08–12 lug 2024
L'Aquila, Italy
Europe/Rome fuso orario

Studies of radioactive background from environment for a potential LXe dark matter experiment at Boulby

10 lug 2024, 16:20
1O 10m
L'Aquila, Italy

L'Aquila, Italy

Plenary sessions: Palazzo dell’Emiciclo, Sala Ipogea Parallel sessions: Palazzo dell’Emiciclo, Sala Ipogea - GSSI Rectorate, Auditorium - GSSI, Sala Rossa (MLH)
Poster Direct detection Poster session

Relatore

Jemima Tranter (University of Sheffield)

Descrizione

Rare event searches, such as those targeting dark matter interactions and neutrinoless double beta decay (0νββ), face challenges from gamma-rays originating in rock, contributing to electron recoil background. This report presents a dual investigation: measurements of natural radioactivity in rock samples from Boulby Mine and a simulation assessing shielding thickness for a future detector. The measurements provide data for normalising conditions in prospective experiments at Boulby. The simulation studies the effectiveness of water shielding around a detector, focusing on the Weakly Interacting Massive Particle (WIMP) energy range (0 – 20 keV) and the energy range near the 0νββ Q-value (2.458 MeV).

The study design features a simplified xenon-based detector with a 70-tonne active volume, encompassed by veto systems and water shielding. Our findings indicate that gamma-ray background is unlikely to persist through analysis cuts in the WIMP energy range. However, for 0νββ decay signal searches, adjustments will be required; the sensitivity of a next-generation detector demands a background of < 1 event per 10 years, necessitating a reduction in the fiducial volume of the detector.

Autore principale

Jemima Tranter (University of Sheffield)

Coautore

Dr. Paul Scovell (Boulby Underground Laboratory, STFC) Prof. Vitaly Kudryavtsev (University of Sheffield)

Materiali di presentazione