NUCLEAR ASTROPHYSICS WITH SECONDARY (RADIOACTIVE) BEAMS

Details NUCLEAR ASTROPHYSICS WITH SECONDARY (RADIOACTIVE) BEAMS NUCLEAR ASTROPHYSICS WITH SECONDARY (RADIOACTIVE) BEAMS

1995-02-15

arxiv.org/abs/nucl-th/9502036v1

Physics

Nuclear Physics

Nuclear Theory

10 Figures not included. Invited Talk, Int. Workshop Nucl. Phys., Oaxtepec, Mexico, 4-7 January '95.

Scientific paper

Some problems in nuclear astrophysics are discussed with emphasize on the ones central to the field which were not solved over the last two decades, including Helium Burning in Massive stars (the 12C(a,g)16O reaction) and the 8B Solar Neutrino Flux Problem (the 7Be(p,g)8B reaction). We demonstrate that a great deal of progress was achieved by measuring the time reverse process(es): the beta-delayed alpha-particle emission of 16N and the Coulomb dissociation of 8B, using radioactive beams (of 16N and 8B). In this way an amplification of the sought for cross section was achieved, allowing a measurement of the small cross section(s) of relevance for stellar (solar) process(es).

Affiliated with

Also associated with

No associations

Rating

NUCLEAR ASTROPHYSICS WITH SECONDARY (RADIOACTIVE) BEAMS 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 NUCLEAR ASTROPHYSICS WITH SECONDARY (RADIOACTIVE) BEAMS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and NUCLEAR ASTROPHYSICS WITH SECONDARY (RADIOACTIVE) BEAMS will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-518811