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Nature, 1970
NOWHERE should the nonlinear features of general relativity show up more clearly than in the collisional interaction of two gravitational waves. One of the direct consequences of the linearity of Maxwell's equations is that electromagnetic waves pass straight through each other, and this is probably one of the best attested facts of physics.
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NOWHERE should the nonlinear features of general relativity show up more clearly than in the collisional interaction of two gravitational waves. One of the direct consequences of the linearity of Maxwell's equations is that electromagnetic waves pass straight through each other, and this is probably one of the best attested facts of physics.
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Sources of gravitational waves
AIP Conference Proceedings, 2001We discuss the characteristic features of the signals emitted by some astrophysical sources of gravitational waves, that are most likely to be seen by gravitational detectors in the near future.
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2015
Introduction Gravitational waves are a consequence of Einstein’s General Theory of Relativity, first presented in 1915 and published in 1916 [1]. Einstein himself linearized his theory and derived wave equations and calculated the gravitational radiation produced by sources in the weak-field, slow-motion limit [2]. As described in the following Chapter,
Berger B. K. +6 more
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Introduction Gravitational waves are a consequence of Einstein’s General Theory of Relativity, first presented in 1915 and published in 1916 [1]. Einstein himself linearized his theory and derived wave equations and calculated the gravitational radiation produced by sources in the weak-field, slow-motion limit [2]. As described in the following Chapter,
Berger B. K. +6 more
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General Relativity and Gravitation, 1997
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GRAVITATIONAL WAVES AND THEIR DETECTION
Non-Accelerator Astroparticle Physics, 2005In these lectures I present the basic principles, the state of the art and the perspectives of gravitational wave detection.
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2006
Gravitational waves may reach the Earth in different forms which depend on the nature of the emitting source: they may be short bursts, outcome of a catastrophic event like the gravitational collapse or the coalescence of a binary system; they may be continuous, weak wavetrains emitted by a non axially symmetric, rotating neutron star or by binary ...
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Gravitational waves may reach the Earth in different forms which depend on the nature of the emitting source: they may be short bursts, outcome of a catastrophic event like the gravitational collapse or the coalescence of a binary system; they may be continuous, weak wavetrains emitted by a non axially symmetric, rotating neutron star or by binary ...
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Challenges and opportunities of gravitational-wave searches at MHz to GHz frequencies
Living Reviews in Relativity, 2021Odylio D Aguiar +2 more
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