Lithium-Containing Crystals for Light Dark Matter Search Experiments
Journal article, 2020

In the current direct dark matter search landscape, the leading experiments in the sub-GeV mass region mostly rely on cryogenic techniques which employ crystalline targets. One attractive type of crystals for these experiments is those containing lithium, due to the fact that 7Li is an ideal candidate to study spin-dependent dark matter interactions in the low mass region. Furthermore, 6Li can absorb neutrons, a challenging background for dark matter experiments, through a distinctive signature which allows the monitoring of the neutron flux directly on site. In this work, we show the results obtained with three different detectors based on LiAlO 2, a target crystal never used before in cryogenic experiments.

Lithium

Cryogenic

Dark matter

Spin-dependent

Neutrons

Author

E. Bertoldo

Max Planck Society

A. H. Abdelhameed

Max Planck Society

G. Angloher

Max Planck Society

P. Bauer

Max Planck Society

A. Bento

Max Planck Society

University of Coimbra

R. Breier

Comenius University in Bratislava

C. Bucci

Laboratori Nazionali del Gran Sasso

L. Canonica

Max Planck Society

A. D’Addabbo

Laboratori Nazionali del Gran Sasso

Gran Sasso Science Institute (GSSI)

S. Di Lorenzo

Gran Sasso Science Institute (GSSI)

Laboratori Nazionali del Gran Sasso

A. Erb

Walther-Meissner-Institute for Low Temperature Research

Technical University of Munich

F. V. Feilitzsch

Technical University of Munich

N. Ferreiro Iachellini

Max Planck Society

S. Fichtinger

Austrian Academy of Sciences

D. Fuchs

Max Planck Society

A. Fuss

Atominstitut der Osterreichischen Universitaten

Austrian Academy of Sciences

P. Gorla

Laboratori Nazionali del Gran Sasso

D. Hauff

Max Planck Society

M. Jes̆kovský

Comenius University in Bratislava

J. Jochum

University of Tübingen

J. Kaizer

Comenius University in Bratislava

A. Kinast

Technical University of Munich

H. Kluck

Austrian Academy of Sciences

Atominstitut der Osterreichischen Universitaten

H. Kraus

University of Oxford

A. Langenkämper

Technical University of Munich

M. Mancuso

Max Planck Society

V. Mokina

Austrian Academy of Sciences

E. Mondragon

Technical University of Munich

M. Olmi

Gran Sasso Science Institute (GSSI)

Laboratori Nazionali del Gran Sasso

T. Ortmann

Technical University of Munich

C. Pagliarone

Universita di Cassino e del Lazio Meridionale

Laboratori Nazionali del Gran Sasso

V. Palus̆ová

Comenius University in Bratislava

L. Pattavina

Laboratori Nazionali del Gran Sasso

Technical University of Munich

F. Petricca

Max Planck Society

W. Potzel

Technical University of Munich

P. Povinec

Comenius University in Bratislava

F. Pröbst

Max Planck Society

F. Reindl

Austrian Academy of Sciences

Atominstitut der Osterreichischen Universitaten

J. Rothe

Max Planck Society

K. Schäffner

Max Planck Society

J. Schieck

Austrian Academy of Sciences

Atominstitut der Osterreichischen Universitaten

V. Schipperges

University of Tübingen

D. Schmiedmayer

Austrian Academy of Sciences

Atominstitut der Osterreichischen Universitaten

S. Schönert

Technical University of Munich

C. Schwertner

Atominstitut der Osterreichischen Universitaten

Austrian Academy of Sciences

M. Stahlberg

Atominstitut der Osterreichischen Universitaten

Austrian Academy of Sciences

L. Stodolsky

Max Planck Society

C. Strandhagen

University of Tübingen

R. Strauss

Technical University of Munich

I. Usherov

University of Tübingen

M. Willers

Technical University of Munich

Vanessa Zema

Laboratori Nazionali del Gran Sasso

Gran Sasso Science Institute (GSSI)

Chalmers, Physics, Subatomic and Plasma Physics

J. Zeman

Comenius University in Bratislava

M. Brützam

Leibniz Association

S. Ganschow

Leibniz Association

Journal of Low Temperature Physics

0022-2291 (ISSN) 1573-7357 (eISSN)

Vol. 199 1-2 510-518

Subject Categories (SSIF 2011)

Accelerator Physics and Instrumentation

Subatomic Physics

Astronomy, Astrophysics and Cosmology

DOI

10.1007/s10909-019-02287-3

More information

Latest update

1/16/2026