Temperatures and excitation energies of hot nuclei in the reactions of S32+Ag and O16+Ag at 30 MeV/nucleon

173Citations
Citations of this article
5Readers
Mendeley users who have this article in their library.
Get full text

Abstract

For the reactions of 30 MeV/nucleon O16 and S32 with Ag, singles and coincidence measurements have been made for heavy residues, fragments (3z14), and light charged particles (z2). Mass-velocity correlations for the residues and fragment-residue coincidences indicate that increasing residue velocities do correspond to increasing excitation energy. Excitation energies as high as 90% of those which would result from complete fusion are reached. The spectra of light particles detected in coincidence with residue groups having different average velocities are analyzed with a moving source fit. When recoil effects are properly taken into account, excellent fits to the data are obtained. From the energy spectra and multiplicities of particles emitted from a fusion-like source the initial temperatures of the primary composite nuclei are determined. The results suggest that a plateau temperature near 6.5 MeV is reached above excitation energies of 3 MeV/nucleon. The temperatures are compared to those resulting from various model calculations. © 1989 The American Physical Society.

Cite

CITATION STYLE

APA

Wada, R., Fabris, D., Hagel, K., Nebbia, G., Lou, Y., Gonin, M., … Tomasi, E. (1989). Temperatures and excitation energies of hot nuclei in the reactions of S32+Ag and O16+Ag at 30 MeV/nucleon. Physical Review C, 39(2), 497–515. https://doi.org/10.1103/PhysRevC.39.497

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free