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PHOTOMETRY OF RELATIVISTIC HEAVY NUCLEI (in Italian)

Journal Article · · Nuovo Cimento (Italy) Divided into Nuovo Cimento A and Nuovo Cimento B
OSTI ID:4810411
The photometric profile of the tracks of relativistic heavy nucled in nuclear emulsions was studied. A model for the track is developed according to which the track is made up of a central part of grains directly affected by the heavy nuclei and a peripheral part in which the darkening is due to the secondary electrons. The experimental results are in accord with this model. By measuring the darkening at a distance of more than 3.5 mu m from the axis of the track, a method is proposed for the identification of the charge Z of the heavy nuclei. This method appears to compete favorably with other standard methods. The possibility of using the half width as a parameter for the identification of the charge of heavy nuclei is also discussed. (auth)
Research Organization:
Istituto Nazionale di Fisica Nucleare, Florence; and Universita, Arcetri (Florence)
NSA Number:
NSA-16-010250
OSTI ID:
4810411
Journal Information:
Nuovo Cimento (Italy) Divided into Nuovo Cimento A and Nuovo Cimento B, Journal Name: Nuovo Cimento (Italy) Divided into Nuovo Cimento A and Nuovo Cimento B Vol. Vol: (10), 21: Suppl. No. 1; ISSN NUCIA
Country of Publication:
Country unknown/Code not available
Language:
Italian

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