6533b834fe1ef96bd129e011
RESEARCH PRODUCT
Atom-at-a-time laser resonance ionization spectroscopy of nobelium
Dieter AckermannA. K. MistryPeter KunzSebastian RaederF. LautenschlägerAlexander YakushevMichael BlockRafael FerrerS. GötzMustapha LaatiaouiThomas WaltherEnrique Minaya RamirezF. P. HeßbergerPiet Van DuppenHartmut BackeWerner LauthF. GiacoppoP. ChhetriJadambaa KhuyagbaatarOliver KalejaC. WraithBradley ChealJulia EvenChristoph E. DüllmannMark Huysesubject
PhysicsMultidisciplinary010308 nuclear & particles physicsFermiumchemistry.chemical_element[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural scienceschemistry13. Climate actionIonization0103 physical sciencesAtomAtomic numberNobeliumPhysics::Atomic PhysicsAtomic physics010306 general physicsSpectroscopyRelativistic quantum chemistryLawrenciumdescription
Resonance ionization spectroscopy of nobelium (atomic number 102) reveals its ground-state transition and an upper limit for its ionization potential, paving the way to characterizing even heavier elements via optical spectroscopy. Characterizing the heaviest elements in the periodic table is a gruelling task because they are radioactive, exist only for split seconds at a time and need to be artificially produced in sufficient quantities by complicated procedures. The heaviest element that has been characterized by optical spectroscopy is fermium, which has an atomic number of 100. Mustapha Laatiaoui et al. extend the methods used for fermium to perform optical spectroscopy on nobelium (atomic number 102). Through laser resonance ionization spectroscopy, they identify the ground-state transition of the atom and manage to investigate highly excited states called Rydberg states. This allows them to determine an upper limit for the atomic ionization potential of nobelium. This study opens the door to the characterization of even heavier elements such as lawrencium using optical spectroscopy. 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 elements1 and theoretical modelling can be performed to high precision2,3, 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 production4, 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 1S0 1P1. 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 calculations5,6,7,8 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 | journal | country | edition | language |
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2016-10-01 | Nature |