文摘
The experimental determination of atomic levels and the first ionization potential of the heaviest elements (<span id="mmlsi23" class="mathmlsrc"><span class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0168583X1630266X&_mathId=si23.gif&_user=111111111&_pii=S0168583X1630266X&_rdoc=1&_issn=0168583X&md5=1d790d33920f124900a54d68b8d01656" title="Click to view the MathML source">Z⩾100span><span class="mathContainer hidden"><span class="mathCode">span>span>span>) is key to challenge theoretical predictions and to reveal changes in the atomic shell structure. These elements are only artificially produced in complete-fusion evaporation reactions at on-line facilities such as the GSI in Darmstadt at a rate of, at most, a few atoms per second. Hence, highly sensitive spectroscopic methods are required. Laser spectroscopy is one of the most powerful and valuable tools to investigate atomic properties. In combination with a buffer-gas filled stopping cell, the Radiation Detected Resonance Ionization Spectroscopy (RADRIS) technique provides the highest sensitivity for laser spectroscopy on the heaviest elements. The RADRIS setup, as well as the measurement procedure, have been optimized and characterized using the <span id="mmlsi24" class="mathmlsrc"><span class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0168583X1630266X&_mathId=si24.gif&_user=111111111&_pii=S0168583X1630266X&_rdoc=1&_issn=0168583X&md5=0e1233178749809e818716d4ef33258b" title="Click to view the MathML source">αspan><span class="mathContainer hidden"><span class="mathCode">span>span>span>-emitter <span id="mmlsi1" class="mathmlsrc"><span class="formulatext stixSupport mathImg" data-mathURL="/science?_ob=MathURL&_method=retrieve&_eid=1-s2.0-S0168583X1630266X&_mathId=si1.gif&_user=111111111&_pii=S0168583X1630266X&_rdoc=1&_issn=0168583X&md5=e06ac1cc4cc31a3da79025c184a9788d" title="Click to view the MathML source"><sup>155sup>span><span class="mathContainer hidden"><span class="mathCode">span>span>span>Yb in on-line conditions, resulting in an overall efficiency well above 1%. This paves the way for a successful search of excited atomic levels in nobelium and heavier elements.