Dark Matter-Electron Scattering from Aromatic Organic Targets
Carlos Blanco, J.I. Collar, Yonatan Kahn, Benjamin Lillard

TL;DR
This paper explores the potential of aromatic organic compounds, like xylene, as targets for detecting sub-GeV dark matter via electron scattering, using scintillator-based detection methods and existing measurements to set new constraints.
Contribution
It develops a formalism for DM-electron scattering in aromatic molecules, calculates expected rates, and applies this to existing scintillator data to establish new constraints on light dark matter.
Findings
Constraints on 3-100 MeV dark matter from scintillator data
Aromatic compounds are sensitive targets for light dark matter detection
Proposed scalable scintillator techniques could enhance detection sensitivity
Abstract
Sub-GeV dark matter (DM) which interacts with electrons can excite electrons occupying molecular orbitals in a scattering event. In particular, aromatic compounds such as benzene or xylene have an electronic excitation energy of a few eV, making them sensitive to DM as light as a few MeV. These compounds are often used as solvents in organic scintillators, where the de-excitation process leads to a photon which propagates until it is absorbed and re-emitted by a dilute fluor. The fluor photoemission is not absorbed by the bulk, but is instead detected by a photon detector such as a photomultiplier tube. We develop the formalism for DM-electron scattering in aromatic organic molecules, calculate the expected rate in p-xylene, and apply this calculation to an existing measurement of the single photo-electron emission rate in a low-background EJ-301 scintillator cell. Despite the fact that…
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