Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

Astrophysical S-Factor for 16 0+ 16 0 within the Adiabatic Molecular Picture

Thumbnail Image

Date

2008

Authors

Diaz-Torres, Alexis
Gasques, Leandro Romero
Wiescher, M.

Journal Title

Journal ISSN

Volume Title

Publisher

World Scientific Publishing Company

Abstract

The astrophysical S-factor for 16O+16O is investigated within the adiabatic molecular picture. It very well explains the available experimental data. The collective radial mass causes a pronounced resonant structure in the S-factor excitation function, providing a motivation for measuring the 16O+16O fusion cross section at deep sub-barrier energies

Description

Keywords

Citation

URI

http://hdl.handle.net/1885/54136

Collections

ANU Research Publications

Source

International Journal of Modern Physics E - Nuclear Physics

Type

Journal article

Book Title

Entity type

Access Statement

License Rights

DOI

10.1142/S0218301308011331

Restricted until

2037-12-31

Downloads

File
Description
01_Diaz-Torres_Astrophysical_S-Factor_for__16_2008.pdf (161.02 KB)

DSpace software copyright © 2002-2026 LYRASIS

abcd