Nuclei – Formation of Elements and Fundamental Properties

The chemical composition of our universe shows some surprising peculiarities: The sun mainly consists of hydrogen and helium; iron is much more abundant on Earth compared to heavy elements like gold. Nucleosynthesis follows reaction paths involving fusion and capture processes, some of them yet mostly unexplained. Since nuclear fusion stops at iron, heavier elements are generated via proton or neutron capture under extreme conditions like in supernova explosions of stars or in hot environments like accretion discs around Black Holes or neutron stars.

Based on Einstein’s principle of mass-energy equivalence, high-precision mass measurements are used to determine nuclear binding energies which are crucial for reaction pathways in nucleosynthesis. In combination with theoretical models, the structure of nuclei even far from stability can be investigated. Mass measurements on these mostly short-lived exotic (e. g. neutron-rich) nuclei are used to explore the “terra incognita” on the chart of nuclides. This helps to figure out how many nuclides exist at all.

The proton mass (simplest nucleus) determined with unprecedented precision was found to be smaller than the previously accepted value. This helps to understand observed discrepancies in the masses of light nuclei.

Division Blaum

Penning Traps: Precision Measurements on Single Ions (pdf)

Ion Traps

Ions can be stored in traps by the superposition of electric and magnetic fields in an extreme vacuum. Penning traps allow storage of a single ion that performs a characteristic oscillating circular motion in the trap. The ion’s mass and further properties can be deduced from the frequency if the charge state and the magnetic field strength are known, even in the case of exotic particles that live only for a few milliseconds. Penning-trap mass spectrometers are operated at MPIK and at radioactive beam facilities like GSI and CERN.

In an electron-beam ion trap (EBIT), highly charged ions are produced by impact of energetic electrons, then spatially confined, and electronically heated up to temperatures of millions of degrees. Both, stationary and mobile EBITs are used to prepare and study atomic matter under extreme conditions. A suite of accurate spectroscopic instrumentation attached to the EBITs collects precise data. A new cryogenic ion trap (Cryogenic Paul Trap Experiment: CryPTEx) has been built at MPIK in cooperation with the university of Aarhus, in which ion crystals can be produced by means of laser cooling and highly charged ions cooled therein.

Division Blaum    Division Pfeifer

Penning Traps: Precision Measurements on Single Ions (pdf)
Captive Stars in the Laboratory: Highly Charged Ions at 100 Millionen Degrees (pdf)

Highly Charged Ions – Matter under Extreme Conditions

Highly charged ions (HCIs) are found in hot environments of more than one million degrees such as stellar atmospheres and cores, supernova remnants or accretion discs around neutron stars and black holes. In fact, most of the visible matter in the Universe is assumed to be highly ionized. Analysis of the observed light (visible, UV, or X-ray) from these ions needs support by theoretical structure calculations which are often not accurate enough to determine e. g. the temperature of the hot environment. The controlled production of highly charged ions in an EBIT combined with high-precision spectroscopy provides direct experimental information. One example is the investigation of the X-ray absorption of highly charged iron ions at the synchrotron PETRA III (DESY) which provided important new insight into the radiation transport within stars.

The cryogenic ion trap CryPTEx provides efficient cooling of trapped HCIs for high-precision laser spectroscopy. In collaboration with the PTB (Braunschweig), the MPIK contributes to the development of novel optical clocks using quantum logic spectroscopy. The ultimate goal will be to test the time dependence of natural constants.

Division Pfeifer     Division Keitel

Captive Stars in the Laboratory: Highly Charged Ions at 100 Millionen Degrees (pdf)