Numerical simulations of black-hole binaries and gravitational wave emission

Ulrich Sperhake*, Emanuele Berti, Vitor Cardoso

*Corresponding author af dette arbejde

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningpeer review

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Abstract

We review recent progress in numerical relativity simulations of black-hole (BH) spacetimes. Following a brief summary of the methods employed in the modeling, we summarize the key results in two major areas of BH physics: (i) BHs as sources of gravitational waves (GWs) and (ii) astrophysical systems involving BHs. We conclude with a list of the most urgent tasks for numerical relativity in these areas. (C) 2013 Academie des sciences. Published by Elsevier Masson SAS. All rights reserved.

OriginalsprogEngelsk
TidsskriftComptes Rendus Physique
Vol/bind14
Udgave nummer4
Sider (fra-til)306-317
Antal sider12
ISSN1631-0705
DOI
StatusUdgivet - apr. 2013
Udgivet eksterntJa

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