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.

In: Comptes Rendus Physique, Vol. 14, No. 4, 04.2013, p. 306-317.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Sperhake, U, Berti, E & Cardoso, V 2013, 'Numerical simulations of black-hole binaries and gravitational wave emission', Comptes Rendus Physique, vol. 14, no. 4, pp. 306-317. https://doi.org/10.1016/j.crhy.2013.01.004

APA

Sperhake, U., Berti, E., & Cardoso, V. (2013). Numerical simulations of black-hole binaries and gravitational wave emission. Comptes Rendus Physique, 14(4), 306-317. https://doi.org/10.1016/j.crhy.2013.01.004

Vancouver

Sperhake U, Berti E, Cardoso V. Numerical simulations of black-hole binaries and gravitational wave emission. Comptes Rendus Physique. 2013 Apr;14(4):306-317. https://doi.org/10.1016/j.crhy.2013.01.004

Author

Sperhake, Ulrich ; Berti, Emanuele ; Cardoso, Vitor. / Numerical simulations of black-hole binaries and gravitational wave emission. In: Comptes Rendus Physique. 2013 ; Vol. 14, No. 4. pp. 306-317.

Bibtex

@article{7a757b6897ce400a8ae5f58d90ffeec9,
title = "Numerical simulations of black-hole binaries and gravitational wave emission",
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.",
keywords = "Numerical relativity, Black holes, Gravitational wave physics, Astrophysics, APPARENT-HORIZON FINDER, SPIN EVOLUTION, INITIAL DATA, FINAL SPIN, MASS, RADIATION, COALESCENCE, MERGERS, MODELS, RECOIL",
author = "Ulrich Sperhake and Emanuele Berti and Vitor Cardoso",
year = "2013",
month = apr,
doi = "10.1016/j.crhy.2013.01.004",
language = "English",
volume = "14",
pages = "306--317",
journal = "Comptes Rendus Physique",
issn = "1631-0705",
publisher = "Elsevier",
number = "4",

}

RIS

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