Correlation Between U/Th and Pb/Os Abundance Ratios and its Application in Nuclear Cosmochronology
The abundance ratios of radioactive elements U/Th and stable elements Pb/Os from the r -process are found to have a strong correlation. This correlation is quite robust with respect to astrophysical conditions. The U/Th–Pb/Os correlation is applied to provide customized initial abundance ratios U/Th...
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| Published in | The Astrophysical journal Vol. 988; no. 1; pp. 22 - 28 |
|---|---|
| Main Authors | , , , |
| Format | Journal Article |
| Language | English |
| Published |
Philadelphia
The American Astronomical Society
20.07.2025
IOP Publishing |
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| Online Access | Get full text |
| ISSN | 0004-637X 1538-4357 1538-4357 |
| DOI | 10.3847/1538-4357/ade390 |
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| Abstract | The abundance ratios of radioactive elements U/Th and stable elements Pb/Os from the r -process are found to have a strong correlation. This correlation is quite robust with respect to astrophysical conditions. The U/Th–Pb/Os correlation is applied to provide customized initial abundance ratios U/Th from the observed abundance ratios Pb/Os for six r -process enhanced metal-poor stars. The ages of these six metal-poor stars are predicted by the U/Th chronometer, which are approximately between 11 and 15 Gyr. Their ages are compatible with the cosmic age of 13.8 billion years predicted from the cosmic microwave background radiation. |
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| AbstractList | The abundance ratios of radioactive elements U/Th and stable elements Pb/Os from the r -process are found to have a strong correlation. This correlation is quite robust with respect to astrophysical conditions. The U/Th–Pb/Os correlation is applied to provide customized initial abundance ratios U/Th from the observed abundance ratios Pb/Os for six r -process enhanced metal-poor stars. The ages of these six metal-poor stars are predicted by the U/Th chronometer, which are approximately between 11 and 15 Gyr. Their ages are compatible with the cosmic age of 13.8 billion years predicted from the cosmic microwave background radiation. |
| Author | Wu, X. H. Huang, Y. Y. Cui, Q. Q. Zhang, S. Q. |
| Author_xml | – sequence: 1 givenname: Y. Y. surname: Huang fullname: Huang, Y. Y. organization: Fuzhou University Department of Physics, Fuzhou 350108, Fujian, wuxinhui@fzu.edu.cn People’s Republic of China – sequence: 2 givenname: Q. Q. surname: Cui fullname: Cui, Q. Q. organization: Fuzhou University Department of Physics, Fuzhou 350108, Fujian, wuxinhui@fzu.edu.cn People’s Republic of China – sequence: 3 givenname: X. H. surname: Wu fullname: Wu, X. H. organization: Peking University State Key Laboratory of Nuclear Physics and Technology, School of Physics, Beijing 100871, People’s Republic of China – sequence: 4 givenname: S. Q. surname: Zhang fullname: Zhang, S. Q. organization: Peking University State Key Laboratory of Nuclear Physics and Technology, School of Physics, Beijing 100871, People’s Republic of China |
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| Snippet | The abundance ratios of radioactive elements U/Th and stable elements Pb/Os from the r -process are found to have a strong correlation. This correlation is... The abundance ratios of radioactive elements U/Th and stable elements Pb/Os from the r-process are found to have a strong correlation. This correlation is... |
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| SubjectTerms | Abundance Background radiation Correlation Cosmic microwave background Measuring instruments Metallicity Nuclear abundances Nuclear astrophysics R-process Radioisotopes Stellar ages Thorium |
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| Title | Correlation Between U/Th and Pb/Os Abundance Ratios and its Application in Nuclear Cosmochronology |
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