next up previous
Next: angular distribution Up: ternary fission Previous: ternary fission

Tsien San-Tsiang et al.;P hys.Rev.71(1947), 128
2 heavy fr
agments + 1 light particle Particle Accompanied 252Cf Fission:


Table 1: Relative emission probabilities of the various ternary particles and first and second moments of the energy distribution for the spontanous fission of 252Cf.
ternary particle <E> [MeV] FWHM [MeV] Yield Lifetime [s]
3H  8.2±0.6  7.2±0.6  950±90  
4He+5He 15.7±0.2 10.9±0.2 104  
4He 16.4±0.2 10.3±0.3 8264±341  
5He 12.4±0.3  8.9±0.5 1736±274 1.1*10-21
6He+7He 12.3±0.5  9.0±0.5  270±30  
6He 12.6±0.5  8.9±0.5  223±26  
7He 11.0±1.5  8±2   47±9 4.1*10-21
8He 10.2±1.0 10.2±1.0   25±5  
Li 14.3±1.0 14.3±1.0   60±10  
Be 17.5±1.0 18±1  175±30  
B 21.2±1.0 19.3±1.0   13.5±4.0  
C 26±1 -   80±30  

About 90% of the ternary particles are tex2html_wrap_inline90 -particles and about 10% tritons, the remaining fraction being constituted by a large variety of particles. The relative emission probabilities of the various ternary particles are summarized in table 1 for the spontanous fission of 252Cf. The hydrogen and helium isotopes are always responsible for 99% of the ternary particle yield, while the heavier particles are very rarely emitted. Nevertheless, strong yield differences are observed between neighboring particles. In table 1, both the first and second moments of the energy distribution of ternary particles are also given. The main feature of the spectrum is a fairly wide Gaussian shape, with a slight excess of intensity at low energies. It is apparent that mean energies of the measured ternary particles increase with the nuclear charge and decrease within each element with increasing mass. The observed decrease of kinetic energy with increasing mass and constant Z can be understood by assuming very similar initial conditions for the vatious ternary particles. Indeed, for a given initial energy, the heavier particles will move more slowly, allowing the fission fragments to move further away before the particle is fully accelerated.

  



last update: 16.08.2002 Hans-Juergen Wollersheim HJW