Researchers from Norway, Hungary, Russia, Turkey, and the U.S. have studied the
least energetic light emitted by heated iron nuclei. This kind of light is also
called gamma radiation. It is about one million times more energetic than
visual light and cannot be seen with the naked eye.
Surprisingly, heated iron nuclei like to emit
low-energy radiation, the more so, the lower its energy. The
researchers found ten times more low-energetic light than
previously assumed. This result was first found out in an
experiment at the University of Oslo. There, researchers from five
institutions investigated the previously unaccessible region of
low-energy (0.5--3 MeV) gamma radiation emitted by warm (6--8 MeV
excited) iron nuclei. The MeV or Mega electron Volt is a
traditional measure of energy for nuclear physicists. It requires
26 quadrillion (a one followed by 15 zeros) MeV equal one food
calorie.
Often color is used to represent the preference to
absorb, scatter, and re-emit light at different energies, with red
light having less energy than blue light. According to this
picture, the experiment showed that heated iron nuclei are
'redder' than thought, by giving out a lot of low-energy gamma
radiation. Standard nuclear theory based on vast experimental data
predicts that radiation should be emitted mostly at much higher
energies of 10--15 MeV, which represent the region of 'blue light'
in nuclear physics. This high-energy light is governed by the well
known phenomena of the Giant Dipole Resonance connected to the
swinging of protons against neutrons, the two constituents of
nuclei. The results from Oslo suggested that besides this 'blue
light' (which is also seen in the experiment with the expected
intensity) a second, weaker source of 'red light' exists in heated
iron nuclei with a fifth of the energy.
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Data points: light emission (expressed as radiative strength) in heated iron
nuclei for different frequencies or gamma energies. Open circle: lowest
previous data point from literature. Solid line: standard nuclear theory
predicts emission in the 'blue' region of nuclear physics. Hatched area: excess
of 'red', low-energy radiation.
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The researchers kept their results quiet for two
years since nobody was able to understand the findings. They
contacted their Hungarian colleagues and a second experiment was
carried out at a Budapest reactor. It confirmed the earlier
results by using a different experimental method, including a
different nuclear reaction and different detection instruments.
Theorists in several countries will now try to
understand why heated iron nuclei emit so much low-energy gamma
radiation. Parallel to this, the experimentalists will continue
their effort and investigate new nuclei like molybdenum. Their
results might impact our understanding of giant star explosions
like supernovae where chemical elements are produced by nuclear
reactions. The outcomes will also be important for the projected
Rare Isotope Accelerator, a Department-of-Energy funded,
one-billion-dollar factory of very short-lived nuclei.
The present results will be published shortly in
the prestigious physics journal 'Physical Review Letters'. Among
the participating U.S. institutions are Ohio University, Lawrence
Livermore National Laboratory, Triangle University Nuclear
Laboratory, North Carolina State University, and Michigan State
University.
Reference: ``Large Enhancement of Radiative Strength for Soft Transitions
in the Quasicontinuum,''
A. Voinov, E. Algin,
U.Agvaanluvsan, T.Belgya, R.Chankova, M.Guttormsen, G.E.Mitchell,
J.Rekstad, A.Schiller, S.Siem,
Phys. Rev. Lett. 93, 142504 (2004).
More information here.
Contact: voinov@ohio.edu