Results 31 to 40 of about 284,905 (340)
GRAVITATIONAL WAVES FROM COMPACT SOURCES [PDF]
New Worlds in Astroparticle Physics, 2006 22 pages, Proceedings of the 5th International Workshop "New Worlds in Astroparticle Physics", Faro, Portugal, 8-10 January ...
Kokkotas, Kostas D. +1 more
openaire +2 more sources
Gravitational Wave Sources: An Overview [PDF]
AIP Conference Proceedings, 2003 With full‐sensitivity operation of the first generation of gravitational wave detectors now just around the corner, and with the LISA space‐based detector entering its final design stage, I review the wide variety of predicted sources from the perspective of what further theoretical work may be needed to assist in their detection. Some sources, such as
openaire +2 more sources
Localization of transient gravitational wave sources: beyond triangulation [PDF]
, 2017 Rapid, accurate localization of gravitational wave transient events has proved critical to successful electromagnetic followup. In previous papers we have shown that localization estimates can be obtained through triangulation based on timing information
S. Fairhurst
semanticscholar +1 more source
Multimessenger Probes of High-energy Sources [PDF]
EPJ Web of Conferences, 2019 Multimessenger observations may hold the key to learn about the most energetic sources in the universe. The recent construction of large scale observatories opened new possibilities in testing non thermal cosmic processes with alternative probes, such as
Guetta Dafne
doaj +1 more source
A new gravitational wave verification source [PDF]
Monthly Notices of the Royal Astronomical Society: Letters, 2014 Abstract We report the discovery of a detached 20-min orbital period binary white dwarf (WD). WD 0931+444 (SDSS J093506.93+441106.9) was previously classified as a WD + M dwarf system based on its optical spectrum. Our time-resolved optical spectroscopy observations obtained at the 8 m Gemini and 6.5 m MMT reveal peak-to-peak radial ...
M. Kilic +5 more
openaire +2 more sources
Inferring the lensing rate of LIGO–Virgo sources from the stochastic gravitational wave background [PDF]
, 2020 Strong lensing of gravitational waves is more likely for distant sources but predicted event rates are highly uncertain with many astrophysical origins proposed. Here we open a new avenue to estimate the event rate of strongly lensed systems by exploring
S. Mukherjee +4 more
semanticscholar +1 more source
Narrow-band search for gravitational waves from known pulsars using the second LIGO observing run
, 2022 Isolated spinning neutron stars, asymmetric with respect to their rotation axis, are expected to be sources of continuous gravitational waves. The most sensitive searches for these sources are based on accurate matched filtering techniques that assume ...
LIGO Scientific Collaboration and Virgo Collaboration +2 more
core +1 more source
CATACLYSMIC VARIABLES AS SOURCES OF GRAVITATIONAL WAVES [PDF]
The Ninth Marcel Grossmann Meeting, 2002 10 pages, 2 eps figures, (A&A) Latex. A&A (in press)
Meliani, M. T. +2 more
openaire +2 more sources
Localizing gravitational wave sources with single-baseline atom interferometers [PDF]
, 2017 Localizing sources on the sky is crucial for realizing the full potential of gravitational waves for astronomy, astrophysics, and cosmology. We show that the mid-frequency band, roughly 0.03 to 10 Hz, has significant potential for angular localization ...
P. Graham, Sunghoon Jung
semanticscholar +1 more source
Measuring the Hubble Constant with Dark Neutron Star–Black Hole Mergers
The Astrophysical Journal, 2023 Detection of gravitational waves (GWs) from neutron star-black hole (NSBH) standard sirens provides local measurements of the Hubble constant ( H _0 ), regardless of the detection of an electromagnetic (EM) counterpart, given that matter effects can be ...
Banafsheh Shiralilou +6 more
doaj +1 more source