Volume 96, Issue 20
26 May 2006
On the Cover
Gravitational-wave energy density as a function of frequency (vertical) and time after a supernova core bounce (horizontal). Gravitational-wave bursts (purple) start about a half a second after the bounce, and may be detectable via LIGO.
From the article:
A New Mechanism for Gravitational-Wave Emission in Core-Collapse Supernovae
Christian D. Ott, Adam Burrows, Luc Dessart, and Eli Livne
Phys. Rev. Lett. 96, 201102 (2006)