Published May 21, 2008 | Version v1
Journal article

Investigation of Stellar 26Si(p,γ)27P Reaction via Coulomb Dissociation

  • 1. Department of Physics, Rikkyo University, Tokyo 171-8501 (Japan)
  • 2. National Institute of Radiological Sciences, Chiba 263-8555 (Japan)
  • 3. RIKEN Nishina Center, RIKEN, Saitama 351-0198 (Japan)

Description

The Coulomb dissociation of the proton-rich nuclei 27P was studied experimentally using 27P beams at 57 MeV/nucleon with a lead target. The radiative widths of the low-lying excited state in 27P were deduced. The resonant capture reaction rate of stellar 26Si(p,γ)27P through these states was estimated using the measured radiative widths. The astrophysical implications obtained from the extracted reaction rate will be discussed

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1016
Journal Issue
1
Journal Page Range
p. 193-198
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
From the dawn of Universe to the formation of solar system
Acronym
10. international symposium on origin of matter and evolution of galaxies
Dates
4-7 Dec 2007
Place
Sapporo (Japan)

Optional Information

Notes
(c) 2008 American Institute of Physics