Using experiments to understand the synthesis of the heaviest nuclei

NUCL 10

W. Loveland, lovelanw@onid.orst.edu, 100 Radiation Center, Oregon State University, Corvallis, OR 97331
The cross section for producing a heavy evaporation residue, σEVR, in a fusion reaction can be written as

σEVR=Σσcapture(Ecm,J)PCN(Ecm,J)Wsur

where σcapture(Ecm, J) is the capture cross section at center of mass energy Ecm and spin J and PCN is the probability that the projectile-target system will evolve inside the fission saddle point to form a completely fused system rather than re-separating (quasifission) and Wsur is the probability that the completely fused system will de-excite by neutron emission rather than fission. For a quantitative understanding of the synthesis of new heavy nuclei, one needs to understand σcapture, PCN, and Wsur for the reaction system under study. The capture cross sections are relatively well understood, but predictions of the values of Wsur and PCN differ by orders of magnitude. I describe some recent experiments that measure PCN by characterizing the fission angular distributions in these reactions and recent experiments that measure Wsur using direct counting of the emitted neutrons in these reactions.