Nuclear reactions in shock wave front during supernova events

Details Nuclear reactions in shock wave front during supernova events Nuclear reactions in shock wave front during supernova events

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....3..203l&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 3 p 203-206 (SEE N85-34862 23-93)

Physics

Shock Fronts, Shock Waves, Supernovae, Xenon Isotopes, Carbon, Deuterons, Helium, High Temperature, Neutrons, Nuclear Reactions, Protons

Scientific paper

The new unique isotopic anomalous coponent of Xe(XeX) was found in the carbonaceous chondrites. It is enriched in light shielded isotopes (124Xe and 126Xe) and in heavy nonshielded isotopes (134Xe and 136Xe. All characteristics of Xe-X can be explained by a model of nucleosynthesis of the Xe isotopes in shock wave front passed through the He envelope during supernova events. The light isotopes are created by p process and the heavy isotopes are created by n process (slow r process). They were captured with high temperature carbon grains condensing by supernova shock waves.

Affiliated with

Also associated with

No associations

Rating

Nuclear reactions in shock wave front during supernova events 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 reactions in shock wave front during supernova events, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nuclear reactions in shock wave front during supernova events will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-755097