relativity, 2018
We present possible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger ...
B. P. Abbott   +1100 more
doaj   +3 more sources

Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo

open access: yesLiving Reviews in Relativity, 2016
We present a possible observing scenario for the Advanced LIGO and Advanced Virgo gravitational-wave detectors over the next decade, with the intention of providing information to the astronomy community to facilitate planning for multi-messenger ...
Benjamin P. Abbott   +2 more
doaj   +3 more sources

Design method for the structure of a gravitational wave detection telescope with low TTL noise [PDF]

open access: yesScientific Reports
As a critical payload of the gravitational wave detection interferometry system, the tilt-to-length (TTL) noise has a significant influence on the detection accuracy of the interferometry system.
Sijun Fang   +8 more
doaj   +2 more sources

Gravitational-wave astronomy: delivering on the promises [PDF]

open access: yesPhilosophical Transactions Series A, Mathematical, Physical, and Engineering Sciences, 2018
Bernard Schutz
exaly   +2 more sources

Testing general relativity with gravitational-wave catalogs: The insidious nature of waveform systematics

open access: yesiScience, 2021
Summary: Gravitational-wave observations of binary black holes allow new tests of general relativity (GR) to be performed on strong, dynamical gravitational fields.
Christopher J. Moore   +3 more
doaj   +1 more source

A Broadband Signal Recycling Scheme for Approaching the Quantum Limit from Optical Losses

open access: yesGalaxies, 2021
Quantum noise limits the sensitivity of laser interferometric gravitational-wave detectors. Given the state-of-the-art optics, the optical losses define the lower bound of the best possible quantum-limited detector sensitivity.
Teng Zhang, Joe Bentley, Haixing Miao
doaj   +1 more source

Squeezing for cosmic symphony

open access: yesAAPPS Bulletin, 2023
We briefly review the status of applying quantum squeezing to aid the search for gravitational waves with km-scale laser interferometers operating in the audio frequency band.
Mengyao Wang, Fan Zhang
doaj   +1 more source

Gravitational-wave asteroseismology with fundamental modes from compact binary inspirals

open access: yesNature Communications, 2020
Independently measuring the tidal deformability and the fundamental oscillation mode (fmode) frequency enables tests of gravity and the nature of compact binaries.
Geraint Pratten   +2 more
doaj   +1 more source

No tension between assembly models of super massive black hole binaries and pulsar observations

open access: yesNature Communications, 2018
Pulsar timing arrays enable the search for the isotropic gravitational-wave (GW) background originating from super massive black hole binary populations, but impose a stringent upper limit on the GW characteristic amplitude.
Hannah Middleton   +4 more
doaj   +1 more source

Home - About - Disclaimer - Privacy