The transduction of sound into light through the implosion of a bubble of g
as leads to a flash of light whose duration is delineated in picoseconds. C
ombined measurements of spectral irradiance, Mie scattering, and flash widt
h (as determined by time-correlated single-photon counting) suggest that so
noluminescence from hydrogen and noble-gas bubbles is radiation from a blac
kbody with temperatures ranging from 6000 K (H-2) to 20,000 K (He) and a su
rface of emission whose radius ranges from 0.1 mum (He) to 0.4 mum (Xe). Th
e state of matter that would admit photon-matter equilibrium under such con
ditions is a mystery. (C) 2001 Optical Society of America.