Gravitational Waves II: Emitting Systems
M.Cattani
TL;DR
This paper calculates gravitational wave emissions from various astrophysical systems using Einstein's theory, providing detailed luminosities and amplitudes for different sources.
Contribution
It offers comprehensive calculations of gravitational wave signals from multiple astrophysical phenomena based on Einstein's equations, serving as an educational resource.
Findings
Luminosities and amplitudes for binary stars and neutron star pulsations calculated.
Gravitational wave emissions from wobbling and oscillating neutron stars quantified.
Wave signals from collapsing supernova cores analyzed.
Abstract
We use the basic equations that predict the emission of gravitational waves according to the Einstein gravitation theory 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. This paper was written to graduate and postgraduate students of Physics.
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Taxonomy
TopicsPulsars and Gravitational Waves Research