「nucleosynthesis」の共起表現一覧(1語右で並び替え)
該当件数 : 31件
gh neutron flux, such as during supernova | nucleosynthesis after core-collapse, and yields neutron-r |
This has some consequences on | nucleosynthesis and the abundance of the chemical element |
g bang cosmology, including baryogenesis, | nucleosynthesis and dark matter. |
dark matter can be inferred from Big Bang | nucleosynthesis, and observations of the cosmic microwave |
in baryogenesis, which underwent Big Bang | nucleosynthesis and was opaque to radiation. |
957, which proposed the theory of stellar | nucleosynthesis and set the frame-work for contemporary n |
ructure formation, the theory of big bang | nucleosynthesis, and the nature of dark energy. |
ng the final elements produced by stellar | nucleosynthesis, and thus the heaviest elements which do |
neutrons per cm2 per second, resulting in | nucleosynthesis by the s-process (slow-neutron-capture-pr |
neutrons per cm2 per second, resulting in | nucleosynthesis by the s-process (slow-neutron-capture-pr |
neutrons per cm² per second, resulting in | nucleosynthesis by the r-process (rapid-neutron-capture-p |
heavy elements is the s-process, which is | nucleosynthesis by means of slow neutron captures, primar |
l nuclear physics parameters for reliable | nucleosynthesis calculations in astrophysics. |
Neutron capture | nucleosynthesis describes two nucleosynthesis pathways: t |
is is the much better understood Big Bang | nucleosynthesis, during which light atomic nuclei began t |
grains preserve an isotopic record of the | nucleosynthesis in individual stars. |
ny other means than creation by r-process | nucleosynthesis in supernovae. |
to the rate of beta decay, as for stellar | nucleosynthesis in some stars, and yields nuclei with sta |
resent universe are the result of stellar | nucleosynthesis in stars, a theory largely developed by B |
accumulation of heavy elements by stellar | nucleosynthesis in the Galaxy. |
chief primordial isotope made in stellar | nucleosynthesis) is not known to be nucleogenic or radiog |
He made additions to the big bang | nucleosynthesis model that built upon the work of the cla |
(supernovae, the solar neutrino problem, | nucleosynthesis), neutrino physics (neutrino oscillations |
ure plays an important role in the cosmic | nucleosynthesis of heavy elements. |
e of the Hoyle state is essential for the | nucleosynthesis of carbon in helium-burning red giant sta |
The r-process is a | nucleosynthesis process, likely occurring in core-collaps |
ae is responsible for most of the natural | nucleosynthesis producing elements heavier than iron. |
Relations between | Nucleosynthesis Rates and the Metal Abundance, 1980, Astr |
Big bang | nucleosynthesis tells us that the early universe consiste |
During Big Bang | nucleosynthesis, the only elements that formed aside from |
In the case of big bang | nucleosynthesis, the problem is that large amounts of ord |
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