Results 91 to 100 of about 18,093 (220)
Environmental noise in advanced LIGO detectors
The sensitivity of the Advanced LIGO detectors to gravitational waves can be affected by environmental disturbances external to the detectors themselves.
Mavalvala, Nergis
core +1 more source
Photonic Metrology with Hierarchic Quantum Frequentist Bounds
This paper proposes photonic metrology with hierarchical quantum frequentist bounds. The present model tightens the Quantum Cramér‐Rao Bound using a hybrid classical‐quantum framework. The experiment validates the hierarchical frequentist bounds for single‐qubit phase estimation.
Xin‐Zhu Liu +6 more
wiley +1 more source
Gravitational waves from supercooled phase transitions in conformal Majoron models of neutrino mass
We study supercooled first-order phase transitions above the QCD scale in a wide class of conformal Majoron-like U(1)′ models that explain the totality of active neutrino oscillation data and produce a detectable stochastic gravitational wave background (
João Gonçalves +3 more
doaj +1 more source
THE PAST AND THE FUTURE OF DIRECT SEARCH OF GW FROM PULSARS IN THE ERA OF GW ANTENNAS
In this paper we will give an overview of the past and present status of Gravitational Wave (GW) research associated with pulsars, taking into account the target sensitivity achieved from interferometric laser GW antennas such as Tama, Geo, Ligo and ...
L. Milano +5 more
doaj +1 more source
Discrepancy in tidal deformability of GW170817 between the Advanced LIGO twin detectors
We find that the Hanford and Livingston detectors of Advanced LIGO derive a distinct posterior probability distribution of binary tidal deformability Λ[over ̃] of the first binary-neutron-star merger GW170817.
Tatsuya Narikawa +6 more
doaj +1 more source
The LIGO–LIGO cross correlation for the detection of relic scalar gravitational waves [PDF]
In the earlier work arXiv:0706.3782 we studied the cross correlation between the Virgo interferometer and the MiniGRAIL resonant sphere for the detection of relic scalar gravitational waves (SGWs). We have shown that the overlap reduction function for the cross correlation between Virgo and the monopole mode of MiniGRAIL is very small, but a maximum ...
openaire +2 more sources
Polarization-Based Tests of Gravity with the Stochastic Gravitational-Wave Background
The direct observation of gravitational waves with Advanced LIGO and Advanced Virgo offers novel opportunities to test general relativity in strong-field, highly dynamical regimes.
Thomas Callister +9 more
doaj +1 more source
Data Access for LIGO on the OSG
6 pages, 3 figures, submitted to ...
Derek Weitzel +5 more
openaire +5 more sources
I worked on this project during my stay at LIGO Hanford site: the seismic isolation control and reduction is a crucial matter of concern on site, because seismic motion affects the performance of the detector.
Di Fronzo, Chiara
core
Noise line identification in LIGO S6 and Virgo VSR2
An important goal for LIGO (the Laser Interferometer Gravitational-Wave Observatory) and Virgo is to find periodic sources of gravitational waves. The LIGO and Virgo detectors are sensitive to a variety of noise of non-astrophysical origin, such as ...
for the Ligo Scientific Collaboration and the Virgo Collaboration +2 more
core +1 more source

