Published January 1, 2018 | Version v1
Journal article Metadata-only

Nucleosynthesis of Mo and Ru isotopes in neutrino-driven winds

Creators

  • 1. Institut für Kernphysik, Technische Universität Darmstadt (Germany)

Description

The solar system origin of the p-isotopes 92,94Mo and 96,98Ru is a long-lasting mystery. Several astrophysical scenarios failed to explain their formation. Moreover, SiC X grains show a different abundance ratio of 95,97Mo than in the solar system. We have investigated if neutrino-driven winds can offer a solution to those problems. (paper)

Availability note (English)

Available from http://dx.doi.org/10.1088/1742-6596/940/1/012030

Additional details

Identifiers

DOI
10.1088/1742-6596/940/1/012030;

Publishing Information

Journal Title
Journal of Physics. Conference Series (Online)
Journal Volume
940
Journal Issue
1
Journal Page Range
[3 p.]
ISSN
1742-6596

Conference

Title
7. Nuclear Physics in Astrophysics Conference
Dates
18-22 May 2015
Place
York (United Kingdom)

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
52066246
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ABUNDANCE; ASTROPHYSICS; MOLYBDENUM 92; MOLYBDENUM 94; MOLYBDENUM 97; NEUTRINOS; NUCLEOSYNTHESIS; RUTHENIUM 96; RUTHENIUM 98; SILICON CARBIDES; SOLAR SYSTEM; STELLAR WINDS
Descriptors DEC
CARBIDES; CARBON COMPOUNDS; ELEMENTARY PARTICLES; EVEN-EVEN NUCLEI; EVEN-ODD NUCLEI; FERMIONS; INTERMEDIATE MASS NUCLEI; ISOMERIC TRANSITION ISOTOPES; ISOTOPES; LEPTONS; MASSLESS PARTICLES; MOLYBDENUM ISOTOPES; NANOSECONDS LIVING RADIOISOTOPES; NUCLEI; PHYSICS; RADIOISOTOPES; RUTHENIUM ISOTOPES; SILICON COMPOUNDS; STABLE ISOTOPES; STELLAR ACTIVITY; SYNTHESIS