Results 71 to 80 of about 381,601 (342)
Event Rate for Extreme Mass Ratio Burst Signals in the LISA Band
, 2006 Stellar mass compact objects in short period orbits about a $10^{4.5}$--$10^{7.5}$ solar mass massive black hole (MBH) are thought to be a significant continuous-wave source of gravitational radiation for the ESA/NASA Laser Interferometer Space Antenna ...
Finn, Lee Samuel +2 more
core +1 more source
Massive double compact object mergers: gravitational wave sources and r-process element production sites [PDF]
, 2013 With our galactic evolutionary code that contains a detailed intermediate-mass and massive binary population model, we study the temporal evolution of the galactic population of double neutron star binaries, mixed systems with a neutron star and black ...
N. Mennekens, D. Vanbeveren
semanticscholar +1 more source
Potential of Radio Telescopes as High-Frequency Gravitational Wave Detectors.
Physical Review Letters, 2021 In the presence of magnetic fields, gravitational waves are converted into photons and vice versa. We demonstrate that this conversion leads to a distortion of the cosmic microwave background (CMB), which can serve as a detector for MHz to GHz ...
V. Domcke, C. Garcia-Cely
semanticscholar +1 more source
Advanced Materials, EarlyView.Biological and biologically‐inspired functional nanostructures with structural, thermal, optical, and sensing applications are reviewed. The role of nanoscale features in biological materials on performance is described, and their blueprints are used for bio‐inspired nanomaterials, synthesized using advanced techniques (i.e., photolithography, bio ...
Chao Hsuan (Joseph) Sung +15 more
wiley +1 more source
The Astrophysical JournalElectromagnetic follow-up observations of gravitational wave events offer critical insights and provide significant scientific gain from this new class of astrophysical transients.
Man Leong Chan +14 more
doaj +1 more source
An Overview of Gravitational-Wave Sources [PDF]
, 2002 We review current best estimates of the strength and detectability of the gravitational waves from a variety of sources, for both ground-based and space-based detectors, and we describe the information carried by the waves.Comment: 40 pages, 5 figures ...
Cutler, Curt, Thorne, Kip S.
core +2 more sources
Detection, Localization and Characterization of Gravitational Wave Bursts in a Pulsar Timing Array [PDF]
, 2010 Efforts to detect gravitational waves by timing an array of pulsars have focused traditionally on stationary gravitational waves: e.g., stochastic or periodic signals.
Accadia +33 more
core +3 more sources
Localization of gravitational wave sources with networks of advanced detectors [PDF]
, 2011 Coincident observations with gravitational wave (GW) detectors and other astronomical instruments are among the main objectives of the experiments with the network of LIGO, Virgo, and GEO detectors.
S. Klimenko +9 more
semanticscholar +1 more source
Autonomous Spatiotemporal Regulation of Reversible Hydrogel Actuators by Chemical Reaction Networks
Advanced Materials, EarlyView.Hydrogel actuators with reversible response to thiols are developed using reversible binding of thiols to Michael acceptors. Autonomous spatiotemporal regulation of reversible movement of these hydrogels is achieved using thiol‐based chemical reaction networks containing both positive and negative feedback.
Fan Liao +3 more
wiley +1 more source
Indication for a Compact Object Next to a LIGO–Virgo Binary Black Hole Merger
The Astrophysical Journal LettersThe astrophysical origin of binary black hole (BBH) mergers remains uncertain, although many events have been observed by the LIGO–Virgo–KAGRA network. Such mergers are potentially originated in the vicinity of massive black holes (MBHs).
Shu-Cheng Yang +4 more
doaj +1 more source