Published September 2005
| Version v1
Journal article
r-process isotopes in the 132Sn region
Creators
- 1. University of Notre Dame, Department of Physics, Notre Dame, IN (United States)
- 2. Virtual Institute for Nuclear Structure and Astrophysics (Germany)
- 3. Universitaet Mainz, Institut fuer Kernchemie, Mainz (Germany)
- 4. Joint Institute for Nuclear Astrophysics (United States)
Description
A correct understanding of r-process nucleosynthesis requires the knowledge of nuclear-structure properties far from β-stability and a detailed description of the possible astrophysical environments. With respect to nuclear data, in recent years the main focus at CERN/ISOLDE has been put on the 132Sn region to explore the role of the N=82 shell closure and its consequences on the r-process matter flow through the A ≅130 Solar-System r-abundance peak. (orig.)
Availability note (English)
Available from: http://dx.doi.org/10.1140/epjad/i2005-06-157-2Additional details
Identifiers
Publishing Information
- Journal Title
- European Physical Journal. A
- Journal Volume
- 25
- Journal Issue
- Suppl.1
- Journal Page Range
- p. 633-638
- ISSN
- 1434-6001
Conference
- Title
- 4. international conference on exotic nuclei and atomic masses
- Acronym
- ENAM '04
- Dates
- 12-16 Sep 2004
- Place
- Pine Mountain, GA (United States)
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- Germany
- INIS RN
- 36103701
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- INTERMEDIATE MASS NUCLEI; NEUTRON-RICH ISOTOPES; NUCLEAR PROPERTIES; NUCLEAR STRUCTURE; NUCLEOSYNTHESIS; R PROCESS
- Descriptors DEC
- BETA DECAY RADIOISOTOPES; BETA-MINUS DECAY RADIOISOTOPES; EVOLUTION; ISOTOPES; NUCLEI; RADIOISOTOPES; STAR EVOLUTION; SYNTHESIS
Optional Information
- Collaborations
- ISOLDE/IS333