Published January 2010
| Version v1
Journal article
Nuclear astrophysics with radioactive beams
Creators
- 1. Department of Physics, Texas A and M University, Commerce, TX 75429 (United States)
- 2. Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824 (United States)
- 3. National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, MI 48824 (United States)
Description
The quest to comprehend how nuclear processes influence astrophysical phenomena is driving experimental and theoretical research programs worldwide. One of the main goals in nuclear astrophysics is to understand how energy is generated in stars, how elements are synthesized in stellar events and what the nature of neutron stars is. New experimental capabilities, the availability of radioactive beams and increased computational power paired with new astronomical observations have advanced the present knowledge. This review summarizes the progress in the field of nuclear astrophysics with a focus on the role of indirect methods and reactions involving beams of rare isotopes.
Availability note (English)
Available from http://dx.doi.org/10.1016/j.physrep.2009.09.002Additional details
Identifiers
- DOI
- 10.1016/j.physrep.2009.09.002;
- arXiv
- arXiv:0909.5693v2;
- PII
- S0370-1573(09)00252-X;
Publishing Information
- Journal Title
- Physics Reports
- Journal Volume
- 485
- Journal Issue
- 6
- Journal Page Range
- p. 195-259
- ISSN
- 0370-1573
- CODEN
- PRPLCM
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41069424
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTROPHYSICS; AVAILABILITY; ISOTOPES; NEUTRON STARS; RESEARCH PROGRAMS
- Descriptors DEC
- PHYSICS; STARS
Optional Information
- Copyright
- Copyright (c) 2009 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.