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Martin Martschini

Publications and source records attributed to Martin Martschini.

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Recent progress on interstellar radionuclides on Earth and the Moon

The detection of interstellar radionuclides in geological archives provides insights into nucleosynthesis in stars and stellar explosions as well as interstellar medium dynamics in the Local Bubble and the Local Interstellar Cloud. In this work, current projects to detect interstellar radionuclides with accelerator mass spectrometry will be reviewed. These projects aim to address unsolved questions regarding the timing and the origin of the influxes and to establish new radionuclides for future searches. For the first time, experimental evidence for an inhomogeneous deposition of interstellar 60Fe onEarthwill be presented and another potential source for 60Fe on Earth and the Moon, primary galactic cosmic rays, will be introduced.

astro-ph.SR

Catastrophic disruption of asteroid 2023 CX1 and implications for planetary defense

Mitigation of the threat from airbursting asteroids requires an understanding of the potential risk they pose for the ground. How asteroids release their kinetic energy in the atmosphere is not well understood due to the rarity of significant impacts. Ordinary chondrites, in particular L chondrites, represent a frequent type of Earth-impacting asteroids. Here, we present the first comprehensive, space-to-lab characterization of an L chondrite impact. Small asteroid 2023 CX1 was detected in space and predicted to impact over Normandy, France, on 13 February 2023. Observations from multiple independent sensors and reduction techniques revealed an unusual but potentially high-risk fragmentation behavior. The nearly spherical 650 $\pm$ 160 kg (72 $\pm$ 6 cm diameter) asteroid catastrophically fragmented around 28 km altitude, releasing 98% of its total energy in a concentrated region of the atmosphere. The resulting shockwave was spherical, not cylindrical, and released more energy closer to the ground. This type of fragmentation increases the risk of significant damage at ground level. These results warrant consideration for a planetary defense strategy for cases where a >3-4 MPa dynamic pressure is expected, including planning for evacuation of areas beneath anticipated disruption locations.

astro-ph.EP

Towards AMS measurements of $^{91}$Nb, $^{94}$Nb and $^{93}$Mo produced in fusion environment

Long-lived radionuclides, such as $^{91}$Nb, $^{94}$Nb and $^{93}$Mo, are expected to be produced in nuclear fusion reactors by reactions of high-energy neutrons with the structural material. Accurate predictions of waste categorization require experimental validation of simulation codes like FISPACT-II. This work explores the use of Ion-Laser InterAction Mass Spectrometry (ILIAMS) at the Vienna Environmental Research Accelerator (VERA) to measure these three radionuclides by accelerator mass spectrometry (AMS). The ILIAMS setup employs laser photodetachment to suppress their respective stable isobars: $^{91}$Zr, $^{94}$Zr and $^{94}$Mo, and $^{93}$Nb. For $^{91,94}$Nb measurements, NbO$_3^-$ is selected, with interferences from ZrO$_3^-$ suppressed by collisions with the He buffer gas in the ion cooler. The suppression can be enhanced by overlapping a 355\,nm laser with the ion beam. The lower limit for the suppression factor is 37000. In that way, we reach $^{91}$Zr/$^{93}$Nb and $^{94}$Zr/$^{93}$Nb levels of $1.2\,\times\,10^{-14}$ and $1.8\,\times\,10^{-14}$, respectively, in targets prepared from commercial Nb$_2$O$_5$. MoO$_3$ is suppressed by a factor of 4360, leading to a $^{94}$Mo/$^{93}$Nb interference of $1.28\,\times\,10^{-10}$ in the same targets. For $^{93}$Mo measurements, MoO$_2^-$ is selected, with interference from $^{93}$NbO$_2^-$ suppressed by 637\,nm photons by a factor of $5.5\,\times\,10^6$. This results in a $^{93}$Nb/$^\text{nat}$Mo level of $1.3\,\times\,10^{-13}$ in targets prepared from commercial MoO$_3$. Suppression factors as high as this are not achieved by isobar suppression techniques based on differences in energy loss, not even by AMS facilities with terminal voltages above 8.5\,MV.

physics.ins-det

Detection of $^{135}$Cs & $^{137}$Cs in environmental samples by AMS

The detection of low abundances of $^{135}$Cs in environmental samples is of significant interest in different fields of environmental sciences, especially in combination with its shorter-lived sister isotope $^{137}$Cs. The method of Ion-Laser InterAction Mass Spectrometry (ILIAMS) for barium separation at the Vienna Environmental Research Accelerator (VERA) was investigated and further improved for low abundance cesium detection. The difluorides BaF$_2^-$ and CsF$_2^-$ differ in their electron detachment energies and make isobar suppression with ILIAMS by more than 7 orders of magnitude possible. By this method, samples with ratios down to the order of $^{135,137}$Cs/$^{133}$Cs $\approx 10^{-11}$ are measurable and the $^{135}$Cs/$^{137}$Cs ratios of first environmental samples were determined by AMS.

physics.ins-det