Physics
Scientist
Kumamoto University, Japan
Adiabatic Exponent for Iron-Helium Transition and Pair Creation
On the Role of 14N in Helium Burning Phase in Stellar Evolution
The (N-14) (e-, nu) (C-14)(alpha, gamma)(O-18) reaction and helium flashes in accreting helium white dwarfs
The revised form of characteristic actions (h/2 pi)(s) in the structure of the universe
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