Our Dark Matter Stopping in the Earth
H.B. Nielsen (Niels Bohr Institut), Colin D. Froggatt (Glasgow, University)

TL;DR
This paper proposes a model where dark matter consists of vacuum bubbles that interact with Earth and atmosphere, emitting specific radiation, potentially explaining why only DAMA-LIBRA detects dark matter signals underground.
Contribution
It introduces a novel dark matter model involving vacuum bubbles and analyzes their stopping behavior and radiation emission within Earth, explaining experimental detection discrepancies.
Findings
Dark matter pearls emit 3.5 keV radiation during Earth passage
They can reach deep underground detectors like DAMA-LIBRA
The model explains why only DAMA-LIBRA observes dark matter signals
Abstract
We have worked for some time on a model for dark matter, in which dark matter consists of small bubbles of a new speculated type of vacuum, which are pumped up by some ordinary matter such as diamond, so as to resist the pressure of the domain wall separating the two vacua. Here we put forward thoughts on, how such macroscopic pearls would have their surrounding dust cleaned off passing through the atmosphere and the Earth, and what their distribution would be as a function of the depth of their stopping point and the distribution of the radiation emitted from them. In our model we assume that they radiate 3.5 keV electrons and photons, after having been excited during their passage into the Earth. The purpose of such an estimation of the radiation distribution is to explain the truly mysterious fact that, among all the underground experiments seeking dark matter colliding with the…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Scientific Research and Discoveries
