Axion Search in DarkSide-20k

Información del proyecto

ASiD

Identificador del acuerdo de subvención: 101031397

DOI

10.3030/101031397

Proyecto cerrado

Fecha de la firma de la CE 9 Marzo 2021

Fecha de inicio 1 Enero 2022

Fecha de finalización 31 Diciembre 2023

Financiado con arreglo a

• EXCELLENT SCIENCE - Marie Skłodowska-Curie Actions

Coste total

€ 212 933,76

Aportación de la UE

€ 212 933,76

Coordinado por

ROYAL HOLLOWAY AND BEDFORD NEW COLLEGE
United Kingdom

Periodic Reporting for period 1 - ASiD (Axion Search in DarkSide-20k)

Período documentado: 2022-01-01 hasta 2023-12-31

Resumen del contexto y de los objetivos generales del proyecto

The existence of dark matter was suggested in the early 20th century independently by multiple astronomers. Further evidence was provided by Vera Rubin’s observations of the velocity curves of the spiral galaxy. Nearly 85 % of the Universe is made up of yet-to-be discovered particles called dark matter. Two of the most promising candidates are relic axions and Weakly Interacting Massive Particles (WIMPs). If they exist, the dark matter particles must be non-baryonic, electrically neutral, and rarely interact with ordinary matter.

The Darkside-20k experiment uses a dual phase argon-based time projection chamber filled with underground liquid argon of 20-ton fiducial mass as target volume to detect the WIMP-nucleon scattering. The time projection chamber is placed inside the Laboratori Nazionali del Gran Sasso underneath the Gran Sasso mountains. The experiment uses photodetector modules made up of state-of-the-art silicon photomultipliers. U.K. is producing nearly a total of 6 sq. meter photodetector units for inner veto of DarkSide 20k.

In addition to searching wimps, the silicon inside the silicon photomultipliers itself can be used as a target for searching solar axions via axioelectric effect. This is analogues to photoelectric effect but with a solar axion instead of a photon. The energy required to promote an electron to conduction band in silicon is much lower than in liquid argon and liquid xenon.

Trabajo realizado desde el comienzo del proyecto hasta el final del período abarcado por el informe y los principales resultados hasta la fecha

The Darkside 20k is a low background search. Therefore, we expect a low occupancy during the experiment. We built a laser test stand at Royal Holloway to mimic the experimental conditions and calibrate the single photoelectron response. We cryogenically tested the tiles inside an ISO7 clean room. We kept the occupancy low by setting the intensity of the laser accordingly. We acquired data at a range of bias voltages above the breakdown and qualified the silicon photomultipliers at 7V above the breakdown. The quantities we qualified were signal to noise ratio, single photo electron response and noise spectra.

During the characterization, we found that the single photo electron response and the signal to noise ratio as a function of bias voltage was linear as expected. The noise spectra showed a characteristic shape which is an artifact of the front-end board electronics of the silicon photomultipliers. During the test, we identified bad tile behavior. These were mainly due to flaky connectors and smushed wire bonds. We used the noise analysis as an early warning system to identify this bad behavior in the test stand.

Avances que van más allá del estado de la técnica e impacto potencial esperado (incluida la repercusión socioeconómica y las implicaciones sociales más amplias del proyecto hasta la fecha)

The proposal went beyond the state-of-the-art and proposed the search for solar axions with the detector itself. Using the assayed silicon-32 beta decay spectrum, a PhD student is currently working on a Monte Carlo simulation to generate a sensitivity plot.

A simple table top setup to cryogenically test the silicon photomultipliers.

A picture of two silicon photomultiplier setup being prepared for cryogenic testing.