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Frontiers of Physics, 2013
We are entering a new era of gravitational-wave astronomy. The ground-based interferometers have reached their initial design sensitivity in the audio band. Several upper limits have been set for anticipated astrophysical sources from the science data. The advanced detectors in the US and in Europe are expected to be operational around 2015.
Gabriela Gonzalez +2 more
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We are entering a new era of gravitational-wave astronomy. The ground-based interferometers have reached their initial design sensitivity in the audio band. Several upper limits have been set for anticipated astrophysical sources from the science data. The advanced detectors in the US and in Europe are expected to be operational around 2015.
Gabriela Gonzalez +2 more
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2021
The theory of General Relativity predicts that objects moving in a gravitational field should emit gravitational waves. This is analogous to the emission of electromagnetic waves by moving charged particles, but the effect is much weaker. Einstein himself at first doubted the reality of the effect, and later, although recognizing the effect, thought ...
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The theory of General Relativity predicts that objects moving in a gravitational field should emit gravitational waves. This is analogous to the emission of electromagnetic waves by moving charged particles, but the effect is much weaker. Einstein himself at first doubted the reality of the effect, and later, although recognizing the effect, thought ...
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Nature Physics, 2019
With the improving sensitivity of the global network of gravitational-wave detectors, we expect to observe hundreds of transient gravitational-wave events per year.
H. Gabbard +4 more
semanticscholar +1 more source
With the improving sensitivity of the global network of gravitational-wave detectors, we expect to observe hundreds of transient gravitational-wave events per year.
H. Gabbard +4 more
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Annalen der Physik, 2000
AbstractGravitational waves, as predicted by the theory of General Relativity, have been studied theoretically for many decades. However, due to the weak coupling of gravitation with matter, it has not yet been possible to measure them directly. Up to now, we only have indirect evidence of the existence and the effect of gravitational radiation by ...
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AbstractGravitational waves, as predicted by the theory of General Relativity, have been studied theoretically for many decades. However, due to the weak coupling of gravitation with matter, it has not yet been possible to measure them directly. Up to now, we only have indirect evidence of the existence and the effect of gravitational radiation by ...
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Classical and quantum gravity
In the first part of this work, we provide a curated overview of the theoretical framework necessary for incorporating dephasing due to environmental effects (EEs) in gravitational wave (GW) templates.
J'anos Tak'atsy +5 more
semanticscholar +1 more source
In the first part of this work, we provide a curated overview of the theoretical framework necessary for incorporating dephasing due to environmental effects (EEs) in gravitational wave (GW) templates.
J'anos Tak'atsy +5 more
semanticscholar +1 more source
Annual Review of Astronomy and Astrophysics, 1972
The "windows" of observational astronomy have become broader. They now include, along with photons from many decades of the electromagnetic spectrum, extraterrestrial "artifacts" of other sorts: cosmic rays, meteorites, particles from the solar wind, samples of the lunar surface, and neutrinos.
Press, William H., Thorne, Kip S.
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The "windows" of observational astronomy have become broader. They now include, along with photons from many decades of the electromagnetic spectrum, extraterrestrial "artifacts" of other sorts: cosmic rays, meteorites, particles from the solar wind, samples of the lunar surface, and neutrinos.
Press, William H., Thorne, Kip S.
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Uspekhi Fizicheskih Nauk, 1988
CONTENTS 1. Introduction. Gravitational-wave astronomy in action 940 2. Astronomical manifestations of gravitational waves 941 2.1. The binary radio pulsar PSR 1913 + 16. 2.2. Cataclysmic variables. 2.3. Type I supernovas. 3. Theory and some new results 942 3.1. Mathematical description of gravitational waves. 3.2. Relativistic celestial mechanics.
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CONTENTS 1. Introduction. Gravitational-wave astronomy in action 940 2. Astronomical manifestations of gravitational waves 941 2.1. The binary radio pulsar PSR 1913 + 16. 2.2. Cataclysmic variables. 2.3. Type I supernovas. 3. Theory and some new results 942 3.1. Mathematical description of gravitational waves. 3.2. Relativistic celestial mechanics.
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2016
The direct detection of gravitational waves announced on 11 February 2016 has opened a new window onto the universe. The gravitational wave spectrum extends from some nHz to several kHz. This chapter will firstly discuss the acoustic detectors, the first historically developed.
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The direct detection of gravitational waves announced on 11 February 2016 has opened a new window onto the universe. The gravitational wave spectrum extends from some nHz to several kHz. This chapter will firstly discuss the acoustic detectors, the first historically developed.
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Towards Gravitational Wave Astronomy
2014This chapter is meant to introduce the reader to the forthcoming network of second-generation interferometric detectors of gravitational waves, at a time when their construction is close to completion and there is the ambition to detect gravitational waves for the first time in the next few years and open the way to gravitational wave astronomy.
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Gravitational-wave physics and astronomy in the 2020s and 2030s
Nature Reviews Physics, 2021Matthew Bailes +2 more
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