Numerical simulations of black-hole binaries and gravitational wave emission
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Numerical simulations of black-hole binaries and gravitational wave emission. / Sperhake, Ulrich; Berti, Emanuele; Cardoso, Vitor.
I: Comptes Rendus Physique, Bind 14, Nr. 4, 04.2013, s. 306-317.Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt
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TY - JOUR
T1 - Numerical simulations of black-hole binaries and gravitational wave emission
AU - Sperhake, Ulrich
AU - Berti, Emanuele
AU - Cardoso, Vitor
PY - 2013/4
Y1 - 2013/4
N2 - 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.
AB - 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.
KW - Numerical relativity
KW - Black holes
KW - Gravitational wave physics
KW - Astrophysics
KW - APPARENT-HORIZON FINDER
KW - SPIN EVOLUTION
KW - INITIAL DATA
KW - FINAL SPIN
KW - MASS
KW - RADIATION
KW - COALESCENCE
KW - MERGERS
KW - MODELS
KW - RECOIL
U2 - 10.1016/j.crhy.2013.01.004
DO - 10.1016/j.crhy.2013.01.004
M3 - Journal article
VL - 14
SP - 306
EP - 317
JO - Comptes Rendus Physique
JF - Comptes Rendus Physique
SN - 1631-0705
IS - 4
ER -
ID: 300165311