Search for low mass WIMP dark matter with DarkSide-50

Author:

Kimura Masato1

Affiliation:

1. Nicolaus Copernicus Astronomical Center

Abstract

DarkSide-50 is a direct dark matter detection experiment at Laboratori Nazionali del Gran Sasso that uses argon as the target material. Exploiting the ionization signal from a dual-phase time projection chamber filled with low-radioactivity argon, it has set the most stringent exclusion limit on WIMPs with a mass of few \mathrm{GeV}/c^2GeV/c2. A new analysis has recently been carried out with a larger exposure, profiting from an improved understanding of the detector response and background model. An improvement of about a factor 10 in sensitivity is expected for a WIMP mass of 2 GeV/c^22.

Funder

Agence Nationale de la Recherche

European Metrology Programme for Innovation and Research

European Regional Development Fund

Fundacja na rzecz Nauki Polskiej

Fundação de Amparo à Pesquisa do Estado de São Paulo

Horizon 2020

Institut National de Physique Nucléaire et de Physique des Particules

Instituto Nazionale di Fisica Nucleare

Ministry of Education and Science of the Russian Federation

Narodowe Centrum Nauki

National Science Foundation

Science and Technology Facilities Council

United States Department of Energy

Publisher

Stichting SciPost

Subject

General Medicine

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