Sensitivity study for s process nucleosynthesis in AGB stars-Reference-Cited by-同舟云学术

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Sensitivity study for s process nucleosynthesis in AGB stars

Published:2016-03 Issue: Volume:108 Page:1-14
ISSN:0092-640X
Container-title:Atomic Data and Nuclear Data Tables
language:en
Short-container-title:Atomic Data and Nuclear Data Tables

Author:

Koloczek A.,Thomas B.,Glorius J.,Plag R.,Pignatari M.,Reifarth R.^ORCID,Ritter C.,Schmidt S.,Sonnabend K.

Funder

HGF Young Investigators Project

Helmholtz International Center

Helmholtz Graduate School HGS-HIRe

DAAD

DFG

German Israeli Foundation

NAVI

EuroGenesis project MASCHE

European Research Council

European Union’s Seventh Framework Programme

SNSF

NuGrid

NSF

EU

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Reference34 articles.

1. Neutron Capture in Low‐Mass Asymptotic Giant Branch Stars: Cross Sections and Abundance Signatures

2. Thesprocess: Nuclear physics, stellar models, and observations

3. THE WEAKs-PROCESS IN MASSIVE STARS AND ITS DEPENDENCE ON THE NEUTRON CAPTURE CROSS SECTIONS

4. s‐Process Nucleosynthesis in Asymptotic Giant Branch Stars: A Test for Stellar Evolution

5. Therma Instability in Non-Degenerate Stars.

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2. Stellar s -process neutron capture cross section of Ce isotopes;Physical Review C;2024-02-29

3. Investigation of ^90,92Zr(n,γ)^91,93Zr in the s-process nucleosynthesis;Zeitschrift für Naturforschung A;2024-02-19

4. Measurement of the Tb159(n,γ) cross section at the CSNS Back-n facility;Physical Review C;2023-04-26

5. Stellar s-process neutron capture cross sections on ^ASe and ^ACe;EPJ Web of Conferences;2023

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