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© Roland Diehl,
MPE.
Impressum
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last update 25Feb2022 by rod
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...more about
my science themes
(for all curious people, rather that just the
specialists)
How can we
understand far-away cosmic objects and the physical
processes in their interiors? This is the general theme of
astrophysics. My own interests herein emphasize the
processes related to atomic nuclei and their physics.
Atomic nuclei are aggregates of neutrons and protons, the
elementary particles part-taking in the nuclear forces. As
created from the initial event of our cosmos, the big
bang, neutrons and protons have later combined and formed
a variety of compositions (atomic nuclei). This "cosmic
evolution of material composition" is far from understood,
yet provides the variety of the chemical elements which we
and our world is made of, such as Carbon, Oxygen, Silicon,
Iron, Gold, or Uranium.
Cosmic extremes in the interiors of stars and of
supernovae (their explosions) are violent enough to enable
transformations of nuclei, the generation of new nuclei.
Such environments are my main interest. This implies that
interaction energies of MeV, or ~a thousand times that of
atomic-electron related processes such as chemical burning
or optical light, are in the main focus. At such energies,
atomic nuclei are combined into new species, and
electromagnetic light at high energies, called gamma rays,
are the messengers of such processes. We now operate
telescopes in space, which record such radiation from
distant sources. The analysis and interpretation of such
data, in the context of theories of astrophysical sources
and processes, and of observations from other messengers,
are my interests pursued in my research.
A variety of publications which I made over the past years
are written in a way which make these themes
accessible to interested people other than experts. Here
is a collection:
Most-relevant for a broader audience:
More:
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