Inhomogeneous big-bang model, revived, and evolution of the light elements in cosmic rays

T. Kajino

doi:10.1016/0375-9474(95)00159-X

Inhomogeneous big-bang model, revived, and evolution of the light elements in cosmic rays

T. Kajino^*

^*此作品的通讯作者

National Astronomical Observatory of Japan

科研成果: 期刊稿件 › 文章 › 同行评审

16 引用（Scopus）

摘要

Inhomogeneous big-bang model for primordial nucleosynthesis allows higher universal mass density parameter of baryons than the standard homogeneous model does, which is marginally consistent with recent astronomical suggestion that some kind of dark matter is made of baryons. Observation of the enhanced heavy elements in metal weak dwarfs is proposed to test the inhomogeneous model. The studies of radioactive nuclear reactions help predict the theoretical abundances more precisely.

源语言	英语
页（从-至）	c339-c343
期刊	Nuclear Physics A
卷	588
期	1
DOI	https://doi.org/10.1016/0375-9474(95)00159-X
出版状态	已出版 - 29 5月 1995
已对外发布	是

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abstract = "Inhomogeneous big-bang model for primordial nucleosynthesis allows higher universal mass density parameter of baryons than the standard homogeneous model does, which is marginally consistent with recent astronomical suggestion that some kind of dark matter is made of baryons. Observation of the enhanced heavy elements in metal weak dwarfs is proposed to test the inhomogeneous model. The studies of radioactive nuclear reactions help predict the theoretical abundances more precisely.",

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DO - 10.1016/0375-9474(95)00159-X

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Inhomogeneous big-bang model, revived, and evolution of the light elements in cosmic rays

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