Cross Section Measurement of ~2H(~8Li, ~9Li)~1H Reaction for Astrophysics Interesting

来源 :Annual Report for China Institute of Atomic Energy | 被引量 : 0次 | 上传用户:ztcld2003
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The standard model (SM) is know to produce fairly good agreement with primordial abundances ofnuclides up to mass 7 amu, and to produce very tiny abundances of the high-mass elements due primarilyto the lack of stable particles at 5 and 8 amu. The recently developed inhomogeneous models (IMs)predict that short-lived isotopes are created which allow for more reaction pathways, such as The standard model (SM) is know to produce fairly good agreement with primordial abundances of nuclides up to mass 7 amu, and to produce very tiny abundances of the high-mass factors due less toto the lack of stable particles at 5 and 8 amu. The recently developed inhomogeneous models (IMs) predict that short-lived isotopes are created which allow for more reaction pathways, such as
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