Dark Matter Search with the Nuclear Isomer Ta-180m
Bjoern Lehnert

TL;DR
This paper explores using the rare isotope Ta-180m to detect or constrain exotic dark matter interactions through direct detection experiments and geochemical analysis, offering a novel approach beyond traditional WIMP searches.
Contribution
It introduces a new method employing nuclear isomers, specifically Ta-180m, for dark matter detection, providing constraints on dark matter models with less resource-intensive experiments.
Findings
Set new limits on dark matter interactions with Ta-180m.
Proposed an indirect geochemical detection method for long-term decay signatures.
Demonstrated the feasibility of using nuclear isomers in dark matter searches.
Abstract
There is compelling cosmological and astrophysical evidence of dark matter comprising 27% of the energy budget of the Universe. However, dark matter has never been observed in direct detection experiments. The long-time favorite model of Weakly Interacting Massive Particles saw a large experimental effort with steady progress over recent decades. Since also these large-scale searches remain unsuccessful to date, it is compelling to look at more exotic dark matter models which can be constrained with new approaches and much less scientific resources. Using nuclear isomers is one of these approaches. Ta is the rarest known isotope with the longest-lived meta-stable state whose partial half-life limits are on the order of 10-10 yr. We investigate how strongly interacting dark matter and inelastic dark dark matter collides with Ta, leading to its…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Scientific Research and Discoveries · Particle physics theoretical and experimental studies
