Synthesis of 4N- and Their Neighboring Nuclei by the Rapid Nuclear Process

Details Synthesis of 4N- and Their Neighboring Nuclei by the Rapid Nuclear Process Synthesis of 4N- and Their Neighboring Nuclei by the Rapid Nuclear Process

May 1963

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1963pthph..29..699t&link_type=abstract

Progress of Theoretical Physics, Vol. 29, No. 5, pp. 699-711

Physics

1

Scientific paper

It is investigated whether or not the nucleogenesis in the range A = 20 {sim} 40 is carried out in terms of the proton capturing process in the outer layer of a supernova envelope. The reaction rates induced by protons and a-particles are calculated for density (10^{-5} {sim} 1) g/cm^3 at temperature (0.5 {sim} 1.5){×} 10^{9} ^{circ}K. As its result, it is found that the α-particle reactions are of negligible effects for the synthesis of elements in the range of interest. If the explosion time of a supernova may be assumed to be (2 {×} 5) {×} 10^3 sec, it is indicated that the relative abundances of the 4N-nuclei, ^{20}Ne, ^{24}Mg, ^{28}Si, ^{32}S, ^{36}A and ^{40}Ca can be explained by the proton capturing process starting from ^{20}Ne alone.

Affiliated with

Also associated with

No associations

Rating

Synthesis of 4N- and Their Neighboring Nuclei by the Rapid Nuclear 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 Synthesis of 4N- and Their Neighboring Nuclei by the Rapid Nuclear Process, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Synthesis of 4N- and Their Neighboring Nuclei by the Rapid Nuclear Process will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1180129