Results 101 to 110 of about 56,908 (217)
Advanced LIGO is currently in the final stages of installation and early commissioning. In the design of Advanced LIGO a key goal was the ability to detect gravitational waves from compact object binary inspirals, as these are thought to be the most likely candidates for early detections with ground based interferometers.
openaire +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
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
Overview of Advanced LIGO adaptive optics
This is an overview of the adaptive optics used in Advanced LIGO (aLIGO), known as the thermal compensation system (TCS). The thermal compensation system was designed to minimize thermally-induced spatial distortions in the interferometer optical modes and to provide some correction for static curvature errors in the core optics of aLIGO.
Brooks, Aidan F. +25 more
openaire +4 more sources
The discovery of gravitational waves (GW) by Advanced LIGO has ushered us into an era of observational GW astrophysics. Compact binaries remain the primary target sources for LIGO, of which neutron star-black hole (NSBH) binaries form an important subset.
Kumar, Prayush +2 more
core +1 more source
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
During 2015 and 2016, the Laser Interferometer Gravitational-Wave Observatory (LIGO) conducted a three-month observing campaign. These observations delivered the first direct detection of gravitational waves from binary black hole mergers.
Bockelman, Brian +5 more
core +1 more source
Multifaceted supercooling: from PTA to LIGO
Supercooled phase transitions, as predicted, e.g., in near-conformal and confining extensions of the Standard Model (SM), are established sources of strong stochastic gravitational wave backgrounds (SGWBs).
Satyabrata Datta, Rome Samanta
doaj +1 more source
Rapid likelihood free inference of compact binary coalescences using accelerated hardware
We report a gravitational-wave parameter estimation algorithm, AMPLFI , based on likelihood-free inference using normalizing flows. The focus of AMPLFI is to perform real-time parameter estimation for candidates detected by machine-learning based compact
D Chatterjee +14 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

