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Gravitational Waves from Core-Collapse Supernovae
Below we present GWs from our most recent simulations. We invite you to check out the repository at StellarCollapse.org for GW generated by other groups.
Non-rotating progenitors
Series A
We present the gravitational wave signatures for a suite of core-collapse supernovae models. These models correspond to progenitors with masses in the range between 12 and 25 solar mass and are axisymmetric. More details of these simulations can be found in our paper Yakunin et al., 2010.
Attachments
- rhplus-B12-WH07.tgz (112.0 KB) - added by reubendb 6 years ago.
- rhplus-B15-WH07.tgz (72.1 KB) - added by reubendb 6 years ago.
- rhplus-B20-WH07.tgz (66.4 KB) - added by reubendb 6 years ago.
- rhplus-B25-WH07.tgz (73.4 KB) - added by reubendb 6 years ago.
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GW_C15-3D_Filter_Polar.dat
(1.1 MB) -
added by lentz 4 years ago.
C15-3D Polar view, filtered
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GW_C15-3D_Filter_Equatorial.dat
(1.1 MB) -
added by lentz 4 years ago.
C15-3D Equatorial view, filtered
