Possibility to determine the astrophysical S factor for the 7Be(p,γ)8B radiative capture from analysis of the 7Be(3He,d)8B reaction

Details Possibility to determine the astrophysical S factor for the 7Be(p,γ)8B radiative capture from analysis of the 7Be(3He,d)8B reaction Possibility to determine the astrophysical S factor for the 7Be(p,γ)8B radiative capture from analysis of the 7Be(3He,d)8B reaction

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phrvc..51.3472m&link_type=abstract

Physical Review C (Nuclear Physics), Volume 51, Issue 6, June 1995, pp.3472-3478

Physics

Nuclear Physics

27

Transfer Reactions, Elementary Particle Processes

Scientific paper

At very low energies of astrophysical interest, the 7Be(p,γ)8B reaction is almost totally peripheral. Consequently, the overall normalization of the cross section for this reaction is defined by the asymptotic normalization coefficient of the bound-state wave function of 8B in the two-body channel 7Be+p. The reaction 7Be(3He,d)8B is suggested as a tool to measure this asymptotic normalization coefficient thereby allowing one to define the absolute value of the astrophysical factor, S17(0), for the 7Be(p,γ)8B reaction.

Affiliated with

Also associated with

No associations

Rating

Possibility to determine the astrophysical S factor for the 7Be(p,γ)8B radiative capture from analysis of the 7Be(3He,d)8B reaction 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 Possibility to determine the astrophysical S factor for the 7Be(p,γ)8B radiative capture from analysis of the 7Be(3He,d)8B reaction, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Possibility to determine the astrophysical S factor for the 7Be(p,γ)8B radiative capture from analysis of the 7Be(3He,d)8B reaction will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-758214