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.

Progenitor Mass	Source	Dh+(t) at 10 kpc
12 Msun	matter	Download
(A12-WH07)	neutrinos	Download
15 Msun	matter	Download
(A15-WH07)	neutrinos	Download
25 Msun	matter	Download
(A25-WH07)	neutrinos	Download

Series B

We provide the gravitational waveforms from four 2D core-collapse supernovae models. These models correspond to progenitors with masses 12, 15, 20 and 25M. Detailed description of these waveforms can be found in the paper ​Yakunin et al., 2015.

Model	Source	Dh+(t)
B12-WH07	matter/neutrino	Download
B15-WH07	matter/neutrino	Download
B20-WH07	matter/neutrino	Download
B25-WH07	matter/neutrino	Download

Series C

The gravitational wave signal (at 10 kpc) reported in ​Mezzacappa et al., 2020 from C15-3D simulation described in ​Lentz et.al, 2015.

Model	Source		Dh+(t), Dhx(t)
C15-3D	matter	Polar view (Default).	Download updated data
	matter	Equatorial view.	Download updated data