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EGAS41 - Swansea University

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41 st EGAS CP 137 Gdańsk 2009<br />

Influence of target surface contamination on experimental UHV<br />

screening energies<br />

N. Targosz-Ślȩczka1 , K. Czerski 1,2 , A. Huke 2 , L. Martin 2 , P. Heide 2 , A.I. Kilic 1 ,<br />

D. Blauth 3 , H. Winter 3<br />

1 Institute of Physics, <strong>University</strong> of Szczecin, ul. Wielkopolska 15, 70-451 Szczecin, Poland<br />

2 Institut für Atomare Physik und Optik, Technische Universität Berlin, Hardenbergstr. 36,<br />

10623 Berlin, Germany<br />

3 Institut fr Physik, Humboldt-Universitt zu Berlin, Berlin, Germany<br />

The enhanced screening of the nuclear Coulomb potential due to the atomic electrons has<br />

lead been confirmed in many laboratory experiments. The electron screening effect in<br />

astrophysical plasmas can enhance nuclear reaction rates in the interior of stars by many<br />

orders of magnitude.<br />

However, a reliable comparison between experimental data and theoretical predictions<br />

is still ambiguous because of some systematic errors in experiments. The measurements<br />

on deuterium inside metals are heavily affected by the formation of surface contamination<br />

layers under beam irradiation even in ultra-high vacuum (UHV) system.<br />

Here, we present our recent experimental results obtained for deuteron fusion reactions<br />

taking place in the metallic Zr environment and give some rigorous calculations of the<br />

influence of surface contamination layers on UHV experimental data. We thoroughly<br />

analyzed the ion induced chemical surface reaction mechanisms and their influence on the<br />

obtained screening energies. Our investigations show that this process has crucial impact<br />

on the interpretation of the raw experimental data.<br />

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