Results 71 to 80 of about 136,037 (243)

Possible direct method to determine the radius of a star from the spectrum of gravitational wave signals [PDF]

open access: yes, 2000
We computed the spectrum of gravitational waves from a dust disk star of radius R inspiraling into a Kerr black hole of mass M and specific angular momentum a. We found that when R is much larger than the wave length of the quasinormal mode, the spectrum
E. W. Leaver   +14 more
core   +2 more sources

Equation-of-state constraints and the QCD phase transition in the era of gravitational-wave astronomy [PDF]

open access: yesXIAMEN-CUSTIPEN WORKSHOP ON THE EQUATION OF STATE OF DENSE NEUTRON-RICH MATTER IN THE ERA OF GRAVITATIONAL WAVE ASTRONOMY, 2019
We describe a multi-messenger interpretation of GW170817, which yields a robust lower limit on NS radii. This excludes NSs with radii smaller than about 10.7 km and thus rules out very soft nuclear matter.
A. Bauswein   +9 more
semanticscholar   +1 more source

The Once and Future Hydrology Is Whole Earth Hydrology

open access: yesPerspectives of Earth and Space Scientists, Volume 6, Issue 1, December 2025.
Abstract We here argue for a new paradigm to advance pursuit of truth in global freshwater science. Our proposed Whole Earth Hydrology is hydrology that is explicitly empirical and discovery‐based, grounded in primary data, detailed at scale, and incorporates humans as essential.
Colin J. Gleason, Casey M. Brown
wiley   +1 more source

Research on High-Stability Composite Control Methods for Telescope Pointing Systems under Multiple Disturbances

open access: yesSensors
During the operation of space gravitational wave detectors, the constellation configuration formed by three satellites gradually deviates from the ideal 60° angle due to the periodic variations in orbits.
Rui Zhang   +9 more
doaj   +1 more source

Electromagnetic follow-up of gravitational wave transient signal candidates

open access: yes, 2012
Pioneering efforts aiming at the development of multi-messenger gravitational wave and electromagnetic astronomy have been made. An electromagnetic observation follow-up program of candidate gravitational wave events has been performed (Dec 17 2009 to ...
Abadie J   +17 more
core   +1 more source

An information-theoretic approach to the gravitational-wave burst detection problem [PDF]

open access: yes, 2017
The observational era of gravitational-wave astronomy began in the Fall of 2015 with the detection of GW150914. One potential type of detectable gravitational wave is short-duration gravitational-wave bursts, whose waveforms can be difficult to predict ...
Essick, Reed   +4 more
core   +3 more sources

High angular resolution gravitational wave astronomy [PDF]

open access: yesExperimental astronomy (Print), 2019
Since the very beginning of astronomy the location of objects on the sky has been a fundamental observational quantity that has been taken for granted.
J. Baker   +21 more
semanticscholar   +1 more source

A Numerical 3D‐2D Coupling Strategy for Simulating Landslide‐Generated Tsunamis in Complex Geometries: The Taan Fiord, Alaska, Case Study

open access: yesJournal of Geophysical Research: Oceans, Volume 130, Issue 12, December 2025.
Abstract Landslide‐generated tsunamis represent a significant hazard, specifically in coastal, fjord, and lake environments. The accurate modeling of these complicated phenomena is crucial for risk assessment and preparation of mitigation strategies.
A. Romano   +4 more
wiley   +1 more source

Unsupervised Machine Learning for Classifying CHIME Fast Radio Bursts and Investigating Empirical Relations

open access: yesThe Astrophysical Journal
Fast radio bursts (FRBs) are highly energetic millisecond-duration astrophysical phenomena typically categorized as repeaters or nonrepeaters. However, observational limitations may result in misclassifications, potentially leading to a higher proportion
Da-Chun Qiang   +3 more
doaj   +1 more source

R-mode instability in compact stars

open access: yes, 2019
R-mode oscillations have been identified as viable and promising targets for continuous gravitational wave searches, meanwhile, it would allow us to probe the interior of compact stars directly.
Wang, Yu-bin, Zhou, Xia, Zhu, Cui
core   +1 more source

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