180Ta production in the classical s-process

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F60461373%3A22340%2F02%3A00007048" target="_blank" >RIV/60461373:22340/02:00007048 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

180Ta production in the classical s-process

Original language description

The production and survival of the quasistable isomer 180Ta during the stellar nucleosynthesis has remained a matter of discussion for years. A careful analysis of the available experimental data and theoretical calculations enabled us to reproducethe observed solar abundance of 180Ta in the classical s-process (kT=28 keV - 33 keV).

Czech name

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Czech description

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Type

A - Audiovisual production

CEP classification

BG - Nuclear, atomic and molecular physics, accelerators

OECD FORD branch

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Project

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Continuities

Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2002

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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