On the Direct Detection of Dark Matter in the Stratosphere
G. Cantatore, H. Fischer, W. Funk, M. Karuza, A. Kryemadhi, M., Maroudas, Y. Semertzidis, K.Zioutas

TL;DR
This paper proposes a novel method for direct dark matter detection using balloon-based measurements in the stratosphere, focusing on dark photons and their potential conversion to photons facilitated by atmospheric conditions.
Contribution
It introduces a new atmospheric detection approach for dark matter, leveraging resonance effects and balloon flights to observe dark photon interactions in the stratosphere.
Findings
Dark photons can convert to photons in the ionospheric plasma.
Balloon missions can feasibly operate for 1-2 months at high altitudes.
The method allows for simultaneous searches of multiple dark matter candidates.
Abstract
We investigate the prospects for direct detection of Dark Matter (DM) particles, such as dark photons, incident on the upper atmosphere. A recent work relates the burst-like temperature excursions in the stratosphere at heights of ~38-47 km with incident invisible streaming matter. Surprisingly, dark photons match the reasoning presented in that work provided they constitute part of the local DM density. Dark photons mix with real photons with the same total energy without the need for an external field as would be required for instance for axions. Furthermore, the ionospheric plasma column above the stratosphere can enhance the dark photon to photon conversion due to resonance. The stratosphere is easily accessible via balloon flights. Balloon missions with up to a few tons of payload can be readily assembled to operate for 1-2 months at such atmospheric heights making for realistic…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Astrophysics and Cosmic Phenomena
