Abstract
The Coulomb dissociation method was applied to several radiative capture processes of astrophysical interest. The method has an advantage of high experimental efficiency, which allow measurements with radioactive nuclear beams. The reactions {sup 13}N(p,{gamma}){sup 14}O and {sup 7}Be(p,{gamma}){sup 8}B are mainly discussed. They are the key reaction in the hot CNO cycle in massive stars and the one closely related to the solar neutrino problem, respectively. (orig.)
Motobayashi, T
[1]
- Dept. of Physics, Rikkyo Univ., Toshima, Tokyo (Japan)
Citation Formats
Motobayashi, T.
Coulomb dissociation studies for astrophysical thermonuclear reactions.
Germany: N. p.,
1998.
Web.
Motobayashi, T.
Coulomb dissociation studies for astrophysical thermonuclear reactions.
Germany.
Motobayashi, T.
1998.
"Coulomb dissociation studies for astrophysical thermonuclear reactions."
Germany.
@misc{etde_613417,
title = {Coulomb dissociation studies for astrophysical thermonuclear reactions}
author = {Motobayashi, T}
abstractNote = {The Coulomb dissociation method was applied to several radiative capture processes of astrophysical interest. The method has an advantage of high experimental efficiency, which allow measurements with radioactive nuclear beams. The reactions {sup 13}N(p,{gamma}){sup 14}O and {sup 7}Be(p,{gamma}){sup 8}B are mainly discussed. They are the key reaction in the hot CNO cycle in massive stars and the one closely related to the solar neutrino problem, respectively. (orig.)}
place = {Germany}
year = {1998}
month = {Jun}
}
title = {Coulomb dissociation studies for astrophysical thermonuclear reactions}
author = {Motobayashi, T}
abstractNote = {The Coulomb dissociation method was applied to several radiative capture processes of astrophysical interest. The method has an advantage of high experimental efficiency, which allow measurements with radioactive nuclear beams. The reactions {sup 13}N(p,{gamma}){sup 14}O and {sup 7}Be(p,{gamma}){sup 8}B are mainly discussed. They are the key reaction in the hot CNO cycle in massive stars and the one closely related to the solar neutrino problem, respectively. (orig.)}
place = {Germany}
year = {1998}
month = {Jun}
}