Number 230, June 14, 1995 by Phillip F. Schewe and Ben Stein
HYPERDEFORMED NUCLEI even more distorted than superdeformed nuclei have
been found in recent experiments at Lawrence Berkeley Laboratory. When
two medium-sized nuclei collide off-center, they can fuse into a highly-spinning,
distorted nucleus which then sheds its rotational energy by emitting a
series of gamma rays. In the past few years, researchers have found numerous
examples of superdeformed nuclei, football-shaped particles with a 2-to-1
long-to-short axis ratio. But in recent experiments at LBL's 88-Inch Cyclotron,
even more oblong (3-to-1) nuclei have apparently been produced. Demetrios
Sarantites (314-935-6504) of Washington University in St. Louis and his
colleagues smashed a 230-MeV beam of vanadium-51 nuclei into a molybdenum-100
foil. Gamma rays and charged particles, detected by LBL's Gammasphere and
Microball arrays respectively, suggested the existence of hyperdeformed
gadolinium-147 nuclei. The existence of such nuclear states challenges
the current understanding of fission and fusion in nuclei with very high
angular momentum. One might expect such highly spinning nuclei to fragment
immediately into two smaller pieces. Instead, a very small fraction of
the hyperdeformed nuclei remain intact and merely get rid of their spins
by emitting gamma rays. (D.R. LaFosse et al., to appear in Physical Review
Letters, 26 June 1995.)
AN ACCELERATION GRADIENT OF 30 GeV/m has been achieved by scientists
from a consortium of labs in Japan. The researchers used short (1 psec)
and powerful (3 TW) laser pulses to excite waves in a plasma. Electrons
which had been injected into the plasma at an energy of 1 MeV were then
accelerated up to an energy of 25 MeV, all in a space of less than 1 mm,
for a net gradient of 30 GeV/m. For such ultrahigh acceleration gradients
to be useful for particle physics applications (squeezing the milelong
SLAC accelerator, say, into a space of only a few meters), the whole process
would have to be scaled up considerably. (K. Nakajima et al., Physical
Review Letters, 29 May 1995.)
THE MOST ELONGATED SOLAR SYSTEM OBJECT YET IMAGED is the asteroid 1620
Geographos. Like the most oblong nucleus described in the paragraph above,
the pototo-shaped Geographos has an aspect ratio (length/width) of about
3 (2.76 to be exact). The 5-km Geographos, which passed to within 0.034
astronomical units of Earth in August 1994, was photographed at radar wavelengths
by Caltech astronomers. Small asteroids are generally thought to be the
result of the breakup or collision of larger bodies. Laboratory fragmentation
studies suggest the average aspect ratio for pieces should be 1.4. Only
1% of fragments should be as oblong as Geographos. (S.J. Ostro et al.,
Nature, 8 June 1995.)
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