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Gravitational Waves from Gravitational Collapse

Author: A Buonanno
A Burrows
A Burrows
A Burrows
A Burrows
A Hayashi
A Hayashi
A Heger
A Heger
A Heger
A Heger
A Hungerford
A Hungerford
A Loeb
A Mezzacappa
A Mezzacappa
AI MacFadyen
AK Schenk
AL Watts
AR King
BF Schutz
BJ Carr
BK Pickett
California Institute of Technology
CD Ott
CJ Hogan
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CL Fryer
CW Misner
D Lai
D Lai
D Lai
D Proga
DJ Eisenstein
DK Nadyozhin
DT Wickramasinghe
E Baron
E Baron
E Baron
E Berger
E Bravo
E Cappellaro
E Müller
E Müller
E Müller
E Müller
E Müller
E Müller
E Müller
E Seidel
E Seidel
EE Salpeter
EMD Symbalisty
EW Leaver
F Brachwitz
FA Jenet
FD Macchetto
FD Swesty
G Bazan
GB Cook
H Dimmelmeier
H Dimmelmeier
H Dimmelmeier
H Dimmelmeier
H-T Janka
H-T Janka
H-T Janka
H-T Janka
H-T Janka
HA Bethe
HA Bethe
Hannover University
HC Spruit
I Baraffe
I Hachisu
I Iben
ID Novikov
J Isern
J Kormendy
J Toman
J Woodward
J-A Marck
J-L Tassoul
JC Wheeler
JD Brown
JD Brown
JE Tohline
JE Tohline
JL Friedman
JL Houser
JM Blondin
JM Centrella
JN Imamura
JN Imamura
JR Wilson
JR Wilson
K Kifonidis
K Kotake
K Kotake
K Kotake
K Nomoto
KCB New
KCB New
KCB New
KS Thorne
KS Thorne
KS Thorne
KS Thorne
L Blanchet
L Ferrarese
L Lindblom
L Lindblom
L Lindblom
L Lindblom
L Rezzolla
L Rezzolla
L Rezzolla
L Scheck
L Villain
LC Loveridge
LR Yungelson
LS Finn
LS Finn
LS Finn
M Alcubierre
M Bardeen
M Hamuy
M Herant
M Herant
M Kato
M Liebendörfer
M Rampp
M Rampp
M Saijo
M Saijo
M Saijo
M Shibata
M Shibata
M Shibata
M Shibata
M Shibata
M Shibata
M Shibata
M Shibata
M Shibata
Max Planck Institute for Astrophysics
Max Planck Institute for Astrophysics
MC Begelman
MD Duez
MG Haehnelt
MG Haehnelt
MG Haehnelt
MHPM Putten van
MHPM Putten van
MJ Rees
MS Turner
N Andersson
N Andersson
N Arnaud
N Stergioulas
N Stergioulas
NASA/ESA
National Astronomical Observatory
O Zanotti
P Arras
P Bodenheimer
P Gressman
P Haensel
P Podsiadlowski
PA Young
PB Jones
PB Jones
R Buras
R Epstein
R Epstein
R Maiolino
R Mayle
R Mönchmeyer
R Popham
R Ruffini
R Walder
RA Managan
RA Saenz
RA Saenz
RA Saenz
RF Stark
RH Durisen
RH Sanders
RL Bowers
RL Bowers
S Akiyama
S Bonazzola
S Cassisi
S Chandrasekhar
S Chandrasekhar
S Chandrasekhar
S Detweiler
S Kobayashi
S Kobayashi
S Ou
S Smith
S Starrfield
S Yamada
S Yu-ichirou
SA Colgate
SA Colgate
SA Colgate
SA Hughes
SC Yooun
SE Woosley
SE Woosley
SE Woosley
SL Shapiro
SL Shapiro
SL Shapiro
SL Shapiro
SN Nazin
SW Bruenn
SW Bruenn
T Abel
T Abel
T Foglizzo
T Nakamura
T Nakamura
T Piran
T Zwerger
TA Thompson
TW Baumgarte
TW Baumgarte
TW Baumgarte
TW Baumgarte
TW Baumgarte
TX Thuan
V Bromm
V Ferrari
V Ferrari
W Hillebrandt
WCG Ho
WD Arnett
Y Eriguchi
Y Sekiguchi
YT Liu
YT Liu
Publication venue: 'Living Reviews'
Publication date: 14/06/2002
Field of study

Gravitational wave emission from the gravitational collapse of massive stars has been studied for more than three decades. Current state of the art numerical investigations of collapse include those that use progenitors with realistic angular momentum profiles, properly treat microphysics issues, account for general relativity, and examine non--axisymmetric effects in three dimensions. Such simulations predict that gravitational waves from various phenomena associated with gravitational collapse could be detectable with advanced ground--based and future space--based interferometric observatories.Comment: 68 pages including 13 figures; revised version accepted for publication in Living Reviews in Relativity (http://www.livingreviews.org

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