Results 51 to 60 of about 136,037 (243)

Compact Binary Coalescences in the Band of Ground-based Gravitational-Wave Detectors

open access: yes, 2010
As the ground-based gravitational-wave telescopes LIGO, Virgo, and GEO 600 approach the era of first detections, we review the current knowledge of the coalescence rates and the mass and spin distributions of merging neutron-star and black-hole binaries.
  +64 more
core   +1 more source

Astrophysical science metrics for next-generation gravitational-wave detectors [PDF]

open access: yes, 2019
The second generation of gravitational-wave detectors are being built and tuned all over the world. The detection of signals from binary black holes is beginning to fulfill the promise of gravitational-wave astronomy.
Adhikari, Rana X   +10 more
core   +2 more sources

TeV Particle Astrophysics II: Summary comments [PDF]

open access: yes, 2006
A unifying theme of this conference was the use of different approaches to understand astrophysical sources of energetic particles in the TeV range and above.
  +42 more
core   +2 more sources

An introduction to Bayesian inference in gravitational-wave astronomy: parameter estimation, model selection, and hierarchical models—Corrigendum

open access: yesPublications Astronomical Society of Australia, 2020
1. In the original version of this article, we included a subsection in Appendix E, “Selection effects with a single event.” This section included formulas with errors including Eq. 89 and Eq. 95 of the arxiv version (Eq. E2 and Eq.
E. Thrane, C. Talbot
semanticscholar   +1 more source

Dynamical Formation Scenarios for GW190521 and Prospects for Decihertz Gravitational-wave Astronomy with GW190521-like Binaries [PDF]

open access: yes, 2020
The gravitational-wave (GW) detection of GW190521 has provided new insights on the mass distribution of black holes and new constraints for astrophysical formation channels.
A. M. Holgado   +2 more
semanticscholar   +1 more source

Nuclear Physics with Gravitational Waves from Neutron Stars Disrupted by Black Holes

open access: yesThe Astrophysical Journal Letters, 2023
Gravitational waves from neutron star–black hole (NSBH) mergers that undergo tidal disruption provide a potential avenue to study the equation of state of neutron stars and hence the behavior of matter at its most extreme densities.
Teagan A. Clarke   +3 more
doaj   +1 more source

The damping of gravitational waves in dust

open access: yes, 2008
We examine a simple model of interaction of gravitational waves with matter (primarily represented by dust). The aim is to investigate a possible damping effect on the intensity of gravitational wave when passing through media.
  +6 more
core   +1 more source

Fast Magnetosonic Waves Driven by Gravitational Waves [PDF]

open access: yes, 2001
The propagation of a gravitational wave (GW) through a magnetized plasma is considered. In particular, we study the excitation of fast magnetosonic waves (MSW) by a gravitational wave, using the linearized general-relativistic hydromagnetic equations. We
Andersson   +27 more
core   +3 more sources

Quantum gravity and gravitational-wave astronomy [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2019
We investigate possible signatures of quantum gravity which could be tested with current and future gravitational-wave (GW) observations. In particular, we analyze how quantum gravity can influence the GW luminosity distance, the time dependence of the ...
G. Calcagni   +5 more
semanticscholar   +1 more source

Exploring the Effects of Reduced Gravitational Field Impacts on Convective Heat Transfer: A Comprehensive Review

open access: yesHeat Transfer, EarlyView.
ABSTRACT This review explores the impact of gravitational instability on convective heat transfer, integrating existing research results and theoretical models. Gravitational instability is vital in promoting or hindering convective actions in different systems, such as atmospheric events, ocean currents, and industrial processes.
Hossam A. Nabwey   +3 more
wiley   +1 more source

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