10.07.2015 Views

Biennial Report 2005-2007 - Saha Institute of Nuclear Physics

Biennial Report 2005-2007 - Saha Institute of Nuclear Physics

Biennial Report 2005-2007 - Saha Institute of Nuclear Physics

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

<strong>Nuclear</strong> Sciences 492.3 Atomic <strong>Physics</strong>2.3.1 Sub-shell Ionisation2.3.1.1 The effect <strong>of</strong> multiple ionization on L subshell ionization <strong>of</strong> Au and U by 5-10 MeV C and Si ionsC +q and Si +q (q = 3, 4) ions in the energy range 5 10 MeV obtained from the Pelletron Accelerator,IOP, Bhubaneswar, were used to bombard thin W, Au and U targets to excite L X-rays. A Si(Li)detector having an energy resolution <strong>of</strong> 160 eV at 5.9 keV were used to detect these X-rays. Tomeasure the efficiency <strong>of</strong> the Si(Li) detector and to calibrate the system very accurately, thintargets <strong>of</strong> KBr, Ni, Zn, Sr, Mo, Ag and Sn targets were bombarded with 3 MeV proton beam.Back scattered particles were measured with a Si surface barrier detector simultaneously with theX-rays so as to avoid the error in target thickness measurements. Energy resolved peaks <strong>of</strong> L α , L β, L γ etc. lines excited by C and Si ions can be easily observed. When these spectra are comparedwith those induced by protons, shifting <strong>of</strong> the peak position towards the higher energy side andwidening <strong>of</strong> the peaks are observed. This is a clear signature <strong>of</strong> the multiple ionization. Evaluation<strong>of</strong> the subshell ionization cross sections and the extent <strong>of</strong> multiple ionization are in progress.D Mitra, S Santra, AC Mandal, M Sarkar, D Bhattacharya, G LapickiNAP2.3.1.2 Measurements <strong>of</strong> the angular distribution <strong>of</strong> L X-rays <strong>of</strong> Au and U in photoionisationLast year, a set <strong>of</strong> data was taken on the angular distribution <strong>of</strong> L X-rays <strong>of</strong> Au and U excited by a109 Cd source. When these data were thoroughly analysed, it was observed that at some points thedata had to be re-measured. In order to have a fresh set <strong>of</strong> data, we decided to repeat the wholeexperiment. Before going into the main experiment, an 241 Am source <strong>of</strong> 1 µCi was placed on anAl frame fixed at the centre <strong>of</strong> the angular distribution Table. With a Si(Li) detector, the L lines (which are isotropic in nature) emitted from the source were detected over the angular range from40 o to 140 o . The anisotropy <strong>of</strong> these lines are found to be 2% due to the misalignment <strong>of</strong> the table.Au and U foils were held vertical to the table with the help <strong>of</strong> the Al frame. The 109 Cd sourcewith the graded collimator was placed near the centre <strong>of</strong> the table so that the emerging X-raysfrom the source make an angle <strong>of</strong> 60 o with the normal to the foils. Keeping the source and thetarget positions fixed, the detector was moved to scan the whole angular range. Data were thenanalysed. It was observed that for Au, the angular anisotropy <strong>of</strong> the emitted L lines are within5% while for U it is within the experimental error. Our observation contradict the results <strong>of</strong> thegroups <strong>of</strong> Patiala, India and that <strong>of</strong> Turkey but are in agreement with the findings <strong>of</strong> the groups<strong>of</strong> Chandigarh and Japan.S Santra, D Mitra, M Sarkar, D Bhattacharya, PK DasNAP2.3.1.3 Numismatic StudyIn collaboration with the Centre for Archaeological Studies and Training (CAST) Kolkata, 15 silvercoins have been analysed with our EDXRF system. These coins were from the period <strong>of</strong> 1200 AD.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!