Published July 13, 2004 | Version v1
Report

Surrogate Nuclear Reactions and the Origin of the Heavy Elements

Description

An innovative method for indirectly determining reaction cross sections via Surrogate Nuclear Reactions is presented. Exploring indirect approaches for obtaining reaction cross sections is important since a large number of nuclear reactions relevant to astrophysics cannot be measured with currently available techniques. A program is outlined for developing a comprehensive framework for planning and interpreting experiments that can yield the cross sections of interest. The applications will focus on reactions involving unstable nuclei that play a key role in the production of the elements between iron and uranium

Availability note (English)

Available from http://www.llnl.gov/tid/lof/documents/pdf/309567.pdf; PURL: https://www.osti.gov/servlets/purl/15014485-qrLy4U/native/

Additional details

Publishing Information

Imprint Pagination
vp.
Report number
UCRL-PROC--205320

Conference

Title
8. International Symposium on Nuclei in the Cosmos
Dates
19-23 Jul 2004
Place
Vancouver, British Columbia (Canada)

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
39050733
Subject category
S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
Resource subtype / Literary indicator
Conference, Non-conventional Literature
Descriptors DEI
ASTROPHYSICS; CROSS SECTIONS; IRON; NUCLEAR REACTIONS; NUCLEI; ORIGIN; UNIVERSE; URANIUM
Descriptors DEC
ACTINIDES; ELEMENTS; METALS; PHYSICS; TRANSITION ELEMENTS

Optional Information

Contract/Grant/Project number
W-7405-ENG-48
Notes
PDF-FILE: 6 ; SIZE: 92.4 KBYTES
Funding organization
US Department of Energy (United States)