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Theoretical studies

Introduction

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 Our numerical facilities are suitable to carry out the study of the time evolution of various astrophysically interesting GW sources such as oscillating stars or stars that undergo a full gravitational collapse while a black hole is formed. We are also able to calculate the gravitational wave production, the form of the signals generated at the location of dynamical processes and the waveforms that can be observed in the distance.
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The RMKI Budapest Virgo Group
 -- GergelyDebreczeni - 19 Nov 2008
 
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