| Literature DB >> 27680707 |
Mustapha Laatiaoui1,2, Werner Lauth3, Hartmut Backe3, Michael Block1,2,4, Dieter Ackermann2, Bradley Cheal5, Premaditya Chhetri6, Christoph Emanuel Düllmann1,2,4, Piet van Duppen7, Julia Even1, Rafael Ferrer7, Francesca Giacoppo1,2, Stefan Götz1,2,4, Fritz Peter Heßberger1,2, Mark Huyse7, Oliver Kaleja2,8, Jadambaa Khuyagbaatar1,2, Peter Kunz9, Felix Lautenschläger6, Andrew Kishor Mistry1,2, Sebastian Raeder1,2,7, Enrique Minaya Ramirez1, Thomas Walther6, Calvin Wraith5, Alexander Yakushev1,2.
Abstract
Optical spectroscopy of a primordial isotope has traditionally formed the basis for understanding the atomic structure of an element. Such studies have been conducted for most elements and theoretical modelling can be performed to high precision, taking into account relativistic effects that scale approximately as the square of the atomic number. However, for the transfermium elements (those with atomic numbers greater than 100), the atomic structure is experimentally unknown. These radioactive elements are produced in nuclear fusion reactions at rates of only a few atoms per second at most and must be studied immediately following their production, which has so far precluded their optical spectroscopy. Here we report laser resonance ionization spectroscopy of nobelium (No; atomic number 102) in single-atom-at-a-time quantities, in which we identify the ground-state transition 1S01P1. By combining this result with data from an observed Rydberg series, we obtain an upper limit for the ionization potential of nobelium. These accurate results from direct laser excitations of outer-shell electrons cannot be achieved using state-of-the-art relativistic many-body calculations that include quantum electrodynamic effects, owing to large uncertainties in the modelled transition energies of the complex systems under consideration. Our work opens the door to high-precision measurements of various atomic and nuclear properties of elements heavier than nobelium, and motivates future theoretical work.Year: 2016 PMID: 27680707 DOI: 10.1038/nature19345
Source DB: PubMed Journal: Nature ISSN: 0028-0836 Impact factor: 49.962