# Measurement of the directional sensitivity of DMTPC detectors

**Authors:** Cosmin Deaconu, Michael Leyton, Ross Corliss, Gabriela Druitt, Richard, Eggleston, Natalia Guerrero, Shawn Henderson, Jeremy Lopez, Jocelyn Monroe,, Peter Fisher

arXiv: 1705.05965 · 2017-06-21

## TL;DR

This paper models the directional response of DMTPC detectors for dark matter detection, demonstrating that a 10-20 kg detector can confirm dark matter signals by correlating recoil directions with incident particle predictions.

## Contribution

The paper develops and validates a model of the directional sensitivity of DMTPC detectors, guiding the design of scalable detectors with dark matter detection capabilities.

## Key findings

- A validated model of detector directional response as a function of recoil energy.
- Scalability analysis indicating 10-20 kg detectors can confirm dark matter signals.
- Potential for decisive confirmation of dark matter interactions using directional detection.

## Abstract

The Dark Matter Time Projection Chamber (DMTPC) is a direction-sensitive detector designed to measure the direction of recoiling $^{19}$F and $^{12}$C nuclei in low-pressure CF$_4$ gas using optical and charge readout systems. In this paper, we employ measurements from two DMTPC detectors, with operating pressures of 30-60 torr, to develop and validate a model of the directional response and performance of such detectors as a function of recoil energy. Using our model as a benchmark, we formulate the necessary specifications for a scalable directional detector with sensitivity comparable to that of current-generation counting (non-directional) experiments, which measure only recoil energy. Assuming the performance of existing DMTPC detectors, as well as current limits on the spin-dependent WIMP-nucleus cross section, we find that a 10-20 kg scale direction-sensitive detector is capable of correlating the measured direction of nuclear recoils with the predicted direction of incident dark matter particles and providing decisive (3$\sigma$) confirmation that a candidate signal from a non-directional experiment was indeed induced by elastic scattering of dark matter particles off of target nuclei.

## Full text

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## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/1705.05965/full.md

## References

27 references — full list in the complete paper: https://tomesphere.com/paper/1705.05965/full.md

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Source: https://tomesphere.com/paper/1705.05965