University of Hertfordshire

By the same authors

Astrophysical Reaction Rates as a Challenge for Nuclear Reaction Theory

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Documents

  • 1005

    Accepted author manuscript, 63.7 KB, PDF document

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Original languageEnglish
Title of host publication10th Int Symposium on Origin of Matter and Evolution of Galaxies
EditorsT. Shima, H.J. Ong, A. Tamii, T. Kishimoto, H. Toki, T. Kajino, S. Kubono
PublisherAmerican Institute of Physics
Pages247-254
Number of pages8
ISBN (Print)978-0-7354-0819-7
Publication statusPublished - 2010
Event10th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG10) - Osaka, Japan
Duration: 8 Mar 201010 Mar 2010

Publication series

NameAIP Conference Proceedings
Volume1269
ISSN (Print)0094-243X

Conference

Conference10th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG10)
Country/TerritoryJapan
CityOsaka
Period8/03/1010/03/10

Abstract

The relevant energy ranges for stellar nuclear reactions are introduced. Low-energy compound and direct reactions are discussed. Stellar modifications of the cross sections are presented. Implications for experiments are outlined.

ID: 1619544