Published January 2010 | Version v1
Journal article

Nuclear astrophysics with radioactive beams

  • 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.2009.09.002

Additional 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.