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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)

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