Measurements of equilibrium and time-dependent energy spectra of beta rays from californium-252 fission fragments
Absolute measurements were made for the equilibrium and time-dependent beta-ray energy spectra from flssion fragments produced bv spontaneous fission of /sup 252/Cf. The beta rays were detected by a plastic scintillator, and the fission rate was monitored by a semiconductor detector. The equilibrium spectrum was measured from a /sup 252/Cf source permanently encapsulated between two Mylar foils thick enough to stop the fragments. The time-dependent measurements used a /sup 252/Cf source supported on a thin nickel foil and covered with a thin collodion foil. Virtually all fragments from this second source escaped the foils. By use of a special transport system, the time dependence of the /sup 252/ Cf beta-ray energy spectrum was measured for two cases: buildup of the spectrum following initiation of fragment collection on clean catcher foils, and decay of the spectrum following a period of fragment collection. The measured spectra were corrected for energy resolution effects by unfolding them with the use of a measured system response function. The measured data were used to generate empirical expressions for the equilibrium and time-dependent beta-ray spectra from /sup 252/Cf fission fragments. The total number of beta rays from one fission was estimated to be 6.7 plus or minus 0.3, while the total beta-ray energy was estimated to be 6.1 plus or minus 0.5 MeV. The results of the measurements were compared with the analogous measurements for thermal-neutron fission of /sup 235/U. High-energy transitions (5 to 10 MeV) found for /sup 235/ U fission were not found for /sup 252/Cf fission. (11 figures) (auth)
- Research Organization:
- Univ. of Illinois, Urbana
- NSA Number:
- NSA-29-017303
- OSTI ID:
- 4353204
- Journal Information:
- Nucl. Sci. Eng., v. 53, no. 1, pp. 47-60, Other Information: Orig. Receipt Date: 30-JUN-74
- Country of Publication:
- Country unknown/Code not available
- Language:
- English
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