Published January 1982
| Version v1
Journal article
Average /sup 186,187,188/Os(n,γ) cross sections and the age of the galaxy via 187Re decay to 187Os
Description
One measure of the age of the galaxy is derived from the Re-Os decay chronometer. The /sup 186,187/Os capture cross sections are crucially important in the use of this chronometer. In this note we describe a small revision of our measurements and point out the high degree of consistency of the measured cross sections with the revised results from other laboratories. Using a standard model of nucleosynthesis and these cross sections, the duration of r-process nucleosynthesis is estimated to be (8.9 +- 2.0) x 109 yr, the age of the galaxy to be roughly-equal13.5 x 109 yr and the universe to be roughly-equal14.5 x 109 yr
Additional details
Publishing Information
- Journal Title
- Phys. Rev., C
- Journal Volume
- 25
- Journal Issue
- 1
- Series
- Phys. Rev., C.
- Journal Page Range
- 208-212
- ISSN
- 0556-2813
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 13682156
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Descriptors DEI
- AGE ESTIMATION; CAPTURE; CROSS SECTIONS; DECAY; GALAXIES; KEV RANGE; NEUTRON REACTIONS; NUCLEOSYNTHESIS; OSMIUM 186 TARGET; OSMIUM 187 TARGET; OSMIUM 188 TARGET; R PROCESS; RHENIUM 187; UNIVERSE
- Descriptors DEC
- BARYON REACTIONS; BETA DECAY RADIOISOTOPES; BETA-MINUS DECAY RADIOISOTOPES; ENERGY RANGE; HADRON REACTIONS; HEAVY NUCLEI; ISOTOPES; NUCLEAR REACTIONS; NUCLEI; NUCLEON REACTIONS; ODD-EVEN NUCLEI; RADIOISOTOPES; RHENIUM ISOTOPES; STABLE ISOTOPES; STAR EVOLUTION; TARGETS; YEARS LIVING RADIOISOTOPES