Determination of the 35Cl(n, p)35S reaction cross section and its astrophysical implications

Details Determination of the 35Cl(n, p)35S reaction cross section and its astrophysical implications Determination of the 35Cl(n, p)35S reaction cross section and its astrophysical implications

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994nupha.573..291d&link_type=abstract

Nuclear Physics A, Volume 573, Issue 2, p. 291-305.

Physics

Nuclear Physics

12

Nuclear Reactions

Scientific paper

The 35Cl(n, p)35S reaction cross section has been measured with thermal neutrons at the High Flux Reactor of the ILL (Grenoble) and with resonance neutrons at the linear accelerator GELINA of the IRMM (Geel). For the thermal cross section, a precise value of 440 +/- 10 mb was obtained. In the region up to about 100 keV neutron energy, several resonances were determined with high resolution. These data were used to calculate the maxwellian averaged cross section at various temperatures. Their impact on stellar-nucleo-synthesis calculations is discussed.

Affiliated with

Also associated with

No associations

Rating

Determination of the 35Cl(n, p)35S reaction cross section and its astrophysical implications 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 Determination of the 35Cl(n, p)35S reaction cross section and its astrophysical implications, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Determination of the 35Cl(n, p)35S reaction cross section and its astrophysical implications will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1506574