(nuclear physics, astrophysics) the relatively slow nucleosynthesis process, in giant stars, in which neutron capture synthesizes elements up to atomic mass number 210 (at which point alpha decay becomes a deterrent to further building)..
현재 검증된 한국어 뜻은 준비 중이며 영어 정의는 “(nuclear physics, astrophysics) the relatively slow nucleosynthesis process, in giant stars, in which neutron capture synthesizes elements up to atomic mass number 210 (at which point alpha decay becomes a deterrent to further building).”입니다.