Gravitational Waves III: Detecting Systems

Details Gravitational Waves III: Detecting Systems Gravitational Waves III: Detecting Systems

2010-04-14

arxiv.org/abs/1004.2470v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

12 pages 2 figures

Scientific paper

In a recent paper we have deduced the basic equations that predict the emission of gravitational waves (GW) according to the Einstein gravitation theory. In a subsequent paper these equations have been used to calculate the luminosities and the amplitudes of the waves generated by binary stars, pulsations of neutron stars, wobbling of deformed neutron stars, oscillating quadrupoles, rotating bars and collapsing and bouncing cores of supernovas. We show here how the GW could be detected in our laboratories. This paper, like the preceding ones, was written to graduate and postgraduate students of Physics.

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