Resonance States in 22Mg, 26Si for Reaction Rates in the Rp-Process

Details Resonance States in 22Mg, 26Si for Reaction Rates in the Rp-Process Resonance States in 22Mg, 26Si for Reaction Rates in the Rp-Process

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005omeg.conf..367s&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2003. Held 17-19 November 2003 in RIKEN, Wako, Saitama, Japan. Edited by M Terasawa,

Astronomy and Astrophysics

Astrophysics

Scientific paper

Motivated by the need of spectroscopic data to better understand the astrophysical rp-process, we developed a new experimental method using the Grand Raiden magnet spectrometer to study proton rich nuclei with α and 3He induced reactions. The results of the 24Mg(4He,6He)22Mg reaction at 205 MeV and 0° are presented, showing states relevant for resonant reaction rate calculations of the proton capture 21Na(p,γ)22Mg and 18Ne(α,p)21Na reaction which controls the break-out of the hot CNO cycles at X-ray burst conditions. In addition, the results of the 28Si(4He,6He)26Si reaction are presented, showing states relevant to the production rate of 26Al in its ground state which provides models of the explosive hydrogen burning process in novae and supernovae.

Affiliated with

Also associated with

No associations

Rating

Resonance States in 22Mg, 26Si for Reaction Rates in the Rp-Process does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Resonance States in 22Mg, 26Si for Reaction Rates in the Rp-Process, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Resonance States in 22Mg, 26Si for Reaction Rates in the Rp-Process will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1466618