Daemons: Detection at Pulkovo, Gran Sasso, and Soudan
E.M. Drobyshevski, M.E. Drobyshevski, S.A. Ponyaev, I.S. Guseva

TL;DR
This paper reports the detection of daemons, hypothesized dark matter particles, using specialized detectors at Pulkovo, Gran Sasso, and Soudan, and interprets experimental data within the daemon paradigm to explain signals in dark matter detection experiments.
Contribution
It introduces a daemon detection method and provides a quantitative interpretation of DAMA and CoGeNT experimental results without additional hypotheses.
Findings
Detected daemon flux from near-Earth orbits with specific flux values.
Reinterpreted DAMA and CoGeNT signals as caused by daemons rather than WIMPs.
Suggested processing improvements for dark matter detection experiments.
Abstract
During a week of the March maximum in 2011, two oppositely installed direction-sensitive TEU-167d Dark Electron Multipliers (DEMs) recorded a flux of daemons from the near-Earth almost circular heliocentric orbits (NEACHOs). The flux measured from above is f \approx (8\pm3)\times10^-7 cm^-2 s^-1, and that from below is twice smaller. The difference may be due both to specific design features of the TEUs themselves, and to dissimilarities in the slope of trajectories along which objects are coming from above or from below. It is shown that the daemon paradigm enables a quantitative interpretation of DAMA and CoGeNT experiments with no additional hypotheses. Both the experiments record a daemon flux of f ~ 10^-6 cm^-2 s^-1 from strongly elongated Earth-crossing heliocentric orbits (SEECHOs), predecessors of NEACHOs. Recommendations are given for processing of DAMA/LIBRA data, which…
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