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2018

Macro detection using fluorescence detectors

Sidhu, Jagjit Singh, Abraham, Roshan Mammen, Covault, Corbin et al.

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Macroscopic dark matter (aka macros) constitutes a broad class of alternatives to particulate dark matter.

We calculate the luminosity produced by the passage of a single macro as a function of its physical cross section.
A general detection scheme is developed for measuring the fluorescence caused by a passing macro in the atmosphere that is applicable to any ground based or space based Fluorescence Detecting (FD) telescopes.
In particular, we employ this scheme to constrain the parameter space ($\sigma_{x} \mbox{ vs} \mbox{ M}_{x}$) of macros than can be probed by the Pierre Auger Observatory and by the Extreme Universe Space Observatory onboard the Japanese Experiment Module (JEM-EUSO).

Macro detection using fluorescence detectors · Around

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