Towards a Reliable Model for Dark Matter Search Experiments

Projektinformationen

SABRE

ID Finanzhilfevereinbarung: 703650

DOI

10.3030/703650

Das Projekt endete am 14 August 2017

EK-Unterschriftsdatum 19 April 2016

Startdatum 1 Juli 2016

Enddatum 30 Juni 2018

Finanziert unter

• EXCELLENT SCIENCE - Marie Skłodowska-Curie Actions

Gesamtkosten

€ 195 454,80

EU-Beitrag

€ 195 454,80

Koordiniert durch

IMPERIAL COLLEGE OF SCIENCE TECHNOLOGY AND MEDICINE
United Kingdom

Periodic Reporting for period 1 - SABRE (Towards a Reliable Model for Dark Matter Search Experiments)

Berichtszeitraum: 2016-07-01 bis 2018-06-30

Zusammenfassung vom Kontext und den Gesamtzielen des Projekts

The SABRE experiment aims to detect dark matter particles through an annual modulation of their interaction rate using thallium-doped sodium iodide (NaI(Tl)) crystals. To fully understand the detector response to a dark matter signal or background radiation, end-to-end simulations are essential: The aim of this project was to include the interaction of the incoming particle/radiation with the detector, signal dispersion and collection including a full optical model, as well as the subsequent processing by the data acquisition electronics. Measurements with a high-purity crystal during the proof of-principle phase will allow their intrinsic radiopurity to be fully characterized, which is a key input to the simulation. A measurement of the optical properties of the materials involved was another crucial part of the end-to-end simulation software. Using these results, we can also optimize the light collection efficiency of the detector and, with that, the sensitivity of the full-scale experiment.

Arbeit, die ab Beginn des Projekts bis zum Ende des durch den Bericht erfassten Berichtszeitraums geleistet wurde, und die wichtigsten bis dahin erzielten Ergebnisse

During the first half of the project, good progress was achieved in all work packages. For the software package, I focused on the Monte Carlo simulations to reproduce the interaction of signal and background with the detector. Such an interaction typically produces light in our setup, which then gets detected by photomultiplier tubes (PMTs). The replication of the PMT response was another important part of the recent work.
Furthermore, I worked with two Master’s students on a setup to measure the reflectivity of different materials. These measurements are important to a) decide, which ones to use in the experiment for an optimum light collection efficiency and b) to then be able to simulate how light travels through the detector. The work also included first optical simulations.

A measurement of the temperature dependency of the scintillation light from sodium iodide crystals was conducted together with Queen’s University, Canada. The initial data analysis shows some interesting effects; final evaluations are still ongoing.

We made good progress in reducing the radioactive contamination inside the NaI(Tl) crystals. However, we still experience problems scaling the procedure up to the required crystal size.

Fortschritte, die über den aktuellen Stand der Technik hinausgehen und voraussichtliche potenzielle Auswirkungen (einschließlich der bis dato erzielten sozioökonomischen Auswirkungen und weiter gefassten gesellschaftlichen Auswirkungen des Projekts)

The beneficiary received an offer from Switzerland and decided to accept it. As a result, thie fellowship was terminated.

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