Searching for Dark Matter with Paleo-Detectors. (arXiv:1806.05991v3 [astro-ph.CO] UPDATED)
<a href="http://arxiv.org/find/astro-ph/1/au:+Baum_S/0/1/0/all/0/1">Sebastian Baum</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Drukier_A/0/1/0/all/0/1">Andrzej K. Drukier</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Freese_K/0/1/0/all/0/1">Katherine Freese</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Gorski_M/0/1/0/all/0/1">Maciej Górski</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Stengel_P/0/1/0/all/0/1">Patrick Stengel</a>
A large experimental program is underway to extend the sensitivity of direct
detection experiments, searching for interaction of Dark Matter with nuclei,
down to the neutrino floor. However, such experiments are becoming increasingly
difficult and costly due to the large target masses and exquisite background
rejection needed for the necessary improvements in sensitivity. We investigate
an alternative approach to the detection of Dark Matter-nucleon interactions:
Searching for the persistent traces left by Dark Matter scattering in ancient
minerals obtained from much deeper than current underground laboratories. We
estimate the sensitivity of paleo-detectors, which extends far beyond current
upper limits for a wide range of Dark Matter masses. The sensitivity of our
proposal also far exceeds the upper limits set by Snowden-Ifft et al. more than
three decades ago using ancient Mica in an approach similar to paleo-detectors.
A large experimental program is underway to extend the sensitivity of direct
detection experiments, searching for interaction of Dark Matter with nuclei,
down to the neutrino floor. However, such experiments are becoming increasingly
difficult and costly due to the large target masses and exquisite background
rejection needed for the necessary improvements in sensitivity. We investigate
an alternative approach to the detection of Dark Matter-nucleon interactions:
Searching for the persistent traces left by Dark Matter scattering in ancient
minerals obtained from much deeper than current underground laboratories. We
estimate the sensitivity of paleo-detectors, which extends far beyond current
upper limits for a wide range of Dark Matter masses. The sensitivity of our
proposal also far exceeds the upper limits set by Snowden-Ifft et al. more than
three decades ago using ancient Mica in an approach similar to paleo-detectors.
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