s-Processing in Asymptotic Giant Branch Stars in the Light of Revised Neutron-Capture Cross Sections
Current AGB stellar models provide an adequate description of the s-process nucleosynthesis that occurs. Nonetheless, they still suffer from many uncertainties related to the modeling of the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"...
| मुख्य लेखकों: | , |
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| स्वरूप: | लेख |
| भाषा: | English |
| प्रकाशित: |
MDPI AG
2021-07-01
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| श्रृंखला: | Universe |
| विषय: | |
| ऑनलाइन पहुंच: | https://www.mdpi.com/2218-1997/7/7/239 |