scholarly journals Gravitational wave extraction in simulations of rotating stellar core collapse

2011 ◽  
Vol 83 (6) ◽  
Author(s):  
C. Reisswig ◽  
C. D. Ott ◽  
U. Sperhake ◽  
E. Schnetter

2009 ◽  
Vol 80 (10) ◽  
Author(s):  
Christian Röver ◽  
Marie-Anne Bizouard ◽  
Nelson Christensen ◽  
Harald Dimmelmeier ◽  
Ik Siong Heng ◽  
...  


2010 ◽  
Vol 514 ◽  
pp. A51 ◽  
Author(s):  
S. Scheidegger ◽  
R. Käppeli ◽  
S. C. Whitehouse ◽  
T. Fischer ◽  
M. Liebendörfer


2017 ◽  
Vol 95 (6) ◽  
Author(s):  
K. Crocker ◽  
T. Prestegard ◽  
V. Mandic ◽  
T. Regimbau ◽  
K. Olive ◽  
...  




2008 ◽  
Vol 678 (2) ◽  
pp. 1142-1157 ◽  
Author(s):  
T. Z. Summerscales ◽  
Adam Burrows ◽  
Lee Samuel Finn ◽  
Christian D. Ott


2011 ◽  
Vol 7 (S279) ◽  
pp. 367-368
Author(s):  
Ken'ichiro Nakazato ◽  
Kohsuke Sumiyoshi

AbstractSome supernovae and gamma-ray bursts are thought to accompany a black hole formation. In the process of a black hole formation, a central core becomes hot and dense enough for hyperons and quarks to appear. In this study, we perform neutrino-radiation hydrodynamical simulations of a stellar core collapse and black hole formation taking into account such exotic components. In our computation, general relativity is fully considered under spherical symmetry. As a result, we find that the additional degrees of freedom soften the equation of state of matter and promote the black hole formation. Furthermore, their effects are detectable as a neutrino signal. We believe that the properties of hot and dense matter at extreme conditions are essential for the studies on the astrophysical black hole formation. This study will be hopefully a first step toward a physics of the central engine of gamma-ray bursts.



2018 ◽  
Vol 14 (S346) ◽  
pp. 397-416
Author(s):  
Michela Mapelli

AbstractWhat are the formation channels of merging black holes and neutron stars? The first two observing runs of Advanced LIGO and Virgo give us invaluable insights to address this question, but a new approach to theoretical models is required, in order to match the challenges posed by the new data. In this review, I discuss the impact of stellar winds, core-collapse and pair instability supernovae on the formation of compact remnants in both isolated and dynamically formed binaries. Finally, I show that dynamical processes, such as the runaway collision scenario and the Kozai-Lidov mechanism, leave a clear imprint on the demography of merging systems.



2009 ◽  
Vol 707 (2) ◽  
pp. 1173-1190 ◽  
Author(s):  
Jeremiah W. Murphy ◽  
Christian D. Ott ◽  
Adam Burrows


2020 ◽  
Vol 1 (2) ◽  
pp. 025014 ◽  
Author(s):  
Alberto Iess ◽  
Elena Cuoco ◽  
Filip Morawski ◽  
Jade Powell


2019 ◽  
Vol 878 (1) ◽  
pp. 13 ◽  
Author(s):  
Michael A. Pajkos ◽  
Sean M. Couch ◽  
Kuo-Chuan Pan ◽  
Evan P. O’Connor


Sign in / Sign up

Export Citation Format

Share Document