J S Yadav
Articles written in Pramana – Journal of Physics
Volume 20 Issue 4 April 1983 pp 287-292 Nuclear Physics
A search for superheavy nuclei tracks in extraterrestrial olivine crystals
J S Yadav A P Sharma G N Flerov V O Perelygin S G Stetsenko P Pellas C Perron R Antanasijevich B Jakupi Y Todorovich
A study is made for the search of superheavy nuclei in Marjalahti, Eagle Station and in other pallasite olivines. The olivine crystals are calibrated for heavy ion track lengths by using heavy ion beams from cyclotrons. The calibration for ultra heavy ions which are presently not available with sufficient energy to produce volume tracks in olivine crystals, is based on Katz and Kobetich model of track formation. The length spectrum of volume tracks, revealed by puncturing them with focussed Nd-glass laser beam, is measured and the abundances of different nuclei groups are calculated. Partial annealing has been used at 430°C for 32 hr which eliminates the interfering tracks due to nuclei of atomic number
Volume 21 Issue 5 November 1983 pp 323-328 Nuclear And Particle Physics
Study of1840Ar ion tracks in cellulose nitrate
Subhash Chander Shyam Kumar J S Yadav A P Sharma
Sample of cellulose nitrate (Russian) is exposed to1840Ar ions. The bulk etch rate has been studied at different etching temperatures and the activation energy for bulk etch rate has been calculated. The etched track lengths are measured for different etching times. The energy loss rate and range of1840Ar ions in CN(R) is also calculated. The critical threshold value for etchable track in CN(R) is determined by comparing the theoretical and experimental values of track length. The response curve of CN(R) is also presented.
Volume 22 Issue 1 January 1984 pp 17-30 Molecular Physics
The longest wavelength
Volume 27 Issue 1-2 July 1986 pp 89-104 Particle Physics
Ionization states of cosmic rays:
S Biswas R Chakraborti R Cowsik N Durgaprasad P J Kajarekar R K Singh M N Vahia J S Yadav N Dutt J N Goswami D Lal H S Mazumdar D V Subhedar M K Padmanabhan
The measurements of the ionization states, composition, energy spectra and spatial distribution of heavy ions of helium to iron of energies 10–100 MeV/amu in the anomalous cosmic rays are of major importance in understanding their origin which is unknown at present.
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