Trojan Horse Investigation for AGB Stellar Nucleosynthesis

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61389005%3A_____%2F22%3A00555175" target="_blank" >RIV/61389005:_____/22:00555175 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.3390/universe8020128" target="_blank" >https://doi.org/10.3390/universe8020128</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3390/universe8020128" target="_blank" >10.3390/universe8020128</a>

Result language
angličtina
Original language name
Trojan Horse Investigation for AGB Stellar Nucleosynthesis
Original language description
Asymptotic Giant Branch (AGB) stars are among the most important astrophysical sites influencing the nucleosynthesis and the chemical abundances in the Universe. From a pure nuclear point of view, several processes take part during this peculiar stage of stellar evolution thus requiring detailed experimental cross section measurements. Here, we report on the most recent results achieved via the application of the Trojan Horse Method (THM) and Asymptotic Normalization Coefficient (ANC) indirect techniques, discussing the details of the experimental procedure and the deduced reaction rates. In addition, we report also on the on going studies of interest for AGB nucleosynthesis.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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