Abstract
41Ca (t1/2 = 9.94 × 104 yrs) is an important stellar radionuclide and its production in the Early Solar System from various irradiation scenarios can help determine the viability of models of early stellar processes. A novel reaction technique has been under development and recently tested at the Nuclear Science Laboratory at the University of Notre Dame. This technique utilizes an “in-cathode” reaction method, where natural CaF2 material is packed into an ion source sample holder (cathode) and then irradiated and subsequently measured using Accelerator Mass Spectrometry (AMS) without the need for chemical processing afterward. The setup for the irradiation was performed using a 3He beam to measure the reaction natCa(3He,x)41Ca. Initial AMS results suggest additional complexity due to ion source sputtering rates and geometry, which will need to be explored further.
| Original language | English |
|---|---|
| Pages (from-to) | 50-55 |
| Number of pages | 6 |
| Journal | Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms |
| Volume | 533 |
| DOIs | |
| State | Published - Dec 15 2022 |
Funding
We would like to thank George Jackson at PRIME Lab for supplying us with all the AMS standard materials used for measurements. We would also like to thank Jerry Lingle of the NSL for helping design and machine all the required pieces for the new cathode holders and the many ND graduate students who sat shift on the FN for experiments. This work is supported by the National Science Foundation under Grant No. PHY-2011890 and the Nuclear Regulatory Commission award number 31310019 M0037.
Keywords
- 41Ca
- AMS
- Early solar system
- In-cathode activation
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